text:
Showing results 21051 to 21100 out of 38103
25023 AT 2018oo 1 14:03:33.307 +56:13:05.77 Pan-STARRS1 Pan-STARRS1 PS18gp PS1 - GPC1 Y Y 19.78 i-Sloan 2018-01-30 14:51:21 PS1_Bot1
16760 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 14:03:33.307 +56:13:05.77 2018-01-30 14:51:21 19.78 i-Sloan 1 PSN PS18gp Pan-STARRS1
25024 AT 2018op 1 13:48:46.240 +45:31:50.91 Pan-STARRS1 Pan-STARRS1 PS18go PS1 - GPC1 Y Y 20.09 i-Sloan 2018-01-30 14:45:36 PS1_Bot1
16761 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 13:48:46.240 +45:31:50.91 2018-01-30 14:45:36 20.09 i-Sloan 1 PSN PS18go Pan-STARRS1
25025 AT 2018oq 1 14:05:29.569 +37:08:17.02 Pan-STARRS1 Pan-STARRS1 PS18gq PS1 - GPC1 Y Y 19.5 i-Sloan 2018-01-31 14:28:19 PS1_Bot1
16762 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 14:05:29.569 +37:08:17.02 2018-01-31 14:28:19 19.5 i-Sloan 1 PSN PS18gq Pan-STARRS1
25219 2018-01-31 14:28:19 19.5 0.08 20.7 ABMag i-Sloan PS1_GPC1 45 Robot
25026 AT 2018or 1 10:54:42.517 +45:13:21.39 Pan-STARRS1 Pan-STARRS1 PS18fx PS1 - GPC1 Y Y 20.14 i-Sloan 2018-01-29 12:10:04 PS1_Bot1
16763 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 10:54:42.517 +45:13:21.39 2018-01-29 12:10:04 20.14 i-Sloan 1 PSN PS18fx Pan-STARRS1
25027 AT 2018os 1 13:28:37.132 +30:43:34.89 Pan-STARRS1 Pan-STARRS1 PS18fz PS1 - GPC1 Y Y 20.1 i-Sloan 2018-01-29 13:32:09 PS1_Bot1
16765 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 13:28:37.132 +30:43:34.89 2018-01-29 13:32:09 20.1 i-Sloan 1 PSN PS18fz Pan-STARRS1
25028 SN 2018ot 1 1 13:04:58.733 +30:30:18.88 SN Ib 0.036 Pan-STARRS1 None Pan-STARRS1 PS18fy PS1 - GPC1 Lick-3m - KAST Y Y 1 19.95 i-Sloan 2018-01-29 13:26:24 PS1_Bot1
16766 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 13:04:58.733 +30:30:18.88 2018-01-29 13:26:24 19.95 i-Sloan 1 PSN PS18fy Pan-STARRS1
25223 2018-01-29 13:26:24 19.95 0.1 20.7 ABMag i-Sloan PS1_GPC1 45 Robot
1717 2018-02-11 00:26:16 UCSCTr_Bot1 G. Dimitriadis, Y.-C. Pan, C. Rojas-Bravo, R. J. Foley (UCSC) None SN Ib 0.036 1 SN Ib. ATel 11284
1722 2018-02-08 07:50:09 Lick-3m_KAST 3090 C. Rojas-Bravo G. Dimitriadis None tns_2018ot_2018-02-08_07-50-09_Lick_3m_KAST.flm Object
1722 2018-02-08 07:50:09 Lick-3m / KAST 3090 C. Rojas-Bravo G. Dimitriadis None tns_2018ot_2018-02-08_07-50-09_Lick_3m_KAST.flm Object
25029 SN 2018ou 1 1 02:00:37.795 +12:10:18.12 SN Ia 0.0701 Pan-STARRS1 ZTF Pan-STARRS1 PS18gb PS1 - GPC1 P60 - SEDM Y Y 1 19.47 i-Sloan 2018-01-30 05:29:45 PS1_Bot1
16767 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 02:00:37.795 +12:10:18.12 2018-01-30 05:29:45 19.47 i-Sloan 1 PSN PS18gb Pan-STARRS1
1684 2018-02-05 15:16:37 neill James Neill ZTF SN Ia 0.0701 1 1 ZTF SNID match to SN1994D at -10 days
tns_2018ou_classrep_1684_ZTF.png Graphics SNID template fit 2018-02-05 15:16:37 neill
1689 2018-02-05 03:24:16 P60_SEDM 3600 Walters/Neill/Blagorodnova Neill ZTF tns_2018ou_2018-02-05_03-24-16_P60_SED-Machine_ZTF.txt Object ZTF
1689 2018-02-05 03:24:16 P60 / SEDM 3600 Walters/Neill/Blagorodnova Neill ZTF tns_2018ou_2018-02-05_03-24-16_P60_SED-Machine_ZTF.txt Object ZTF
25030 AT 2018ov 1 04:40:40.890 +11:59:11.47 Pan-STARRS1 Pan-STARRS1 PS18gd PS1 - GPC1 Y Y 20.31 i-Sloan 2018-01-30 08:28:19 PS1_Bot1
16769 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 04:40:40.890 +11:59:11.47 2018-01-30 08:28:19 20.31 i-Sloan 1 PSN PS18gd Pan-STARRS1
25031 SN 2018ow 1 1 02:51:04.415 +09:06:44.32 SN IIb 0.01 Pan-STARRS1 None Pan-STARRS1 PS18gc PS1 - GPC1 Lick-3m - KAST Y Y 1 19.39 i-Sloan 2018-01-30 05:42:43 PS1_Bot1
16770 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 02:51:04.415 +09:06:44.32 2018-01-30 05:42:43 19.39 i-Sloan 1 PSN PS18gc Pan-STARRS1
1714 2018-02-11 00:26:16 UCSCTr_Bot1 G. Dimitriadis, Y.-C. Pan, C. Rojas-Bravo, R. J. Foley (UCSC) None SN IIb 0.01 1 SN IIb. We measure an H alpha velocity of -12,400 km/s. ATel 11284
1719 2018-02-08 03:13:18 Lick-3m_KAST 2460 C. Rojas-Bravo G. Dimitriadis None tns_2018ow_2018-02-08_03-13-18_Lick_3m_KAST.flm Object
1719 2018-02-08 03:13:18 Lick-3m / KAST 2460 C. Rojas-Bravo G. Dimitriadis None tns_2018ow_2018-02-08_03-13-18_Lick_3m_KAST.flm Object
25032 AT 2018ox 1 10:41:36.105 +61:54:48.35 Pan-STARRS1 Pan-STARRS1 PS18gf PS1 - GPC1 Y Y 19.93 z-Sloan 2018-01-26 15:54:43 PS1_Bot1
16771 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 10:41:36.105 +61:54:48.35 2018-01-26 15:54:43 19.93 z-Sloan 1 PSN PS18gf Pan-STARRS1
25228 2018-01-26 15:54:43 19.93 0.13 20.4 ABMag z-Sloan PS1_GPC1 120 Robot
25033 AT 2018oy 1 08:24:35.407 +62:36:41.35 Pan-STARRS1 Pan-STARRS1 PS18ge PS1 - GPC1 Y Y 20.16 i-Sloan 2018-01-30 09:51:50 PS1_Bot1
16772 2018-02-04 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 08:24:35.407 +62:36:41.35 2018-01-30 09:51:50 20.16 i-Sloan 1 PSN PS18ge Pan-STARRS1
25034 SN 2018oz 1 1 03:34:19.760 +39:35:34.55 SN Ic 0.032 GaiaAlerts ZTF GaiaAlerts Gaia18aii Gaia - Gaia-photometric P60 - SEDM Y Y 1 18.3 G-Gaia 2018-02-03 05:58:33 Gaia_Bot1
16773 2018-02-04 21:06:41 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 03:34:19.760 +39:35:34.55 2018-02-03 05:58:33 18.3 G-Gaia 2 PSN Gaia18aii GaiaAlerts candidate SN in galaxy 2MASX J03341957+3935382
25231 2018-02-03 05:58:33 18.3 0.2 ABMag G-Gaia Gaia_Gaia-photometric 60 Robot
25230 2017-09-16 18:18:43 21.5 ABMag G-Gaia Gaia_Gaia-photometric Robot [Last non detection]
1690 2018-02-06 04:10:42 neill James Neill ZTF SN Ic 0.032 1 1 ZTF SNID match to SN1994I at -3 days
tns_2018oz_classrep_1690_ZTF.png Graphics SNID template match 2018-02-06 04:10:42 neill
1695 2018-02-06 02:43:50 P60_SEDM 3600 Walters/Neill/Blagorodnova Neill ZTF tns_2018oz_2018-02-06_02-43-50_P60_SED-Machine_ZTF.txt Object ZTF
1695 2018-02-06 02:43:50 P60 / SEDM 3600 Walters/Neill/Blagorodnova Neill ZTF tns_2018oz_2018-02-06_02-43-50_P60_SED-Machine_ZTF.txt Object ZTF
25035 AT 2018pa 1 18:15:55.900 +02:43:43.64 GaiaAlerts GaiaAlerts Gaia18aik Gaia - Gaia-photometric Y Y 18.09 G-Gaia 2018-02-03 01:53:45 Gaia_Bot1
16775 2018-02-04 21:16:05 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 18:15:55.900 +02:43:43.64 2018-02-03 01:53:45 18.09 G-Gaia 2 PSN Gaia18aik GaiaAlerts blue hostless transient near Galactic plane
25235 2018-02-03 01:53:45 18.09 0.2 ABMag G-Gaia Gaia_Gaia-photometric 60 Robot
25036 AT 2018pb 1 20:40:17.500 +39:04:58.62 GaiaAlerts GaiaAlerts Gaia18ail Gaia - Gaia-photometric Y Y 18.63 G-Gaia 2018-02-03 07:06:14 Gaia_Bot1
16776 2018-02-04 21:17:34 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 20:40:17.500 +39:04:58.62 2018-02-03 07:06:14 18.63 G-Gaia 2 Other Gaia18ail GaiaAlerts red source shows two dimming events, candidate YSO
25038 AT 2018pd 1 19:34:26.460 +26:10:28.78 GaiaAlerts GaiaAlerts Gaia18aim Gaia - Gaia-photometric Y Y 18.21 G-Gaia 2018-02-03 01:23:31 Gaia_Bot1
16780 2018-02-05 11:44:12 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 19:34:26.460 +26:10:28.78 2018-02-03 01:23:31 18.21 G-Gaia 2 PSN Gaia18aim GaiaAlerts Galactic plane transient on faint PanSTARRS source
25039 AT 2018pe 1 18:13:51.680 +00:28:32.23 GaiaAlerts GaiaAlerts Gaia18ain Gaia - Gaia-photometric Y Y 18.71 G-Gaia 2018-02-03 19:56:38 Gaia_Bot1
16781 2018-02-05 11:45:58 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 18:13:51.680 +00:28:32.23 2018-02-03 19:56:38 18.71 G-Gaia 2 PSN Gaia18ain GaiaAlerts Hostless Galactic plane transient, declining
25040 AT 2018pf 1 07:34:37.120 -26:56:18.56 GaiaAlerts GaiaAlerts Gaia18aio Gaia - Gaia-photometric Y Y 18.64 G-Gaia 2018-02-03 22:35:02 Gaia_Bot1
16782 2018-02-05 11:47:02 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 07:34:37.120 -26:56:18.56 2018-02-03 22:35:02 18.64 G-Gaia 2 PSN Gaia18aio GaiaAlerts Apparently hostless Galactic plane transient
25044 SN 2018pj 3 1 07:10:31.737 +32:38:45.34 SN Ia 0.055 2MASX J07103280+3238411 ASAS-SN, ATLAS, Pan-STARRS1 None ASAS-SN, ATLAS, Pan-STARRS1 ASASSN-18bw ASASSN-4 - Leavitt, ATLAS1 - ACAM1, PS1 - GPC1 Lick-3m - KAST Y Y 1 18 g-Sloan 2018-02-04 04:04:48 Stanek
17075 2018-02-27 18:41:05 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 07:10:31.737 +32:38:45.34 2018-02-20 05:36:57 18.22 w-PS1 1 PSN PS18ju Pan-STARRS1
16795 2018-02-08 15:01:01 ATLAS_Bot1 J. Tonry, B. Stalder, L. Denneau, A. Heinze, H. Weiland (IfA, University of Hawaii), A. Rest (STScI), K.W. Smith, S. J. Smartt, M. Fulton, O. McBrien (Queen's University Belfast) ATLAS 07:10:31.760 +32:38:45.82 2018-02-04 10:03:21 18.005 orange-ATLAS 2 PSN ATLAS18lzh ATLAS
16787 2018-02-06 03:25:18 KZStanek J. Brimacombe, J. V. Shields, K. Z. Stanek, for the ASAS-SN team ASAS-SN 07:10:31.733 +32:38:46.43 2018-02-04 04:04:48 18 g-Sloan 2 PSN 2MASX J07103280+3238411 ASASSN-18bw ASAS-SN On the rise, confirmed in follow-up imaging, unknown redshift host galaxy
25257 2018-02-04 04:04:48 18 ABMag g-Sloan ASASSN-4_Leavitt
25256 2018-01-28 01:55:12 17.3 ABMag g-Sloan ASASSN-4_Leavitt [Last non detection]
1715 2018-02-11 00:26:16 UCSCTr_Bot1 G. Dimitriadis, Y.-C. Pan, C. Rojas-Bravo, R. J. Foley (UCSC) None SN Ia 0.055 1 SN Ia at -4 days. We measure an Si II 6355 velocity of -14,500 km/s. ATel 11284
1720 2018-02-08 04:00:01 Lick-3m_KAST 1845 C. Rojas-Bravo G. Dimitriadis None tns_2018pj_2018-02-08_04-00-01_Lick_3m_KAST.flm Object
1720 2018-02-08 04:00:01 Lick-3m / KAST 1845 C. Rojas-Bravo G. Dimitriadis None tns_2018pj_2018-02-08_04-00-01_Lick_3m_KAST.flm Object
25045 AT 2018pk 1 05:03:16.770 -60:10:17.20 OGLE-GAL-LMC585.26-1165.993-2835.017 OGLE OGLE OGLE-1.3m - OGLEIV-Cam Y Y 19.702 I-Cousins 2018-02-05 02:28:20 Wyrzykowski
16788 2018-02-06 04:18:43 lukasz Lukasz Wyrzykowski OGLE 05:03:16.770 -60:10:17.20 2018-02-05 02:28:20 19.702 I-Cousins 3 PSN OGLE-GAL-LMC585.26-1165.993-2835.017 OGLE late discovery of a transient 2.3'' away from the centre of a faint galaxy, light curve roughly flat, with sharp rise, probably SN IIP.
25259 2018-02-05 02:28:20 19.702 0.061 22 VegaMag I-Cousins OGLE-1.3m_OGLEIV-Cam 150 OGLE-IV
25258 2017-12-16 05:10:46 22 VegaMag I-Cousins OGLE-1.3m_OGLEIV-Cam 150 OGLE-IV [Last non detection]
25046 AT 2018pl 1 05:12:42.750 -49:58:23.70 OGLE-GAL-LMC693.20-199.188-3990.530 None OGLE-1.3m - OGLEIV-Cam Y Y 19.769 I-Cousins 2018-02-06 04:39:44 Gromadzki
16789 2018-02-06 05:16:49 mariusz Mariusz Gromadzki None 05:12:42.750 -49:58:23.70 2018-02-06 04:39:44 19.769 I-Cousins 2 PSN OGLE-GAL-LMC693.20-199.188-3990.530
25262 2018-02-06 04:39:44 19.769 0.068 22 VegaMag I-Cousins OGLE-1.3m_OGLEIV-Cam 150 OGLE4
25261 2017-02-23 00:00:00 22 VegaMag I-Cousins OGLE-1.3m_OGLEIV-Cam 150 OGLE4 [Last non detection]
25047 SN 2018pm 1 1 08:19:07.890 +44:56:44.00 SN II 0.06 SDSS J081907.87+445648.2 TNTS None TNTS BAO-0.6m - BATC Lick-3m - KAST Y Y 1 19.6 Clear- 2018-02-05 14:24:00 Li
16790 2018-02-06 09:32:46 M51 Zhijian Xu,Wenxiong Li(THU),Tianmeng Zhang (NAOC), Zesheng Yang(THU), Hanjie Tan(CCU),Hao Song(THU), Xiaofeng Wang(THU), Jun Mo(THU),Xu Zhou(NAOC) on behalf of the TNTS TNTS 08:19:07.890 +44:56:44.00 2018-02-05 14:24:00 19.6 Clear- 1 PSN SDSS J081907.87+445648.2 TNTS This possible supernova was discovered by the 0.6 m schmidt telescope at Xinglong Observatory during the Tsinghua-NAOC Transient Survey (TNTS). The transient is located 0" west and 4" south of the center of SDSS J081907.87+445648.2
25263 2018-02-05 14:24:00 19.6 VegaMag Clear- BAO-0.6m_BATC
1716 2018-02-11 00:26:16 UCSCTr_Bot1 G. Dimitriadis, Y.-C. Pan, C. Rojas-Bravo, R. J. Foley (UCSC) None SN II 0.06 1 SN II. ATel 11284
1721 2018-02-08 06:50:44 Lick-3m_KAST 3090 C. Rojas-Bravo G. Dimitriadis None tns_2018pm_2018-02-08_06-50-44_Lick_3m_KAST.flm Object
1721 2018-02-08 06:50:44 Lick-3m / KAST 3090 C. Rojas-Bravo G. Dimitriadis None tns_2018pm_2018-02-08_06-50-44_Lick_3m_KAST.flm Object
25048 SN 2018pn 1 1 07:56:11.300 +45:31:36.40 SN IIP 0.048 SDSS J075611.44+453138.3 TNTS TNTS TNTS BAO-0.6m - BATC Lijiang-2.4m - YFOSC Y Y 1 17.9 Clear- 2018-02-05 14:24:00 Li
1701 2018-02-07 09:36:04 jujia Jujia Zhang, Yuxin Xin (YNAO), Wenxiong Li, Xiaofeng Wang (Tsinghua University), Hanjie Tan (Chinese Culture University) TNTS SN IIP 0.048 1 TNTS The spectrum of SN 2018pn matches with the type IIP supernova SN 2004dj at t = +0 days relative to the maximum light.
1706 2018-02-06 16:47:59 Lijiang-2.4m_YFOSC 1700 Jujia Zhang TNTS tns_2018pn_2018-02-06.7_Lijiang-2.4m_YFOSC_TNTS.dat Object TNTS
1706 2018-02-06 16:47:59 Lijiang-2.4m / YFOSC 1700 Jujia Zhang TNTS tns_2018pn_2018-02-06.7_Lijiang-2.4m_YFOSC_TNTS.dat Object TNTS
25049 SN 2018po 1 1 11:32:51.982 -38:45:41.62 SN Ia 0.032 ASAS-SN None ASAS-SN ASASSN-18bx ASASSN-5 - Payne-Gaposchkin SOAR - Goodman Y Y 1 16.9 g-Sloan 2018-02-06 22:33:36 Stanek
16792 2018-02-07 11:19:16 KZStanek K. Z. Stanek, for the ASAS-SN team ASAS-SN 11:32:51.982 -38:45:41.62 2018-02-06 22:33:36 16.9 g-Sloan 2 PSN ASASSN-18bx ASAS-SN In several epochs, flat light curve, no match in Vizier or DSS, probably a CV, but could also be a hostless SN
25266 2018-02-06 22:33:36 16.9 ABMag g-Sloan ASASSN-5_Payne-Gaposchkin
25265 2018-02-02 21:21:36 17.4 ABMag g-Sloan ASASSN-5_Payne-Gaposchkin [Last non detection]
1719 2018-02-12 13:40:14 strader Jay Strader None SN Ia 0.032 1 Ia near peak, with Si II ~ -11,600 km/s.
1724 2018-02-12 01:54:34 SOAR_Goodman Jay Strader None tns_2018po_2458161.57957_SOAR_Goodman.txt Object
1724 2018-02-12 01:54:34 SOAR / Goodman Jay Strader None tns_2018po_2458161.57957_SOAR_Goodman.txt Object
25050 AT 2018pp 1 00:42:34.399 +40:44:26.02 M31 ASAS-SN ASAS-SN ASASSN-18ca ASASSN-4 - Leavitt Y Y 16.5 g-Sloan 2018-02-08 01:40:48 Stanek
16793 2018-02-08 03:15:41 KZStanek K. Z. Stanek, for the ASAS-SN team ASAS-SN 00:42:34.399 +40:44:26.02 2018-02-08 01:40:48 16.5 g-Sloan 2 PNV M31 ASASSN-18ca ASAS-SN Likely nova in M31, rapid rise, so could also be (unlikely) a young SN
25268 2018-02-08 01:40:48 16.5 ABMag g-Sloan ASASSN-4_Leavitt
25052 SN 2018pr 1 1 12:49:56.970 +28:52:23.10 SN Ia 0.092 SDSS J124956.78+285222.5 TNTS TNTS TNTS BAO-0.6m - BATC Lijiang-2.4m - YFOSC Y Y 1 18.7 Clear- 2018-02-07 16:47:59 Li
16796 2018-02-08 15:21:43 M51 Zhijian Xu,Wenxiong Li(THU),Tianmeng Zhang (NAOC), Zesheng Yang(THU), Hanjie Tan(CCU),Hao Song(THU), Xiaofeng Wang(THU), Jun Mo(THU),Xu Zhou(NAOC) on behalf of the TNTS TNTS 12:49:56.970 +28:52:23.10 2018-02-07 16:47:59 18.7 Clear- 1 PSN SDSS J124956.78+285222.5 TNTS This possible supernova was discovered by the 0.6 m schmidt telescope at Xinglong Observatory during the Tsinghua-NAOC Transient Survey (TNTS). The transient is located 3" east and 1" north of the center of SDSS J124956.78+285222.5
1711 2018-02-10 13:36:56 jujia Jujia Zhang, Jianguo Wang (YNAO), Wenxiong Li, Xiaofeng Wang (THU), Hanjie Tan (CCU), Tianmeng Zhang, Xu Zhou (NAOC) TNTS SN Ia 0.092 1 TNTS The spectrum of SN 2018pr matches with the type Ia supernova SN 2007ca at t = +9 days relative to the maximum light.
1716 2018-02-09 17:31:12 Lijiang-2.4m_YFOSC 1700 Jujia Zhang TNTS tns_2018pr_2018-02-09.73_Lijiang-2.4m_YFOSC_TNTS.dat Object TNTS
1716 2018-02-09 17:31:12 Lijiang-2.4m / YFOSC 1700 Jujia Zhang TNTS tns_2018pr_2018-02-09.73_Lijiang-2.4m_YFOSC_TNTS.dat Object TNTS
25054 SN 2018pt 2 1 12:56:06.195 +32:03:15.70 SN Ia-91T-like 0.127 SDSS J125606.27+320314.6 TNTS, Pan-STARRS1 TNTS Pan-STARRS1, TNTS BAO-0.6m - BATC, PS1 - GPC1 Lijiang-2.4m - YFOSC Y Y 1 18.4 Clear- 2018-02-07 16:47:59 Li
19037 2018-06-02 18:25:04 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 12:56:06.195 +32:03:15.70 2018-02-09 11:54:14 19.66 i-Sloan 1 PSN PS18vx Pan-STARRS1
1712 2018-02-10 13:42:14 jujia Jujia Zhang, Jianguo Wang (YNAO), Wenxiong Li, Xiaofeng Wang (THU), Hanjie Tan (CCU), Tianmeng Zhang, Xu Zhou (NAOC) TNTS SN Ia-91T-like 0.127 1 TNTS The spectrum of SN 2018pt matches with the 91T-like type Ia supernova SN 2005eq at t = -4 days relative to the maximum light. Given a redshift of 0.127 (from SNID fit) for its host galaxy, an expansion velocity of about 9300 km/s can be deduced from the Si II 635.5 absorption minimum. Given this redshift (z~0.127) the absolute brightness of this SN is about -20.2 mag.
1717 2018-02-09 18:14:24 Lijiang-2.4m_YFOSC 1700 Jujia Zhang TNTS tns_2018pt_2018-02-09.76_Lijiang-2.4m_YFOSC_TNTS.dat Object TNTS
1717 2018-02-09 18:14:24 Lijiang-2.4m / YFOSC 1700 Jujia Zhang TNTS tns_2018pt_2018-02-09.76_Lijiang-2.4m_YFOSC_TNTS.dat Object TNTS
25056 SN 2018pv 3 1 11:52:55.760 +36:59:10.36 SN Ia 0.0031 NGC3941 None, ATLAS, GaiaAlerts None ATLAS, GaiaAlerts Other - Other, ATLAS1 - ACAM1, Gaia - Gaia-photometric Kanata - HOWPol Y Y 1 15.1 Clear- 2018-02-03 15:09:07 Tsuboi
17812 2018-04-17 23:26:07 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 11:52:55.760 +36:59:10.36 2018-04-16 11:19:40 15.35 G-Gaia 2 PSN Gaia18ayx GaiaAlerts confirmed SN Ia in galaxy NGC3491, aka SN 2018pv
17008 2018-02-19 00:00:02 ATLAS_Bot1 J. Tonry, B. Stalder, L. Denneau, A. Heinze, H. Weiland (IfA, University of Hawaii), A. Rest (STScI), K.W. Smith, S. J. Smartt, M. Fulton, O. McBrien (Queen's University Belfast) ATLAS 11:52:55.745 +36:59:10.19 2018-01-10 14:36:57 17.128 orange-ATLAS 2 PSN ATLAS18mci ATLAS
16800 2018-02-08 18:23:28 mtsuboi Masaki Tsuboi None 11:52:55.700 +36:59:11.60 2018-02-03 15:09:07 15.1 Clear- 2 2 PSN NGC3941 Offsets:3″ Eand0″NofNGC3941
25279 2018-02-03 15:09:07 15.1 17.7 VegaMag Clear- Other_Other 20 M.Tsuboi Telescope:0.35-m f/4.6 reflector
25278 2018-01-25 16:06:55 17.4 VegaMag Other- Other_Other 20 M.Tsuboi [Last non detection] Telescope:0.35-m f/4.6 reflector
tns_2018pv_atrep_16800.jpg Graphics 2018-02-08 18:23:28 mtsuboi
tns_2018pv_atrep_16800_0.jpg Graphics 2018-02-07 15:37:38(UT) Telescope:0.35-m f/4.6 reflector 2018-02-08 18:23:28 mtsuboi
1707 2018-02-08 18:48:56 myamanaka Masayuki Yamanaka None SN Ia 0.0031 1 SN Ia at the premaximum phase
1712 2018-02-08 16:47:59 Kanata_HOWPol 600 T. Nakaoka, M. Kawabata, R. Huang M. Yamanaka None tns_2018pv_2018-02-08.7_Kanata_HOWPol.txt Object The spectrum resembles with that of a normal Type Ia supernova (SN Ia) at the pre-maximum stage. Using the automatic SN classification tool, GELATO (Harutyunyan et al., 2008, A&A, 488, 383), the spectrum would be similar to that of SN 1992A at the 5 days before maximum. We identified the absorption lines of the CaII IR triplet, OI 7774, SiII 6355, SiII 5972, SII W-shape feature, and Fe II multiplet in our spectrum. The CaII IR triplet, OI 7774, and SiII 6355 line velocities were measured to be ~16500, ~16500, and ~13000 km/s, respectively. The SiII 5972 absorption line was significantly deeper than that of SN 1992A, suggesting that this SN might be a more subluminous event. We measured the equivalent width (EW) of the NaID line as to 0.9 angstrom, suggesting that the host galactic extinction could be very large (A_V~0.5-2.0). Even if the extinction is corrected for, this SN could be still in the rising phase. Follow-up observations could be encouraged.
1712 2018-02-08 16:47:59 Kanata / HOWPol 600 T. Nakaoka, M. Kawabata, R. Huang M. Yamanaka None tns_2018pv_2018-02-08.7_Kanata_HOWPol.txt Object The spectrum resembles with that of a normal Type Ia supernova (SN Ia) at the pre-maximum stage. Using the automatic SN classification tool, GELATO (Harutyunyan et al., 2008, A&A, 488, 383), the spectrum would be similar to that of SN 1992A at the 5 days before maximum. We identified the absorption lines of the CaII IR triplet, OI 7774, SiII 6355, SiII 5972, SII W-shape feature, and Fe II multiplet in our spectrum. The CaII IR triplet, OI 7774, and SiII 6355 line velocities were measured to be ~16500, ~16500, and ~13000 km/s, respectively. The SiII 5972 absorption line was significantly deeper than that of SN 1992A, suggesting that this SN might be a more subluminous event. We measured the equivalent width (EW) of the NaID line as to 0.9 angstrom, suggesting that the host galactic extinction could be very large (A_V~0.5-2.0). Even if the extinction is corrected for, this SN could be still in the rising phase. Follow-up observations could be encouraged.
25057 AT 2018pw 2 01:50:33.366 +11:13:54.56 Pan-STARRS1, ATLAS ATLAS, Pan-STARRS1 PS18gs PS1 - GPC1, ATLAS1 - ACAM1 Y Y 18.44 w-PS1 2018-02-04 05:38:24 PS1_Bot1
17041 2018-02-20 20:34:01 ATLAS_Bot1 J. Tonry, B. Stalder, L. Denneau, A. Heinze, H. Weiland (IfA, University of Hawaii), A. Rest (STScI), K.W. Smith, S. J. Smartt, M. Fulton, O. McBrien (Queen's University Belfast) ATLAS 01:50:33.365 +11:13:54.77 2017-10-29 10:33:36 19.731 orange-ATLAS 2 PSN ATLAS18mev ATLAS
16801 2018-02-08 23:50:02 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 01:50:33.366 +11:13:54.56 2018-02-04 05:38:24 18.44 w-PS1 1 PSN PS18gs Pan-STARRS1
25058 AT 2018px 2 06:30:25.670 +40:04:02.17 ATLAS, GaiaAlerts ATLAS, GaiaAlerts ATLAS18lzd ATLAS1 - ACAM1, Gaia - Gaia-photometric Y Y 18.091 orange-ATLAS 2018-02-01 09:50:24 ATLAS_Bot1
16953 2018-02-15 10:53:53 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 06:30:25.670 +40:04:02.17 2018-02-11 17:52:48 18 G-Gaia 2 PSN Gaia18akw GaiaAlerts candidate SN near galaxy MCG +07-14-001
25523 2018-02-11 17:52:48 18 0.2 ABMag G-Gaia Gaia_Gaia-photometric 60 Robot
16802 2018-02-09 00:00:03 ATLAS_Bot1 J. Tonry, B. Stalder, L. Denneau, A. Heinze, H. Weiland (IfA, University of Hawaii), A. Rest (STScI), K.W. Smith, S. J. Smartt, M. Fulton, O. McBrien (Queen's University Belfast) ATLAS 06:30:25.697 +40:04:02.57 2018-02-01 09:50:24 18.091 orange-ATLAS 2 PSN ATLAS18lzd ATLAS
25282 2018-02-01 09:50:24 18.091 0.173 18.4 ABMag orange-ATLAS ATLAS1_ACAM1 30 Robot
25063 AT 2018qc 1 18:36:16.630 +05:32:11.87 GaiaAlerts GaiaAlerts Gaia18aip Gaia - Gaia-photometric Y Y 17.58 G-Gaia 2018-02-05 09:37:26 Gaia_Bot1
16808 2018-02-09 09:56:23 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 18:36:16.630 +05:32:11.87 2018-02-05 09:37:26 17.58 G-Gaia 2 Other Gaia18aip GaiaAlerts 1.5 mag rise on a faint Galactic Plane star
25064 AT 2018qd 1 07:18:14.190 -23:43:39.32 GaiaAlerts GaiaAlerts Gaia18aiq Gaia - Gaia-photometric Y Y 18.79 G-Gaia 2018-02-05 00:27:21 Gaia_Bot1
16809 2018-02-09 10:04:22 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 07:18:14.190 -23:43:39.32 2018-02-05 00:27:21 18.79 G-Gaia 2 Other Gaia18aiq GaiaAlerts 2 mag rise on previously variable Galactic Plane source, strong WISE signal, probably YSO
25065 AT 2018qe 1 21:30:27.890 +48:14:10.43 GaiaAlerts GaiaAlerts Gaia18air Gaia - Gaia-photometric Y Y 18.92 G-Gaia 2018-02-04 00:54:43 Gaia_Bot1
16810 2018-02-09 10:07:13 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 21:30:27.890 +48:14:10.43 2018-02-04 00:54:43 18.92 G-Gaia 2 PSN Gaia18air GaiaAlerts Hostless Galactic plane transient
25066 AT 2018qf 1 05:32:31.500 +14:52:09.80 GaiaAlerts GaiaAlerts Gaia18ais Gaia - Gaia-photometric Y Y 18.71 G-Gaia 2018-02-03 23:25:26 Gaia_Bot1
16811 2018-02-09 10:12:14 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 05:32:31.500 +14:52:09.80 2018-02-03 23:25:26 18.71 G-Gaia 2 PSN Gaia18ais GaiaAlerts candidate SN near galaxy 2MASX J05323154+1452101
25067 AT 2018qg 1 05:23:25.340 +18:10:41.59 GaiaAlerts GaiaAlerts Gaia18ait Gaia - Gaia-photometric Y Y 17.86 G-Gaia 2018-02-03 23:29:45 Gaia_Bot1
16812 2018-02-09 10:16:45 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 05:23:25.340 +18:10:41.59 2018-02-03 23:29:45 17.86 G-Gaia 2 PSN Gaia18ait GaiaAlerts transient on top of g=17.7 SDSS source, declining. Candidate CV, aka PS1-14pq
25068 AT 2018qh 1 05:21:11.700 +21:09:59.15 GaiaAlerts GaiaAlerts Gaia18aiu Gaia - Gaia-photometric Y Y 18.77 G-Gaia 2018-02-04 11:32:38 Gaia_Bot1
16813 2018-02-09 10:18:56 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 05:21:11.700 +21:09:59.15 2018-02-04 11:32:38 18.77 G-Gaia 2 PSN Gaia18aiu GaiaAlerts transient near PanSTARRS and X-ray source, and a faint extended source
25069 AT 2018qi 1 17:22:09.860 -18:46:56.86 GaiaAlerts GaiaAlerts Gaia18aiv Gaia - Gaia-photometric Y Y 18.6 G-Gaia 2018-02-03 22:07:40 Gaia_Bot1
16814 2018-02-09 10:22:28 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 17:22:09.860 -18:46:56.86 2018-02-03 22:07:40 18.6 G-Gaia 2 PSN Gaia18aiv GaiaAlerts Galactic plane hostless transient, rising
25070 AT 2018qj 1 17:47:54.670 -11:32:05.60 GaiaAlerts GaiaAlerts Gaia18aiw Gaia - Gaia-photometric Y Y 18.66 G-Gaia 2018-02-04 09:57:36 Gaia_Bot1
16815 2018-02-09 10:26:07 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 17:47:54.670 -11:32:05.60 2018-02-04 09:57:36 18.66 G-Gaia 2 PSN Gaia18aiw GaiaAlerts hostless Galactic plane transient
25071 AT 2018qk 1 18:34:45.480 +06:53:11.44 GaiaAlerts GaiaAlerts Gaia18aix Gaia - Gaia-photometric Y Y 19.2 G-Gaia 2018-02-03 21:34:33 Gaia_Bot1
16816 2018-02-09 13:31:00 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 18:34:45.480 +06:53:11.44 2018-02-03 21:34:33 19.2 G-Gaia 2 PSN Gaia18aix GaiaAlerts Rising, hostless Galactic plane transient, near a faint galaxy-like PanSTARRS object
25072 AT 2018ql 1 15:13:24.570 -50:02:05.89 GaiaAlerts GaiaAlerts Gaia18aiy Gaia - Gaia-photometric Y Y 18.15 G-Gaia 2018-02-04 15:04:19 Gaia_Bot1
16817 2018-02-09 13:33:44 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 15:13:24.570 -50:02:05.89 2018-02-04 15:04:19 18.15 G-Gaia 2 PSN Gaia18aiy GaiaAlerts Galactic plane transient near DSS sources
25073 AT 2018qm 1 16:37:43.680 -32:07:26.87 GaiaAlerts GaiaAlerts Gaia18aiz Gaia - Gaia-photometric Y Y 18.73 G-Gaia 2018-02-04 02:38:24 Gaia_Bot1
16818 2018-02-09 13:34:39 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 16:37:43.680 -32:07:26.87 2018-02-04 02:38:24 18.73 G-Gaia 2 PSN Gaia18aiz GaiaAlerts Galactic plane transient
25074 AT 2018qn 1 16:59:08.580 -29:18:17.14 GaiaAlerts GaiaAlerts Gaia18aja Gaia - Gaia-photometric Y Y 18.72 G-Gaia 2018-02-04 14:34:04 Gaia_Bot1
16819 2018-02-09 13:37:18 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 16:59:08.580 -29:18:17.14 2018-02-04 14:34:04 18.72 G-Gaia 2 PSN Gaia18aja GaiaAlerts Galactic plane transient
25075 AT 2018qo 1 16:46:33.040 -32:40:14.95 GaiaAlerts GaiaAlerts Gaia18ajb Gaia - Gaia-photometric Y Y 14.66 G-Gaia 2018-02-04 14:38:24 Gaia_Bot1
16820 2018-02-09 13:38:48 Gaia_Bot1 A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team GaiaAlerts 16:46:33.040 -32:40:14.95 2018-02-04 14:38:24 14.66 G-Gaia 2 Other Gaia18ajb GaiaAlerts Erratic variability in red Galactic plane star
25077 AT 2018qq 1 1 09:58:33.029 -27:49:50.09 CV 0 LEDA 749345 ASAS-SN ePESSTO ASAS-SN ASASSN-18cd ASASSN-2 - Cassius, ASASSN-3 - Paczynski ESO-NTT - EFOSC2-NTT Y Y 1 17 g-Sloan 2018-02-10 04:48:00 Stanek
16822 2018-02-10 16:45:14 KZStanek K. Z. Stanek, for the ASAS-SN team ASAS-SN 09:58:33.029 -27:49:50.09 2018-02-10 04:48:00 17 g-Sloan 2 PSN LEDA 749345 ASASSN-18cd ASAS-SN In several epochs, on the rise, faint match in PS1 images, could also be a CV
25318 2018-02-10 04:48:00 17 ABMag g-Sloan ASASSN-3_Paczynski
25317 2018-02-09 03:21:36 17.5 VegaMag V-Johnson ASASSN-2_Cassius [Last non detection]
1726 2018-02-14 18:50:07 ePESSTO_Bot1 Jesse T. Palmerio, Ken W. Smith, David O'Neill, O. Yaron, N. Knezevic on behalf of ePESSTO ePESSTO CV 0 1 ePESSTO
1731 2018-02-14 04:00:32 ESO-NTT_EFOSC2-NTT 600 Jesse T. Palmerio, Ken W. Smith David O'Neill ePESSTO tns_2018qq_2018-02-14_04-00-32_ESO-NTT_EFOSC2-NTT_ePESSTO.asci tns_2018qq_2018-02-14_04-00-32_ESO-NTT_EFOSC2-NTT_ePESSTO.fits Object ePESSTO
1731 2018-02-14 04:00:32 ESO-NTT / EFOSC2-NTT 600 Jesse T. Palmerio, Ken W. Smith David O'Neill ePESSTO tns_2018qq_2018-02-14_04-00-32_ESO-NTT_EFOSC2-NTT_ePESSTO.asci tns_2018qq_2018-02-14_04-00-32_ESO-NTT_EFOSC2-NTT_ePESSTO.fits Object ePESSTO
25078 AT 2018qr 1 01:03:31.157 +09:28:36.03 Pan-STARRS1 Pan-STARRS1 PS18hv PS1 - GPC1 Y Y 19.88 w-PS1 2018-02-04 05:31:12 PS1_Bot1
16824 2018-02-10 18:41:07 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 01:03:31.157 +09:28:36.03 2018-02-04 05:31:12 19.88 w-PS1 1 PSN PS18hv Pan-STARRS1
25079 AT 2018qs 1 01:08:25.642 +12:56:35.44 Pan-STARRS1 Pan-STARRS1 PS18hw PS1 - GPC1 Y Y 19 w-PS1 2018-02-04 05:26:52 PS1_Bot1
16825 2018-02-10 18:41:07 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 01:08:25.642 +12:56:35.44 2018-02-04 05:26:52 19 w-PS1 1 PSN PS18hw Pan-STARRS1
25321 2018-02-04 05:26:52 19 0.04 22 ABMag w-PS1 PS1_GPC1 45 Robot
25080 AT 2018qt 1 01:37:54.046 +14:23:42.67 Pan-STARRS1 Pan-STARRS1 PS18hx PS1 - GPC1 Y Y 21.06 w-PS1 2018-02-04 05:35:31 PS1_Bot1
16826 2018-02-10 18:41:07 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 01:37:54.046 +14:23:42.67 2018-02-04 05:35:31 21.06 w-PS1 1 PSN PS18hx Pan-STARRS1
25081 AT 2018qu 2 09:33:54.613 +51:31:45.15 Pan-STARRS1, TNTS Pan-STARRS1, TNTS PS18hr PS1 - GPC1, BAO-0.6m - BATC Y Y 19.54 i-Sloan 2018-02-03 09:56:09 PS1_Bot1
16860 2018-02-11 01:54:19 M51 Zhijian Xu,Wenxiong Li(THU),Tianmeng Zhang (NAOC), Zesheng Yang(THU), Hanjie Tan(CCU),Hao Song(THU), Xiaofeng Wang(THU), Jun Mo(THU),Xu Zhou(NAOC) on behalf of the TNTS TNTS 09:33:54.580 +51:31:45.30 2018-02-09 14:24:00 19.2 Clear- 1 PSN CGCG 265-026 TNTS This possible supernova was discovered by the 0.6 m schmidt telescope at Xinglong Observatory during the Tsinghua-NAOC Transient Survey (TNTS). The transient is located 1" east and 7" south of the center of CGCG 265-026
16827 2018-02-10 18:41:07 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 09:33:54.613 +51:31:45.15 2018-02-03 09:56:09 19.54 i-Sloan 1 PSN PS18hr Pan-STARRS1
25082 AT 2018qv 1 09:55:56.908 +55:24:17.09 Pan-STARRS1 Pan-STARRS1 PS18hm PS1 - GPC1 Y Y 19.52 i-Sloan 2018-02-03 10:04:48 PS1_Bot1
16828 2018-02-10 18:41:07 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 09:55:56.908 +55:24:17.09 2018-02-03 10:04:48 19.52 i-Sloan 1 PSN PS18hm Pan-STARRS1
25083 AT 2018qw 1 00:54:57.467 +11:52:23.00 Pan-STARRS1 Pan-STARRS1 PS18hs PS1 - GPC1 Y Y 20.87 w-PS1 2018-02-04 05:25:26 PS1_Bot1
16829 2018-02-10 18:41:07 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 00:54:57.467 +11:52:23.00 2018-02-04 05:25:26 20.87 w-PS1 1 PSN PS18hs Pan-STARRS1
25084 AT 2018qx 1 00:59:22.643 +14:17:38.96 Pan-STARRS1 Pan-STARRS1 PS18ht PS1 - GPC1 Y Y 20.44 w-PS1 2018-02-04 05:26:52 PS1_Bot1
16830 2018-02-10 18:41:07 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe, J. Bulger (IfA, University of Hawaii), S. J. Smartt, K. W. Smith (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright (University of Minnesota), D. R. Young (Queen's University Belfast) Pan-STARRS1 00:59:22.643 +14:17:38.96 2018-02-04 05:26:52 20.44 w-PS1 1 PSN PS18ht Pan-STARRS1
25326 2018-02-04 05:26:52 20.44 0.1 22 ABMag w-PS1 PS1_GPC1 45 Robot


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The Mixed 10 m platform synchro competition of the 2018 European Aquatics Championships was held on 11 August 2018.

Results
The final was started at 15:30.

References

Mixed 10 m platform synchro
European Aquatics Championships

redpajama_set_name: RedPajamaWikipedia


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Photo Credit To Komatsu
Komatsu to acquire GHH in Germany
Komatsu today announced that it has entered into an agreement to acquire GHH Group GmbH, a manufacturer of underground mining, tunnelling and special civil engineering equipment headquartered in Gelsenkirchen, Germany.
Founded in the 1960s and currently part of the German-owned Schmidt Kranz Group, GHH offers a wide range of equipment focused on loaders (LHDs) and articulated dump trucks in the mid-seam mass mining, narrow vein and low-profile market segments The company also supports customers with aftermarket parts and service support through the entire life of each machine.
With this acquisition, Komatsu will add GHH's factories and rebuild facilities in key markets, in addition to its robust product offerings and talented staff.
"We are very excited about this acquisition as it represents a great opportunity for Komatsu to expand its offerings for underground mining equipment and accelerate new product development through synergies with Komatsu's existing team and product offerings," said Peter Salditt, president and CEO, Komatsu Mining Corp. "By adding GHH's factories and rebuild facilities in key markets in Europe, South Africa, India and Chile. We also aim to strengthen production and service capabilities for our customers."
Komatsu intends to continue the excellent service GHH provides and plans to support business as usual post-acquisition. The combined team will then work together to expand Komatsu's offering for underground mining equipment and increase customer access to products in new territories.
"GHH is excited to be able to start a new journey with a strong player in the mining world. This opens huge doors for our people and our products to develop further and grow beyond what we could have hoped for," said GHH Group CEO Dr. Jan Petzold. "This is the next logical step in becoming a true global player and we look forward to becoming part of the Komatsu family".
The official close of the acquisition is projected for the first half of 2023.
Per the company's ongoing mid-term management plan "DANTOTSU Value – Together, to 'The Next' for sustainable growth," Komatsu is working to expand offerings for underground hard rock mining, creating new value for customers with the development of new equipment, processes and technologies that will help operations step forward to the next stage for the workplace of the future and provide a more sustainable environment for the next generation.
Post source : Komatsu
Tags:AcquisitionConstructionEquipmentGHHKomatsuMining
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A key signature in music means the set of flats and sharps that are based on any root note. Keys have a big impact on the tone and mood of musical piece. An understanding of music keys is essential, particularly when you wish to jam with other artists. It can be tough to find a key, particularly if you lack prior music training. Here are some ways to know which key you are playing.
In a key signature, the tonic is the root note on which the remainder of the scale is based. Tonic is vital given that any specified set of flats and sharps could match either a Minor or a Major Key. If the remainder of the composition seems to be created on a chord, the root note of the chord is likely to be the tonic note.
The Circle of Fifths happens to be an easy way to remember the flats and sharps in a specific Major Key. It is, in a lot of ways, the most vital tool in the world of Western Music. Count how many spaces are there clockwise from C between a note, if you want to know the number of sharps in a key. C is located in the Circle of Fifths at the top, which makes it easily countable. Count the number of sharps in a clockwise fashion. The Major key will be the spot where you stop at.
A song's final note, in many cases, can bring back the composition to the root tonic note. A lot of music composers use a tonic note to end with, in order to give a sense of finality to their work. Use the give flats and sharps for cross-reference of your final note.


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Read an Extract from Crooked Heart by Lissa Evans
January 8, 2016 // Books // lissa evans / historic fiction / extracts / fiction
Lissa Evans' Crooked Heart is an emotional, moving and vivid tale laced with dark humour and wit. Set in London at the start of World War Two, we meet smart and loveable ten year old Noel who lives happily with his strong-willed godmother Mattie. But as the Blitz begins, Noel is evacuated to St Alban's where he is taken in by Vee; a woman who lives with her idle son Donald and poorly mother Flora. Vee is desperate to make money, and she'll use every trick in the book to get it. It isn't long before Noel is involved in her underhand schemes and the pair begin to form a strong but unusual friendship in the most desperate and dangerous of times.
Heartwarming, unique and funny, Crooked Heart isn't your usual World War Two story. Noel and Vee's everyday struggles and the blossoming friendship that develops because of them are very much the stars of the story, while the chaotic background of World War Two London ensures an absorbing and poignant read.
Meet Noel and his godmother Mattie in the below extract from Crooked Heart and prepare to become engrossed in their story.
She was losing words. At first it was quite funny. 'The box of things,' Mattie would say, waving her mauve-veined hands vaguely around the kitchen.
'The box of things for making flames. It's a song, Noel!
'The box of things for making flames
I can't recall their bloody names.'
Or 'that church', she'd say, standing at the top of Hampstead Heath, gazing down at the scribble of blue and grey that was London. 'The one with the dome – remind me of what it's called.'
His godmother would teeter around the drawing room, slippered feet not quite keeping up with her heavy body.
'St Paul's Cathedral.'
'Of course it is. The architect has a bird's name. Owl . . .Ostrich . . .'
'Wren.'
'Right again, young Noel, though I can't help thinking "Sir Christopher Ostrich" has a tremendous ring to it . . .'
After a while, it stopped being funny. 'Where's my . . . my . . .'
'Where's that damn thing, the blue thing, goes round my shoulders, the blue thing . . .'
Some words would resurface after a few days; others would sink for ever. Noel started writing labels: 'SHAWL', 'WIRELESS', 'GAS MASK', 'CUTLERY DRAWER'.
'Helpful little man,' Mattie said, bending to kiss his forehead.
'Be sure to take them down before Geoffrey comes to check on me,' she added, suddenly shrewd again.
Uncle Geoffrey and Auntie Margery lived a mile away, in Kentish Town.
Once a month, Uncle Geoffrey came for Sunday tea, and once a year he dropped by for Mattie's birthday, always bringing a gift that had been made either by himself or by Auntie Margery.
'There are times,' said Mattie, examining yet another crossstitched antimacassar, 'when it's very useful to have an open fire. What is the one thing that is more important than money, Noel?'
'Taste.'
'Which is something that Geoffrey and . . .' she paused, '. . .bosoms . . .'
'Margery.'
'. . . will never have.'
At the monthly teas, Uncle Geoffrey smiled all the time and talked about his job in rate-collection, the marquetry picture frames he made in his spare time, and Auntie Margery's delicate health, which prevented her from ever leaving the house. His teeth were regular and well-spaced, like battlements. Noel liked to imagine tiny soldiers popping up between them, firing arrows across the room or pouring molten lead down Uncle Geoffrey's chin.
'Hobbies are for people who don't read books,' said Noel; it was one of Mattie's sayings.
'And what have you been up to, young Noel?' his uncle would ask. 'Keeping busy with hobbies? Model aircraft? Stamp collecting?'
After tea, Uncle Geoffrey would ask whether there was anything he could do around the house, and Mattie always found something awkward or messy – shifting furniture, oiling a door. When the blackout regulations were published, Uncle Geoffrey was set to work sticking brown paper on the doorpanes and checking every shutter for soundness.
'After all,' as Mattie said, 'you are our war expert.' He had enrolled as an air-raid warden the day after Mr Chamberlain came back from Munich. He had a hat, a whistle and an armband.
'So all you need now is an air-raid!' said Mattie.
She didn't believe that there would be a war.
Mattie's house was a spacious brick box, with a fancy ironwork verandah and a garden full of azaleas. 'A Victorian gentleman's residence,' she said. 'Or, more likely, the place where a Victorian gentleman secreted his mistress. Family in Mayfair, lady friend in Hampstead. It would have been considered frightfully out of town.'
The road ran along a little crease in the fabric of the Heath, coming to a dead end at a bolt of rabbit-cropped turf; from the rear windows of the house you could see only trees.
'Who would know we were in London?' said Mattie, nearly every day.
It was a hot, slow summer. In the early morning, when it was still cool, they walked the mile to Parliament Hill and back, leaving dark tracks through the wet grass, singing songs of protest to the skylarks:
As we come marching, marching,
We bring the greater days.
The rising of the women
Means the rising of the race.
No more the drudge and idler,
ten that toil while one reposes,
But a sharing of life's glories:
Bread and Roses!
Our lives shall not be sweated
From birth until life closes;
Hearts starve as well as bodies;
Give us bread, but give us roses!
On the final chorus repeats, Mattie would simultaneously hum and whistle. 'A rare and underrated skill,' she'd remark, 'and one that, sadly, has never brought me the acclaim it deserves.'
In the silence that followed, Noel rolled over and looked at her. Her square, sure face was suddenly unfamiliar; her expression one he'd never seen before. It was panic, he realized.
During the afternoon heat, she slept in a deckchair and Noel lay on the lawn and read detective stories, noting down clues as he went along. Wood pigeons crooned in the trees.
'Who'd know,' sighed Mattie, 'who'd know we were in . . .in . . .'
Somewhere inside herself she was teetering on a ledge.
'London,' he said, 'it's London.'
'Ah yes, London,' she repeated, inching back.
The mechanical digger arrived one day when they were at the library. By the time they came home, the first lorry was already roaring back past their house, leaving a frill of sand along the verges behind it.
'What are you doing?' called Mattie to the driver, but he ignored her.
They followed the gritty trail to the end of the road, and there stood the great red digger. It had already scalped the grass from fifty yards of heath, and was taking savage bites out of the sandy slope. Another lorry was waiting for a load.
'No!' shouted Mattie.
Three neighbours arrived, sweating and gesticulating, and then a fourth, grim with knowledge.
'It's official,' he said. 'I've been talking to the council. It's for sandbags, they say they're going to need thousands if bombing starts. They're grubbing up Hyde Park, too . . .'
Within the week, there were four diggers, not one, and aconstant stream of lorries rattling up past the house and then grinding down again. The hole in the Heath grew daily, the cut edge a palette of yellows: ochre, mustard, butter, gold. When the wind blew, Mattie's front garden was more beach than grass.
There was no possible reply to this. She had been gaoled five times as a suffragette; she still had the scars of handcuffs on her wrists.
Every floor in the house crunched underfoot. Mrs Harley, the char, said the extra work was too much for her, and left.
A man came to the door, offering filled sandbags at £5 for a hundred, or empty ones for 3d each. 'And then you can do them yourself,' he said. 'Lucky for you, you're right on the spot.'
Mattie closed the door in his face.
Their morning walk was changing. The detour they took to avoid the hole at the end of the road added another mile to the round trip; it was just too far for Noel, with his gammy leg, to manage comfortably, and meant he was always limping by the time they arrived home. There was a gun emplacement behind Parliament Hill now, and shelters being dug along the fields by the railway line. Mattie would stand and stare at the horizon, at the silver blimps motionless on invisible wires, and shake her head in disbelief. 'Isn't it strange,' she said, 'that there's always enough money in the coffers for war?'
During his August teatime visit, Uncle Geoffrey talked about the international situation before patting Noel on the head.
'And I wonder where this young shaver will be off to?' he said, smiling as usual.
'What d'you mean, "off to"?' asked Mattie, very sharply.
The smile wavered. 'You'll have registered him, I suppose, for evacuation?'
'No, why would I have done that?'
Geoffrey looked flustered. 'I didn't mean to annoy you, Mattie dear,' he said, advancing a hand as if to pat one of Mattie's, and then wisely withdrawing it again. 'It's just that the government . . .' With an effort, he hoisted the smile back on to his face, where it hung a little crookedly, '. . . the government considers that the best place for children, in the event of a war, is away from the areas of likely bombardment.'
'There is no war.'
'Not yet, perhaps, but I think the likelihood is—'
'And since when have I ever taken any notice of what the government says?' asked Mattie.
'Do you want to be evacuated?' Mattie asked Noel, afterwards.
'No,' he said.
'I'm sure Roberta would have you to stay in . . . where is it that Roberta lives? Ipswich? I'm sure you'd be safe there.'
'I don't want to go anywhere,' he said. He was a little bit worried by the thought of bombs. He was far, far more worried by the fact that Mattie seemed to have forgotten that her best friend Roberta was dead. The funeral had been eighteen months ago. Mattie had worn her old sash, and a white, green and purple rosette.
Poland was being invaded and the summer holidays were almost over. On the Saturday before the start of the Michaelmas term, Noel went to the library. He had read every Lord Peter Wimsey on the shelves, and every Albert Campion. The tall librarian with the moustache suggested he tried a thriller instead of a detective story. 'You'll find Eric Ambler very good,' she said. Noel was brooding over the choice of titles when he received a blow between the shoulder blades.
Find Related Content // Books / books / extracts / fiction / historic fiction / january 2016 / Lissa Evans
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As part of MPD's embrace of a community-based policing philosophy and desire to build partnerships with our citizens, officers in the Central District have been participating in "Coffee with a Cop" as a way to reach out and meet with people in the neighborhood. Similar to other such programs that many police departments across the nation have already been engaged in, Coffee with a Cop serves as an informal meeting space where MPD and the members of the community can meet without any agendas or formal presentations.
So far this year, topics of conversation have ranged from crime trends in the area neighborhoods and concerns about drug activity to traffic enforcement in school zones and crime prevention tips.
Coffee with a Cop happens every Wednesday morning at 9:00am at Madison Sourdough Company (916 Williamson St). If a call for service comes in during this time, it is possible that officers may need to leave early.
Coffee with a Cop is a way for residents of Madison to become involved, one cup of coffee at a time.


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Becoming Daddy Owen
It's late in the evening when Owen Mwatia, otherwise known as Daddy Owen, calls to tell me he is ready for this interview. He asks me whether we can meet
PublishedOctober 7, 2019
It's late in the evening when Owen Mwatia, otherwise known as Daddy Owen, calls to tell me he is ready for this interview. He asks me whether we can meet at Java at the Junction Mall and I reply in the affirmative. I came to learn in the course of the interview that he has a soft spot for this particular café as it is here that he fell in love with his wife – Farida Wambui.
"I recall that day clearly. I had earlier performed at her work place and though we interacted, it was on a professional note. I was meeting a friend thereafter at this café and coincidentally, she was also meeting her sister here," Daddy Owen recollects.
Their love came as natural as their meeting. Daddy Owen asked Farida out and when they started talking and getting to know each other, they realised that their worlds were far apart. However, when Daddy Owen eventually asked Farida to be his girlfriend, his celebrity status and humble background did not matter one bit to her.
"I said yes to Owen the man who needed to be loved back and not the celebrity," Farida, a regional marketing manager with a Swiss pharmaceutical firm, says.
Meanwhile, as he awaited her answer, Daddy Owen's heart was beating hard against his ribcage. He wasn't sure whether Farida would accept his advances seeing as it is that he came from Eastlands while Farida was born and raised in the leafy suburbs of Lavington. Yet, it is in these differences that their love would find a perfect resting place and blossom. Indeed, opposites do attract.
The couple dated low key for three years before eventually tying the knot in a grand, colourful wedding in Nairobi in 2016. In July last year, the couple was blessed with a son. However, his entry to the world was marred with a scare.
"I was excited about the prospect of becoming a father again. So I accompanied my wife to the last scan, which showed that the umbilical cord had wrapped around the baby's neck. Some of our friends had lost their babies to this complication and this reality hit us hard. The doctor ordered for an emergency Caesarean section to save the baby. We thank God because the procedure went well and to top it up, our son did not need to be incubated for he had the right weight and his lungs were developed," the father of two narrates.
Disrupting gospel music industry
The new parents thus spent a better part of last year tending to their newborn. Even then, Daddy Owen was working on an album that would disrupt the gospel music industry once more.
"I got saved while I was still a teenager and I used to crave for music that I could relate with. My peers, too, were looking for this kind of music. What was available was secular and hence many of them went to discotheques to satisfy their musical thirst. When I eventually got into music, I knew the kind of music I wanted to do and who it would appeal to," he says resolutely.
Growing up in Kakamega, Daddy Owen used to spend most his free time helping out in his father's music shop. Congolese music used to rule the airwaves then and Daddy Owen got to listen to a lot of songs from this genre. It is here that he also got to understand music in its entirety – the beat, notes and arrangement. He started writing songs while in high school and these songs would be sung during sports days to cheer up his team.
"My brother Rufftone and I have always been creative. We were particularly adept at drawing and we both won national drawing competitions. We weren't really into singing," he offers.
When he cleared form four, Daddy Owen moved to Nairobi to stay with his father and brother. He enrolled for a diploma course in travel and ticketing. Upon completion, he resorted to selling clothes in Gikomba and Mutindwa markets in Nairobi. The eight to five job did not appeal to him. Before venturing into clothes business, he worked at a chip's outlet peeling potatoes and making samosas and yoghurt.
"I thereafter got a job with a bus body manufacturing company to do matatu graffiti," Daddy Owen narrates.
All this while, his elder brother Rufftone was making inroads in the music industry. Whenever he had time, Daddy Owen dabbled up as his brother's right hand man. Again, this gave him the perfect opportunity to interact with the music industry. It was as if the universe was aligning him with his destiny. And so when his brother challenged him to do a verse on one of his songs, Daddy Owen did not hesitate. Rufftone's producer then, the revered R Kay, was impressed and he told him as much.
"I would say that R Kay's words were what I needed to push me into music. I knew I could write and sing songs but it took R Kay's pronouncement for me to finally believe in my ability," he says.
And so in 2002, Daddy Owen released his first song Haijalishi, which became a massive hit as many youths finally found a beat they could dance and worship to. As the song's popularity grew, so did Daddy Owen's star. However, behind the scenes, things were not as rosy.
"I wanted to change how gospel music was done in the country and this did not sit well with our fairly conservative churches. Even performing in jeans was unheard of yet these were the waters we were testing. Radio stations were also not playing gospel songs and my team and I had to innovate if we were to survive," he recalls.
Daddy Owen used to perform a lot in high schools. After the shows, he would request the students to call radio stations and ask for his song when they were on holiday. His songs then started to get airplay. Also, together with Starehe MP Charles 'Jaguar' Njagua, he would personally distribute his song to DJs and request them to play it in clubs.
Internationally, there was a wave of contemporary gospel music sang by the likes of Makoma, Kirk Franklin, Mary Mary and the likes. This stood him in good stead as gospel music, as it was known then, was undergoing a transformation and he was at the forefront of this change.
"Another challenge was money. No one was paying us for our songs. It took me six years to break even and I only held on because I had a vision that gospel music would one day take over the music industry. I would share this vision with other gospel musicians and they would laugh it off as wishful thinking. I am happy I have been vindicated," he shares.
Daddy Owen says his big break in music happened in 2008 with the release of System ya Kapungala and Tobina. Interestingly, he did the songs when he was contemplating quitting music altogether so as to focus on more sustainable ventures.
After System ya Kapungala and Tobina, the calls, endorsements and awards started streaming in. Daddy Owen was the man of the moment. He went on to release well-known songs such as Mbona ft Denno, Kazi ya Msalaba, Saluti and Vanity. He was the Groove Awards male artist of the year from the year 2009 to 2011. He eventually turned down any further nomination so as to give other gospel artists a chance.
He has five albums to his name and he is currently working on the sixth, which he promises is going to be a game changer in the gospel music industry. In what way? I inquire.
"For the longest time, gospel musicians have been releasing what I refer to as 'popcorn' songs known for their longevity or, rather, lack of it. Our songs are not sung in churches during praise and worship as it was in days long gone and this is what I want to bring back. I am working on songs that people will sing to in churches, songs that will inspire congregants as well as connect them with God," he reveals.
I had the privilege of listening to one of the songs he is working on and true to his word, it is revolutionary; nothing your ears have ever heard before!
Daddy Owen unapologetically describes his music as a complex mix of Kapuka and Lingala. Content wise, he is categorical that his music is inspired by the Holy Spirit. He also draws inspiration from the environment around him including what he sees on social media.
"Packaging of the music is also very essential and this is what makes my music tick. Together with my team, we work on every aspect of the song and it takes months before we release it as we want to ensure it is of good quality. I have people, including my wife, who give me honest reviews and I use their feedback to refine my songs," the 37-year-old reveals the secret behind his success in music.
And this is what he has to say on being a gospel musician: "It's not easy. You are judged more harshly, everyone is watching your every step and not everyone will believe you are genuine about your salvation."
Founding Malaika Awards
For many years, in fact since his foray into music, Daddy Owen has always been spotted wearing dark sunglasses. This was his attempt to cover his squinted right eye. He is also not able to see with it. He says his disability is acquired and I prod on how he got it. He is uncomfortable to talk about it, brushing off my question with a nervous laugh. Clearly, it is a chapter in his book of life that he would gladly tear off if he had the power.
I prod further even mentioning a blog that implied he lost his vision during a mugging incident. He neither confirms nor denies the rumour and we leave it that. But how did his life change after the incident? He shuffles in his seat, clasps his hand in front of him and leans forward, his face facing down. A somber mood suddenly engulfs us and everything around us freezes for a moment.
"My eye was affected when I was at the cusp of launching my music career. I feared people would not accept me. There is this notion that a celebrity needs to be perfect in all ways and more so physically. My self-esteem took a beating and sunglasses became my signature as I didn't want people to see my flaw," he says wistfully.
Talking of self-esteem, Daddy Owen says he has suffered from low self-esteem for the longest time. When he was a child, ringworms and rashes covered his skin. In high school, he suffered a serious bout of acne and when he outgrew them, he heaved a sigh relief but not for long for he lost his right eye.
"All these incidents made me feel inadequate. It was only recently that I accepted myself. This came with the realisation that people don't really care about my eye but what I have to offer them. My take to anyone who feels inadequate for one reason or the other is, if you are really good at what you do, people will focus on it and not your shortfall, real or imagined," he asserts.
Daddy Owen, an ardent footballer, founded Malaika Tribute Awards in 2013 to celebrate persons living with disability and who are impacting their communities despite their challenges. He proudly refers to this group of people as unsung heroes who are silently transforming the society.
Malaika Charity Organisation, the foundation overseeing Malaika Tribute Awards, also annually organises the Malaika Disability Walk to create awareness on the plight of persons living with disability. Each year sees the number of participants double up, something that scares and excites him in equal measure.
Daddy Owen wears many hats. He was the ambassador for NHIF Supa Cover for the whole of 2018 and Twaweza with Safaricom. He is also a 'restrapreneur' – he owns a chain of restaurants, which he is not keen to reveal.
With his seemingly busy schedule, does he find time for family? "My family means everything to me. Since my schedule runs late into the night, I ensure I spend my morning hours with them. We also go for a lot of vacations together," he says as his wife nods in agreement.
Daddy Owen's dad passed on in 2017 and the pain is, understandably, still fresh. He talks highly of him. "My father had a very difficult childhood having been born out of wedlock. He endured stigma and I am proud of him for he raised us decently," the third born in a family of eight says, adding, "He didn't go to school yet he was the wisest man I have ever met. He imparted in me life lessons that I hold dear. He once told me that the world will never pay what you are worth but what you negotiated for. He also said that one's reward is equal to the quality of their work," he shares.
Himself a father, Daddy Owen wants nothing but the best for his children. Even more importantly for him, he would want his two sons to be footballers. Hs eldest son is seven years old. Daddy Owen supports the Phoenix Football Team in Nairobi and is a close ally of Tottenham Hotspurs skipper Victor Wanyama who he fondly refers to as his brother.
Job loss: 5 ways to prepare before it happens
GLADYS SOME-MWANGI – On determination, forgiveness and keeping the faith


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Deep Neural Network Predicting the EMI Induced Offset of a Differential Amplifier Stage including Training and Test Data
Dominik Zupan & Daniel Kircher
Software published via Graz University of Technology
Implementation of a neural network for predicting the EMI induced offset of a differential amplifier stage. This neural network is implemented in the Pyhton library Tensorflow. This dataset also includes data, that can be used as training and test data for the developed network.
https://doi.org/10.3217/1q54y-dsc31 Cite
TRNSYS Type 840: Simulation model for PCM/water storage tanks (Version 3.0)
Christoph Moser, Andreas Heinz & Hermann Schranzhofer
The simulation model Type 840 was developed at the Institute of Thermal Engineering, Graz University of Technology, within the framework of the European Project PAMELA (2004), the IEA SHC TASK 32 and a national research project (2006). The model enables a detailed simulation of water tanks with integrated PCM modules of different geometries (cylinders, spheres and plates) or tanks filled with a PCM slurry. An update was made by Christoph Moser in the European project...
https://doi.org/10.3217/f1k4a-gg440 Cite
Deep Neural Network Framework Predicting the EMI Induced Offset of a Differential Amplifier Stage including Training and Test Data
https://doi.org/10.3217/jnfrs-g4c04 Cite
https://doi.org/10.3217/d453f-0z754 Cite
https://doi.org/10.3217/5b8b3-15b63 Cite
TRNSYS Type 842: Model for the transient simulation of bulk PCM tanks with immersed fin and tube heat exchanger (Version 2.0)
Andreas Heinz
The simulation model Type 842 was developed at the Institute of Thermal Engineering, Graz University of Technology, within a national research project (2006). The model enables the detailed simulation of PCM (phase change material) tanks with an immersed fin and tube heat exchanger. The storage is assumed to be of rectangular shape and charged/discharged via an integrated fin and tube heat exchanger. Heat transfer (conduction) within the PCM is only considered in the direction...
https://doi.org/10.3217/0716a-69t63 Cite
https://doi.org/10.3217/mg0ve-jqr68 Cite


Look great, feel great—that's what Men's Health Weight Loss helps you do. Whether you want to trim away a few pounds from your middle, or you need a total body overhaul, we'll give you the tools you need to get the job done. We focus on simple, healthy, practical ways of controlling your weight—from smart low-carb meal plans, and effective fat-burning workouts to sneaky style tips that will make you look slimmer. Backed with the latest research and written with the usual dose of Men's Health wit, Men's Health Weight Loss is the best diet tool since the scale.


First featured here, Seattle based artist Olivia Knapp creates cross-hatched pen and ink drawings influenced by old European woodblock engravings. Specifically, Knapp pulls her inspiration from 16th through 18th century blocks, which were in all genres including religion, art, history, science and medicine. She borrows ideas from medical illustrations for her current exhibit at Hellion Gallery in Portland, "Prehensility". The title refers to the quality of an appendage adapted for grasping, for example, as a monkey's tail has adapted to grasping to a branch. The show is an extension of Knapp's previous works in both style and theme, where she explores a relationship between psychology and biology in the context of one's environment.
"Prehensility" by Olivia Knapp will be on view at Hellion Gallery from August 6th through 29th, 2015.


Call it a case of youthful naïveté – in 1994, artist Cain Motter received a convenience check in the mail for $50 – and he spent it believing it was a gift. It wasn't, of course; it was a standard marketing strategy used by many credit card companies. He learned that lesson when he received a bill in the mail for that amount plus the usual charges a credit card company applies.
Either way, it made him start thinking about credit cards in different ways, and led to a credit meltdown of an entirely different kind.
Using heat, scissors and a lot of imagination, he turns the cards he receives in the mail or collects for his art into sculptures that make a big statement about that little piece of plastic in your wallet and corporatism in general.
Whether it's the day laborers bursting from the Home Depot™ credit card, or the American soldier crawling across the face of the flag, his work looks to examine the meaning behind the symbolism and the culture that credit cards use. They're strong statements in miniature, which seems to be the point – these little cards have a lot of influence over our lives and our lifestyles. That requires thought, patience, and thorough research.
Motter may have made that mistake when he was younger, but his art serves to inspire people who see it to look at their credit cards in quite a different way.
And that's something everyone can agree is a smart thing to do.
You can find Cain Motter here on Facebook.


new prints will be here soon!
as I said we are just about ready to have our new print of the painting that inspired the Hop Cat mural... THE GEAR HEAD! we will have two types to chose from one hand embellished and one with out, both will be 11x14 in size and just right to hang anywhere in your home or office.


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Chris Brown Releases Yet Another 'Back to Sleep' Remix -- This Time Featuring Tank, Anthony Hamilton, and R. Kelly [New Music]
April 10, 2016 11:39 AM PST
Chris Brown's "Back to Sleep" has received its third remix.
The first remix included Usher and Zayn.
Trey Songz, Miguel, and August Alsina contributed to the second.
And now, Chris tapped Tank, R. Kelly, and Anthony Hamilton for what he calls the 'Legend Remix.'
Get into it below.
Tags:Anthony HamiltonChris BrownR. Kelly


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Lancashire Equalities
HomeAbout— Our Vision and Mission— Our Services— Our Members— Policy & InfluencingTrainingResearchJob ClubsBoard & Staff NewsContact Us
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One Lancashire & European Strategy
As part of the Countywide Infrastructure Support Programme Selnet Ltd have put on some briefing events. The briefing sessions are aimed to support and develop real active inclusion for the residents of Lancashire using funds being provided as part of the new European Funding Programmes 2014-20.
The sessions outlined the Big Lottery Fund plans, to match fund money within the new round of the European Social Fund (ESF).
The event covered
The background to EU funding in Lancashire
The role of the LEP and the scope of ESF
The opportunities provided to VCSE organisations in Lancashire.
The opportunities provided through the Big Lottery Fund ESF Opt In Programme
An opportunity for organisations to found out how they might get involved.
There will be a further 3 events held later in the New Year to develop further project ideas with organisations who can take the next step towards developing high quality Big Lottery Funded projects.
The aim is to boost the impact and scope of projects in Lancashire, provide a more straightforward route for engagement and ensure that all opportunities are maximised.
Lancashire Equalities is a Registered charity no : 1137828 and a Company limited by Guarantee No ; 08072150, governed by a board of trustees. Previously known as Project BME
Lancashire Equalities aims to
As an infrastructure organisation Project BME would like to encourage voluntary sector organisations to be healthy and to support the most marginalised people in our communities. We have a membership ranging of over fifty voluntary community faith member groups across the Lancashire.
Lancashire Equalities was set up to help multi disadvantaged communities access mainstream services and support provision. The team are experienced and have the expertise to assist individuals and groups to overcome health inequalities and combat exclusion, discrimination and injustice. Lancashire Equalities is strategically positioned within ONE Lancashire to act as a conduit for engagement with service providers and advocate for Social inclusion in Lancashire.
The health and wellbeing of BME communities of Lancashire, By supporting the integration, empowerment and civic engagement of BME communities to address exclusion, discrimination and injustice.
As an infrastructure organisation Lancashire Equalities would like to encourage voluntary sector organisations to be healthy and to support the most marginalised people in our communities.
Contribute to the joint strategic needs assessment (JSNA) Improve equity of access to health care and health promotion activities Improve equity in treatment and care of Black and other minority groups using health services Increase awareness and understanding of differing community needs Ensure that planning, policy development and monitoring of local health services reflect the views of black and other minority groups "


After an even start the game sparked into life on the ten minute mark. Good work from Sarah Ewens and Keeva Keenan on the Celtic left resulted in a ball being whipped into the area which the Rangers defence were able to hook clear.
A minute later though the visitors were one up. From the resulting throw in Keenan launched the ball in to the box and with the home defence struggling to properly clear their lines the ball fell to Josi Giard who curled the ball into the corner from the edge of the area and four minutes later the lead was doubled. A left wing corner made its a way to a cluster of players positioned at the far post and from the melee Celtic captain Kelly Clark rose the highest to knock the ball in from a couple of yards out.
Rangers were unable to get a foothold in the game and found themselves 3-0 down with just 17 minutes on the clock. Rangers keeper Jade Baillie came rushing out of her area to deal with a ball but didn't do enough to clear it leaving Natalie Ross with the opportunity to lob the ball into the empty net from 35 yards out. Rangers may have felt that there was a foul on Baillie in the build up but the Celtic midfielder should be credited with the composure she showed in putting away the long range effort.
In attack Rangers were resorting to long range efforts whilst bouncing balls in their own area continued to cause problems.
As the game restarted Rangers came out quickly with the always game Brown denied again this time by Cunningham as the winger cut in from the left only for the keeper to push her shot wide and out for a corner.
Those moments of Rangers attacking quality would however prove to be fleeting as Celtic were soon 4-0 up. On the 55th minute Kathleen McGovern became the latest Celtic player to benefit from the ball bouncing around the Rangers penalty area to stick a header home. Celtic continued to have chances with Baillie in the Rangers goal denying both Keenan and Ewens respectively but the fourth goal effectively killed the game.
Rangers did get on the scoresheet through Brown who, having been unlucky to see her 35 yard effort strike the crossbar a few minutes previous, found herself in the box to nod home an injury time consolation for the home side.


I found Sean Carroll's "A No Nonsense Introduction to General Relativity" (about page here. pdf here), a 24-page overview of the topic, very helpful for beginning study. It all got me over the hump of learning the meaning of various terms associated with GR, most of which I had heard before without understanding. It also outlined the most important examples.
Is there a similar document for quantum field theory, which presents the main equations, briefly describes the main ideas, and summarizes the most important applications and results so that the reader can feel the lay of the land before studying in depth?
What I would like to point out is that renormalizability is just one step in an evolutionary process of quantum field theory. In order to illuminate this point of view I will present a survey of the evolution of quantum field theory into its present form. However we will not follow the historical development, but rather, for my convenience, the lines of logic. As is well known, that is quite something different.
The conceptual basis of Quantum Field Theory. Gerard 't Hooft. In Philosophy of Physics (J. Butterfield & J. Earman, eds., Elsevier/North-Holland: Amsterdam, 2007). Author's eprint.
This reads more like a textbook geared at readers with fairly solid quantum mechanics and a good understanding of special relativity, and covers a rather wide range of topics, so it is a little more advanced.
Veltman's book Diagrammatica is awesome when it comes to the basics of field theory and what it all means.
Reading through that one is in my opinion getting it right from the horse's mouth. Not heavy on the calculations but more on how the QFT and it's tools all work together to form a coherent picture of the subject.
It's true that it's a 300 page book, but I think you'll find that it's really easy to read. It's not high powered math and honestly I haven't found anything that got to the heart of the matter as quickly or with less math. QFT is a big subject and GR is more standalone. Reading a chapter in that book will run you about 20 min and it doesn't hurt the brain because it's all stuff an undergrad can easily do. The other reviews of QFT I've seen are very technical and extremely dense. Let me know if you find a better shorter alternative: I'd like to read something that succinct myself!
Feynman's book QED: The Strange Theory of Light and Matter is probably your best bet. He spells out what is going on in the equations of quantum electrodynamics in about 120 pages and briefly touches on how these equations generalize in other parts of QFT.
There is a great introduction called "This is How Quantum Field Theory Works" which, I think, is exactly what you are looking for.
All essential concepts are introduced and the basic idea how one gets from the fundamental equations to cross sections, i.e. quantities that can be measured in experiments is sketched.
Good book on quantum field theory to start learning as an undergraduate?
Self Study Textbook Progression from QM to QFT?
Literature on Quantum Field Theory/Standard Model Physics?


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https://www.mysanantonio.com/entertainment/arts-culture/article/San-Antonio-artist-has-made-more-than-50-paleta-8328032.php
San Antonio artist has made more than 50 paleta sculptures Alamo City residents are taking a bite of
By Madalyn Mendoza, mySanAntonio.com
Published 11:40 am CDT, Tuesday, June 28, 2016
"Ordinaced Out," the paleta sculpture David Blancas made and is situated on the yard of a home in Pleasanton, Calif.
Photo: Provided By David Blancas
Paletas have become art in the studio of a local artist who has sculpted metal into more than 50 renditions of a San Antonio summertime classic.
David Blancas, a visual artist and muralist, has incorporated the sculptures into his resume, culminating a catalog of metal and resin pieces varying in size from handheld works to ones that reach 10 feet tall, he told mySA.com on Monday.
RELATED: 14 summer festivities today's San Antonio kids know nothing about
"It's a nostalgia thing," Blancas said. "Summertime memories of chasing down the paleta man."
The artist said his paleta pieces have gone to local businesses like Alamo Beer Company and private collections around San Antonio as well as California where a towering, 10-foot-tall red paleta is an eye-catcher on the yard of a home in Pleasanton.
He said people, especially kids, love seeing the over-sized paletas and are eager to get a photo beside one.
RELATED: New San Antonio paleteria's treats are food art locals will 'fall in love with'
One of the local families eating up Blancas' quirky art is that of Marissa Star, a fellow San Antonio sculpture artist.
Starr won the $600 bid in a silent auction at the 2nd annual Party for the Arts hosted by the University of Texas at San Antonio on June 15. She took home a few pieces that night, including a melting paleta sculpture of her own.
RELATED: 13 places to get the best frozen treats in San Antonio
She said her daughters — ages 9, 5, 2 — are enjoying the family's new piece where it's situated in their living room and she's sure baby No. 3 will too once she is born.
Starr said her home follows a mostly grey, neutral tone, but the 3-foot-tall paleta serves a punch of vibrancy which makes it difficult to ignore.
"I like to put art in unexpected places, I like to catch people off guard," she said.
RELATED: San Antonio model creates 'Love, Not Hate' campaign to promote acceptance after Orlando massacre
Like Blancas, paletas are tied to Starr's childhood memories of eating the icy treats from El Paraiso on Fredericksburg Road.
The artist said the prices of his pieces vary depending on size. Click through the gallery above to see some of his work.
mmendoza@mysa.com
Twitter: @MaddySkye
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Tommy Haas was the defending champion, but lost in the second round this year.

Andre Agassi won the tournament, beating Gilles Müller in the final, 6–4, 7–5.

Seeds

Draw

Finals

Top half

Bottom half

External links
 Main draw
 Qualifying draw

Los Angeles Open (tennis)
2005 ATP Tour


(1) The Legislature finds and declares that this state faces increasing competition from other states and other countries for the location and retention of private enterprises within its borders. Furthermore, the Legislature finds that there is a need to enhance and expand economic activity in the counties of this state by attracting and retaining manufacturing development, business enterprise management, and other activities conducive to economic promotion, in order to provide a stronger, more balanced, and stable economy in the state; to enhance and preserve purchasing power and employment opportunities for the residents of this state; and to improve the welfare and competitive position of the state. The Legislature declares that it is necessary and in the public interest to facilitate the growth and creation of business enterprises in the counties of the state.
(2) The governing body of a county may expend public funds to attract and retain business enterprises, and the use of public funds toward the achievement of such economic development goals constitutes a public purpose. The provisions of this chapter which confer powers and duties on the governing body of a county, including any powers not specifically prohibited by law which can be exercised by the governing body of a county, must be liberally construed in order to effectively carry out the purposes of this section.
(3) For the purposes of this section, it constitutes a public purpose to expend public funds for economic development activities, including, but not limited to, developing or improving local infrastructure, issuing bonds to finance or refinance the cost of capital projects for industrial or manufacturing plants, leasing or conveying real property, and making grants to private enterprises for the expansion of businesses existing in the community or the attraction of new businesses to the community.
(4) A contract between the governing body of a county or other entity engaged in economic development activities on behalf of the county and an economic development agency must require the agency or entity receiving county funds to submit a report to the governing body of the county detailing how county funds were spent and detailing the results of the economic development agency's or entity's efforts on behalf of the county. By January 15, 2011, and annually thereafter, the county must file a copy of the report with the Office of Economic and Demographic Research and post a copy of the report on the county's website.
1. Direct financial incentives of monetary assistance provided to a business from the county or through an organization authorized by the county. Such incentives include, but are not limited to, grants, loans, equity investments, loan insurance and guarantees, and training subsidies.
2. Indirect incentives in the form of grants and loans provided to businesses and community organizations that provide support to businesses or promote business investment or development.
3. Fee-based or tax-based incentives, including, but not limited to, credits, refunds, exemptions, and property tax abatement or assessment reductions.
4. Below-market rate leases or deeds for real property.
(b) A county shall report its economic development incentives in the format specified by the Office of Economic and Demographic Research.
(c) The Office of Economic and Demographic Research shall compile the economic development incentives provided by each county in a manner that shows the total of each class of economic development incentives provided by each county and all counties.
History.—s. 1, ch. 95-309; H.C.R. 2741 (1995); s. 1, ch. 2010-147; s. 19, ch. 2011-34; s. 51, ch. 2011-142.


The ultimate accessory to any dress has to be the jewellery that the lady wears. Taking an already stunning elegant gown and adding a necklace of freshwater pearls creates an elegant classy look that will not be forgotten in a hurry. If pearls are not suitable then we have other colour options such as silver and gold chains, simple black, or perhaps a multi-coloured necklace to complete the outfit you have chosen.


Visit your Open Interviews page to manage and easily edit your open interviews.
Job: This will sort your open interviews by the job title they are associated with.
Status: This will sort your open interviews by their status (active or inactive).
Absolute: This will sort your open interviews by their absolute deadline.
Relative: This will sort your open interviews by their relative deadline.
Created by: This will sort your open interviews by the name of the user who created them.
To sort your interviews, you can use the sorting dropdown or clicking the column headers.
To quickly view your active or inactive open interviews, check the filters boxes in the right sidebar.
To activate or deactivate an open interview, click the button under the open interview you want to activate/deactivate.
To share your open interview on social media, click the share button under the open interview you want to share.
To edit your open interview, click the edit button under the open interview you want to edit.
When you're editing an Open Interview, you'll have the option to Save as active or Save as inactive.
Save as active: This will save your open interview as active so candidates will be able to complete interviews via the link.
Save as inactive: This will save your open interview as inactive meaning candidates will not be able to complete interviews via the link.


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  	<display-name>VersionNumber</display-name>
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redpajama_set_name: RedPajamaGithub


In addition to the traditional Colonial Castings business, Glenn is also responsible for guiding the Colonial Castings Security brand from its infancy into a market leading, security door solution for fabricators and consumers.
Let's take a look at a typical day for Glenn.
How have you found it settling into your role at ALG?
Starting any job in a new place presents its challenges and my first week was a major adjustment especially learning all the new faces at a place as large as ALG. Using the staff directory on the intranet was great because it let me put a face to a name.
Overall in terms of adjusting, it didn't take much time roughly a couple of weeks and that was due to the staff of ALG being so welcoming and inclusive. By the first month I felt very welcomed by the entire company and comfortable in the sense of feeling right at home.
It's always an early start for me – either I wake up on my own or my boys will around 6.30am every morning. From there, we have breakfast which is usually Weetbix with fruit and honey. After breakfast, I get the kids ready and we make the dash for school.
After doing the school run and get into work, how do you kick off your work day?
I usually get into work between 8.30-9 am and the first thing I do is check my emails and sales progress. Once a month we also have a sales meeting, this way it allows for the reps to have more time out on the road.
Do you drink a lot of coffee throughout the day?
I'm actually not a big coffee drinker at all. I might have a cappuccino every now and then when we're out for meetings, but I'm not a regular coffee drinker. Instead of getting a caffeine fix, I like to graze on snacks during the day to keep my energy levels up.
Colonial Castings is a relatively new brand from the perspective that we're establishing them in the market so I spend a lot of time reviewing Colonial Castings products, pricing and positioning.
A lot of my time is also spent in meetings or catch ups, whether it's with other departments, speaking with other National Business Managers to get a perspective on their processes, touching base with key customers, or chatting with my team.
How do you wind your day after getting home from work?
After getting the boys settled and in their beds, I put on some TV to relax for the night. My go-to show is currently Seinfeld – a classic!


Stay right on trend this winter with our gorgeous 100% real fur keyrings. The perfect way to accessorise your keys, purse, gym bag or clutch, whether you're running errands or going out on the town. Available in nine beautiful shades, from neutrals to brights, and measuring approximately 18cm, our Bobbl keyrings make an instant style statement.


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Kenya: Government must increase protection of people living in Garissa
02 Apr 2015, 05:42pm
Responding to this morning's horrific attack on a university college in Garissa northern Kenya, Amnesty International urged the Kenyan authorities to urgently increase protection of people living in that region. Garissa University College, a constituent college of Moi University, is located in a region known to be vulnerable to Al Shabaab attacks.
Amnesty International's East Africa Regional Director Muthoni Wanyeki said:
"Citizens and public servants in the north have repeatedly expressed fears about their vulnerability to Al Shabaab attacks which the Kenyan government has failed to appropriately address. Learning institutions are meant to be safe places for students and their teachers. Their protection must be fully guaranteed.
"It is the government's responsibility to guarantee the security of all its citizens, including those in the north – and to do everything legally in their power to prevent such attacks from taking place at all.
"We urge the Government of Kenya to act decisively and within the Constitution and the law to ensure protection for those under or at risk of attack in Garissa and other areas of the north."
Amnesty also urges the authorities to conduct a prompt, impartial and effective investigation to bring the perpetrators to justice.
According to the Kenya Red Cross, so far, the attack has resulted in 65 casualties including an unspecified number of students and residents. Five casualties have been airlifted to Nairobi for treatment. Additional people are believed to be missing and are presumed kidnapped. Both local and International media have reported the armed group Al Shabaab claimed responsibility for the attack.
View latest press releases


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Kościół katolicki obrządku syryjskiego –  jeden z katolickich Kościołów wschodnich, działający na obszarze Syrii, Iraku, Libanu, Jordanii i Izraela oraz wśród diaspory syryjskiej.

Historia
Kościół powstał w VI wieku w Syrii, głównie za sprawą biskupa Edessy Jakuba Baradeusza (aram. burd'ono - "w łachmanach", od jego imienia pochodzi potoczna nazwa Kościół jakobicki) i za poparciem cesarzowej bizantyjskiej Teodory. Wędrując po Syrii w przebraniu żebraka Jakub Baradeusz własnym wysiłkiem stworzył organizację kościoła, konsekrując 27 biskupów i setki księży. Organizacja ta pozwoliła jakobitom przetrwać prześladowania ze strony władz bizantyjskich w VI i w VII wieku, najazd krzyżowców w XI wieku, masakrę dokonaną przez Tamerlana około 1400, ucisk osmański, masakrę 25 tysięcy Syryjczyków w południowej Turcji w latach 1895-1896, rzeź 90 tysięcy Syryjczyków w 1915 i wreszcie powstanie Kurdów w latach 1925-1926. W szczytowym okresie swego rozwoju (XIV wiek) Kościół jakobicki liczył 20 metropolii i 103 diecezje, sięgające na wschód do Afganistanu. Są również dowody istnienia skupisk wiernych tego kościoła w Turkiestanie i w Sinciangu. Charakterystyczną cechą hierarchii duchownej Kościoła jakobickiego był dualizm władzy - w zachodniej Syrii biskupi podlegali patriarsze, a na terenach Persji i dalej na wschód - mafrianowi (metropolicie z uprawnieniami patriarchy).

Próby unii z Rzymem podejmowano w Kościele jakobickim od XVII wieku. Na początku XVIII wieku biskup Aleppo wraz z grupą wiernych nawiązał unię z Rzymem. Od tego czasu istnieje unicki katolicki Kościół jakobicki, którego patriarcha rezyduje w Bejrucie. Kościół nie używa nazwy "jakobicki", ponieważ została ona nadana przez bizantyjskich przeciwników tego Kościoła i sugeruje, że nie jest to Kościół założony przez Apostołów.

Obecnie głową Kościoła syryjskiego jest Ignacy Józef III Younan, wybrany 20 stycznia 2009 patriarchą Antiochii.

Przypisy

Kościół katolicki w Iraku
Kościół katolicki w Libanie
Kościół katolicki w Izraelu
Kościół katolicki w Jordanii
Kościół katolicki w Autonomii Palestyńskiej
Kościół katolicki w Turcji
Kościół katolicki w Egipcie
Kościół katolicki w Sudanie
Kościół katolicki w Sudanie Południowym
Kościół katolicki w Stanach Zjednoczonych
Kościół katolicki w Kanadzie
Kościół katolicki w Wenezueli
Kościół katolicki w Kuwejcie