adsabs/AstroCLIMB huggingface dataset:
Paper: Feasibility of High-resolution Transmission Spectroscopy for Low-velocity Exoplanets
Authors: Connor J. Cheverall, Nikku Madhusudhan
Figure caption: Recovery of an NH3 signal injected with zero orbital velocity. The detection S/N across K p−V sys space is shown when an NH3 signal is injected into the spectra with no semi-amplitude radial velocity (K p = 0 km s−1) and no barycentric velocity correction and then recovered as in Figure 2. A signal with a S/N of 4.7, unconstrained in K p, is recovered at the correct V sys.
Paper: A MeerKAT Polarization Survey of Southern Calibration Sources
Authors: A. R. Taylor, L. S. Legodi
Figure caption: Fractional polarization spectra of J1939-6342 on 2019 August 19 (top) and 2020 August 29 (bottom). For each run, traces are shown for Q/I (blue), U/I (green), and V/I (red).
Paper: A MeerKAT Polarization Survey of Southern Calibration Sources
Authors: A. R. Taylor, L. S. Legodi
Figure caption:  Gaincal solutions for hourly observations of J0408-6545 during the observing run of 2020 August 29. The x-axis shows observation time stamps with solution amplitude and phase given on the y-axis. The left-hand panel shows gain amplitude vs. time, and the right-hand panel shows the gain phase vs. time. The vertical red line shows the approximate time of astronomical sunrise.
Paper: A MeerKAT Polarization Survey of Southern Calibration Sources
Authors: A. R. Taylor, L. S. Legodi
Figure caption: The observed polarization position angle vs. frequency for 3C 286 on 2019 August 19 (black dots) and 2020 August 29 (blue dots). The solid black line is the revised model for the polarization position angle of 3C 286 from B. Hugo & Perley (2023, private communication). The red and green dots are the data from 2019 to 2020 with an additional correction to align with the B. Hugo & R. A. Perley (2023, private communication) model (see text).
Paper: A MeerKAT Polarization Survey of Southern Calibration Sources
Authors: A. R. Taylor, L. S. Legodi
Figure caption: The residual x − y phase angle (degrees) measured from the Stokes U and V spectra of J1331+3030 (3C 286). The top panel shows ϕ  xy  vs. frequency for the first run and the bottom panel for the second run. The lines are a linear fit.
Paper: A MeerKAT Polarization Survey of Southern Calibration Sources
Authors: A. R. Taylor, L. S. Legodi
Figure caption: Left panel: the distribution of in-band spectral indices, α. Right panel: the distribution of in-band curvature indices. The blue bars are for sources with spectral index α < −0.5, and the red for α > −0.5.
Paper: Probing the Relationship Between Early Star Formation and CO in the Dwarf Irregular Galaxy WLM with JWST
Authors: Haylee N. Archer, Deidre A. Hunter, Bruce G. Elmegreen, Monica Rubio, Phil Cigan, Rogier A. Windhorst, Juan R. Cortés, Rolf A. Jansen
Figure caption: Top left: mass distribution of type 1 objects (red). Top center: mass distribution of type 2 objects (blue). Top right: mass distribution of type 3 objects (yellow). Bottom left: mass distribution comparing only objects in FUV knots—those near CO (red with circle hatches, type 1) and those away from CO (blue, type 2). Bottom center: mass distribution comparing objects near (red with circle hatches, type 1) and away from CO (green, types 2 and 3), independent of proximity to FUV. Bottom right: mass distribution comparing objects near (purple with star hatches, types 1 and 2) and away from (yellow, type 3) FUV, independent of proximity to CO. We note some bins contain one object and appear only as thicker lines at log(number of objects) = 0. Mass is in units of M ⊙.
Paper: Probing the Relationship Between Early Star Formation and CO in the Dwarf Irregular Galaxy WLM with JWST
Authors: Haylee N. Archer, Deidre A. Hunter, Bruce G. Elmegreen, Monica Rubio, Phil Cigan, Rogier A. Windhorst, Juan R. Cortés, Rolf A. Jansen
Figure caption: Color–color diagrams of F090W–F150W vs. F250M–F430M for all objects (red circles: in FUV knots and near CO; blue circles: in FUV knots and away from CO; and yellow circles: away from FUV knots and away from CO). Objects that overlap 8 μm sources are marked with a  ×  instead of a circle (top), and objects that overlap V-band sources are marked with a ∇ instead of a circle (bottom). A reddening vector of A  V  = 1 assuming SMC-like extinction is included in the upper left of the plot, and the black line shows the effective temperature of a blackbody.