text:
16162 AT 2015bx 1 17:52:08.380 +13:14:25.20 PIKA PIKA PIKA Other - Other Y Y 17.6 R-Cousins 2015-07-06 23:18:22.000 Mikuz
6676 2016-11-13 13:43:00 bmikuz S. Maticic PIKA PIKA 17:52:08.380 +13:14:25.20 2015-07-06 23:18:22.000 17.6 R-Cousins 1 1 PSN PIKA Supernova was discovered by S. Maticic at Crni Vrh Observatory (mag. 17.6) on four R filter CCD images, taken on 2015 July 06.976 UT with the 60-cm f/3.3 Cichocki reflector in the course of the Comet and Asteroid Search Program (PIKA).
9611 2015-07-06 23:18:22 17.6 ABMag R-Cousins Other_Other 60 S. Maticic CCD photometry obtained on images taken with the 60-cm, f/3.3 Cichocki telescope at Crni Vrh Observatory.
tns_2015bx_atrep_6676_PIKA.JPG Graphics 2016-11-13 13:43:01 bmikuz
18263 AT 2017aue 3 16:24:18.900 +51:23:44.16 PIKA, GaiaAlerts, Pan-STARRS1 PIKA, GaiaAlerts, Pan-STARRS1 GaiaAlerts, Pan-STARRS1, PIKA Gaia - Gaia-photometric, Other - Other, PS1 - GPC1 Y Y 17.9 R-Cousins 2017-02-15 04:06:14.000 Mikuz
10270 2017-03-28 23:28:25 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe (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, D. R. Young (Queen's University Belfast) Pan-STARRS1 Pan-STARRS1 16:24:18.907 +51:23:44.21 2017-03-18 14:31:12.000 19.73 i-Sloan 1 PSN PS17bxm Pan-STARRS1
9870 2017-03-02 19:17:38 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 GaiaAlerts 16:24:18.900 +51:23:44.16 2017-03-01 00:05:45.000 18.87 G-Gaia 2 PSN Gaia17aob GaiaAlerts blue, hostless, transient GS-TEC predicts SN Ia, aka AT 2017aue
9019 2017-02-15 14:24:36 hmikuz Herman Mikuz PIKA PIKA 16:24:18.850 +51:23:44.10 2017-02-15 04:06:14.000 17.9 R-Cousins 1 1 PSN PIKA
13238 2017-02-15 04:06:14 17.9 ABMag R-Cousins Other_Other 60 H. Mikuz Supernova was discovered by H. Mikuz at Crni Vrh Observatory on four R-filter CCD images, taken on 2017 February 15.171-15.209 UT with the 60-cm f/3.3 Cichocki reflector in the course of the Comet and Asteroid Search Program (PIKA).
tns_2017aue_atrep_9019_PIKA.jpg Graphics 2017-02-15 14:24:36 hmikuz
18340 AT 2017axd 3 09:54:28.290 +67:39:41.98 LEDA 2703724 0.03469 GaiaAlerts, Pan-STARRS1 GaiaAlerts, Pan-STARRS1 GaiaAlerts, Pan-STARRS1 Gaia - Gaia-photometric, Other - Other, PS1 - GPC1 Y Y 16.75 R-Cousins 2017-02-16 19:46:33.000 Denisenko
10777 2017-04-15 23:23:19 PS1_Bot1 K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, A. Schultz, T. Lowe (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, D. R. Young (Queen's University Belfast) Pan-STARRS1 Pan-STARRS1 09:54:28.269 +67:39:41.94 2017-04-07 06:08:38.000 19.04 i-Sloan 1 PSN PS17cgm Pan-STARRS1
9418 2017-02-23 13:38:17 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 GaiaAlerts 09:54:28.290 +67:39:41.98 2017-02-17 17:42:43.000 17.69 G-Gaia 2 PSN Gaia17all GaiaAlerts candidate SN in outskirts of galaxy LEDA 2703724, aka AT 2017axd
9109 2017-02-18 18:15:39 BigDen Denis Denisenko, Dirk Cornelis 09:54:28.200 +67:39:42.00 2017-02-16 19:46:33.000 16.75 R-Cousins 2 1 PSN LEDA 2703724 0.03469 Discovered by D. Denisenko on the images obtained by D. Cornelis with 0.185-m f/6.8 APO refractor + SBIG STL-11000 CCD at e-EyE observatory (Fregenal de la Sierra, Spain). PSN was located in the same 93'x62' FOV with Gaia17aiq = 2017ati. Offset from the nucleus of host galaxy LEDA 2703724 is 9.5" East and 1.6" North.
13373 2017-02-17 05:02:24 16.66 0.08 19.5 STMag R-Cousins Other_Other 240 D. Cornelis 0.185-m f/6.8 APO refractor + SBIG STL-11000 CCD at e-EyE observatory
tns_2017axd_atrep_9109.jpg Graphics Color-combined discovery image by D. Cornelis on 2017-02-16.84 UT 2017-02-18 18:15:40 BigDen
22582 SN 2017hbg 2 1 07:27:37.350 +35:36:30.56 SN II 0.016 MCG+06-17-007 ASAS-SN, GaiaAlerts ASAS-SN, GaiaAlerts NUTS ASAS-SN, GaiaAlerts ASASSN-17nb ASASSN-1 - Brutus, Gaia - Gaia-photometric NOT - ALFOSC Y Y 1 17.3 R-Cousins 2017-09-25 13:55:12.000 Stanek
14783 2017-11-17 12:06:03 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 GaiaAlerts 07:27:37.350 +35:36:30.56 2017-10-27 09:48:57.000 18.53 G-Gaia 2 PSN Gaia17cyc GaiaAlerts confirmed SN II near galaxy MCG+06-17-007, SN2017hbg
13897 2017-10-03 20:35:19 KZStanek K. Z. Stanek, for the ASAS-SN team ASAS-SN ASAS-SN 07:27:37.320 +35:36:28.37 2017-09-25 13:55:12.000 17.3 R-Cousins 2 PSN MCG+06-17-007 ASASSN-17nb ASAS-SN In several epochs, fading, close to relatively bright galaxy, but with an unknown redshift
20866 2017-09-25 13:55:12 17.3 VegaMag R-Cousins ASASSN-1_Brutus
20865 2017-09-08 15:07:12 17 VegaMag V-Johnson ASASSN-1_Brutus [Last non detection]
1270 2017-10-06 08:27:50 Harmanen Jussi Harmanen NUTS SN II 0.016 1 NUTS Redshift from SNID. Consistent with type II SNe a few weeks after the explosion. ATel #10823 2017TNSCR1079....1H
1274 2017-10-05 03:50:24 NOT_ALFOSC 2100 Tapio Pursimo Jussi Harmanen NUTS tns_2017hbg_2017-10-05.16_NOT_ALFOSC_NUTS. tns_2017hbg_2017-10-05.16_NOT_ALFOSC_NUTS.fits Object NUTS
1274 2017-10-05 03:50:24 NOT / ALFOSC 2100 Tapio Pursimo Jussi Harmanen NUTS tns_2017hbg_2017-10-05.16_NOT_ALFOSC_NUTS. tns_2017hbg_2017-10-05.16_NOT_ALFOSC_NUTS.fits Object NUTS
23059 SN 2017htp 1 1 04:26:19.460 -10:27:45.90 SN Ic-BL 0.328 PSOJ042619.553-102745.801 0.328 STARGATE STARGATE STARGATE STARGATE GRB171010A SN VLT-UT3 - VIMOS VLT-UT2 - X-Shooter Y Y 1 21.8 R-Cousins 2017-11-01 06:00:00.000 Malesani
14429 2017-11-03 18:03:54 dmalesani Antonio de Ugarte Postigo (HETH/IAA-CSIC), Jonatan Selsing (DARK/NBI), Daniele Malesani (DARK/NBI) STARGATE STARGATE 04:26:19.460 -10:27:45.90 2017-11-01 06:00:00.000 21.8 R-Cousins 1 Other PSOJ042619.553-102745.801 0.328 GRB171010A SN STARGATE Optical counterpart of the long GRB 171010A (detected by Fermi GBM and LAT on 2017 October 10 at 19:00:50.58 UT; Omodei et al., GCN 21985). The optical afterglow was initially discovered by Thorstensen & Halpern (GCN 21897) on 2017 October 11 at 08:31 UT. Spectroscopic signatures of the associated SN were discovered by our group on 2017 November 1.
21740 2017-10-31 06:00:00 21.8 0.05 25.5 VegaMag R-Cousins VLT-UT3_VIMOS 600 VLT UT3 staff This photometry is probably heavily contaminated by the host (maybe 50/50); subtraction not possible at the present time.
1386 2017-11-03 22:32:28 dmalesani Antonio de Ugarte Postigo (HETH/IAA-CSIC), Jonatan Selsing (DARK/NBI), Daniele Malesani (DARK/NBI) STARGATE SN Ic-BL 0.328 1 1 STARGATE Spectrum taken 16.5 days (rest frame) after the GRB explosion, when the SN was dominating after the bright afterglow had faded. There is significant host contamination at the location of the afterglow, which was approximately removed using a spectrum of the adjacent region (the nucleus of the host) rescaled assuming no SN contribution at 3500 AA. 2017TNSCR1209....1P
tns_2017htp_classrep_1386_STARGATE.png Graphics The plot shows the comparison between the spectrum at the location of the GRB afterglow and some other broad-lined type Ic GRB-associated SNe (SN 1998bw from Patat et al. 2001, ApJ, 555, 900; SN 2006aj from Pian et al., Nature, 442, 1011). 2017-11-03 22:32:28 dmalesani
1390 2017-11-01 06:00:00 VLT-UT2_X-Shooter 4800 VLT UT2 staff Jonatan Selsing STARGATE tns_2017htp_2017-11-01.25_VLT-UT2_X-Shooter_STARGATE.txt Object STARGATE 2018-11-03 This is the spectrum at the afterglow location after subtracting a host template taken from the galaxy nucleus; the spectrum is rebinned by a factor 100 to increase the S/N.
1390 2017-11-01 06:00:00 VLT-UT2 / X-Shooter 4800 VLT UT2 staff Jonatan Selsing STARGATE tns_2017htp_2017-11-01.25_VLT-UT2_X-Shooter_STARGATE.txt Object STARGATE 2018-11-03 This is the spectrum at the afterglow location after subtracting a host template taken from the galaxy nucleus; the spectrum is rebinned by a factor 100 to increase the S/N.
25696 SN 2015cp 1 1 03:09:12.761 +27:31:16.95 SN Ia-91T-like 0.0413 SDSS J030912.11+273106.9 0.0413 None iPTF15fel P48 - CFH12k ESO-NTT - EFOSC2-NTT Y Y 1 19.06 R-Cousins 2015-12-28 02:27:03.000 Nugent
17553 2018-03-29 18:26:05 nugent68 Peter Nugent 03:09:12.761 +27:31:16.95 2015-12-28 02:27:03.000 19.06 R-Cousins 2 PSN SDSS J030912.11+273106.9 0.0413 iPTF15fel
26574 2015-12-28 02:27:03 19.06 0.07 20.53 ABMag R-Cousins P48_CFH12k 60 Kulkarni
26573 2014-07-16 11:44:43 20.27 ABMag R-Cousins P48_CFH12k 60 Kulkarni [Last non detection]
1818 2018-03-29 19:23:33 nugent68 Chris Frohmaier None SN Ia-91T-like 0.0413 1 2018TNSCR.418....1F
1823 2016-01-02 12:49:31 ESO-NTT_EFOSC2-NTT 900 Firth, Dimitriadis, Frohmaier Firth, Dimitriadis, Frohmaier None tns_2015cp_2016-01-02_12-49-31_ESO-NTT_EFOSC2-NTT.asci Object
1823 2016-01-02 12:49:31 ESO-NTT / EFOSC2-NTT 900 Firth, Dimitriadis, Frohmaier Firth, Dimitriadis, Frohmaier None tns_2015cp_2016-01-02_12-49-31_ESO-NTT_EFOSC2-NTT.asci Object
26823 AT 2013jw 1 08:07:32.400 +05:32:03.12 SDSS J080731.98+053203.1 0.031 CTIO-4m - DECAM Y Y 19.07 R-Cousins 2013-01-04 07:11:07.000 Nowell
18972 2018-05-30 14:20:10 Richard Nowell W. Meeussen, R. Nowell, C. Macmillan, A. Jonkeren 08:07:32.400 +05:32:03.12 2013-01-04 07:11:07.000 19.07 R-Cousins 1 PSN SDSS J080731.98+053203.1 0.031 This transient was first noticed on the Galaxy Zoo website in a discussion begun by participant Wouter Meeussen. Other participants were: Richard Nowell, ChristineM, A.F. Jonkeren . The link to the discussion is: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/20285037 . The link to the DECaLS browser where the object is visible is: http://legacysurvey.org/viewer?ra=121.8850&dec=5.5342&zoom=15&layer=decals-dr5 . Host galaxy SDSS J080731.98+053203.1 link is: http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237661064940945793
29217 2013-01-04 07:11:07 19.07 0.5 23.4 ABMag R-Cousins CTIO-4m_DECAM The magnitude value was calculated using APT and r-band values. A reference star was used: SDSS J080732.42+053238.0 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237661064940946153 . The flux values obtained using APT are: 13209 (star) and 17998 (transient). The original r-band DECaLS photometric value is 19.41. The photometric value given by DECaLS for the transient is 19.09 but I have chosen to use the value I calculated with reference to the star SDSS J080732.42+053238.0, which is 19.07, as above.
26826 AT 2016jib 1 11:55:50.472 -02:15:00.72 SDSS J115550.41-021457.9 0.345 CTIO-4m - DECAM Y Y 20.27 R-Cousins 2016-04-08 03:37:13.000 Nowell
18976 2018-05-31 14:23:38 Richard Nowell S. Pednekar, R. Nowell, A. Jonkeren, R. Jackson, C. Macmillan, W. Keel 11:55:50.472 -02:15:00.72 2016-04-08 03:37:13.000 20.27 R-Cousins 1 PSN SDSS J115550.41-021457.9 0.345 This transient was first noticed on the Galaxy Zoo website in a discussion started by participant Sharad Pednekar. Other participants are: Rick Nowell, CeciliaB, A.F. Jonkeren, Jacko99, ChristineM., W. Keel . The link to the discussion is: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/20926993 . The link to the DECaLS browser image for the transient is: http://www.legacysurvey.org/viewer?ra=178.9603&dec=-2.2502&zoom=16&layer=decals-dr5 . The host galaxy link is: SDSS J115550.41-021457.9 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237650371018358950 . Its redshift z=0.345 is an SDSS photometric value.
29223 2016-04-08 03:37:13 20.27 0.5 23.4 ABMag R-Cousins CTIO-4m_DECAM The r-band magnitude was calculated using APT. An r-band reference star was used: SDSS J115549.01-021532.9 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237650371018358940 (DECaLS mag 19.82). The calculated flux values are: transient=5803.5, star=8763.8 .
26872 AT 2016jic 1 13:02:08.136 -03:05:51.72 SDSS J130208.13-030556.6 0.088 CTIO-4m - DECAM Y Y 20.51 R-Cousins 2016-04-09 04:15:55.000 Seguin
19051 2018-06-03 16:56:22 LynnSeguin Lynn Seguin,Rick Nowell,Alex Jonkeren 13:02:08.136 -03:05:51.72 2016-04-09 04:15:55.000 20.51 R-Cousins 1 PSN SDSS J130208.13-030556.6 0.088 Galaxy Zoo volunteer, Lynn Seguin, first reported PSN to the discovery/investigative team: Rick Nowell, Alex Jonkeren, CecliaB and ChristieM on May 20, 2018, for analysis and verification. A record of the discussion can be viewed here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1267/632280?comment=1090556&page=1
29399 2016-04-09 04:15:55 20.51 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The r-band magnitude was calculated using APT and reference star: SDSS J130208.56-030522.6 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237650760786706714 . This has a DECaLS r-band value of 17.90.
26879 AT 2014fs 1 10:28:42.792 -00:08:39.48 SDSS J102842.76-000840.1 0.035 CTIO-4m - DECAM Y Y 17.65 R-Cousins 2014-12-30 08:14:17.000 Nowell
19062 2018-06-04 11:26:35 Richard Nowell A. Jonkeren, R. Nowell, M. Walmsley, L. Seguin 10:28:42.792 -00:08:39.48 2014-12-30 08:14:17.000 17.65 R-Cousins 1 PSN SDSS J102842.76-000840.1 0.035 This transient was first noticed in a discussion on the Galaxy Zoo website started by participant ak11. Other participants are: A. Jonkeren, R. Nowell, M. Walmsley, L. Seguin and Justinnnn. The discussion's link is: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/20531255 . Participant ak11 had two messages sent to that name, but there has been no reply and so no proper name can be given.
29425 2014-12-30 08:14:17 17.65 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The r-band magnitude was calculated using APT and a reference star SDSS J102842.71-000803.4 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237648721220731072 . This has a DECaLS r-band value of r=19.53. Because of the very strong source intensity of the transient, I calculated another magnitude value which used the total source intensity 66963 minus the source intensity of the host galaxy in December 2016 which is 12319. This gave a value of source intensity = 54644 for just the transient alone, as far as I could surmise. This calculation gave a r-band value = 17.87.
26888 AT 2012is 1 02:15:45.264 +00:51:38.16 SDSS J021545.50+005135.6 0.142 CTIO-4m - DECAM Y Y 19.71 R-Cousins 2012-11-16 03:07:02.000 Seguin
19072 2018-06-04 18:08:00 LynnSeguin Lynn Seguin 02:15:45.264 +00:51:38.16 2012-11-16 03:07:02.000 19.71 R-Cousins 1 1 PSN SDSS J021545.50+005135.6 0.142 Galaxy Zoo volunteer, Lynn Seguin first reported PSN to discovery/investigation team: Rich Nowell, Alex Jonkeren, CeciliaB on May 31, 2018 for analysis and investigation. A record of the discussion can be viewed here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1267/652313?comment=1087045&page=1
29444 2012-11-16 03:07:02 19.71 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The R-band magnitude is calculated using APT and the reference star = SDSS J021543.35+005145.9 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237660027202961633 DECaLS r-band ref = 19.03 https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1267/632280?comment=1090897 The AB Magnitude setting is from DECaLS description: http://legacysurvey.org/dr1/description/
tns_2012is_atrep_19072.jpg Graphics 2018-06-04 18:08:00 LynnSeguin
26911 AT 2013jx 1 22:30:50.424 -00:31:23.88 2MASX J22305050-0031267 0.081 AFJ_008 CTIO-4m - DECAM Y Y 19.05 R-Cousins 2013-09-10 01:43:45.000 Jonkeren
19106 2018-06-05 20:52:01 A.F. Jonkeren Alexander Jonkeren 22:30:50.424 -00:31:23.88 2013-09-10 01:43:45.000 19.05 R-Cousins 1 PSN 2MASX J22305050-0031267 0.081 AFJ_008 This discovery is made possible with the help of the moderators and zooites from the Zooniverse project Galaxy Zoo.
29522 2013-09-10 01:43:45 19.05 ABMag R-Cousins CTIO-4m_DECAM
26960 AT 2013jy 1 01:26:36.000 +00:24:45.00 SDSS J012636.07+002440.3 0.119 CTIO-4m - DECAM Y Y 20.47 R-Cousins 2013-10-05 07:33:55.000 Seguin
19170 2018-06-07 14:06:14 LynnSeguin S.Beer,R.Nowell,A.Jonkeren 01:26:36.000 +00:24:45.00 2013-10-05 07:33:55.000 20.47 R-Cousins 1 PSN SDSS J012636.07+002440.3 0.119 Galaxy Zoo volunteer, S.Beer first reported PSN for investigation on June 6, 2018. Analysis and verification conducted by R.Nowell, A.Jonkeren and Cecilia B. A record of the discussion can be viewed here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1267/656093?comment=1095959&page=1
29629 2013-10-05 07:33:55 20.47 1 23.6 ABMag R-Cousins CTIO-4m_DECAM "This calculation was made using APT and reference star SDSS J012640.93+002451.7 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237656512816087207 . Its R-band=16.60."
26961 AT 2013jz 1 00:26:34.248 +00:29:55.68 SDSS J002633.89+002953.5 0.071 CTIO-4m - DECAM Y Y 20.02 R-Cousins 2013-11-22 02:00:04.000 Seguin
19171 2018-06-07 15:43:07 LynnSeguin L.Seguin,R.Nowell,A.Jonkeren 00:26:34.248 +00:29:55.68 2013-11-22 02:00:04.000 20.02 R-Cousins 1 PSN SDSS J002633.89+002953.5 0.071 Galaxy Zoo volunteer, Lynn Seguin, first reported PSN to R.Nowell and A.Jonkeren for analysis and verification on June 5, 2018. A record of the conversation can be reviewed here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1267/656387?comment=1094718&page=1
29630 2013-11-22 02:00:04 20.02 1 23.6 ABMag R-Cousins CTIO-4m_DECAM "This r-band magnitude calculation used APT and reference star SDSS J002631.33+003207.8 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237663716017242141". A g-band calculation resulted in a value of 20.12."
27301 AT 2013ka 1 13:18:17.712 -02:51:43.92 SDSS J131818.07-025129.6 0.085 CTIO-4m - DECAM Y Y 20.52 R-Cousins 2013-04-02 06:16:36.000 Seguin
19662 2018-06-22 15:52:01 LynnSeguin Lynn Seguin 13:18:17.712 -02:51:43.92 2013-04-02 06:16:36.000 20.52 R-Cousins 1 PSN SDSS J131818.07-025129.6 0.085 Discovery made by Galaxy Zoo volunteer, Lynn Seguin on May 30, 2018. Analysis and verification provided by R.Nowell, A.Jonkeren and CeciliaB.
30565 2013-04-02 06:16:36 20.52 1 23.6 ABMag R-Cousins CTIO-4m_DECAM
27535 AT 2016jie 1 13:13:25.512 +00:41:20.40 SDSS J131325.47+004114.5 0.073 CTIO-4m - DECAM Y Y 19.26 R-Cousins 2016-06-07 00:37:59.000 Nowell
19971 2018-07-04 12:05:18 Richard Nowell R. Nowell 13:13:25.512 +00:41:20.40 2016-06-07 00:37:59.000 19.26 R-Cousins 1 PSN SDSS J131325.47+004114.5 0.073 This transient was noticed on the Galaxy Zoo website in a discussion started by participant Wilde1. Other participants are: Rick Nowell, A. F. Jonkeren. The address of that discussion is here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/20685458. The DECaLS browser address that shows the transient image is here: http://www.legacysurvey.org/viewer?ra=198.3563&dec=0.6890&zoom=16&layer=decals-dr5.
31120 2016-06-07 00:37:59 19.26 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The Apparent magnitude was calculated by using APT and reference star: SDSS J131328.15+004140.7 http://cas.sdss.org/dr9/en/tools/explore/obj.asp?id=1237648722312495339 (DECaLS photometry). As the object is only visible in one DECaLS r-band cutout, additional calculations were made to find the Absolute magnitude, which is -18.46 (no K correction). This matches well with other known Absolute magnitudes for transients and so serves as confirmation.
28483 AT 2016jij 1 12:37:31.296 -01:43:45.48 SDSS J123730.88-014347.7 0.081 CTIO-4m - DECAM Y Y 20.17 R-Cousins 2016-04-08 04:17:46.000 Seguin
21156 2018-08-02 14:24:11 LynnSeguin Lynn Seguin 12:37:31.296 -01:43:45.48 2016-04-08 04:17:46.000 20.17 R-Cousins 1 PSN SDSS J123730.88-014347.7 0.081 Galaxy Zoo volunteer first reported transient on July 20, 2018. Verified by CeciliaB and Rick Nowell. http://www.legacysurvey.org/viewer/cutouts/?ra=189.3803&dec=-1.7297&layer=decals-dr5
28545 AT 2012it 1 02:24:39.792 -01:06:16.56 SDSS J022439.42-010614.3 0.068 CTIO-4m - DECAM Y Y 19.19 R-Cousins 2012-11-16 02:22:27.000 Seguin
21229 2018-08-04 14:15:41 LynnSeguin Lynn Seguin 02:24:39.792 -01:06:16.56 2012-11-16 02:22:27.000 19.19 R-Cousins 1 PSN SDSS J022439.42-010614.3 0.068 First reported by Galaxy Zoo volunteer Lynn Seguin on July 28, 2018. Additional verification provided by CeciliaB, A.Jonkeren and Rick Nowell. http://www.legacysurvey.org/viewer/cutouts/?ra=36.1657&dec=-1.1048&layer=decals-dr5 http://www.legacysurvey.org/viewer?ra=36.16427699381626&dec=-1.1039785347859754&zoom=15&layer=decals-dr5
33066 2012-11-16 02:22:27 19.19 1 23.6 ABMag R-Cousins CTIO-4m_DECAM Flux Values provided by R.Nowell. FITS file: decam 151716 N7 r decam/NonDECaLS/CP201211/c4d_121116_022227_ooi_r_a1.fits.fz GUIDE STAR: SDSS J022438.96-010543.6 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237663782602604626 r-band mag. = 15.62 SN Coordinates: 36.1658 -1.1046 GS Coordinates: 36.162339154 -1.095461352 Using APT: SN Source Intensity: +25396 GS Source Intensity: +679836 mag target = mag reference – 2.5 * log (flux target / flux reference) mag target = 15.62 - 2.5 x log(25396/679836) mag target = 19.1890 https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1267/680499?comment=1168583&page=1
28767 AT 2018exw 1 00:37:26.663 +42:27:45.40 RC2_18 Other - Other Y Y 18.5 R-Cousins 2018-08-12 18:15:30.000 chinchwadkar
21502 2018-08-12 18:58:03 rohit_astro rohit chinchwadkar, malhar kendurkar 00:37:26.663 +42:27:45.40 2018-08-12 18:15:30.000 18.5 R-Cousins 1 1 PNV RC2_18
33623 2017-09-11 04:44:06 18.5 VegaMag R-Cousins Other_Other 60 ELESCOPE TYPE-CORRECTED DALL-KIRKHAM, FOCAL LENGTH- 2938MM(115.71"), CAMERA MODEL- PL16803, TELESCOPE MANUFACTURER- PLANEWAVE, NATIVE FOCAL RATIO= f/6.8, EFFECTIVE FOCAL RATIO=f/6.8, EFFECTIVE APERTURE- 432MM(17"), FOCAL REDUCER- NONE, CAMERA MANUFACTURER- FINGER LAKES INSTRUEMENTS
tns_2018exw_atrep_21502.PNG Graphics 2018-08-12 18:58:03 rohit_astro
28947 AT 2018feu 1 00:38:57.676 +42:42:59.00 M31 RC18 Other - Other Y Y 18.5 R-Cousins 2018-08-17 18:15:00.000 chinchwadkar
21721 2018-08-18 05:08:58 rohit_astro Rohit Chinchwadkar 00:38:57.676 +42:42:59.00 2018-08-17 18:15:00.000 18.5 R-Cousins 1 1 PNV M31 RC18
34023 2018-08-16 23:19:40 18.5 VegaMag R-Cousins Other_Other 20 Observations are made using Slooh Observatories in Canary Islands, Spain. Informations --> Telescope Type: Corrected Dall-Kirkham Telescope Manufacturer: PlaneWave Effective Aperture: 432mm (17") Focal Length: 2938mm (115.71") Native Focal Ratio: f/6.8 Focal Reducer: None Effective Focal Ratio: f/6.8 Camera Manufacturer: Finger Lakes Instruments Camera Model: PL16803 CCD Type: Kodak KAF-16803
tns_2018feu_atrep_21721.PNG Graphics 2018-08-18 05:08:58 rohit_astro
29008 AT 2014fu 1 02:44:04.848 +00:46:28.92 SDSS J024403.83+004629.6 0.045 CTIO-4m - DECAM Y Y 22.19 R-Cousins 2014-09-30 06:56:13.000 Nowell
21796 2018-08-21 11:54:59 Richard Nowell Richard Nowell, Glenn Lindsey 02:44:04.848 +00:46:28.92 2014-09-30 06:56:13.000 22.19 R-Cousins 1 PSN SDSS J024403.83+004629.6 0.045 This transient was first noticed in a discussion on the Galaxy Zoo website at this address: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/21665590. The discussion was started by Glenn Lindsey (participant snugthejoiner), Rick Nowell made the initial discovery that was confirmed by participant CeciliaB. DECaLS address is: http://www.legacysurvey.org/viewer?ra=41.0202&dec=0.7747&zoom=16&layer=decals-dr5
34177 2014-09-30 06:56:13 22.19 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The apparent magnitude was calculated using APT and the guide object SDSS J024400.64+004723.0 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237678617435766979. The DECaLS r-band magnitude of 19.05 was used as a reference. As the apparent magnitude was quite dim, probably because the transient had not yet reached its full luminosity, the absolute magnitude was also calculated as -14.2583 (no k-correction).
30235 AT 2014fv 1 10:51:58.488 -00:43:30.36 SDSS J105158.38-004327.0 0.108 CTIO-4m - DECAM Y Y 21.98 R-Cousins 2014-03-01 08:41:01.000 Nowell
23329 2018-10-04 09:03:46 Richard Nowell J.H.M. van Belzen, C. Macmillan 10:51:58.488 -00:43:30.36 2014-03-01 08:41:01.000 21.98 R-Cousins 1 PSN SDSS J105158.38-004327.0 0.108 This transient was first noticed in a discussion started by J.H.M van Belzen on the Galaxy Zoo website. Participants who also took part in the discussion are Christine Macmillan, Irena Copeland (user name cowslip) and Richard Nowell. The address of the discussion is: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/25811835.
37156 2014-03-01 08:41:01 21.98 0.1 23.6 ABMag R-Cousins CTIO-4m_DECAM The r-band magnitude value is taken from the DECaLS DR7 catalog. The other values are: g-band=20.58 and z-band=22.17.
30383 AT 2018hhm 1 20:54:18.430 +19:34:44.00 PIKA PIKA PIKA Other - Other Y Y 16.1 R-Cousins 2018-09-26 20:39:56.000 Mikuz
23506 2018-10-13 17:19:58 bmikuz Blaz Mikuz PIKA PIKA 20:54:18.430 +19:34:44.00 2018-09-26 20:39:56.000 16.1 R-Cousins 2 1 PNV PIKA Object was discovered by B. Mikuz at Crni Vrh Observatory on four R filter CCD images, taken on 2018 Sept. 26.861 - 26.899UT with the 60-cm f/3.3 Cichocki reflector in the course of the Comet and Asteroid Search Program (PIKA).
37517 2018-10-12 18:51:58 16.1 ABMag Clear- Other_Other 60 B. Mikuz CCD photometry obtained on images taken with the 60-cm, f/3.3 Cichocki telescope at Crni Vrh Observatory.
37516 2018-09-26 20:39:56 16.1 ABMag R-Cousins Other_Other 60 B. Mikuz CCD photometry obtained on images taken with the 60-cm, f/3.3 Cichocki telescope at Crni Vrh Observatory.
tns_2018hhm_atrep_23506_PIKA.PNG Graphics 2018-10-13 17:19:58 bmikuz
30444 AT 2013kb 1 10:06:26.640 +00:57:51.12 SDSS J100627.07+005753.2 0.046 CTIO-4m - DECAM Y Y 22.1 R-Cousins 2013-01-08 07:37:06.000 Nowell
23585 2018-10-15 12:13:09 Richard Nowell I. Theunissen-limpens, R. Nowell 10:06:26.640 +00:57:51.12 2013-01-08 07:37:06.000 22.1 R-Cousins 1 PSN SDSS J100627.07+005753.2 0.046 This transient was first noticed on the Galaxy Zoo website in a thread started by I. Theunissen-limpens at this address: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/26443737. Participants Richard Nowell and CeciliaB pointed out and confirmed the transient.
37673 2013-01-08 07:37:06 22.1 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The r-band magnitude was calculated by R. Nowell using APT. The reference star used was SDSS J100624.13+005823.9 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237651752387281368. As the Apparent magnitude seemed a low value, an Absolute magnitude was calculated, giving the approximate value of -14.41 (with K-correction).
30779 AT 2018hwp 3 02:01:10.324 -33:12:31.89 PGC 7664 Pan-STARRS1, ASAS-SN Pan-STARRS1, ASAS-SN ASAS-SN, Pan-STARRS1 ASASSN-2 - Cassius, ASASSN-5 - Payne-Gaposchkin, Other - Other, PS1 - GPC1 Y Y 17.3 R-Cousins 2018-11-05 21:45:30.000 Brosio
63144 2020-02-29 03:04:29 KZStanek K. Z. Stanek, for the ASAS-SN team ASAS-SN ASAS-SN 02:01:10.123 -33:12:28.19 2020-02-27 18:28:48.000 16.9 g-Sloan 2 PSN WISEA J020110.33-331231.8 0.035555 ASASSN-20cq ASAS-SN Present in several epochs, on the rise
123319 2020-02-27 18:28:48 16.9 ABMag g-Sloan ASASSN-5_Payne-Gaposchkin
59139 2020-01-19 01:09:13 PS1_Bot1 K. C. Chambers, T. de Boer, J. Bulger, J. Fairlamb, M. Huber, C.-C. Lin, T. Lowe, E. Magnier, A. Schultz, R. J. Wainscoat, M. Willman (IfA, University of Hawaii), K. W. Smith, D. R. Young, O. McBrien, J. Gillanders. S. Srivastav, S. J. Smartt, D. O'Neill, P. Clark, S. Sim (Queen's University Belfast), D. E. Wright (University of Minnesota) Pan-STARRS1 Pan-STARRS1 02:01:10.324 -33:12:31.89 2019-11-12 07:50:52.000 19.07 i-Sloan 1 PSN PS20el Pan-STARRS1
114518 2019-11-12 07:50:52 19.07 0.1 20.7 ABMag i-Sloan PS1_GPC1 45 Robot
24038 2018-11-05 21:54:41 abrosio Antonino Brosio, Antonio De Pieri 02:01:10.300 -33:12:30.00 2018-11-05 21:45:30.000 17.3 R-Cousins 1 1 PSN PGC 7664
38635 2018-11-05 21:45:30 17.3 Other R-Cousins Other_Other 300 RC 500 mm f8
tns_2018hwp_atrep_24038.jpg Graphics 2018-11-05 21:54:41 abrosio
31131 AT 2014fw 1 00:26:14.490 +00:32:44.16 SDSS J002614.76+003246.7 0.064 CTIO-4m - DECAM Y Y 19.87 R-Cousins 2014-11-13 01:35:12.000 Nowell
24872 2018-11-12 12:18:00 Richard Nowell L. Seguin 00:26:14.490 +00:32:44.16 2014-11-13 01:35:12.000 19.87 R-Cousins 1 PSN SDSS J002614.76+003246.7 0.064 This transient was first noticed in a discussion started by Lynn Seguin on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/21661144. Other participants were: CeciliaB, A.F. Jonkeren, GenieBresh, C. Macmillan and R. Nowell.
41449 2014-11-13 01:35:12 19.87 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The apparent magnitude was calculated by Richard Nowell using APT and guide star: SDSS J002607.33+003316.7 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237663716017176821. Absolute magnitude was calculated as -17.47 (with k-correction).
31230 AT 2013kc 1 10:43:49.272 +00:51:49.32 SDSS J104349.06+005155.3 0.118 CTIO-4m - DECAM Y Y 17.9 R-Cousins 2013-03-16 01:48:25.000 Nowell
25084 2018-11-17 16:32:37 Richard Nowell L. Seguin, J.H.M. van Belzen 10:43:49.272 +00:51:49.32 2013-03-16 01:48:25.000 17.9 R-Cousins 1 PSN SDSS J104349.06+005155.3 0.118 This transient was first noticed in a discussion started by J.H.M. van Belzen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/25812083. Other participants were: S. Beer (bluemagi), CeciliaB, AdTheImpaler and Rick Nowell.
42242 2013-03-16 01:48:25 17.9 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The magnitude was calculated by Richard Nowell using APT and reference star: SDSS J104343.95+005214.1 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237654671350956139. Absolute magnitude was calculated as -20.72 (with k-correction).
31237 AT 2013kd 2 13:51:47.568 +02:44:53.16 SDSS J135147.61+024450.6 0.069 CTIO-4m - DECAM, PS1 - GPC1 Y Y 19.15 R-Cousins 2013-04-02 07:55:18.000 Nowell
34548 2019-05-08 14:33:59 Richard Nowell R. Nowell, A. Bellinghausen 13:51:47.553 +02:44:53.34 2012-04-19 03:50:37.000 20.93 r-Sloan 1 PSN SDSS J135147.61+024450.6 0.069387 This transient was first noticed in a discussion started by Angelika Bellinghausen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/27360130. Other participants are Christine Macmillan and CeciliaB. This transient was originally reported as AT 2013kd but a more recent observation was found.
64977 2012-04-19 03:50:37 20.93 1 23.2 ABMag r-Sloan PS1_GPC1 784 The Pan-STARRS r-band Apparent magnitude was calculated by R. Nowell using APT and reference star: SDSS J135145.92+024535.1 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237674602676814210. An r-band Absolute magnitude of -16.59 was also calculated.
25093 2018-11-18 16:11:35 Richard Nowell R. Nowell, A. Bellinghausen 13:51:47.568 +02:44:53.16 2013-04-02 07:55:18.000 19.15 R-Cousins 1 PSN SDSS J135147.61+024450.6 0.069 This transient was first noticed in a discussion started by Angelika Bellinghausen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/27360130. Other participants are: Christine Macmillan (ChristineM), CeciliaB and Rick Nowell.
42260 2013-04-02 07:55:18 19.15 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The magnitude was calculated by Richard Nowell using APT and reference star: SDSS J135145.92+024535.1 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237674602676814210. Absolute magnitude was calculated as -18.37 (with K-correction).
32534 AT 2016jiw 1 11:49:28.128 +01:54:12.60 SDSS J114928.25+015415.9 0.137 CTIO-1.5m - LORAL Y Y 20.23 R-Cousins 2016-04-08 02:57:27.000 Nowell
26972 2018-12-23 14:15:14 Richard Nowell S. Beer, C. Macmillan 11:49:28.128 +01:54:12.60 2016-04-08 02:57:27.000 20.23 R-Cousins 1 PSN SDSS J114928.25+015415.9 0.137 This transient was first noticed in a discussion started by Sylvia Beer (Bluemagi) on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/26444004. Other participants are: Christine Macmillan (ChristineM) and Richard Nowell.
47739 2016-04-08 02:57:27 20.23 1 23.6 ABMag R-Cousins CTIO-1.5m_LORAL The Apparent magnitude was calculated by Richard Nowell using APT and reference star: SDSS J114932.45+015524.6 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237671128589795496. An Absolute magnitude of -18.76 was also calculated.
32882 SN 2018kzc 1 1 06:28:58.250 +38:43:31.00 SN Ia 0.0378 PIKA PIKA Padova-Asiago PIKA Other - Other Ekar - AFOSC Y Y 1 17.5 R-Cousins 2018-12-27 23:03:12.000 Mikuz
27460 2018-12-28 15:16:18 hmikuz Herman Mikuz PIKA PIKA 06:28:58.250 +38:43:31.00 2018-12-27 23:03:12.000 17.5 R-Cousins 2 1 PSN PIKA Discovered by S. Maticic on four images taken with 60-cm, f/3.3 Cichocki telescope and R filter at Crni Vrh Observatory in the course of the Comet and Asteroid Search Program (PIKA).
48652 2018-12-27 23:03:12 17.5 19 ABMag R-Cousins Other_Other 60 S. Maticic 0.60-m, f/3.3 Deltagraph
48651 2018-12-15 23:49:00 19.8 ABMag Clear- Other_Other 60 S. Maticic [Last non detection] 0.60-m, f/3.3 Deltagraph
tns_2018kzc_atrep_27460_PIKA.jpg Graphics Image 2018-12-28 15:16:18 hmikuz
3321 2018-12-29 07:48:19 linatoma Benetti, Tomasella, Cappellaro, Turatto Padova-Asiago SN Ia 0.0378 1 Padova-Asiago Spectrum very similar to that of SN 1995D about 6 days before B maximum. The expansion velocity deduced from the SiII 635.5nm minimum is about 11300 km/s. The redshift has been deduced from the SN spectral fitting. 2018TNSCR2004....1B
3329 2018-12-28 20:52:48 Ekar_AFOSC 2400 benetti benetti Padova-Asiago tns_2018kzc_2018-12-28.87_Ekar_AFOSC_Padova-Asiago.dat tns_2018kzc_2018-12-28.87_Ekar_AFOSC_Padova-Asiago.fits Object Padova-Asiago
3329 2018-12-28 20:52:48 Ekar / AFOSC 2400 benetti benetti Padova-Asiago tns_2018kzc_2018-12-28.87_Ekar_AFOSC_Padova-Asiago.dat tns_2018kzc_2018-12-28.87_Ekar_AFOSC_Padova-Asiago.fits Object Padova-Asiago
33741 AT 2018lmm 1 15:28:11.800 +30:17:04.00 SDSS J152811.89+301708.0 EGR_001 CTIO-4m - DECAM Y Y 21.06 R-Cousins 2018-03-17 08:26:08.000 Galvez Ranera
28830 2019-01-14 23:10:10 EmilioGR Emilio Galvez Ranera 15:28:11.800 +30:17:04.00 2018-03-17 08:26:08.000 21.06 R-Cousins 2 PSN SDSS J152811.89+301708.0 EGR_001 This discovery is made possible with the help of the Legacy Survey discussion board and specially to Alexander Jonkeren. Images in http://legacysurvey.org/viewer?ra=232.0491&dec=30.2843&zoom=15&layer=decals-dr7
51492 2018-03-19 08:09:40 21.51 ABMag g-Sloan CTIO-4m_DECAM
34717 AT 2017kds 1 11:41:08.774 +10:20:03.03 2MASX J11410850+1020145 0.118578 CTIO-4m - DECAM Y Y 17.72 R-Cousins 2017-03-31 03:35:30.000 Nowell
30189 2019-02-26 10:00:37 Richard Nowell I. Theunissen-limpens, R. Nowell, A. Jonkeren 11:41:08.774 +10:20:03.03 2017-03-31 03:35:30.000 17.72 R-Cousins 1 PSN 2MASX J11410850+1020145 0.118578 This transient was first noticed by Ine Theunissen-limpens in a discussion on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/28488522. Also taking part in the discussion were CeciliaB, Alexander Jonkeren and Richard Nowell.
54298 2017-03-31 03:35:30 17.72 0.1 24 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude of 17.72 is taken from the DECaLS DR7 catalogue. An Absolute magnitude of -20.94 was also calculated.
35757 AT 2017kdt 1 14:29:48.408 +01:20:15.00 SDSS J142948.59+012012.4 0.14315 CTIO-4m - DECAM Y Y 20.44 R-Cousins 2017-03-01 08:46:12.000 Nowell
31816 2019-04-01 08:31:16 Richard Nowell C. Macmillan, M. A. Kovic 14:29:48.408 +01:20:15.00 2017-03-01 08:46:12.000 20.44 R-Cousins 1 PSN SDSS J142948.59+012012.4 0.14315 This transient was discovered in a discussion on the Galaxy Zoo website started by participant timbertom1957 here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/27362279. Also taking part in the discussion were Ine Theunissen-Limpens, Sylvia Beer and participant Kendawg42.
58320 2017-03-01 08:46:12 20.44 0.1 24 ABMag R-Cousins CTIO-4m_DECAM The r-band magnitude was found by using the DECaLS DR7 catalogue which has a value already calculated.
37732 AT 2017kdw 1 01:34:48.880 +21:25:20.14 NGC 606 0.03326 CTIO-4m - DECAM Y Y 21.73 R-Cousins 2017-07-26 10:05:34.000 Nowell
35317 2019-05-18 08:57:13 Richard Nowell Ine Theunissen-Limpens 01:34:48.880 +21:25:20.14 2017-07-26 10:05:34.000 21.73 R-Cousins 2 PSN NGC 606 0.03326 This transient was first discussed on the Galaxy Zoo website by Ine Theunissen here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1268/996160. Melina Thévenot also took part in the discussion.
66390 2017-09-15 06:36:43 22.24 1 24.6 ABMag g-Sloan CTIO-4m_DECAM The g-band Apparent magnitude was calculated by Melina Thévenot using APT and reference star: SDSS J013449.93+212640.6 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237679542435184643. A g-band Absolute magnitude of -13.43 was also calculated.
66389 2017-07-26 10:05:34 21.73 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude was calculated by R. Nowell using APT and reference star: SDSS J013446.32+212616.9 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237679542435119373. An r-band Absolute magnitude of -14.15 was also calculated.
38213 AT 2015cy 1 11:55:49.584 +00:01:44.40 SDSS J115549.70+000143.2 0.108996 CTIO-4m - DECAM Y Y 20.11 R-Cousins 2015-04-11 03:02:05.000 Nowell
36084 2019-05-31 08:55:49 Richard Nowell Marco A. Kovic 11:55:49.584 +00:01:44.40 2015-04-11 03:02:05.000 20.11 R-Cousins 1 PSN SDSS J115549.70+000143.2 0.108996 This transient was first noticed by Marco Kovic on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/32408470.
67731 2015-04-11 03:02:05 20.11 1 23.6 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude value was taken from the DECaLS DR7 catalogue. A r-band Absolute magnitude of -18.51 was also calculated.
39164 AT 2017kdx 1 15:26:29.988 +14:32:04.44 SDSS J152630.04+143211.1 0.133642 CTIO-4m - DECAM Y Y 22.28 R-Cousins 2017-03-28 09:31:29.000 Nowell
37940 2019-06-16 12:41:57 Richard Nowell Ine Theunissen-Limpens 15:26:29.988 +14:32:04.44 2017-03-28 09:31:29.000 22.28 R-Cousins 2 PSN SDSS J152630.04+143211.1 0.133642 This transient was first noticed by Ine Theunissen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/34060241.
71935 2017-03-29 08:50:07 22.06 1 ABMag g-Sloan CTIO-4m_DECAM The g-band Apparent magnitude was calculated by Richard Nowell using APT and reference star:SDSS J152630.75+143211.7 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237668311625695500. A g-band Absolute magnitude of -16.88 was also calculated.
71934 2017-03-28 09:31:29 22.28 1 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude was calculated by Richard Nowell using APT and the reference star: SDSS J152630.75+143211.7 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237668311625695500. An r-band Absolute magnitude of -16.66 was also calculated.
42341 AT 2015db 1 01:31:02.328 -10:17:15.00 2MASX J01310241-1017122 0.065135 CTIO-4m - DECAM Y Y 21.3 R-Cousins 2015-08-18 09:40:24.000 Nowell
42872 2019-08-02 08:24:13 Richard Nowell Marco A. Kovic 01:31:02.328 -10:17:15.00 2015-08-18 09:40:24.000 21.3 R-Cousins 1 PSN 2MASX J01310241-1017122 0.065135 This transient was found by Marco Kovic using the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/34211970.
81384 2015-08-18 09:40:24 21.3 1 ABMag R-Cousins CTIO-4m_DECAM The Apparent r-band magnitude was taken from the values found on the DECaLS browser. An r-band Absolute magnitude of -16.0 was also calculated.
43425 AT 2016jjc 1 09:12:26.784 +13:59:52.44 2MASX J09122660+1359535 0.0774 CTIO-4m - DECAM Y Y 20.04 R-Cousins 2016-01-11 06:38:53.000 Nowell
44250 2019-08-19 09:35:39 Richard Nowell Y.F.A. Epitropoulos, M.A. Kovic 09:12:26.784 +13:59:52.44 2016-01-11 06:38:53.000 20.04 R-Cousins 1 PSN 2MASX J09122660+1359535 0.0774 This transient was first observed by Yannis Epitropoulos and Marco Kovic on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/35623547.
83971 2016-01-11 06:38:53 20.04 1 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude was taken from the DECaLS DR7 catalog. An Absolute magnitude of -17.62 was also calculated.
44491 AT 2018lqg 1 16:22:54.144 +14:21:00.00 SDSS J162254.51+142100.8 0.051246 CTIO-4m - DECAM Y Y 19.68 R-Cousins 2018-05-18 03:36:43.000 Nowell
46042 2019-09-04 10:15:18 Richard Nowell Ine Theunissen-Limpens 16:22:54.144 +14:21:00.00 2018-05-18 03:36:43.000 19.68 R-Cousins 1 PSN SDSS J162254.51+142100.8 0.051246 This transient was first observed by Ine Theunissen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/35622636.
87912 2018-05-18 03:36:43 19.68 1 ABMag R-Cousins CTIO-4m_DECAM 87 The r-band Apparent magnitude was calculated by Richard Nowell using APT and reference star: SDSS J162258.52+142032.4 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237665549439926864. An r-band Absolute magnitude of -17.06 was also calculated.
45016 AT 2017kea 1 11:08:45.519 +02:02:46.00 PKS 1106+023 0.15742 CTIO-4m - DECAM Y Y 21.79 R-Cousins 2017-03-04 04:51:36.000 Nowell
47034 2019-09-16 11:58:15 Richard Nowell Ine Theunissen-Limpens 11:08:45.519 +02:02:46.00 2017-03-04 04:51:36.000 21.79 R-Cousins 1 PSN PKS 1106+023 0.15742 This transient was first observed by Ine Theunissen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/35623082. Marco Kovic started the discussion.
90218 2017-03-04 04:51:36 21.79 1 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude was calculated by Richard Nowell using APT and reference star: SDSS J110849.41+020337.6 http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237651753467838615. The r-band Absolute magnitude of -17.44 was also calculated.
46065 AT 2019rsh 1 04:14:01.210 -55:56:52.50 Germes V4 Other - Other Y Y 17.3 R-Cousins 2019-10-02 13:36:42.000 Denisenko
48458 2019-10-02 15:15:46 BigDen Denis Denisenko 04:14:01.210 -55:56:52.50 2019-10-02 13:36:42.000 17.3 R-Cousins 2 Other Germes V4 Red dwarf flare discovered on iTelescope.Net T32 images
92932 2019-10-02 13:36:42 17.3 0.1 19 ABMag R-Cousins Other_Other 60 D. Denisenko iTelescope.Net T32 (0.43-m f/6.8 reflector + CCD) in Siding Spring
92931 2019-10-02 13:35:18 19 ABMag R-Cousins Other_Other 60 D. Denisenko [Last non detection] iTelescope.Net T32 (0.43-m f/6.8 reflector + CCD) in Siding Spring
46282 AT 2016jjd 1 10:34:38.592 +01:51:27.00 SDSS J103438.60+015127.1 0.137 CTIO-4m - DECAM Y Y 18.09 R-Cousins 2016-01-12 08:19:58.000 Nowell
48759 2019-10-06 09:51:50 Richard Nowell Richard Nowell 10:34:38.592 +01:51:27.00 2016-01-12 08:19:58.000 18.09 R-Cousins 1 PSN SDSS J103438.60+015127.1 0.137 This transient was first observed by Rick Nowell in a discussion started by Angelika Bellinghausen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/26443475. Ine Theunissen, Christine Macmillan and CeciliaB also discussed the transient.
93509 2016-01-12 08:19:58 18.09 1 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude was taken from the DR7 catalogue. The r-band Absolute magnitude of -20.83 was also calculated using the SDSS PhotoZ estimate.
46429 AT 2016jje 1 09:11:05.160 +04:38:43.80 SDSS J091105.32+043841.5 0.110428 CTIO-4m - DECAM Y Y 20.78 R-Cousins 2016-01-16 05:12:04.000 Nowell
49000 2019-10-08 15:18:45 Richard Nowell Marco Kovic 09:11:05.160 +04:38:43.80 2016-01-16 05:12:04.000 20.78 R-Cousins 1 PSN SDSS J091105.32+043841.5 0.110428 This transient was first observed by Marco Kovic on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/36250950. Ine Theunissen and Claude Cornen also took part in the discussion. The transient is visible in HSC DR2 in February 2016.
47124 AT 2018lqn 1 15:22:27.096 +26:22:11.28 SDSS J152227.12+262215.6 0.080908 CTIO-4m - DECAM Y Y 18.83 R-Cousins 2018-02-25 00:00:00.000 Theunissen
50681 2019-10-24 15:21:24 Ine Theunissen Limpens Ine Theunissen-Limpens 15:22:27.096 +26:22:11.28 2018-02-25 00:00:00.000 18.83 R-Cousins 1 PSN SDSS J152227.12+262215.6 0.080908 This transient was first noticed by Ine Theunissen-Limpens on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/37390699. Richard Nowell also took part in the discussion.
97928 2018-02-25 00:00:00 18.83 1 ABMag R-Cousins CTIO-4m_DECAM
48021 AT 2017keh 1 10:22:58.536 -00:10:27.48 SDSS J102258.60-001023.9 0.113118 CTIO-4m - DECAM Y Y 20.22 R-Cousins 2017-03-01 04:02:45.000 Theunissen
52370 2019-11-12 12:19:41 Ine Theunissen Limpens Ine Theunissen-Limpens 10:22:58.536 -00:10:27.48 2017-03-01 04:02:45.000 20.22 R-Cousins 1 PSN SDSS J102258.60-001023.9 0.113118 This transient was first observed by Ine Theunissen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/37904336. Richard Nowell also took part in the discussion.
101654 2017-03-01 04:02:45 20.22 1 ABMag R-Cousins CTIO-4m_DECAM
49275 AT 2015di 1 08:31:19.152 +26:36:37.44 SDSS J083119.73+263638.3 0.0975 CTIO-4m - DECAM Y Y 19.23 R-Cousins 2015-04-11 00:11:27.000 Theunissen
54329 2019-12-11 17:03:53 Ine Theunissen Limpens Ine Theunissen-Limpens 08:31:19.152 +26:36:37.44 2015-04-11 00:11:27.000 19.23 R-Cousins 1 PSN SDSS J083119.73+263638.3 0.0975 This transient was first observed by Ine Theunissen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/36227773 Christine Macmillan also took part in the discussion.
54081 AT 2018lrb 1 12:19:05.472 +27:17:47.04 IC 3143 0.023316 DES DES CTIO-4m - DECAM Y Y 20.5 R-Cousins 2018-02-18 07:23:03.000 Theunissen
61711 2020-02-13 12:23:34 Ine Theunissen Limpens Ine Theunissen-Limpens DES 12:19:05.472 +27:17:47.04 2018-02-18 07:23:03.000 20.5 R-Cousins 1 PSN IC 3143 0.023316 DES This transient was first discovered by Ine Theunissen while examining galaxy IC 3143 in the Legacy Survey Sky Viewer here: http://www.legacysurvey.org/viewer?ra=184.7728&dec=27.2964&layer=decals-dr7&zoom=15. Rick Nowell also took part in the discussion started by Ine Theunissen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1269/1203627 and here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1268/1185971.
120025 2018-02-18 07:23:03 20.5 1 ABMag R-Cousins CTIO-4m_DECAM
55379 AT 2016jji 1 04:01:45.720 -06:22:03.72 2MASX J04014560-0622026 0.057148 CTIO-4m - DECAM Y Y 19.29 R-Cousins 2016-12-21 04:50:26.000 Nowell
63790 2020-03-08 11:51:19 Richard Nowell Sylvia Beer 04:01:45.720 -06:22:03.72 2016-12-21 04:50:26.000 19.29 R-Cousins 1 PSN 2MASX J04014560-0622026 0.057148 This transient was first observed by Sylvia Beer (aka Bluemagi) on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/subjects/21667511. Christine Macmillan and Alexander Jonkeren also took part in the discussion.
124707 2016-12-21 04:50:26 19.29 1 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude was calculated by Richard Nowell using APT and reference star: SDSS J040152.30-062206.3 http://skyserver.sdss.org/dr12/en/tools/explore/Summary.aspx?id=1237652899700605074. The r-band Absolute magnitude of -17.64 was also calculated.
55427 AT 2017kel 1 11:31:39.384 +17:02:23.28 SDSS J113139.16+170223.5 0.082564 CTIO-4m - DECAM Y Y 17.93 R-Cousins 2017-05-21 00:23:19.000 Theunissen
63861 2020-03-09 01:39:38 Ine Theunissen Limpens Ine Theunissen-Limpens 11:31:39.384 +17:02:23.28 2017-05-21 00:23:19.000 17.93 R-Cousins 1 PSN SDSS J113139.16+170223.5 0.082564 This transient was first discovered by Ine Theunissen on the Galaxy Zoo Mobile website here: https://www.zooniverse.org/projects/mikewalmsley/galaxy-zoo-mobile/talk/subjects/40282075. Richard Nowell also took part in the discussion started by Ine Theunissen on the Galaxy Zoo website here: https://www.zooniverse.org/projects/zookeeper/galaxy-zoo/talk/1269/1203627.
124800 2017-05-21 00:23:19 17.93 1 ABMag R-Cousins CTIO-4m_DECAM The r-band Apparent magnitude of 17.93 was calculated by Richard Nowell using APT, reference star SDSS J113138.83+170400.3 and DECaLS magnitudes. http://skyserver.sdss.org/dr14/en/tools/explore/Summary.aspx?id=1237668585434578952. http://www.legacysurvey.org/viewer?ra=172.9118&dec=17.0666&layer=decals-dr7&zoom=15. The r-band Absolute magnitude of -19.89 was calculated by Ine Theunissen.
56062 SN 2020epi 4 1 12:22:08.778 +06:05:59.07 SN Ic 0.024 PGC 40043 0.024562 TAROT, ATLAS, Pan-STARRS1, YSE TAROT, ATLAS, Pan-STARRS1 None ATLAS, Pan-STARRS1, TAROT ATLAS1 - ACAM1, Other - Other, PS1 - GPC1 Other - Other Y Y 2 18.5 R-Cousins 2020-03-19 02:53:00.000 Conseil
69212 2020-04-29 16:35:02 YSE_Bot1 D. O. Jones (UC Santa Cruz), K. D. French (Carnegie, Illinois), A. Agnello, C. R. Angus, Z. Ansari, N. Arendse, C. Gall, C. Grillo, S. H. Bruun, C. Hede, J. Hjorth, L. Izzo, H. Korhonen, S. Raimundo, D. Kodi Ramanah, A. Sarangi, R. Wojtak (DARK, U Copenhagen), K. Auchettl (DARK, UC Santa Cruz, U Melbourne), K. C. Chambers, M. E. Huber, E. A. Magnier, T. J. L. de Boer, J. R. Fairlamb, C. C. Lin, R. J. Wainscoat, T. Lowe, M. Willman, J. Bulger, A. S. B. Schultz (IfA, Hawaii), A. Engel, A. Gagliano, G. Narayan, M. Soraisam (Illinois), Q. Wang (JHU), A. Rest (JHU, STScI), S. J. Smartt, K. W. Smith (Queen's University Belfast), K. Alexander, A. Baldeschi, P. Blanchard, D. Coppejans, L. DeMarchi, A. Hajela, W. Jacobson-Galan, R. Margutti, D. Matthews, C. Stauffer, M. Stroh, G. Terreran (Northwestern), M. Drout (U Toronto), D. A. Coulter, G. Dimitriadis, R. J. Foley, T. Hung, C. D. Kilpatrick, C. Rojas-Bravo, M. R. Siebert (UC Santa Cruz), E. Ramirez-Ruiz (UC Santa Cruz, DARK) YSE Pan-STARRS1 12:22:08.778 +06:05:59.07 2020-04-17 10:37:55.200 20.1 g-Sloan 1 PSN PS20aji Pan-STARRS1
133785 2020-04-17 10:37:55 20.1 0.21 21 ABMag g-Sloan PS1_GPC1 27 Robot
65162 2020-03-28 15:57:37 PS1_Bot1 K. C. Chambers, T. de Boer, J. Bulger, J. Fairlamb, M. Huber, C.-C. Lin, T. Lowe, E. Magnier, A. Schultz, R. J. Wainscoat, M. Willman (IfA, University of Hawaii), K. W. Smith, D. R. Young, O. McBrien, J. Gillanders. S. Srivastav, S. J. Smartt, D. O'Neill, P. Clark, S. Sim (Queen's University Belfast), D. E. Wright (University of Minnesota) Pan-STARRS1 Pan-STARRS1 12:22:08.774 +06:05:59.05 2020-03-25 11:19:40.800 17.92 w-PS1 1 PSN PS20aji Pan-STARRS1
64763 2020-03-23 00:58:19 ATLAS_Bot1 J. Tonry, L. Denneau, A. Heinze, H. Weiland, H. Flewelling (IfA, University of Hawaii), B. Stalder (LSST), A. Rest (STScI), C. Stubbs (Harvard University), K. W. Smith, S. J. Smartt, D. R. Young, S. Srivastav, O. McBrien, D. O'Neill, P. Clark, M. Fulton, J. Gillanders, M. Dobson (Queen's University Belfast), T.-W. Chen (MPE), D. E. Wright (University of Minnesota), J. Anderson (ESO) ATLAS ATLAS 12:22:08.748 +06:05:58.63 2020-03-22 11:42:43.200 18.032 cyan-ATLAS 2 PSN ATLAS20ier ATLAS
64609 2020-03-20 07:35:34 econseil Emmanuel Conseil TAROT TAROT 12:22:08.760 +06:06:01.30 2020-03-19 02:53:00.000 18.5 R-Cousins 3 2 PSN PGC 40043 0.024562 TAROT Emmanuel Conseil, on behalf of the TAROT collaboration, reports the discovery of a probable supernova in the galaxy PGC 40043 located at R.A = 12 22 08.76 and Decl = +06 06 01.3 (J2000.0), which is 13.5" E and 13.1"S from the nucleus of PGC 40043. The transient was visible on 2 images (120s exposures), taken by the TAROT Calern telescope on 2020-03-19 at 02h53 UTC, at magnitude 18.5 (Red filter, limiting R mag 19.0). Nothing was visible at this location on previous images taken by the same telescope on 2020-03-16 at 03h08 UTC (limiting R mag 18.5). Image is visible here : https://www.flickr.com/photos/econseil/49678972857 The transient is also visible on images taken by Alain Klotz and Antoine Cailleau on 2020-03-19 at 21h30 UTC with the "observatoire de Cuq-les-Vielmur" telescope (T510mm + camera Andor 486, France), at magnitude 17.8 (V filter). Image is visible at this location : https://www.flickr.com/photos/econseil/49678152808
125368 2020-03-19 21:28:48 17.8 19 VegaMag V-Johnson Other_Other 460 Alain Klotz; Antoine Cailleau The transient is also visible on images taken by Alain Klotz and Antoine Cailleau on 2020-03-19 at 18h00 UTC with the "observatoire de Cuq-les-Vielmur" telescope (T510 + camera Andor 486, France), at magnitude 17.8 (V filter). Image is visible at this location : https://www.flickr.com/photos/econseil/49678152808
125367 2020-03-19 02:53:00 18.5 19 VegaMag R-Cousins Other_Other E. Conseil The transient was visible on 2 images (120s exposures), taken by the TAROT Calern telescope on 2020-03-19 at 02h53 UTC, at magnitude 18.5 (Red filter, limiting R mag 19.0)
125366 2020-03-16 03:08:00 18.5 VegaMag R-Cousins Other_Other [Last non detection] Nothing was visible at this location on previous images taken by the TAROT Calern telescope on 2020-03-16 at 03h08 UTC (limiting R mag 18.5).
tns_2020epi_atrep_64609_TAROT.png Graphics Discovery image with the Tarot Calern telescope 2020-03-20 07:35:34 econseil
tns_2020epi_atrep_64609_TAROT_0.png Graphics Confirmation image by Alain Klotz and Antoine Cailleau, with the T510mm telescope from "observatoire de Cuq-les-Vielmur", France 2020-03-20 07:35:34 econseil
6429 2020-03-31 14:02:02 THO Robin Leadbeater None SN Ic 0.024 2 3 Low resolution R~130 spectra taken 2020-03-26 and 2020-03-30 show broad features with matches using SNID (Blondin, S. & Tonry, J. L. 2007. ApJ, 666, 1024) to both normal and broad lined type Ic supernovae a few days after maximum. (The redshift given is that of the proposed host PGC4003) 2020TNSCR.926....1L
tns_2020epi_classrep_6429.ps Graphics 2020-03-31 14:02:02 THO
tns_2020epi_classrep_6429_0.ps Graphics 2020-03-31 14:02:02 THO
6438 2020-03-26 23:23:06 Other_Other 3603 R Leadbeater R Leadbeater None tns_2020epi_2020-03-26_23-23-06_Other_Other.dat tns_2020epi_2020-03-26_23-23-06_Other_Other.fit Object R~130 spectrum obtained using modified ALPY spectrograph at Three Hills Observatory as described here http://www.threehillsobservatory.co.uk/astro/spectroscopy_20.htm
6439 2020-03-30 23:03:31 Other / Other 4804 R Leadbeater R Leadbeater None tns_2020epi_2020-03-30_23-03-31_Other_Other.dat tns_2020epi_2020-03-30_23-03-31_Other_Other.fit Object R~130 spectrum obtained using modified ALPY spectrograph at Three Hills Observatory as described here http://www.threehillsobservatory.co.uk/astro/spectroscopy_20.htm


Dear Lord Jesus I just want to lift up my heart to you today as this is our anniversary, and yet Lord, recently things between us have become strained and difficult and I feel sad and confused and quite alone.
Lord I don't know where things went wrong and I don't know how I could have done things differently, but Lord I am sorry for the part that I have played. I know that in many ways I have been selfish and wanted things my way, when Your word says that we should do nothing from selfish ambition or conceit, but in humility consider the other person as more significant than ourselves.
Lord I ask Your forgiveness and pray that You would help me to start to live a life that is honouring to You. Heal my marriage I pray and show me Lord how I can bridge the gap that is widening between us. Teach me Your ways, lead me on a straight path and graciously teach me How to live as unto the Lord, in Jesus name I pray.


Till the advent of Parama Guru Sri Sri Sri Mahavatar Babaji, the highest spiritual Master of Kriya Yoga, this practice had remained a strictly guarded secret handed over by disciplic succession from guru(spiritual master) to shishya(disciple). This tradition had remained within guru and disciple parampara (family) and with a few select yogis of the Himalayas. It demanded physical endurance of the highest degree and several hours of meditation in a single sitting.
Mahavatar Babaji was initiated into Kriya Yoga by Parama Guru Sri Sri Sri Bhoga Siddhar. He had undertaken the mission of spreading Kriya Yoga, to the door steps of suffering humanity and mankind. He has initiated and taught Kriya Yoga practice to several devotees and seekers and is the icon of Kriya Yoga tradition. At the behest of Parama Guru Sri Sri Sri Bhoga Siddhar (spiritual master) of Mahavatar Babaji, Babaji further simplified Kriya Yoga, according to the needs of the times and made it accessible in general to common folk, the householder and city dweller, who were unable to renounce their families / worldly duties and go to secluded places like the Himalayas but also benefit from the age old Kriya Yoga technique. The earliest known luminaries who were initiated in to Kriya Yoga are Sri Adi Shankaracharya, Kabir Das, Shirdi Sai Baba and Lahari Mahasaya.
It is since the 19th century onwards that a few thousand people around the globe were blessed with Kriya Yoga, chiefly through Babaji's disciple Sri Lahari Mahasaya and his subsequent disciples. Even this method of Kriya Yoga turned out to be difficult to practice / cumbersome by the current generation of people, as one single session required almost three hours which included asanas, pranayama techniques and meditation.
This is when, Parama Guru Sri Sri Sri Bhoga Siddhar who had lived for 12,000(Twelve thousand) years, had chosen Pujyasri Aathmanandamayi Maathaji to impart the knowledge of the essence of Kriya Yoga and through Her spread the knowledge of Kriya Yoga among the seeking and deserving lot of mankind irrespective of class, cultures, creeds and faiths across the globe. The Masters blessed Her with a new technique called SUSHUMNA KRIYA YOGA, in a divine intervention of Maathaji's meditative spell, on the auspicious day of Vinayaka Chavithi (Chathurthi) in the Brahma Muhurtha time (early hours) of 7th September 2005.


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text:
Home latest State Domicile Law Shows Its Saffron Colours: Monga
Domicile Law Shows Its Saffron Colours: Monga
Terming the Central Government's order defining domicile law for Jammu and Kashmir against the interests of people of the erstwhile state, J&K Pradesh Congress Committee (JKPCC) Vice President and former MLC G N Monga today said when the entire world has been engulfed by coronavirus pandemic, the BJP government rubbed further salt into the wounds of people of J&K.
In a statement, he said it shows the true colours of the BJP. "The order has been deliberately issued at a time when the entire world, the country as well as Jammu and Kashmir is facing a dreadful threat due to the outbreak of the deadly coronavirus resulting in a complete lockdown."
"Instead of focusing on fighting against the deadly disease, the BJP government at the Center issued domicile law to further humiliate and subjugate people of J&K. The order is against the wishes and interests of people of J&K, especially its youth. The order contains no word related the protection of land and jobs and has been issued just for the sake of issuance," Monga said.
Asking the government of India to immediately roll back the order, the Congress leader said, "The priority of the government should be to contain the spread of COVID-19 in the country as well as in Jammu and Kashmir."

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text:
New Zealand crime
Drunk motorist who killed taxi driver jailed
1:01 pm on 2 July 2019
Anneke Smith, Court Reporter
@aneksmith anneke.smith@rnz.co.nz
A drunk motorist who ran a red light, killing a taxi driver in Auckland's CBD, has been jailed for three years and eight months.
The scene of the crash on Symonds Street. Photo: www.snpa.co.nz
Farshad Bahadori Esfehani was behind the wheel of a Mercedes when he ran a red light on Symonds Street in the early hours of 23 December, 2017.
The 22-year-old smashed into the side of the Toyota Prius Abdul Raheem Fahad Syed was driving; killing the young father who had only recently moved to New Zealand for a better life.
Esfehani appeared before Justice Woolford in the High Court at Auckland for sentencing this morning after pleading guilty to excess breath alcohol causing death, dangerous driving causing death and failing to stop and ascertain injury.
Crown prosecutor Emma Smith told the court Mr Sayed was a hardworking man who was devoted to his son, who was just 5-months-old at the time of his death.
Now a toddler, Mr Syed's son sat on his wife's lap in the front row of the public gallery during this morning's sentencing hearing.
Auckland taxi driver Abdul Raheem Fahad Syed, who leaves behind a wife and baby. Photo: Supplied
The court heard Esfehani sped through three red lights at about 4.30am between Waterloo Quadrant and the crash scene at the intersection of Alex Evans St and Symonds St.
He had just fled the Chancery Basement Carpark in the CBD after an altercation with security staff, who had called police.
The court heard he travelled at an average speed of 87km/h and hit Mr Sayed's car at 61km/h and 74km/h; shunting the Toyota Prius 10 metres sideways.
Esfehani did not make any attempts to call emergency services and Mr Syed died from severe blunt force trauma to his chest.
Justice Woolford said the defendant got out of his car after the crash and told members of the public 'Don't call the cops', 'Can you call me a taxi?'and 'I hope that guy has insurance'.
Esfehani had a breath alcohol reading of 908 micrograms of alcohol per litre of breath, more than three times the legal limit of 250 micrograms.
Farshad Bahadori Esfehani in court for sentencing. Photo: RNZ / Anneke Smith
Ms Smith said there were a number of aggravating factors in the case and submitted a sentence of 5.5 years' imprisonment was appropriate.
Esfehani's defence lawyer Mark Ryan asked for a lesser sentence of 12 months' home detention and 200 hours of community work.
He told the court his client was 20-years-old at the time of the crash and submitted Esfehani's youth, lack of driving experience and the "volume of literature" that showed young male brains did not fully develop until 27-years-old went some way towards explaining his actions that night.
Mr Ryan said the now 22-year-old's genuine remorse was illustrated in a restorative justice conference held with Mr Syed's familly.
"He's going to carry this mistake with him like a millstone around his neck for the rest of his life. Nothing he does is going to bring back the victim."
A family support person read a victim impact statement written by Mr Syed's father, who visits his son's grave in India every day after prayers.
"It is very painful for me and my family. It's a sad demise of my beloved son who was a 29-year-old loving husband and caring father of a five month old at the time of his death.
"I go to my son's grave every single day after praying the mass. It's very painful and I ask Allah to give my son back if possible. After that I cry a lot as I miss my son."
He said Esfehani's failure to help Mr Syed had added to the family's grief and he had not forgiven the defendant for his "grave mistake".
"It was his moral duty to stay beside my son until emergency services arrived or, if possible, provide first aid but he preferred to escape from the scene."
Justice Woolford sentenced Esfehani to three years and eight months' imprisonment, disqualified him from holding or obtaining a driver's license for four years and ordered he pay $12,000 to Mr Syed's family.
Esfehani, who was supported by friends and family in court, shielded his face from cameras in court and bowed his head during most of the sentencing hearing.
Southern DHB staff shortages: Patients 'feeling really angry and frustrated'
Thunderstorm, wind warnings in place around New Zealand


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After a brief stint as a Daily Show correspondent, former Saturday Night Live writer Michael Che is returning to the NBC late-night show as co-host of "Weekend Update". Che, the first black host of "Weekend Update", will join Colin Jost. Cecily Strong, who served as co-anchor for two seasons, first with Seth Meyers and then with Jost, will return to being a full-time cast member. Unlike other "Weekend Update" hosts, she had been juggling both roles, doing the fake newscast and appearing in the majority of skits every week. I hear she felt that she wanted to focus on performing.
Fast-rising New York comedian Che joined The Daily Show as a new correspondent in June, after wrapping SNL, which he joined as a full-time writer last September after a guest-writing stint the previous season. The 40th season of SNL begins September 27 with host Chris Pratt and musical guest Ariana Grande.


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Home Page > Tours and Experiences > Traveller Stories > New Zealand's Hottest Spots
New Zealand's Hottest Spots
Centered on the North Island, the Thermal Explorer Highway is a 457 kilometre route anchored in Auckland and stretches throughout the land to Napier, giving visitors a taste of life on the edge of the Pacific Ring of Fire. Just be sure not to get burned.
You don't have to stray far from the city to get a feel for New Zealand's geothermal activities: the ground beneath Auckland's feet is home to over 40 volcanic cones and explosion craters. The hills and craters were important places for pa-fortified Māori villages, with many of the craters used as large earthen forts.
The biggest volcanic force in the area is Rangitoto, a young and restless volcano at 600 years old. Despite jutting defiantly from the harbour, today it's more of a picturesque hiking and picnic spot.
The upside of Auckland's volcanic pedigree is that you can experience an active volcanic field in a budget-friendly way. One of those ways? Take a walk up Auckland's highest volcano, the evergreen Mt Eden, for some of the best panoramic views over Auckland and Waitemata Harbour.
Take a side trip from the Thermal Explorer Highway for the worthwhile and mysterious White Island lurking in the Bay of Plenty about 50 kilometres offshore. The smoking volcanic crater and ethereal lunar landscape makes White Island the ultimate villain's lair – although visit when the weather is favourable and you'll find daytrippers taking a walk on the wild side.
Considered one of the world's most accessible marine volcanoes, the bulk of the volcanic mountain rests below the surface with easy access for visitors. However, it's also uneasy ground. There was a volcanic temper tantrum a century ago – and if that's not intimidating enough, the intoxicating white smoke that bellows from the crater fumes at around 800 degrees.
Daytrippers come by both boat and helicopter from Whakatāne and you can plan your trip online.
In many ways, Rotorua is the Kiwi version of Las Vegas: big, bubbling and built for tourists. However, its steamy tourist appeal has firm roots in geothermal wonder and stunning beauty.
Pack the camera to capture the sinter terraces and spouting geysers throughout the area, including Pohutu, the southern hemisphere's largest active geyser which blasts up to 30 metres high around twenty times per day (proving patience is a virtue). Take a stroll along the bubbling mud pools on the Craters of the Moon geothermal walk, or visit the largest hot-water waterfall in the Southern Hemisphere at Tikitere, also known as Hell's Gate, a sacred Māori site with over 20 hectares of hot pools, steaming lakes, cooking pools, bush walks and a mud volcano.
And if you're keen to test the medicinal properties of a mud bath, this is the place to indulge your inner spa prince or princess, with high-end mud spas and a sulphur spa.
LAKE TAUPŌ
On the surface, Lake Taupō looks at peace with its surroundings. But beneath the surface of New Zealand's largest lake lies the caldera of a dormant super volcano that caused epic destruction.
Today, Lake Taupō is the centre of an incredible network of geothermal parks and caves popular with families and locals. One of the highlights is Orakei Korako Geothermal Park and Cave, accessible by ferry and home to 23 active natural geysers, boiling hot springs, sinter terraces as well as the Ruatapu Cave.
Also known as the Sacred Hole, the cave descends 35 metres into a hot pool known as the Pool of Mirrors, the only geothermal cave known to exist in New Zealand, and one of two caves known in the world. You can't get too close! Stop by the cave entrance and take a peek from the viewing platform.
Long before Frodo and his friends made New Zealand famous, Tongariro National Park's claim to fame was as New Zealand's first National Park, achieving World Heritage Status in 1993.
Consisting of three huge volcanoes: Ruapehu, Ngauruhoe and Tongariro, the park has been a favourite with hikers and landscape lovers for a century.
However, Ruapehu's starring role as Mount Doom in the Lord of the Rings film trilogy saw the park's popularity boom. Ruapehu clocks in the biggest and most restless volcano, although Tongariro was the last to erupt in August 2012.
The constant volcanic activity in the park draws visitors in their thousands with the Tongariro crossing considered one of the best day-walks in New Zealand, the most popular trek with its fuming vents, thermal lakes and crater hikes (not to mention convenient pick-up/drop-off shuttle service from nearby National Park, Ohakune and Taupo).
While the Thermal Explorer highway ends on the coast in Syrah-inclined Napier, New Zealand's hottest spots continue on the South Island. The South's hottest? The alpine village of Hanmer Springs is known for its thermal pools warmed by the earth's toasty core. The rainwater-to-hot-springs process takes 173 years, much to the delight of hot water relishers who flock to the alkaline waters rich in minerals in search for the ultimate in unwinding.
Treasures lost forever: the Pink and White Terraces
Tourists first flocked to Rotorua in the 1800s to visit New Zealand's "eighth natural wonder of the world", the Pink and White Terraces. A natural wonder, the geothermal creation was captured first by landscape painters and later, the first photographers.
Located just a few hundred metres apart, the Pink Terraces were known as Otukapuarangi, the fountain of the clouded sky, while the white terrace were called Te Tarata, the tattooed rock. Their popularity even extended to a visit by Prince Alfred, the Duke of Edinburgh who visited the area in 1870.
However, in 1886 Mount Tarawera erupted in the early morning and consumed the Pink and White Terraces in volcanic ash and sediment. The eighth wonder of the natural world was lost - until 2011 when researchers announced they had found sections of the terraces lying at the bottom of Lake Tarawera.
Sceptics have challenged the discovery but romantics can imagine what might have been on a visit to the buried village of Te Wairoa near Rotorua.
Similar to Pompeii, the 19th-century Māori villages were engulfed by ash during the same eruption and today have been excavated and opened to the public near the site of the original terraces.
FREE & FEELING HOT HOT HOT
While some of New Zealand's geothermal spas burn your wallet as much as your bottom, there are a handful of natural hot springs that are completely free.
Head to Hot Water Beach on the Coromandel Peninsula at low tide, where two underground fissures – and a handy shop renting spades – allow you to dig your own warm spa in the sand (check the tides first).
Fancy a little waterfall with your hot spring? Half an hour south of Rotorua is Kerosene Creek, where hot water pulsing up underground mixes with the cold water from the creek.
There's a similar experience just outside of Taupo at Otumuheke Stream in SpaPark, where geothermal activity warms the Waikato River.
For those who don't feel like scrambling over rocks, at Mangatutu Hot Springs in Kaweka Forest Park the thermal waters are channeled into two neatly constructed pools for picnickers. If the trails aren't in flood, then a cold water plunge in the Mohaka River is also a must.
And just to make sure the South Island isn't feeling left out, visitors can soak their bones at the Welcome Flat Hot Springs on the overnight Copland Track, the perfect reward for a decent day's tramp into the wilderness. Or at the edge of a river in the Lewis Pass at Sylvia Flats.
YHA Auckland International
auckland@yha.co.nz
YHA Auckland City
aucklandcity@yha.co.nz
rotorua@yha.co.nz
taupo@yha.co.nz
YHA Ohakune
ohakune@yha.co.nz
YHA National Park
nationalpark@yha.co.nz
YHA Hanmer Springs
hanmersprings@yha.co.nz
This story first appeared in the February 2016 issue of Backpacker Essentials. Read the latest edition now!


Lebih-lebih lagi, this app enables you to track not only cell phones, in fact, but it also helps you in tracking text messages, e-mel, and messages from the application. Although every app has functions of their own, each one of them comes with a function different from the other. Such as listening to the actual conversations through the remote access dashboard.
iSpyoo spy app is installed by accessing the device directly. Malangnya, this feature is not available on every phone. Phones like iPhones (need a jailbreaker), Android Phone (need a root or not) kepada install a mobile spy application. Regardless of the jailbreaker, the application requires your email address or iCloud details.
In such circumstances, every woman needs a spying app at the device, so you are aware of your children's conversations with other people, and of course, your husband's as well. iSpyoo spy app will connect you to your people indirectly. Ini mobile spy application is one of the best apps on an Android device or iOS device specifically formulated to spy on people. It comes with a tremendous number of beneficial ciri-ciri and once the spy app has been downloaded in the targeted person's phone, you will be free of all sorts of stresses.
If your teenage daughter is trying to hide her conversations with a guy in her class, you can easily find out about it and even prevent an unforeseen mishap from happening. It helps in getting all the details. From mesej teks kepada video calls, kepada e-mel whether you are online or offline. All you have to do is register yourself and you can get all the required information.
Any application with appropriate pricing will work well. Applications such as another phone spy app come under the reliable mobile spy app categories and it is also user-friendly. Aplikasi ini does not require any sort of rocket science to work it. Most of the applications come with a monthly and annual subscription offer. The method of payment depends upon your feasibility. You are logged into the application after the subscription and download instructions are shown. Once the application has been installed you will be briefed with all the details. Make sure you are connected to the internet throughout the process though. Most applications also have a customer care service in case you go through any problems during the installation and setup.
Spy a phone free has the ability to monitor internet activities. The internet can be sued for several things, but with the help of a spy app, awak boleh monitor every user's activity on the internet and phone. You can keep a track of all the shows and channels your children watch over the internet, enabling parental control accordingly. Keeping track of what they do when you are not around is very easy through this application.
Awak boleh get details of all the calls, dan know whether they are incoming or they are outgoing calls.
Ini mobile app helps you to spy on all the activities that have been done through Whatsapp as well. The complete messages will be available that have been sent or received through Whatsapp.
Sebenarnya, make sure that the phone is not used for any personal uses except that. Several employees think that it is okay to use their phones for work other than their job, which is not the right thing to do. The reason why most are given a phone is, so they keep their work and personal life separate, and obviously, their phone is never busy when their boss needs to contact them for any work purposes.
Lebih-lebih lagi, the entrepreneurs are not the only ones who can see the benefits of a cell phone spy application. Stay at home moms, spouses, and families keep track of each other through this application. It helps them know about their family's whereabouts, and it also enables you to track a lost or stolen phone. God forbid if that happens, you can wipe it clean.
Nobody knows about what the future has in store for them. It can either be good or bad, we cannot be sure about it. Walau bagaimanapun, if you ever come across some mishap, do you think you will ever be able to tackle the problem or overcome it? The truth needs to be admitted, you cannot always be around the people you love and protect them. It is not possible to go wherever they are. But if you download the iSpyoo spy apps on your phone, you can be with them at all times virtually and watch their backs.


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FRISKY Family: Spread the Love
Let's show support: Peace, Love, Cure
One of the most special parts of the underground music community is the energy that we all share from around the world. Together we experience the heights and depths in music that are ultimately reflected through our lives, and together we unite to spread the love that underlies it all. Today we'd like to ask you to help not only one of your friends in the underground electronic music community, but a member of the FRISKY Family. Miss Disk has been sharing her deep tech vibes with us for over 7 years, giving us a part of herself through the music. Paradigm is always a unique and distinctive experience, but there is an extra power in her May episode: dedicated to her boyfriend Helly Larson (whose beautiful tracks open and close the set) who has been diagnosed with terminal brain cancer. Miss Disk shares her love and inspires us to help them spend more time together.
By donating to his cause you can make a difference.
Please share your words, energy, and love to them too.
Thank you FRISKY Family.
FRISKY Family: Spread the Love was last modified: May 9th, 2017 by Lauren Krieger
Are You Really Listening?
Our Underground Electronic Music Community: A Reflection
Home is Where The Vinyl Is
Can You Survive on Music?
Blade Runner & Electronic Music: A Timeless Connection


Searching for Hot air balloon trips in Burbank? You have found to the end of your search! Finding a pilot to provide Hot air balloon trips is easy. Additionally, you can visit our Balloon Ride Directory, or look in the local yellow pages.
Enjoying Hot air balloon trips is something anyone can participate in, but it is also a popular way to celebrate a birthday! When you speak with the company you are considering booking with, be sure to ask how many other passengers will be aboard the balloon.


Alan Levine Letter to the Editor – NY Times – published May 8 | Jews Say No: Not In Our Name!
Pamela Geller is an Islamophobe whose public remarks about Muslims have rightly been condemned by the Southern Poverty Law Center as hate speech. But she has the last word in your article ("Organizer of Cartoon Contest Trumpets the Results," news article, May 5), wrapping herself in the mantle of the First Amendment as if she had made a useful contribution to a public dialogue about Islam.
She has not. While hate speech is protected by the Constitution, the sole purpose of such speech is to inflame bigotry and to inflict injury. Your reference to the case of Debbie Almontaser is a case in point.
Ms. Almontaser, a respected educator and community leader, was selected by the New York City Department of Education to head the Khalil Gibran International Academy, the city's first Arabic dual-language school. In the months after the announcement of the school's creation, Ms. Geller and her allies unleashed a hate-filled barrage of false and Islamophobic accusations about Ms. Almontaser and the school.
Capitulating to the campaign, city officials forced her to resign. She then filed a complaint with the Equal Employment Opportunity Commission.
Ms. Almontaser's reputation and career survived Ms. Geller's onslaught. However, her ordeal should be a reminder that those who propagate hate speech are not proponents of First Amendment rights, but destroyers of lives.
The writer is a civil rights lawyer who represented Ms. Almontaser in her suit against the Department of Education.
This entry was posted on May 8, 2015 at 10:34 pm and is filed under articles.	You can follow any responses to this entry through the RSS 2.0 feed. Both comments and pings are currently closed.


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Home News COVID-19 hospitalizations on the rise in Canada
COVID-19 hospitalizations on the rise in Canada
Local News — COVID-19 hospitalizations on the rise in Canada that we obtained from news agencies. opinions and stunning details about the COVID-19 hospitalizations on the rise in Canada that you have never heard before.
Toronto, Ontario (CTV Network) — More than two-and-a-half years into the pandemic and hospitals across the country continue to grapple with the effects of COVID-19.
Among the hardest hit provinces, Quebec reported over 2,000 COVID-19 hospitalizations for the first-time since August as the province's minister of health urged residents to get their boosters for added protection.
Infectious disease experts have previously reported an uptick in COVID-19 cases was likely to happen in the fall as the influenza season approaches. However, a myriad of factors like emerging variants, other viruses and health concerns have put a strain on hospitals.


There are certain reasons why certain videos go viral. Mainly they do because they are either amazing and mindblowing, or they touch a cord in our humanity. This one does both.
The city of Grand Rapids, Michigan was listed as a dying city by Newsweek magazine. This music video was the city's response. It's quite impressive especially since it was done in one take. My hat is off to Status Creative, the creative videographers who produced this video.


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Our City » City News
Cleanup from February 14 Mudslide Likely to Begin in Late July, Significant Impacts Expected
Post Date:05/31/2019 3:45 PM
Clean up of debris from the February 14 mudslide in Sausalito's Hurricane Gulch neighborhood is expected to begin in late July 2019, according to an update presented to the City Council on May 28. The update was provided by David Bracken, the City's interim director of public works, and Eric Vaughan and Michael McCormick of Harris & Associates, an engineering and disaster recovery firm that is advising the City.
During the week of June 3, the City will post a notice inviting bids on a project to remove debris from the mudslide site. Respondents to the bid notice will have 30 days to submit a bid. The City Council then expects to award a contract to the lowest qualified bidder at its meeting on July 16. Debris removal should begin soon after the contract is signed.
Total costs to the City associated with the initial cleanup are expected to exceed $1 million. If the City complies with all regulations related to the cleanup, up to 93.75% of those costs could be covered by state and federal sources like the Federal Emergency Management Agency (FEMA) and the State of California Office of Emergency Services (Cal OES). Funds will be disbursed only after all cleanup work is completed and the City has been fully audited by funding sources.
Mudslide cleanup is likely to have significant impacts on the residents of Hurricane Gulch, including noise from machinery and traffic delays caused by trucks hauling debris. Among the decisions to be made by the City Council in July will be the allowed hours for cleanup. Work could proceed more quickly if the Council authorizes the operation of construction equipment outside of the hours allowed by the Sausalito Municipal Code (Monday to Friday from 8:00 a.m. to 6:00 p.m. and Saturday from 9:00 a.m. to 5:00 p.m.), e.g. Monday to Saturday from 7:00 a.m. to 7:00 p.m. The interim director of public works estimates that the cleanup will take a minimum of 30 days.
Further updates about mudslide cleanup will appear on the February 14 mudslide page on the City website and in forthcoming editions of Sausalito Currents. When available, information will also be published about support from Harris & Associates for individuals affected by the mudslide who are seeking state and federal disaster assistance.
Any questions about debris removal at the mudslide site may be directed to Interim Director of Public Works David Bracken at (415) 289-4176 or dbracken@sausalito.gov.
LEARN MORE ABOUT THE FEBRUARY 14 MUDSLIDE
WATCH THE PRESENTATION TO THE CITY COUNCIL ON MAY 28