adsabs/AstroCLIMB huggingface dataset:
Paper: AspGap: Augmented Stellar Parameters and Abundances for 37 Million Red Giant Branch Stars from Gaia XP Low-resolution Spectra
Authors: Jiadong Li, 佳东 李, Kaze W. K. Wong, David W. Hogg, Hans-Walter Rix, Vedant Chandra
Figure caption: The left panel shows the two-dimensional distribution of the median Galactocentric Cartesian X position vs. the Cartesian Y position for Gaia XP. On the right panel, a similar two-dimensional distribution is displayed for APOGEE data. By utilizing the sample provided by XP, we can assess whether the larger and all-sky Gaia XP sample covers the same physical extent as the APOGEE data.
Paper: AspGap: Augmented Stellar Parameters and Abundances for 37 Million Red Giant Branch Stars from Gaia XP Low-resolution Spectra
Authors: Jiadong Li, 佳东 李, Kaze W. K. Wong, David W. Hogg, Hans-Walter Rix, Vedant Chandra
Figure caption: Validation of AspGap-derived labels from Gaia XP spectra (XP) vs. APOGEE labels (AP). This figure is analogous to Figure 5, except that the color coding now denotes AspGap's estimate of the label prediction’s uncertainty. Most objects with more discrepant AspGap vs. APOGEE label estimates have correctly identified larger AspGap label uncertainties.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: The [Fe/H] (left panel) and [α/Fe] (right panel) calibrations between the APOGEE and LAMOST data sets. The dashed black lines represent the one-to-one relations, and the solid red lines are linear fits to the data. There is a minimum of four stars per bin, with [Fe/H] and [α/Fe] spaced in 0.02 and 0.02 dex, respectively.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: Spatial distribution in the R–Z plane of the sample stars, color coded by the stellar number density. There is a minimum of eight stars per bin, spaced 0.1 kpc in both axes.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: The Δ[Fe/H]/ΔR as a a function of the ∣Z∣ of the thin (upper left) and thick (upper right) disks, and the Δ[Fe/H]/Δ∣Z∣ as a function of the R of the thin (bottom left) and thick (bottom right) disks.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: Metallicity gradients of the azimuthal velocity (left panel) and azimuthal velocity dispersion (right panel) as a function of R and Z.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: Fractional number density (f = N  i /N tot) distributions of the vertical direction (upper left), radial direction (upper right), [Fe/H] (bottom left), and V  ϕ  (bottom right) for the thin and thick disks. N  i  is the number of stars in the ith radial/vertical bin, and N tot is the total number of stars of the individual populations. The different color lines represent different populations, which are marked as labeled in the top corner.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: Metallicity distribution in the R–Z plane of the thin (left panel) and thick (right panel) disks.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: Radial (upper panels) and vertical (bottom panels) metallicity profiles of the thin (left panels) and thick (right panels) disks.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: Histograms of the eccentricities for the thin- (blue line) and thick-disk (orange line) stars in different [α/Fe] bins, as indicated in the legend of each panel. The [α/Fe] range increases from panels (a) to (e).
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: The corrected vertical metallicity gradient as a function of R for the thin (left panel) and thick (right panel) disks.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: The [Fe/H]−[α/Fe] distribution of the final sample stars, overplotted with contours of equal densities, color coded by the logarithmic number density. The horizontal and vertical axis are spaced by 0.025 and 0.02 dex, respectively, with a minimum of 15 stars per bin. The two dashed lines are used to separate thick- (above the lines) and thin- (below the lines) disk stars.
Paper: Mapping the Chemodynamics of the Galactic Disk Using the LAMOST and APOGEE Red Clump Stars
Authors: Weixiang Sun, Han Shen, Biwei Jiang, Xiaowei Liu
Figure caption: The [α/Fe]–velocity dispersion for the metal-poor (left panel) and metal-rich (right panel) populations.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Color composite of Hα (red), [O III] λ5007 (blue), and broad RGB images of the G13.3-1.3 remnant. Only the short line of red filaments seen here along the remnant’s southeastern region were known previously.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Top: wide FOV [O III] image of the G13.3-1.3 now shown in Galactic coordinates. Bottom: cropped [O III] image with colored 11 cm (left) and 21 cm (right) radio overlays showing the coincidence of the remnant’s bright [O III] filaments with the remnant’s radio emission with fainter filaments outlining the radio extension toward l = 14°.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Close-up views of G13.3-1.3's unusual [O III] λ5007 emission filaments. Top: [O III] emission image plus broadband RGB filters. Bottom: higher-resolution MDM [O III] image showing finer filament details.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: MDW 9.°5 × 8.°5 Hα image of G70.0-21.5 showing the region and orientation of our images (black box).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Same data as in Figure 8 for G82.2+5.3 (W63) but now shown as positive images with the stars removed by software to make the remnant’s Hα (top) and [O III] (bottom) emissions and dust features more readily visible. Note the extensive [O III] emission to the west and southwest of the remnant’s prominent emission shell.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Top panels: Hα and [O III] images of G89.0+4.7 (HB 21) with overlay of WENSS 92 cm radio intensity contours. Bottom: our [O III] image plus RGB images of G89.0+4.7's northern and western emission filaments.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Optical [O III] λ5007, radio 4.8 GHz, and color optical/radio composite images of G82.2+5.3 (W63) showing positional overlap of western and southern emissions features outside of main remnant shell.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Hα and [O III] images of the central regions of G70.0-21.5 along with a matching color composite image.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Color composite of Hα (red), [O III] λ5007 (blue), and broad RGB images of the G70.0-21.5 remnant. Image FOV is 5.°2 × 6.°2. North is up, and east is to the left.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Close-up of the Hα and [O III] λ5007 filter images plus color composite for the northeastern limb of G70.0-21.5.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Top: Hα image of G82.2+5.3 (W63). Bottom: [O III] λ5007 image of G82.2+5.3 (W63).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Hα and [O III] images of G89.0+4.7 (HB 21). The bright star in the lower right is 51 Cyg.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: A color composite formed from Hα (red) and [O III] λ5007 (blue) images of G82.2+5.3 (W63).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Top: color composite made from [O III] (blue) and Hα (red) plus broad RGB images of G150.3+4.5. North is up, and east is to the left. Bottom: enlargement of a section along the remnant’s northwestern limb showing an [O III] emission shell centered on the variable X-ray binary B[e] star, CI Camelopardalis (CI Cam).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Same data as in Figure 14 on CTA 1 (G119.5+10.2) but now shown as a positive images with the stars removed by software to make the remnant’s Hα (top) and [O III] (bottom) emission features more readily visible.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: The left panel our [O III] + RBG image of G150.3+4.5 displayed in Galactic coordinates, with the right panel showing an overlay of the remnant’s color-coded 6 cm radio emission and brightness contours from Gao & Han (2014).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Composite [O III] and Hα plus RGB images of the southern limb of G150.3+4.5 showing both the presence of sharp [O III] filaments along with scattered emission extending farther to the south, and the lack of associated filamentary Hα.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Hα and [O III] images of CTA 1 (G119.5+10.2).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Color composite of CTA 1 (G119.5+102) with Hα (red) and [O III] (blue) emissions along with RGB images. The top panel shows the entire remnant as imaged. The bottom panel is a blowup of its southern region. North is up, and east is to the left.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Top panels: deep Hα and [O III] images of the faint radio SNR G181.1+9.5. Bottom panels: same images but now with stars removed using software.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Composite [O III] plus RGB images of G150.3+4.5. Note the appearance of several dust clouds in the region.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Effelsberg 6 cm image of G181.1+9.5 (Kothes et al. 2017).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Matching 3.°2 × 3.°2 Hα and [O III] images of the large Nereides SNR G107.7-5.1.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Top: comparison of optical [O III] emission vs. radio SUMSS 843 MHz emission in Galactic coordinates. Bottom: color composite of the SNR G321.3-3.9. Blue: [O III], red: [S II], yellow: Hα. North is up, and east is to the left.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Top: deep [O III] image (left) and composite [O III]+Hα (right) images of the SNR G288.8-6.3. Bottom: color composite of [O III], Hα + RGB images of the G288.8-6.3 SNR.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: A 14.°7 × 12.°4 MDW Hα mosaic image covering the area around SNR G181.1+9.5 showing the appearance of a faint and incomplete Hα emission shell roughly 9.°0 in diameter. If it is an unrecognized SNR, it would be called G181.3+12.1.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: [O III] image of G288.8-6.3 with 943 MHz radio emission contours adapted from Filipović et al. (2023).
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Enlargement of [O III] image of G321.3-3.9 highlighting a northern and a large western shock “breakout.”
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Color Hα, [O III], and RGB composite image of SNR G181.1+9.5.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: MDM [O III] and Hα images of G181.1+9.5's northwestern (top) and western (bottom) regions.
Paper: Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Authors: Robert A. Fesen, Marcel Drechsler, Xavier Strottner, Bray Falls, Yann Sainty, Nicolas Martino, Richard Galli, Mathew Ludgate, Markus Blauensteiner, Wolfgang Reich, Sean Walker, Dennis di Cicco, David Mittelman, Curtis Morgan, Aziz Ettahar Kaeouach, Justin Rupert, Zouhair Benkhaldoun
Figure caption: Matching Hα and [O III] images of the SNR G321.3-3.9.
Paper: Sample and Statistical Analysis on NEOWISE Variability of ATLASGAL Sources
Authors: Ying Lu, Xi Chen, Shi-Min Song, Jun-Ting Liu, Tian Yang, You-Xin Wang, Yan-Kun Zhang, Shi-Jie Zhang
Figure caption: Cumulative distribution of fitted period and fractional amplitude for all the sin and sin+linear variables. The blue and orange solid curves represent the sin and sin+linear types. The p-values from the K-S tests are presented in each panel.
Paper: Sample and Statistical Analysis on NEOWISE Variability of ATLASGAL Sources
Authors: Ying Lu, Xi Chen, Shi-Min Song, Jun-Ting Liu, Tian Yang, You-Xin Wang, Yan-Kun Zhang, Shi-Jie Zhang
Figure caption: Comparison of the cumulative distributions of physical parameters of different types of variables and nonvariables in three evolutionary stages. The displayed distributions correspond to the protostellar, YSO, and H II region stages from left to right. Dust temperature, bolometric luminosity, volume density, radius, and mass distributions are shown from top to bottom. Among them, the statistics in the top three rows are based on all sample sources, while the statistics in the bottom two rows are based on the samples after applying a distance restriction (2–4 kpc) described in Urquhart et al. (2022). The blue, orange, and green solid curves represent the secular variables, stochastic variables, and nonvariables. The p-values from the K-S tests are presented in each panel.