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arxivcap_2012.05350_7 | Title: Automatic Diagnosis of Malaria from Thin Blood Smear Images using Deep Convolutional Neural Network with Multi-Resolution Feature Fusion | Caption: Variations of relative improvements in DeepFusionNet with respect to the individual networks operating with different resolutions: All the metrics provide improvement in the fusion scheme from the individual networks. Kappa score provides the largest variance in relative improvements for the steepest rise. | 2012.05350_7.jpg |
arxivcap_2108.09610_2 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Redshift distributions for each cluster. The black dotted line marks the central redshift of the cluster, while the dotted grey lines indicate three times the velocity dispersion on each side. The fitted gaussian for the objects between the grey dotted lines is also shown in red colour. Note that the redshift distribution for clusters RXJ0123.2+3327 and RXJ0123.6+3315 are mixed (bottom panel) as they are in the same field of view. | 2108.09610_2.jpg |
arxivcap_2206.01867_4 | Title: SPGNet: Spatial Projection Guided 3D Human Pose Estimation in Low Dimensional Space | Caption: Clustered column charts (a) and (b) illustrate the comparisons of different sittings and input frames, respectively. The error shows a decreasing trend as the model is applied from the Baseline to our SPGNet or the size of input frames increases. Notably, in Figure <ref>, Baseline is the model only learned from MPJPE loss, and Baseline* represents the Baseline adding kinematic constraints. In the chart <ref>, \(J\) represents the number of frames in the input sequence. | 2206.01867_4.jpg |
arxivcap_astro-ph_0104286_2 | Title: THE NEARBY FIELD GALAXY SURVEY | Caption: Example of the geometry of the periodic drift scan to obtain integrated spectra. The total distance over which the slit is moved back and forth is half the blue minor-axis optical diameter. This distance was chosen to match the expected surface brightness limit of the 1.5 m Telescope and FAST spectrograph. The spectra were extracted into 1D spectra using an objectively defined aperture of size 0.7 times the major-axis diameter at $\mu_B=26$ mag arcsec$^{-1}$, as determined from our $B$-filter photometry. The ellipse drawn in the image was fitted to the $B_{26}$ isophote. In the case of galaxy A10368+4811, we sample $\sim$80% of the light within this isophote, or 68% of the total galaxian light. | astro-ph_0104286_2.jpg |
arxivcap_2305.05260_4 | Title: Guided Focal Stack Refinement Network for Light Field Salient Object Detection | Caption: Overview of GFRNet. The overall architecture is shown in the upper left. "CP" is the compression module, "CA" denotes the channel attention module, "CF" denotes the cross-fusion operation, and "AWM" indicates the alignment weighting module. Details of these modules/operations are described in Sec. <ref>. | 2305.05260_4.jpg |
arxivcap_2202.01537_8 | Title: Bending Graphs: Hierarchical Shape Matching using Gated Optimal Transport | Caption: To show the effectiveness of our GFP module, we visualize correspondences before and after the GFP. Here a model is trained on SURREAL <cit.> and during evaluation on FAUST <cit.>, we visualize the results from the first and final Sinkhorn. a) Correspondence map of target shape. b) Predicted correspondences from the first Sinkhorn (before GFP). c) Predicted correspondences from the final Sinkhorn (after the GFP). | 2202.01537_8.jpg |
arxivcap_1503.07328_3 | Title: Spectral weight redistribution in (LaNiO3)n/(LaMnO3)2 superlattices from optical spectroscopy | Caption: Temperature dependence of the spectral weight $W(T)$ integrated up to $\omega_p$, for the $n$=3,4,5 and LNO compounds. For $n$=3 and $n$=4, $W(T)$ increases with increasing temperature, thus signaling the presence of incoherent excitations at low energies. For both $n$=5 and LNO the spectral weight can be fitted (continuous line) according to the quadratic relation $W(T)=W_0-BT^2$. | 1503.07328_3.jpg |
arxivcap_2206.12127_1 | Title: Implicit Channel Learning for Machine Learning Applications in 6G Wireless Networks | Caption: Impact of channel estimation (CE) for image (IC) and speech classification (SC) performance on the validation datasets. The details for the datasets and the learning models are given in Table <ref>. | 2206.12127_1.jpg |
arxivcap_2202.00263_2 | Title: Fully Online Meta-Learning Without Task Boundaries | Caption: Overview of learning: updates the online parameters $\phi$ using only the most recent $K$ datapoints from the buffer $\mathcal{B}$. Meta-learning learns a regularizer, parameterized by meta-parameters $\theta$, via second-order MAML-style updates. The goal of meta-learning is to make $\phi$ perform well on randomly sampled prior datapoints after performing $K$ steps with the meta-trained regularizer. | 2202.00263_2.jpg |
arxivcap_1902.03928_3 | Title: The Degree of Fine-Tuning in our Universe -- and Others | Caption: Length and mass scales of the universe, given in units of the proton mass and size (adapted from <cit.>). The left end point of the blue line corresponds to the mass and radius of the proton (marked by the triangle at the origin), and its right end point corresponds to a Planck mass black hole (lower triangle). The red line extends from the location of the Planck black hole to the size/mass of the entire observable universe (upper right triangle). Below the red line, objects are smaller than their Schwarzschild radii and are black holes. Below the blue line, objects are smaller than their Compton wavelength and lie in the quantum regime. The three dashed lines show contours of constant density, for nuclear density (lower), atomic density (middle), and cosmic density (upper). The left end point of the middle dashed line corresponds to the Hydrogen atom. The range of life forms is depicted as the heavy green line segment. The range of known black holes is depicted as the heavy black line segment. The circles show the locations of stars, with masses $M_\ast$ = 0.1, 1, 10, and 100 $M_\odot$ (left to right). The squares show the locations of planets, analogs of Earth, Neptune, and Jupiter (left to right). Galaxies lie in the shaded region in the upper right portion of the diagram. | 1902.03928_3.jpg |
arxivcap_2004.03425_12 | Title: Elemental abundances in M31: [Fe/H] and [{\alpha}/Fe] in M31 Dwarf Galaxies Using Coadded Spectra | Caption: The same as Figure <ref>, but for our sample of dSphs with deep observations. | 2004.03425_12.jpg |
arxivcap_1211.6964_5 | Title: On the Bauschinger effect in supercoooled melts under shear: results from mode coupling theory and molecular dynamics simulations | Caption: Bauschinger effect as illustrated by a generalized Maxwell model (see text). Solid lines are $\sigma(t)$ as a function of normalized time, $|\dot\gamma|t$, for the case $\gamma_w=0.1$ corresponding to $\gamma_w^\text{max}$ and $\gamma_w=0.8$ corresponding to $\gamma_w^\text{s}$. Dashed lines display the contributions $\sigma_\text{I}(t)$ (upper, red) and $\sigma_\text{II}(t)$ (lower, blue). | 1211.6964_5.jpg |
arxivcap_2108.09610_3 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: $M_{500}$ mass from <cit.> as a function of the $M_{200}$ mass we estimated from the velocity dispersion for each cluster. The filled and open grey points correspond to the clusters analysed in <cit.>, the open symbols corresponding to the four clusters that we have in common. The blue points correspond to the clusters analysed in this work. | 2108.09610_3.jpg |
arxivcap_2303.14662_9 | Title: OTAvatar: One-shot Talking Face Avatar with Controllable Tri-plane Rendering | Caption: 3D Consistency on monocular dataset. We demonstrate additional visualization comparison on the HDTF dataset <cit.>, with more drastic camera view variation. All methods use the source frame to extract the identity feature, then use the coefficients of pose and expression as visualized by the face meshes to generate talking faces. This subject is not included in the training set of any methods. | 2303.14662_9.jpg |
arxivcap_1806.08643_2 | Title: Diffusiophoretically induced interactions between chemically active and inert particles | Caption: Bispherical ($\theta$, $\eta$, $\phi$) and Cartesian ($x$, $y$, $z$) coordinates for two spheres. The catalytic sphere $S_1$ (red) with radius $R_1$ and noncatalytic sphere $S_2$ (blue) with radius $R_2$, separated by a distance $L$, can be specified by variables $\eta=\eta_1$ and $\eta=\eta_2$, respectively. The system is axisymmetric in the angle $\phi$ about the $z$ axis that lies along the line connecting the centers of the two spheres. The hat notation is used to indicate unit vectors. | 1806.08643_2.jpg |
arxivcap_2212.13102_12 | Title: Piezoelectric effect and diode effect in anapole and monopole superconductors | Caption: Results of the mixed model: $\alpha$ dependence of (a) $q_0$, (b) $d^{\textrm{(SC)}}_{xxx}$ in the $A_g + i B_{3u}$ anapole state, and (c) $d^{\textrm{(SC)}}_{yzx}$ in the $A_g + i A_{u}$ monopole state. We set $\alpha = \alpha_x = -\alpha_y$, $\beta = 1$ or $0.7$, and $T = 0.01$. | 2212.13102_12.jpg |
arxivcap_1709.03144_31 | Title: The 12C(a,g)16O reaction and its implications for stellar helium burning | Caption: (Color online) Comparison of the $R$-matrix fit to the angular distribution data of {Dyer1974495} (green diamonds), <cit.> (brown stars), <cit.> (black circles), and <cit.> (blue squares). Note that the data at $E_\alpha$ = 2.28 and 3.677 MeV have been scaled for plotting convenience. The data from {Fey2004} show a systematic deviation from the $R$-matrix fit and other data sets at backward angles. This is most clearly visible at $E_\alpha$ = 1.740 MeV where the data from {PhysRevC.73.055801, Fey2004} were measured at the same energy. | 1709.03144_31.jpg |
arxivcap_1912.05125_11 | Title: Bayesian Framework for Simultaneous Registration and Estimation of Noisy, Sparse and Fragmented Functional Data | Caption: Posterior means of the amplitude (top) and phase (bottom) components based on the proposed model with the shape restricted amplitude prior with (a) $H = 2$ and (b) $H = 4$. (c) Estimated amplitude (top) and phase (bottom) functions using WPACE. | 1912.05125_11.jpg |
arxivcap_2206.01867_7 | Title: SPGNet: Spatial Projection Guided 3D Human Pose Estimation in Low Dimensional Space | Caption: General workflow of our SPGNet, take 2D key points as input, and estimate the 3D pose with its global position. The 2D re-projection combines both estimations and loss to optimize the model. | 2206.01867_7.jpg |
arxivcap_2108.09610_4 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Top panel: colour-magnitude diagram for the galaxies of all the clusters grey symbols. The black dotted line highlights the colour $g-r$ $\leq$ 1.0 mag used to discard background galaxies. Bottom panel: Mean surface brightness of the galaxies that have passed the first colour cut as a function of their absolute magnitude (grey symbols). For a fixed absolute magnitude, we considered cluster members to be those galaxies below the black dotted line. See text for more details. In both panels, green and red points represent spectroscopically confirmed cluster members and background galaxies, respectively. | 2108.09610_4.jpg |
arxivcap_2303.06733_3 | Title: Probing the Origin of Changing-look Quasar Transitions with Chandra | Caption: Edge-on view of the fundamental plane of black hole activity. The sources in black are from <cit.>, including QSOs (stars), Seyferts (circles), low-luminosity AGN in LINERs (triangles), XRBs (diamonds), and Sgr A$^*$ and M32 (squares). The colored dots are the four CLQs observed by VLA in the faint state, with filled circles denoting sources with unresolved radio emission, and filled diamonds denoting extended radio emission. | 2303.06733_3.jpg |
arxivcap_1111.0053_5 | Title: Exploiting Subgraph Structure in Multi-Robot Path Planning | Caption: A simple planning problem that can be solved with naive prioritised planning but not with the subgraph abstraction. The goal is to swap the positions of robots $a$ and $b$. With priority ordering $a,b$ the subgraph planner will choose for robot $a$ to remain inside the hall. Robot $b$ is then trapped, because $a$ blocks the only exit to $y$ (note that the edges $(x_1, y)$ and $(y, x_4)$ are directed). | 1111.0053_5.jpg |
arxivcap_1906.05303_3 | Title: Calculations for deep inelastic scattering using fast interpolation grid techniques at NNLO in QCD and the extraction of $\alpha_s$ from HERA data | Caption: Results for (lower panel) and corresponding values for (upper panel) from fits to inclusive jet data points arranged in groups of similar . The upper panel is obtained by applying the expectation from the QCD renormalisation group equation, as it also enters the NNLO predictions. The inner error bars indicate experimental uncertainties, and the full error bars the total uncertainty. The upper triangles show results from H1 data, which were previously fit in Ref. <cit.> and are here partially updated with NNLO predictions with higher statistical accuracy. The lower triangles indicate the new results from ZEUS data. The full circles show the combined results from H1 and ZEUS data taken together and are labeled HERA inclusive jets. The shaded band indicates the world average value with its uncertainty, and the dashed line and hatched band indicate the result obtained from the fit to all inclusive jet data and its uncertainty. | 1906.05303_3.jpg |
arxivcap_2010.12170_1 | Title: Is PSR J0855$-$4644 responsible for the 1.4 TeV electron spectral bump hinted by DAMPE? | Caption: SED of inner compact part of the PWN G267.0$-$01.0. The Chandra data are taken from <cit.>, and the HESS data are taken from <cit.>. The HESS data are used as an upper limit in view of possible pollution from the overlapping SNR Vela Junior. | 2010.12170_1.jpg |
arxivcap_2212.13102_14 | Title: Piezoelectric effect and diode effect in anapole and monopole superconductors | Caption: Results of the mixed model: temperature dependence of (a) $q_0$, (b) $d^{\textrm{(SC)}}_{xxx}$ in the $A_g + i B_{3u}$ anapole state, and (c) $d^{\textrm{(SC)}}_{yzx}$ in the $A_g + i A_{u}$ monopole state. We set $\alpha = \alpha_x = - \alpha_y = 0.4$ and $\beta = 1$ or $0.7$. | 2212.13102_14.jpg |
arxivcap_1111.4939_13 | Title: Josephson and Andreev transport through quantum dots | Caption: Phase diagram of the S-QD-S system in the $\Gamma_R,\epsilon_0$ plane for fixed $U$ and different values of $\Gamma_L/\Gamma_R$ obtained using the NRG method. Reprinted figure with permission from Y. Tanaka {et al.}, New Journal of Physics 9, 115, 2007 <cit.>. Copyright (2007) by IOP Publishing Ltd. | 1111.4939_13.jpg |
arxivcap_2202.00263_3 | Title: Fully Online Meta-Learning Without Task Boundaries | Caption: {Ablation experiments: a) We vary the number of online updates $K$ used before the meta-update, to see how it affects the performance of our method. The performance of FOML improves as the number of online updates is increased. b) This experiment shows how FOML performs with and without meta updates, to confirm that the meta-training is indeed an essential component of our method. With meta-updates, FOML learns more quickly, and performance improves with more tasks.} | 2202.00263_3.jpg |
arxivcap_1109.6664_7 | Title: Conditional pair distributions in many-body systems: Exact results for Poisson ensembles | Caption: (Color online) Contributions due to (ii$b$), (iii) and (iv) pair configurations (solid, short dashed and long dashed lines, respectively) to the CPDF $g_v(\omega)$ as a function of $v$, for one dimensional Poisson ensembles and different distances as measured by $\omega$ (values $n\omega$ indicated on the plots). The total CPDF is shown by the dotted line. | 1109.6664_7.jpg |
arxivcap_1503.07328_4 | Title: Spectral weight redistribution in (LaNiO3)n/(LaMnO3)2 superlattices from optical spectroscopy | Caption: Comparison between the room temperature $\sigma_{1,n}$, and $\sigma^*_{1,n}$ (see text) for $n$=2,3,4,5. The blue (red) area corresponds to spectral weight lost (gained) by the SL in the far- (mid-) infrared range due to the presence of interfacial effects. The green area highlights the transfer of spectral weight from higher energies. | 1503.07328_4.jpg |
arxivcap_1802.01331_5 | Title: Relaminarization by steady modification of the streamwise velocity profile in a pipe | Caption: Streamwise rms profile measured at $\Rey=5000$ scaled on inner variables. The dashed line shows the results from <cit.> for comparison. | 1802.01331_5.jpg |
arxivcap_2206.01867_10 | Title: SPGNet: Spatial Projection Guided 3D Human Pose Estimation in Low Dimensional Space | Caption: Clustered column charts (a) and (b) illustrate the comparisons of different sittings and input frames, respectively. The error shows a decreasing trend as the model is applied from the Baseline to our SPGNet or the size of input frames increases. Notably, in Figure <ref>, Baseline is the model only learned from MPJPE loss, and Baseline* represents the Baseline adding kinematic constraints. In the chart <ref>, \(J\) represents the number of frames in the input sequence. | 2206.01867_10.jpg |
arxivcap_2305.05309_2 | Title: PSP Framework: A novel risk assessment method in compliance with ISO/SAE-21434 | Caption: ISO/SAE-21434 Development Life Cycle | 2305.05309_2.jpg |
arxivcap_1308.0826_3 | Title: Elemental Topological Insulator with a Tunable Fermi Level: Strained
\alpha-Sn on InSb(001) | Caption: a) ARPES measurements on , performed at 119 eV, i.e., at the $\Gamma$-point of the BZ resolve the $\Gamma_8^+$ and the $\Gamma_7^-$ valence bands, marked by yellow lines. b) At h$\nu$ = 21.22 eV (He-I) a linearly dispersing feature is observed and marked by red dashed lines. (c - e) Photon-energy dependent measurements, i.e., at h$\nu$ = 21.22 eV (c) and 16.86 eV (Ne-I) (d) clarify the surface character of the state. Blue circles and orange triangles in e) represent the fitted peak positions from c) and d), respectively. Note that the sample of b) - e) is doped with Te, as described in the text. All measurements taken along the -direction at room temperature in our home lab (b - e) and at the ALS (a). The faint replicas at higher binding energies in d) are due to a satellite line in the Ne discharge. | 1308.0826_3.jpg |
arxivcap_2108.09610_5 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Number of dwarfs excluded by visual classification as function of the number of dwarfs expected to be background galaxies (from a blank field). Error bars correspond to Poisson uncertainties based on the actual number of objects. | 2108.09610_5.jpg |
arxivcap_2012.05350_8 | Title: Automatic Diagnosis of Malaria from Thin Blood Smear Images using Deep Convolutional Neural Network with Multi-Resolution Feature Fusion | Caption: Variations of performance in different metrics for training with increasing amount of available data: Considerable performance is achieved even with $10\%$ of the available training data. With increasing data, performanmce gets better in all the metrics. | 2012.05350_8.jpg |
arxivcap_1111.4939_15 | Title: Josephson and Andreev transport through quantum dots | Caption: Experimental setup used in Ref. <cit.> for analyzing the $0-\pi$ transition in CNT QDs (upper panel). The middle panel shows the reversal of the oscillatory pattern of the current as a function of the magnetic flux through the SQUID across the transition. The lower panel shows the correlation of the $\pi$-phase region with the Kondo ridges in the normal state (indicated by the dashed line). Reprinted by permission from Macmillan Publishers Ltd: Nature Physics <cit.>, copyright (2006). | 1111.4939_15.jpg |
arxivcap_2210.09481_4 | Title: FPGA Hardware Acceleration for Feature-Based Relative Navigation Applications | Caption: SURF feature detection and extraction, shown on two images of a terrain named Rheasilvia. Image 1 is taken from a reference position and image 2 is taken after the camera is transformed to a different position. The matched features between images 1 and 2 are also shown. | 2210.09481_4.jpg |
arxivcap_2212.13102_15 | Title: Piezoelectric effect and diode effect in anapole and monopole superconductors | Caption: Temperature dependence of the nonreciprocal critical current $\Delta J_{\textrm{c}}$ in the (a) group velocity model, (b) geometric effect model, and (c) mixed model of the $A_g + i B_{3u}$ anapole state. The parameters $(\alpha, \beta)$ are (a) $(0.4,1)$, (b) $(0.4,0)$, and (c) $(0.4,1)$ as in Figs. <ref>, <ref> and <ref>. | 2212.13102_15.jpg |
arxivcap_2108.09610_6 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Individual cumulative functions of the clustercentric distances of dwarfs (yellow dashed line) and giants (green line) on each cluster. The number at the corner of each panel corresponds to the p-value coming from a Kolmogorov-Smirnov test which gives the probability that giants and dwarfs are taken from the same radial distribution. | 2108.09610_6.jpg |
arxivcap_1401.8257_9 | Title: Online Clustering of Bandits | Caption: Results on synthetic datasets in the case of unbalanced ($z=2$) cluster sizes. The rest is the same as in Figure <ref>. | 1401.8257_9.jpg |
arxivcap_2206.12127_2 | Title: Implicit Channel Learning for Machine Learning Applications in 6G Wireless Networks | Caption: Various ML applications for 6G use-cases and the corresponding transmit data types. The edge devices send the ML data to the PS through wireless medium. Once the channel acquisition is performed, the received ML data is input to the learning models. The recognition task is carried out at the PS that sends back the prediction output to the edge devices. | 2206.12127_2.jpg |
arxivcap_2202.01537_9 | Title: Bending Graphs: Hierarchical Shape Matching using Gated Optimal Transport | Caption: We show the visual difference of the ablation study on the number of GFP layers (corresponding to #1 #2 and #3 on table <ref>. The human models from left to right are (a) The target shape map (b) The coarse matching result of model #1, (c) the coarse matching result of model #2, (d) the coarse matching result of model #3, (e) the dense matching result of model #2, (f) the ground truth dense matching result and (g) normalized L2 error map of model #2. | 2202.01537_9.jpg |
arxivcap_2303.14694_1 | Title: A stability theorem for bigraded persistence barcodes | Caption: The barcode corresponding to the Vietoris-Rips complex in Figure <ref>. The image is generated by Ripser for Python. | 2303.14694_1.jpg |
arxivcap_2004.03425_18 | Title: Elemental abundances in M31: [Fe/H] and [{\alpha}/Fe] in M31 Dwarf Galaxies Using Coadded Spectra | Caption: Histograms showing the distribution of S/N (per angstrom) of individual stars in our Milky Way globular cluster sample (top) and our validation M31 dSph stars (bottom). The solid-filled histograms represent the entire sample of member stars, with the lines showing the sample used for validating our coaddition pipeline (Section <ref>). | 2004.03425_18.jpg |
arxivcap_1211.6964_6 | Title: On the Bauschinger effect in supercoooled melts under shear: results from mode coupling theory and molecular dynamics simulations | Caption: Linear stress responses $G_{\text{eff}}=d\sigma/d\gamma|_{|\gamma-\gamma_{0}|=0.025}$ from simulation, fits of the schematic model, and Maxwell model as labeled for various waiting strains $\gamma_{w}$. The inset gives the strain $\gamma_{w}-\gamma_{0}$ required for the stress to reduce to zero after shear reversal. To include the simulation point for $\gamma_w^s=75$, this value has been divided by 200, using that the precise value of $\gamma_w$ is irrelevant in the steady state. | 1211.6964_6.jpg |
arxivcap_2206.01901_2 | Title: Enabling Heterogeneous, Multicore SoC Research with RISC-V and ESP | Caption: Modifications to the ESP processor tile and CVA6 L1 cache to enable multicore execution. | 2206.01901_2.jpg |
arxivcap_1806.08643_3 | Title: Diffusiophoretically induced interactions between chemically active and inert particles | Caption: The velocity $V$ of the noncatalytic $S_2$ sphere as a function of the separation $L$ between the $S_2$ and $S_1$ catalytic spheres. The black solid line is the exact solution calculated from continuum hydrodynamic theory in Eq. (<ref>) and the black dashed line is the approximate velocity $V_a$ from Eq. (<ref>) that is valid for large $L$. The red circles with error bars are the results of microscopic simulations. Averages were obtained from 80 realizations of the dynamics. | 1806.08643_3.jpg |
arxivcap_1111.0053_7 | Title: Exploiting Subgraph Structure in Multi-Robot Path Planning | Caption: The results of Experiment 1a. In graph (a) the boxes show the first and third quartile and whiskers to show the complete range. When an experiment failed to complete due to time or memory limits or incompleteness of the search, the run time was treated as infinite. No value is plotted for cases where more than 50% of experiments failed. In graph (c) the goal depth for the naive complete and subgraph priority approaches are identical for graphs of 30 to 60 vertices, so the lines overlap. The naive complete planner could not solve problems with more than 60 vertices. | 1111.0053_7.jpg |
arxivcap_2108.09610_7 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Sérsic index ($n$) as a function of clustercentric distance for early type dwarfs (orange points) and late type dwarfs (green points). Note that cluster RXJ0123.2+3327 and RXJ0123.2+3315 are not included in this figure. | 2108.09610_7.jpg |
arxivcap_2303.06733_4 | Title: Probing the Origin of Changing-look Quasar Transitions with Chandra | Caption: Relation between X-ray photon index, $\Gamma_X$, and Eddington ratio (${\rm L_{bol}/L_{Edd}}$) in logarithm, for AGN and XRBs. The color dots are our five CLQs, including J0206 (red), J0224 (blue), J0829 (green), J1226 (magenta), and J1338 (cyan). The dotted lines connect the CLQ in bright state and faint state. The black squres are measurements from AGN in <cit.>. There are some individual XRBs, including Swift J1753.5$-$0127 (open square), H1743$-$322 (cross), and GX 339$-$4 (open triangle). One can see the same trend, softer when brighter, in AGN and XRBs. The individual CLQs follow this trend well. J1338 was unfortunately not captured in its faint state during our {Chandra} observation. | 2303.06733_4.jpg |
arxivcap_1308.0826_4 | Title: Elemental Topological Insulator with a Tunable Fermi Level: Strained
\alpha-Sn on InSb(001) | Caption: SARPES on . a) Mott polarimetry of an MDC at E$_B$=190 meV along the -direction (marked by a white dashed line in both insets), reveals a strong spin-asymmetry that we assign to the surface state. b) The derived spin-resolved intensity distribution gives one highly spin-polarized peak per spin direction, i.e., a spin down-peak ($\downarrow$) at -k$_x$ and a spin up-peak ($\uparrow$) at +k$_x$ (blue and red triangles/lines, respectively). The polarization vector points fully along the y-direction, which gives a counter-clockwise spin helicity as shown in the constant energy surface in the lower inset. All measurements at h$\nu$=19.5 eV and at T$\sim$20 K. Spin-resolved and spin-integrated measurements were performed at COPHEE and HRPES endstations at SLS, respectively. | 1308.0826_4.jpg |
arxivcap_2212.13102_16 | Title: Piezoelectric effect and diode effect in anapole and monopole superconductors | Caption: Temperature dependence of the SDE efficiency $r$ in the (a) group velocity model, (b) geometric effect model, and (c) mixed model of the $A_g + i B_{3u}$ anapole state. The parameters $(\alpha, \beta)$ are (a) $(0.4,1)$, (b) $(0.4,0)$, and (c) $(0.4,1)$ as in Figs. <ref>, <ref> and <ref>. | 2212.13102_16.jpg |
arxivcap_2303.14783_2 | Title: A macroscopic constitutive relation for isotropic-genesis, polydomain liquid crystal elastomers | Caption: The shaded regions indicate the (a) allowable domain order parameters ${\mathcal A}_S$ and (b) allowable spontaneous deformation parameters ${\mathcal A}_G$. The values of the parameters corresponding to the isotropic $I$, monodomain $M$ and planar equiaxed $P$ are also indicated. | 2303.14783_2.jpg |
arxivcap_2010.12170_2 | Title: Is PSR J0855$-$4644 responsible for the 1.4 TeV electron spectral bump hinted by DAMPE? | Caption: The electron spectrum observed near Earth, fitted with the contribution from PSR J0855-4644. The background e$^\pm$s are contributed by other nearby sources such as SNRs. The DAMPE data are taken from <cit.>, CALET data from <cit.>, and AMS positron data from <cit.>. | 2010.12170_2.jpg |
arxivcap_1802.01331_6 | Title: Relaminarization by steady modification of the streamwise velocity profile in a pipe | Caption: Still pictures from supplementary movie 1 (see online materials) of a short section of the pipe at $\Rey=4000$. The camera was following the flow downstream the obstacle-FMD at the mean velocity $U$. The difference between turbulent flow (at $z=3$) and laminar flow (at $z=50$) is unambiguous. | 1802.01331_6.jpg |
arxivcap_2305.05309_6 | Title: PSP Framework: A novel risk assessment method in compliance with ISO/SAE-21434 | Caption: CAL determination based on impact and attack vector parameters table extracted by ISO/SAE-21434 | 2305.05309_6.jpg |
arxivcap_1503.07328_5 | Title: Spectral weight redistribution in (LaNiO3)n/(LaMnO3)2 superlattices from optical spectroscopy | Caption: Schematics of the spectral weight redistribution in LNO/LMO. a) Transfer of spectral weight from coherent (blue) to in-coherent (red) excitations in LNO, due to the reduction in the Ni oxidation state. b) Spectral weight transfer in LMO from the high energy Jahn-Teller band (green) to the mid and far infrared (red), due to the increased Mn valence. c) Sketch of the spectral weight transfer in LNO/LMO SLs, due to the valence mixing associated with interfacial effects. | 1503.07328_5.jpg |
arxivcap_1912.05125_12 | Title: Bayesian Framework for Simultaneous Registration and Estimation of Noisy, Sparse and Fragmented Functional Data | Caption: Posterior draws (transparent), mean (solid black), and credible interval (dashed) when $H = 2$ and (top) $H = 4$ (bottom), with a comparison to the WPACE fitted function (red) for three different subjects. | 1912.05125_12.jpg |
arxivcap_2205.02281_7 | Title: Three-Body Problem in Modified Dynamics | Caption: The effective potential, in units of $GM/(d_{1}+d_{2})$, for different values of the dimensionless energy in the rotating frame $E^{\prime} \equiv E/(GM/(d_{1}+d_{2}))$ and the ratio $\epsilon$, in the case $\mu = 0.3$. | 2205.02281_7.jpg |
arxivcap_1109.6664_11 | Title: Conditional pair distributions in many-body systems: Exact results for Poisson ensembles | Caption: (Color online) Contributions $g^{(\nu)}(\omega)$ due to $\nu=$i, ii, iii and iv pair configurations (solid, short dashed, long dashed and point-dashed lines, respectively) to the PDF $g(\omega)$ vs the volume $\omega$, for Poisson ensembles at dimensions $D=1,2,3$ and $\infty$. The total PDF is shown by a dotted line. | 1109.6664_11.jpg |
arxivcap_2108.09610_8 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Effective radius ($R_{\rm eff}$) as a function of clustercentric distance for early type dwarfs (orange points) and late type dwarfs (green points). Note that cluster RXJ0123.2+3327 and RXJ0123.2+3315 are not included in this figure. | 2108.09610_8.jpg |
arxivcap_2005.06188_9 | Title: Star clusters near and far; tracing star formation across cosmic time | Caption: $\Gamma$ vs. $\Sigma_{\rm SFR}$ plane. We combine the observed data available in the literature (filled grey symbols), i.e, the data are not separated by age ranges used to estimate $\Gamma$ (see Section <ref> and Figure <ref> for description of the observed data). We also include median and 25 and 75 % quartiles of the observed data (filled black symbols) estimated in $\Sigma_{\rm SFR}$ bins, of size indicated by the horizontal bars. {Left}: We include the resulting $\Gamma$ vs. $\Sigma_{\rm SFR}$ extracted from the simulation sets by <cit.>. The curves show the median and quartiles of different sets of simulations using different feedback prescriptions. {Right}: We include the extracted $\Gamma$ and $\Sigma_{\rm SFR}$ for the E-MOSAICS simulations (filled square symbols) by <cit.>. The values have been extracted from galaxies at redshift 0 and are plotted color-coded by the galaxy stellar mass in the same snapshot. | 2005.06188_9.jpg |
arxivcap_2102.12804_7 | Title: Compact Groups of Galaxies in Sloan Digital Sky Survey and LAMOST Spectral Survey. II. Dynamical Properties of Isolated and Embedded Groups | Caption: The comparison of the embedded CGs and mock CGs from Monte Carlo simulation. Left: velocity dispersion of the embedded CGs ($\sigma_{\text{LOS}}$) versus that of their parent groups ($\sigma_{\text{LOS}}^{\text{par}}$). The open hexagons represent the median $\sigma_{\text{LOS}}$ of the embedded CGs in each $\sigma_{\text{LOS}}^{par}$ bin, whose vertical error bars represent the errors of the median $\sigma_{\text{LOS}}$ and horizontal error bars represent the median absolute deviation of $\sigma_{\text{LOS}}^{\text{par}}$ in each bin. The shaded area shows the 16$\text{th}$ and 84$\text{th}$ percentiles of the $\sigma_{\text{LOS}}$ distribution at a given $\sigma_{\text{LOS}}^{\text{par}}$, whereas the three dashed lines show the 16$\text{th}$, 50$\text{th}$, and 84$\text{th}$ percentiles for the mock CGs. The bottom shows the histograms of the radial distance of observed (filled) and mock (open) CGs within the parent groups in each $\sigma_{\text{LOS}}^{\text{par}}$ bin. Right: The CGs located at $R/R_{\text{med}}>1$ (red) and $R/R_{\text{med}}<1$ (green), respectively. The triangles show the observed embedded CGs, while the shaded and hatched areas represent the standard deviation of the median $\sigma_{\text{LOS}}$ of mock CGs, respectively. The bold lines in both panels are the one-to-one correspondence between $\sigma_{\text{LOS}}$ and $\sigma_{\text{LOS}}^{\text{par}}$. | 2102.12804_7.jpg |
arxivcap_2206.12106_1 | Title: TreeDRNet:A Robust Deep Model for Long Term Time Series Forecasting | Caption: Left: TreeDRNet forecasting sequences with model trained using different input horizons. Right: Autoformer forecasting sequences with model trained using different input horizons. Input horizons: the yellow (also including the blue and purple) is 1008; the blue (also including the purple) is 672; the purple is 336. | 2206.12106_1.jpg |
arxivcap_astro-ph_0104286_3 | Title: THE NEARBY FIELD GALAXY SURVEY | Caption: Gallery of several example optical rotation curves. At {top left}, a greyscale $B$-filter image is given for one galaxy with the orientation of the spectrograph slit indicated. The resulting 2D spectrum image, spanning the range 6000-7000Å in wavelength, is presented with the strongest emission lines marked. The extracted rotation curve for this galaxy is presented in the {upper left panel} of the gallery, showing that this galaxy is similar in size, luminosity and mass to our own Milky Way galaxy. | astro-ph_0104286_3.jpg |
arxivcap_2212.13299_1 | Title: Leveraging Collaboration for Multifaceted Design and Product Teams: A Financial Perspective | Caption: This snapshot provides a quick overview of how squads within and outside of the Design Team collaborate together. The User Experience Squad Member acts as an intermediary between the Business and Product Team and the Design Team. | 2212.13299_1.jpg |
arxivcap_1906.05331_1 | Title: Twin-beam sub-shot-noise raster-scanning microscope with a hybrid detection scheme | Caption: Simulation of precision ratio using twin-beams and feed-forward. The plot compares Poisson-limited light (horizontal blue line at ratio of 1) to transmittance estimation with twin-beam strategies. The key refers to the different values of overall source Klyshko efficiency, which are symmetric for direct twin-beam exposure (dotted lines) and asymmetric for feed-forward (solid lines) due to the 15$\%$ loss in the switch and 10$\%$ leakage of unheralded photons. | 1906.05331_1.jpg |
arxivcap_1709.03144_32 | Title: The 12C(a,g)16O reaction and its implications for stellar helium burning | Caption: (Color online) Comparison of destructive (red dashed lines) and constructive (red solid lines) $E1$ solutions. A 1$^-$ background pole is included in the ground state $\gamma$ ray channel in these cases. The energy of the pole is held constant in both cases and the fitted $\alpha$ widths are very similar. For the constructive case $\Gamma_{\gamma_0}$ = 1.8 eV, while the destructive case gives 21.7 eV. | 1709.03144_32.jpg |
arxivcap_2202.13752_5 | Title: Discrete unified gas kinetic scheme for the conservative Allen-Cahn equation | Caption: The phase-field contour ($\phi=0$) of vortex deformation of a circle at (a) t=T/2 and (b) t=T. From left to right, the results are obtained by LBE-AC, DUGKS-AC, DUGKS-I and DUGKS-II. Black dashed lines denotes the initial profile and red solid line represents the reconstructed interface. | 2202.13752_5.jpg |
arxivcap_2108.09610_9 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Colour-magnitude diagram for all the red sequence elliptical galaxies (green points) of all cluster of the sample espectrally confirmed as a cluster member. Upper green line corresponds to the fit line for these galaxies while the bottom green line is the same line shifted three sigmas (standard deviation of the distance of the the green points to the fitting line) below. Grey points correspond to the remaining galaxies from each cluster. | 2108.09610_9.jpg |
arxivcap_2305.05309_7 | Title: PSP Framework: A novel risk assessment method in compliance with ISO/SAE-21434 | Caption: The figure A) shows the attack feasibility weights, defined by ISO-21434, for outsider threats B) On the contrary, the insider threats get attack feasibility weights tuned by PSP framwork | 2305.05309_7.jpg |
arxivcap_2303.14783_3 | Title: A macroscopic constitutive relation for isotropic-genesis, polydomain liquid crystal elastomers | Caption: Domain pattern evolution. Adapted from Figure 8 of Tokumoto {et al.} <cit.> | 2303.14783_3.jpg |
arxivcap_1802.01331_7 | Title: Relaminarization by steady modification of the streamwise velocity profile in a pipe | Caption: Downstream evolution of mean streamwise velocity profiles $(\bar w)$ in the plane $y=0$ measured at (a) $\Rey=3800$ and (b) $\Rey=4500$. In each plot the profile of uncontrolled turbulent flow is shown for reference (ref) at the left. (c) Respective levels of the axially developing centerline velocity. | 1802.01331_7.jpg |
arxivcap_2202.01466_1 | Title: Quantifying knowledge synchronisation in the 21st century | Caption: Wikipedia knowledge network and genealogy vector of a subject. a. Example of a page-category hyperlink in English Wikipedia (left). The page has hyperlinks to several categories to which the page belongs. One can express such relations using the network (graph), where the node represents an entity (which can be a page, a category, or their union) with the links representing the hyperlink relationship between them. The identical page is titled in French Wikipedia (right). Note that the hyperlink structures of two language editions are different, even for the identical entities. Between these two language editions, there are dotted and gray lines denoting the existence of language links between them, indicating that the two subjects are identical. b. Method for calculating the genealogy vector of a focal node. We obtain the genealogy vector using the personalized Page Rank algorithm, which calculates the probability that a random walker starting from the focal node visits other nodes. The random walker starts at the focal node and traverses with probability $1-\alpha$ to its nearest neighbors. The walker also occasionally returns to the focal node with a teleport probability, $\alpha$. The focal genealogy vector of the focal node is the random walker's stationary distribution for the visited nodes. | 2202.01466_1.jpg |
arxivcap_1806.08643_4 | Title: Diffusiophoretically induced interactions between chemically active and inert particles | Caption: Plot of the distance between the fixed catalytic and moving noncatalytic spheres as a function of time. Five realizations of the dynamics are shown, each with an initial separation $L/\sigma = 10$. Contact occurs at approximately $L/\sigma \sim 2.3$. The time where the distance achieves its minimum value is the capture time (see Fig. <ref>). | 1806.08643_4.jpg |
arxivcap_2210.09481_5 | Title: FPGA Hardware Acceleration for Feature-Based Relative Navigation Applications | Caption: OLTAE HW/SW co-design: The modules on the OLTAE core on the PL evaluate the least squares based attitude estimation logic (Eq. <ref>). The PS facilitates the communication of measurement data and estimation results via Advanced eXtensible Interface (AXI4) bus interface. | 2210.09481_5.jpg |
arxivcap_1308.0826_5 | Title: Elemental Topological Insulator with a Tunable Fermi Level: Strained
\alpha-Sn on InSb(001) | Caption: Doping control. On varying the Te concentration, we shift the Dirac-point from 10 meV above (a) for a Te-concentration of 6% to 30 meV (b) and 60 meV (c) below for Te-concentrations of 8% and 15%, respectively. Colored lines in a) - c) are linear regressions to the fitted MDC peak positions (colored symbols). All measurements taken along the -direction, at h$\nu$=21.22 eV, and at room temperature in our home lab. | 1308.0826_5.jpg |
arxivcap_1211.6964_7 | Title: On the Bauschinger effect in supercoooled melts under shear: results from mode coupling theory and molecular dynamics simulations | Caption: View on the $t-t'$-plane, with the three different time regimes for the density correlator $\Phi$. As the $h$-function depends only on the absolute value of $\dot\gamma$, the one-time-solutions $\Phi^{(+\dot\gamma)}$ and $\Phi^{(-\dot\gamma)}$ are equal. | 1211.6964_7.jpg |
arxivcap_1902.03928_4 | Title: The Degree of Fine-Tuning in our Universe -- and Others | Caption: Experimentally measured quark masses. The spikes correspond to the six known quarks $(u,d,s,c,b,t)$, from left to right. The quark masses are relatively evenly spaced on a logarithmic scale (see <cit.>). | 1902.03928_4.jpg |
arxivcap_2303.13078_6 | Title: Real Hopf Insulator | Caption: Various topological insulators appearing in $\mathcal{PT}$ symmetric spinless fermion systems. Topological invariants of 1D,2D,and 3D are the Berry phase, the Euler class, and the real Hopf invariants, respectively. | 2303.13078_6.jpg |
arxivcap_1104.3722_9 | Title: Investigating the Distribution of Password Choices | Caption: Number of users whose passwords are cracked by using the password ordering from different distribution on the Gawker.com password hashes. | 1104.3722_9.jpg |
arxivcap_2206.01901_4 | Title: Enabling Heterogeneous, Multicore SoC Research with RISC-V and ESP | Caption: Execution time of the CRONO benchmark suite on 1, 2, and 4 CVA6 cores in ESP. | 2206.01901_4.jpg |
arxivcap_2012.05322_5 | Title: Deep Learning Segmentation of Complex Features in Atomic-Resolution Phase Contrast Transmission Electron Microscopy Images | Caption: Three examples comparing Bragg and U-net filtering. (a) Output masks where both filters performed well, (b) masks where Bragg filter produced false positive regions, and (c) masks where Bragg filter produced false negative regions. In both (b) and (c), the U-Net filter produced a more accurate result. | 2012.05322_5.jpg |
arxivcap_2108.09610_10 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: Individual cumulative fractions as a function of the distance to the cluster centre for the blue and red galaxies. Blue and red dashed lines correspond to the 'blue' dwarfs and 'red' dwarf respectively, while blue and red filled lines lines correspond to 'blue' giants and 'red' giants respectively. | 2108.09610_10.jpg |
arxivcap_1912.05125_13 | Title: Bayesian Framework for Simultaneous Registration and Estimation of Noisy, Sparse and Fragmented Functional Data | Caption: (a) BMD measurements colored by ethnicity: Asian (blue), Black (red), Hispanic (green) and Caucasian (magenta). (b) Posterior estimates of mean BMD functions, with $95\%$ credible intervals, for the four ethnic groups. | 1912.05125_13.jpg |
arxivcap_2004.03425_19 | Title: Elemental abundances in M31: [Fe/H] and [{\alpha}/Fe] in M31 Dwarf Galaxies Using Coadded Spectra | Caption: Histogram of the differences between coadded abundances and weighted averages, weighted by their corresponding uncertainties, for [Fe/H] (top) and [$\alpha$/Fe] (bottom). The solid black histogram represents the normalized sum of all validation coadds for all GCs in our sample. The solid black curve indicates the best-fit Gaussian for the sample of all validation coadds from all GCs, and the dashed red curve indicates a normalized unit Gaussian with $\sigma = 1$. | 2004.03425_19.jpg |
arxivcap_2210.09481_6 | Title: FPGA Hardware Acceleration for Feature-Based Relative Navigation Applications | Caption: This figure illustrates the hardware/software co-design and the flow of operations for the 6-DOF pose estimation using OLTAE algorithm. | 2210.09481_6.jpg |
arxivcap_1503.07274_1 | Title: Initialization Strategies of Spatio-Temporal Convolutional Neural Networks | Caption: 3D Convolutional Kernels $W^{(3D)}=(W^{(3D)}_{1},W^{(3D)}_{2},W^{(3D)}_{3})$ learned by the first 3D Convolutional Layer initialized by IA, IS, ZWI and NWI respectively. In Spatio-Temporal ConvNet initialized by averaging or scaling, $W^{(3D)}_{2}$ and $W^{(3D)}_{3}$ look very similar to $W^{(3D)}_{1}$. Whereas in ConvNet initialized by NWI, $W^{(3D)}_{2}$ and $W^{(3D)}_{3}$ look different from $W^{(3D)}_{1}$. Also, despite having limited labelled training video data, $W^{(3D)}_{2}$ and $W^{(3D)}_{3}$ look like edge and color blobs detectors in Spatio-Temporal ConvNet initialized by ZWI. | 1503.07274_1.jpg |
arxivcap_1308.0826_6 | Title: Elemental Topological Insulator with a Tunable Fermi Level: Strained
\alpha-Sn on InSb(001) | Caption: LDA+U calculation of 6 layers embedded in a semi-infinite bulk. The TSS is visible as linear dispersion on a weak bulk projection background. | 1308.0826_6.jpg |
arxivcap_2303.06733_5 | Title: Probing the Origin of Changing-look Quasar Transitions with Chandra | Caption: Relation between the UV-to-X-ray spectral index ($\alpha_{\rm OX}$) and the logarithm of the Eddington ratio log(${\rm L_{bol}/L_{Edd}}$), for AGN and XRBs. Both $\alpha_{\rm OX}$ and $L_{bol}$ are taken from our SED fitting. Colored solid dots are our 5 {Chandra} CLQs as in Figure <ref>. The gray symbols are from CLQs in the faint states (open circles) and lower limits in the bright states (open circle with arrows) in <cit.>, and CLQs in the faint states (open diamonds) and lower limits in the bright states (open diamonds with arrows) in <cit.>. The black symbols are CLQs with X-ray observations in both states for J0159 (squares) analyzed in <cit.> and J2252 (star) and J2333 (cross) in <cit.>. The dotted line connects one CLQ observed in two states. The asterisks show results from the Galactic XRB GRO J1655-40 <cit.> in hard state (sky blue) and soft state (pink), extrapolated via mass scaling to Type 1 AGN (see their Figure 4). | 2303.06733_5.jpg |
arxivcap_2212.13295_1 | Title: Structure-based drug discovery with deep learning | Caption: Structure-based drug discovery tasks discussed in this review: (a) drug-target interaction prediction, which aims to predict the affinity between a protein and a ligand, using the structural information of both molecular entities; (b) binding site detection, which aims to identify `druggable' cavities in the protein structure, (c) de novo design, aiming to design bioactive molecules from scratch using the information of a protein target. | 2212.13295_1.jpg |
arxivcap_2303.14783_5 | Title: A macroscopic constitutive relation for isotropic-genesis, polydomain liquid crystal elastomers | Caption: Demonstration of the proposed model. Each row represents a different loading mode described in Table <ref>. The first column shows the true stress vs. stretch, the second column the state variables vs. stretch and the final column the evolution of the state variables. | 2303.14783_5.jpg |
arxivcap_1906.05331_3 | Title: Twin-beam sub-shot-noise raster-scanning microscope with a hybrid detection scheme | Caption: Experimental setup and its characterisation. a) Photon-pairs are generated by SPDC in a PPKTP crystal, feed-forward of the idler photons is implemented using a polarisation independent switch, as described in Ref. <cit.>. Heralded photons are focused first through the sample and subsequently refocused to a point on a CCD camera for detection. The sample is raster scanned in two dimensions, allowing an image to be reconstructed. A mechanical shutter before the crystal is triggered by activation of the camera sensor, initializing the experiment and allowing the pump beam into the crystal. The shutter prevents undesired exposure of the sample during the camera's dead time. The acquisition time of the SPAD is synchronized to the CCD using a software interface that communicates with a time tagging electronics system which only records counts during the acquisition time of the camera, minimising uncorrelated reference channel noise. b) Precision ratio of transmittance between our setup and a theoretically ideal Poisson-limited light source measured with the same detection efficiency, (horizontal blue line at a ratio of 1, which corresponds to the shot-noise limit). Data points are the ratio between the variance of our transmittance estimate and the calculated variance of the same measurement for an ideal coherent state, at different levels of sample transmittance (red circles). In each case, the data was normalized relative to the number of input photons incident on the sample. Points above the blue line exhibit sub-shot-noise performance. Each point corresponds to 13 series of 40 measurements with an integration time of 1 s at a rate of 40000 counts per second. Error bars correspond to the experimental standard deviation of the mean from the different data series. c) Electron beam microscope image of the platinum deposited target used for resolution characterisation. d) Results of imaging the resolution target using correlated photon pairs. Two distinct strips are apparent in the optical image for 3 $\mu$m spacing, but for smaller spacings the gap between parallel strips is not discernible. From this, we estimate that the spatial resolution of the SSN microscope to be 3 $\mu$m. | 1906.05331_3.jpg |
arxivcap_2303.13078_10 | Title: Real Hopf Insulator | Caption: Wannier sheet crossing of a real Hopf insulator model in Eq. (<ref>) with $(\chi_z,\chi_w)=(1,1)$. (a) One of the bulk Wannier sheets of $|u_{1}^{c}\rangle+i |u_{2}^{c}\rangle$ of Eq. (<ref>), which is the $\lambda_1=\lambda_2=0$ limit of Eq. (<ref>). In the $(k_x,k_y)$ plane, the green dotted line connects $\Gamma$ and $\mathrm{M}$ without passing through the $C_{2z}$-invariant momenta along the way, thus being a path $\gamma$ as described in the main text. Along $\gamma$, the Wannier center travels two unit layers (red solid line). (b) Cross-section of the Wannier sheet in (a) along the $\Gamma \mathrm{M}$ line. The red solid line is the cross-section of the Wannier sheet in (a) and the blue solid line is its $\mathcal{PT}$ symmetric partner. The red (blue) dashed lines are given by the parallel translation of the red (blue) solid line and depict Wannier sheets of adjacent unit cells. (c) One of the bulk Wannier sheets of $|u_{1}^{c}\rangle+i |u_{2}^{c}\rangle$ of Eq. (<ref>) with $\lambda_{1}=\lambda_{2}=0.7$. (d) Cross-section of the Wannier sheets in (c) and their partners along $\Gamma \mathrm{M}$. | 2303.13078_10.jpg |
arxivcap_2108.09610_11 | Title: The dwarf galaxy population in nearby clusters from the KIWICS survey | Caption: { Top panels}: Dwarf fraction inside $R_{200}$ as a function of cluster mass $M_{500}$ (left) and cluster velocity dispersion (right). Green colour points indicate whether the distribution of dwarfs and giants is different (based on the KS-test), while orange indicates that both distribution are similar. {Bottom panels}:Ratio of the dwarf fraction in the inner region and in the outermost regions of the cluster versus the same quantities. | 2108.09610_11.jpg |
arxivcap_2206.01858_1 | Title: Efficient Manipulation of Bose-Einstein Condensates in a Double-Well Potential | Caption: Left panels: the phase space of system (<ref>) for $v=0$ (top) and $v=10$ (bottom), with the ground state marked with a black star, showing that two fixed points have bifurcated from the bounding circle as $v$ was raised, now sitting at approximately $(q,p)=(\pm0.7550,0)$. Right panels, same parameter values, show in black the ground state standing wave and in red/blue the odd-symmetric standing waves (top) and the symmetry broken standing waves $\psi_0$ and $\psid$ (bottom). | 2206.01858_1.jpg |
arxivcap_2205.02281_8 | Title: Three-Body Problem in Modified Dynamics | Caption: The evolution of a test particle around two massive objects of $m_{1}=10~ \mathcal{M}$ and $m_{2}=7~ \mathcal{M}$ with the distance of $d=20~ \mathcal{D}$. The evolution time is $3000~\mathcal{T}$, the initial position of $m_{3}$ is chosen randomly to be within $(x_{0}\pm 0.1x_{0},~y_{0} \pm 0.1y_{0})$ and this particle rotates initially in the same direction of $m_{1} $ and $m_{2}$. The ejection in Newtonian models is more common than the MOD models. | 2205.02281_8.jpg |
arxivcap_astro-ph_0104286_4 | Title: THE NEARBY FIELD GALAXY SURVEY | Caption: Effective $B-R$ colours as a function of morphological type and absolute $B$ magnitude. Points are coded according to type as follows. Ellipticals and S0s ($T<0$) are indicated by {open circles}, early-type spirals ($0\leq T<3$) by {open triangles}, intermediate spirals ($3\leq T<6$) by {solid triangles}, and late-type spirals and irregulars by {asterisks}. Active nucleated galaxies are indicated by {crosses} and starburst galaxies by {open stars}. | astro-ph_0104286_4.jpg |
arxivcap_1308.0826_7 | Title: Elemental Topological Insulator with a Tunable Fermi Level: Strained
\alpha-Sn on InSb(001) | Caption: LEED patterns of a) an undoped and b) a Te-doped sample. Incorporating Te during the growth leads to an increased surface quality, as obvious from the sharper LEED spots in b) and to a (1 $\times$ 1) surface reconstruction, while the pristine sample in a) is (2 $\times$ 1) reconstructed. | 1308.0826_7.jpg |
arxivcap_2206.12106_2 | Title: TreeDRNet:A Robust Deep Model for Long Term Time Series Forecasting | Caption: The overall TreeDRNet structure. (a) shows the doubly residual structure, motivated by the robust iterative reweighted algorithm as in Eq. (<ref>). (b) shows the multi-branch block with feature selection (through gating mechanisms), doubly residual structure, and model ensemble (through multiple branch), motivated by the Kolmogorov-Arnold theorem as in Eq. (<ref>). (c) shows the high-level architecture of the TreeDRNet model with binary-tree structure, where each node of the tree is a multi-branch block with feature selection. | 2206.12106_2.jpg |
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