adsabs/AstroCLIMB huggingface dataset:
Paper: Accurate Distances of Massive Young Stars in the Scutum Spiral Arm
Authors: J. J. Li, K. Immer, M. J. Reid, A. Sanna, K. L. J. Rygl, Y. Xu, B. Zhang, A. Brunthaler, K. M. Menten
Figure caption: Parallax and proper-motion data and fits for G031.28+00.06. Plotted are position offsets for six maser spots at V LSR = 105.7 (red triangles), 106.0 (green triangles), 107.5 (blue triangles), 110.0 (cyan triangles), 110.7 (yellow triangles), and 111.1 (magenta triangles) km s−1 and two maser spots (red and green squares) at 110.4 km s−1, calibrated relative to the background sources J1834−0301, J1846−0003, J1853−0048, and J1857−0048. A description of the three panels is given in the caption for Figure 1.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Broadening function of KIC06844489 showing three probable spectral components. The black dotted curve is the BF, the red curves are Gaussian components, the blue curve is the sum of the Gaussian components, and the green x’s represent the model velocity profile of the best-fitting PHOEBE model (which does not include a tertiary). The normalization of both the BF and model velocity profile is arbitrary.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Three competing PHOEBE models for KIC08913061 in comparison to the light curve and velocity data. The nominal variable-temperature-ratio model (magenta) indicates q ≈ 4, in marked disagreement with the velocity curve, while either of the T 2/T 1 = 1 models yields approximately the correct mass ratio.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Posterior probability distributions for combinations of seven free system parameters for the KIC08913061 system, including a hotspot on the primary. There is considerable degeneracy among i, q, and l3, but the models still place strong constraints on the system parameters.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Posterior probability distributions for combinations of five free system parameters from the T 2 ≈ T 1 models for the KIC06844489 system.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Folded light-curve and velocity measurements of KIC06844489, along with best-fitting PHOEBE model light curve, light-curve residuals, and velocity curve.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Broadening function of KIC08913061 showing two distinct components with very disparate luminosities.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Posterior probability distributions for combinations of four free system parameters for the KIC08913061 system when T 2/T 1 = 1.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Folded Kepler light curve of KIC08913061 and mean light-curve shape (red curve) generated from the sum of low-order Fourier coefficients.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Folded Kepler light curve of KIC09164694.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Broadening function and model line profile function of KIC09840412. The discrepancy between the BF and the model line profile (green x’s) suggests substantial third-light contribution, an inference also supported by the light-curve modeling.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Three competing model light curves and velocity curves in comparison to the data of the detached system KIC09953894.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Broadening function and model line profile of KIC09953894. The green x’s are for the best-fitting detached model including irradiation, which significantly underpredicts the velocity semiamplitudes unless the spectroscopically determined M 1 = 1.3 M ⊙ is used in place of the default M 1 = 1 M ⊙.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: O-C eclipse timing residuals of KIC09840412, including one epoch of recent ZTF photometry.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Posterior probability distribution for combinations of five parameters in the KIC09840412 system.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Light curves and velocity curves of KIC09840412, along with best-fitting contact binary models.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Posterior probability distributions for combinations of seven parameters in the KIC09345838 system when a hot spot on the primary is included.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Folded Kepler light curve of the detached system KIC09953894.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Folded Kepler light curve of KIC09840412.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Mass ratio vs. orbital period as in Figure 63. The colored tracks show the evolution of contact binaries—from upper left toward lower right—of contact systems with initial mass ratios q ini = 0.1–0.9, as labeled. Diamonds mark equal time intervals every 2 Gyr. Decreasing/increasing the total system mass shifts models slightly to the left/right, as indicated by arrows.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: 50th-percentile absolute mass ratios q a vs. P for probable contact binaries and ambiguous systems.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: The power-law index α relating the change in size of the primary star to its changing mass as a function of mass ratio. The solid black line is α RL, the change in the equivalent Roche lobe radius. The red dashed and green dotted–dashed lines mark α MS, the indices for equilibrium main-sequence stars at 1 Gy age and mass 0.9 and 1.3 M ⊙, respectively. Stable accretion onto the primary can occur where α RL > α MS.
Paper: A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
Authors: Henry A. Kobulnicky, Lawrence A. Molnar, Evan M. Cook, Lauren E. Henderson
Figure caption: Differences or ratios of 50th-percentile parameters comparing detached models and the T 2 ≈ T 1 contact models for the 114 probable detached binaries. Parameters from best detached model can be very different from the best contact model.
Paper: Monitoring AGNs with Hβ Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar–Green Quasars
Authors: Dong-Wei Bao, Michael S. Brotherton, Pu Du, Jacob N. McLane, T. E. Zastrocky, Kianna A. Olson, Feng-Na Fang, Shuo Zhai, Zheng-Peng Huang, Kai Wang, Bi-Xuan Zhao, Sha-Sha Li, Sen Yang, Yong-Jie Chen, Jun-Rong Liu, Zhu-Heng Yao, Yue-Chang Peng, Wei-Jian Guo, Yu-Yang Songsheng, Yan-Rong Li, Bo-Wei Jiang, David H. Kasper, William T. Chick, My L. Nguyen, Jaya Maithil, H. A. Kobulnicky, D. A. Dale, Derek Hand, C. Adelman, Z. Carter, A. M. Murphree, M. Oeur, S. Schonsberg, T. Roth, Hartmut Winkler, Paola Marziani, Mauro D'Onofrio, Chen Hu, Ming Xiao, Suijian Xue, Bożena Czerny, Jesús Aceituno, Luis C. Ho, Jin-Ming Bai, Jian-Min Wang
Figure caption: Time-series analysis of PG 1613+658. The meanings of the panels, lines, and histograms are the same as in Figure 2.
Paper: Monitoring AGNs with Hβ Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar–Green Quasars
Authors: Dong-Wei Bao, Michael S. Brotherton, Pu Du, Jacob N. McLane, T. E. Zastrocky, Kianna A. Olson, Feng-Na Fang, Shuo Zhai, Zheng-Peng Huang, Kai Wang, Bi-Xuan Zhao, Sha-Sha Li, Sen Yang, Yong-Jie Chen, Jun-Rong Liu, Zhu-Heng Yao, Yue-Chang Peng, Wei-Jian Guo, Yu-Yang Songsheng, Yan-Rong Li, Bo-Wei Jiang, David H. Kasper, William T. Chick, My L. Nguyen, Jaya Maithil, H. A. Kobulnicky, D. A. Dale, Derek Hand, C. Adelman, Z. Carter, A. M. Murphree, M. Oeur, S. Schonsberg, T. Roth, Hartmut Winkler, Paola Marziani, Mauro D'Onofrio, Chen Hu, Ming Xiao, Suijian Xue, Bożena Czerny, Jesús Aceituno, Luis C. Ho, Jin-Ming Bai, Jian-Min Wang
Figure caption: Velocity-resolved lags. The upper subpanel in each panel is the velocity-resolved lags, and the lower subpanel is the rms or mean spectrum. The horizontal dash lines and yellow horizontal spans are the mean time lags and their uncertainties. The vertical dashed lines mark the edges of the velocity bins. The peak correlation coefficient is denoted in each bin at the top subpanels.
Paper: Monitoring AGNs with Hβ Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar–Green Quasars
Authors: Dong-Wei Bao, Michael S. Brotherton, Pu Du, Jacob N. McLane, T. E. Zastrocky, Kianna A. Olson, Feng-Na Fang, Shuo Zhai, Zheng-Peng Huang, Kai Wang, Bi-Xuan Zhao, Sha-Sha Li, Sen Yang, Yong-Jie Chen, Jun-Rong Liu, Zhu-Heng Yao, Yue-Chang Peng, Wei-Jian Guo, Yu-Yang Songsheng, Yan-Rong Li, Bo-Wei Jiang, David H. Kasper, William T. Chick, My L. Nguyen, Jaya Maithil, H. A. Kobulnicky, D. A. Dale, Derek Hand, C. Adelman, Z. Carter, A. M. Murphree, M. Oeur, S. Schonsberg, T. Roth, Hartmut Winkler, Paola Marziani, Mauro D'Onofrio, Chen Hu, Ming Xiao, Suijian Xue, Bożena Czerny, Jesús Aceituno, Luis C. Ho, Jin-Ming Bai, Jian-Min Wang
Figure caption: Pairwise correlations between the measurements from ICCF, χ 2, and MICA. The points in the same color are the time lags of different seasons (and the entire light curve) for individual objects.
Paper: Monitoring AGNs with Hβ Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar–Green Quasars
Authors: Dong-Wei Bao, Michael S. Brotherton, Pu Du, Jacob N. McLane, T. E. Zastrocky, Kianna A. Olson, Feng-Na Fang, Shuo Zhai, Zheng-Peng Huang, Kai Wang, Bi-Xuan Zhao, Sha-Sha Li, Sen Yang, Yong-Jie Chen, Jun-Rong Liu, Zhu-Heng Yao, Yue-Chang Peng, Wei-Jian Guo, Yu-Yang Songsheng, Yan-Rong Li, Bo-Wei Jiang, David H. Kasper, William T. Chick, My L. Nguyen, Jaya Maithil, H. A. Kobulnicky, D. A. Dale, Derek Hand, C. Adelman, Z. Carter, A. M. Murphree, M. Oeur, S. Schonsberg, T. Roth, Hartmut Winkler, Paola Marziani, Mauro D'Onofrio, Chen Hu, Ming Xiao, Suijian Xue, Bożena Czerny, Jesús Aceituno, Luis C. Ho, Jin-Ming Bai, Jian-Min Wang
Figure caption: Time-series analysis of PG 1534+580. The meanings of the panels, lines, and histograms are the same as in Figure 2.
Paper: Simulating the Legacy Survey of Space and Time Stellar Content with TRILEGAL 
Authors: Piero Dal Tio, Giada Pastorelli, Alessandro Mazzi, Michele Trabucchi, Guglielmo Costa, Alice Jacques, Adriano Pieres, Léo Girardi, Yang Chen, Knut A. G. Olsen, Mario Juric, Željko Ivezić, Peter Yoachim, William I. Clarkson, Paola Marigo, Thaise S. Rodrigues, Simone Zaggia, Mauro Barbieri, Yazan Momany, Alessandro Bressan, Robert Nikutta, Luiz Nicolaci da Costa
Figure caption: Top panel: LFs in the r band for stars within 5° of the SGP, for both single and binary stars (that is, for the f bin = 0 and f bin = 1 simulations, respectively). The bottom panel shows the ratio between the f bin = 1 and f bin = 0 simulation. In addition, both panels present the real LFs derived from DES data, to be discussed in Section 4.1 below: one of them is more conservative (EXT_COADD = 0), and the other one more complete (EXT_COADD = [0,1]). For the sake of comparison, the gray shaded area shows the Poisson noise expected in the case of single stars; this noise becomes negligible in the magnitude interval covered by the DES data.
Paper: Simulating the Legacy Survey of Space and Time Stellar Content with TRILEGAL 
Authors: Piero Dal Tio, Giada Pastorelli, Alessandro Mazzi, Michele Trabucchi, Guglielmo Costa, Alice Jacques, Adriano Pieres, Léo Girardi, Yang Chen, Knut A. G. Olsen, Mario Juric, Željko Ivezić, Peter Yoachim, William I. Clarkson, Paola Marigo, Thaise S. Rodrigues, Simone Zaggia, Mauro Barbieri, Yazan Momany, Alessandro Bressan, Robert Nikutta, Luiz Nicolaci da Costa
Figure caption: CMD (r vs. g − r) of the simulated number density per mag2 of the Magellanic Clouds (LMC and SMC, left and right panels, respectively) and the corresponding MW foreground. These are Hess diagrams, with the color scale illustrating the counts of stars in small color–magnitude bins. In the less populated regions of the CMD these stellar densities are replaced by a simple scatter plot of the simulated stars. The MW foreground appears mainly as two almost-vertical features: a marked one at g − r ≃ 1.5, and a more diffuse one located just redward of g − r = 0.3 mag (partially overlapping the He-burning and main sequences of the Magellanic Clouds).
Paper: Simulating the Legacy Survey of Space and Time Stellar Content with TRILEGAL 
Authors: Piero Dal Tio, Giada Pastorelli, Alessandro Mazzi, Michele Trabucchi, Guglielmo Costa, Alice Jacques, Adriano Pieres, Léo Girardi, Yang Chen, Knut A. G. Olsen, Mario Juric, Željko Ivezić, Peter Yoachim, William I. Clarkson, Paola Marigo, Thaise S. Rodrigues, Simone Zaggia, Mauro Barbieri, Yazan Momany, Alessandro Bressan, Robert Nikutta, Luiz Nicolaci da Costa
Figure caption: The two maps that define how the sky is split into smaller areas: the extinction map derived from (Planck Collaboration et al. 2014, top panel) and the surface mass density derived from the Girardi et al. (2012) calibration of TRILEGAL (bottom panel).
Paper: Simulating the Legacy Survey of Space and Time Stellar Content with TRILEGAL 
Authors: Piero Dal Tio, Giada Pastorelli, Alessandro Mazzi, Michele Trabucchi, Guglielmo Costa, Alice Jacques, Adriano Pieres, Léo Girardi, Yang Chen, Knut A. G. Olsen, Mario Juric, Željko Ivezić, Peter Yoachim, William I. Clarkson, Paola Marigo, Thaise S. Rodrigues, Simone Zaggia, Mauro Barbieri, Yazan Momany, Alessandro Bressan, Robert Nikutta, Luiz Nicolaci da Costa
Figure caption: Top-left panel shows the CMD (or Hess diagram) for all simulated single stars in the n side = 64 pixels whose centers lie within 5° of the South Galactic Pole (SGP). Subsequent panels present their distributions of surface gravity, initial mass, Galactic components, distances, metallicity, and evolutionary phase.
Paper: Simulating the Legacy Survey of Space and Time Stellar Content with TRILEGAL 
Authors: Piero Dal Tio, Giada Pastorelli, Alessandro Mazzi, Michele Trabucchi, Guglielmo Costa, Alice Jacques, Adriano Pieres, Léo Girardi, Yang Chen, Knut A. G. Olsen, Mario Juric, Željko Ivezić, Peter Yoachim, William I. Clarkson, Paola Marigo, Thaise S. Rodrigues, Simone Zaggia, Mauro Barbieri, Yazan Momany, Alessandro Bressan, Robert Nikutta, Luiz Nicolaci da Costa
Figure caption: Stellar density (star counts at r < 27.5 mag per square degree) in the LSST simulation with f bin = 0, in both equatorial and Galactic coordinates (Aitoff projection).
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 4536.
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 4527.
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 7421.
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 4666.
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 4496.
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 7418.
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 4632.
Paper: ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
Authors: Bumhyun Lee, Jing Wang, Aeree Chung, Luis C. Ho, Ran Wang, Tomonari Michiyama, Juan Molina, Yongjung Kim, Li Shao, Virginia Kilborn, Shun Wang, Xuchen Lin, Dawoon E. Kim, Barbara Catinella, Luca Cortese, Nathan Deg, Helga Denes, Ahmed Elagali, Bi-Qing For, Dane Kleiner, Bärbel S. Koribalski, Karen Lee-Waddell, Jonghwan Rhee, Kristine Spekkens, Tobias Westmeier, O. Ivy Wong, Frank Bigiel, Albert Bosma, Benne W. Holwerda, Jan M. van der Hulst, Sambit Roychowdhury, Lourdes Verdes-Montenegro, Martin A. Zwaan
Figure caption: NGC 4517.