adsabs/AstroCLIMB huggingface dataset:
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 4592.
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: CN distribution (contours) of three group galaxies (NGC 4527, NGC 4536, and NGC 4666) is overlaid on the DSS2 blue images. The contour levels are 30% and 70% of the peak emission (Table 5) for three group galaxies, and the outermost contour corresponds to the 3σ value of each CN map. The yellow cross indicates the stellar disk center. The bar in the bottom-left corner represents the physical scale of 2 kpc. The synthesized beam of the CN data is shown in the bottom-right corner.
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: 3 mm continuum distribution (contours) of four group galaxies (NGC 4527, NGC 4536, NGC 4666, and NGC 4772) is overlaid on the DSS2 blue images. The contour levels are 20, 40, 60, and 80% of the peak emission (Table 6) for three galaxies. For NGC 4666, the contour levels are 40, 60, and 80% of the peak emission (2.4 mJy beam−1). The red cross indicates the stellar disk center. The bar in the bottom-left corner represents the physical scale of 2 kpc. The synthesized beam of the 3 mm continuum data is shown in the bottom-right corner.
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: Deep optical images (the Hyper Surprime-Cam (HSC) r-band wide DR2) of NGC 4632 (left) and NGC 4772 (right) from the HSC Strategic Program (HSC-SSP; Aihara et al. 2019), which are extracted using Aladin Sky Atlas (Bonnarel et al. 2000).
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: Optical images (DSS2 blue) of the galaxies with nondetection of CO in the I1459G and the N4636G. The dashed circle(s) are the primary beam(s) of the ACA observations. The names of the group members in the I1459G are shown in blue color.
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: UGC 08041.
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 4772.
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: UGC 07982.
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 curve and velocity curve of KIC04853067, along with best-fitting contact binary models (magenta: variable-temperature-ratio; green: fixed-temperature-ratio). Individual points represent Kepler photometric data and residuals (upper and middle panels) or spectroscopic measurements (lower panel). Labels denote 16th-, (best) 50th-, 84th-percentile values for the principal model parameters. The components’ line profiles are likely blended and contaminated by third light so that individual velocity amplitudes cannot be measured for this low-inclination extreme-mass-ratio binary.
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 KIC04999357 showing two velocity components. The black dotted curve is the BF, the red curves are two Gaussian components fitted to the BF, the blue curve is the sum of the Gaussian components, and the green x’s represent the model line profile of the best-fitting PHOEBE model. The normalization of both the data and the model 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: 2D contours and 1D histograms depicting the posterior probability distribution for combinations of free parameters for the fixed-temperature-ratio models (left) and variable-temperature-ratio models (right) used to model the KIC04853067 light curve. The inner and outer contours enclose 39% and 86% of the samples, respectively, corresponding to 1σ and 2σ uncertainties for normal distributions, but note the significantly non-Gaussian histograms in each parameter. Degeneracies between temperature ratio and other parameters are prominently visible by the elongated contours in the right panel.
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 KIC06844489. The red curve shows a parabolic fit corresponding to a constant negative period derivative. The green dashed curve shows a sinusoidal fit corresponding to light travel time effects arising from an orbit about a third body.
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 KIC04999357, along with best-fitting PHOEBE model light curves, residuals (model minus data), and velocity curves without irradiation effects (magenta curves) and with irradiation (green curves).
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: 2D contours and 1D histograms depicting the posterior probability distribution for combinations of six free parameters (plus two ancillary derived parameters R 1/﹩{R}_{1\max }﹩ and R 2/﹩{R}_{2\max }﹩) for the detached configuration models of KIC04853067. Model parameters remain well constrained, and most probable values overlap with the fixed-temperature-ratio models indicating low inclination, extreme q, and significant third light.
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 in the KIC04999357 system from the nominal T 2 ≈ T 1 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: Folded Kepler light curve of KIC04999357 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 KIC06844489 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: Broadening function of KIC10292413. The BF does not include light from the third star. The computed BF is noisier than previous examples owing to the faintness of the source. The model line profile function is generated with q = 0.53 (green x’s) while the two-component Gaussian fit to the BF (red curves) suggests q = 0.37.
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: Bayesian probability distribution of KIC09953894 system parameters when modeled as a detached configuration, and a primary mass of M 1 = 1 M ⊙is assumed.
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 curve and velocity curve of KIC10292413, along with a best-fitting contact model.
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 light-curve parameters in the KIC10292413 system, indicating very tight constraints on all 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:  O − C eclipse timing residuals of KIC10292413.
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: Pan-STARRS g/r/i image of the KIC10292413 field with the contact binary source labeled.
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 KIC10292413.
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 residuals of KIC11097678.
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 KIC11097678.
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 1501+106. The meanings of the panels, lines, and histograms are the same as in Figure 3.
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 1351+640. The black dotted and solid lines in panels (d)–(h) are the original and cleaned (e.g., Fe II, He II, narrow Hβ, and [O III]λ λ 4959,5007) mean spectra. The meanings of the other panels, lines, and histograms are the same as in Figure 3.
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 1202+281. The meanings of the panels, lines, and histograms are the same as in Figure 2. In the narrow-line-correct mean spectra in panels (d)–(i).
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 1001+054. The black dotted and solid lines in panels (d)–(h) are the original and cleaned (e.g., Fe II, He II, narrow Hβ, and [O III]λ λ 4959,5007) mean spectra. The meanings of the other 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: Time-series analysis of PG 1211+143. The black dotted and solid lines in panel (d) are the original and cleaned (e.g., Fe II, He II, narrow Hβ, and [O III]λ λ 4959,5007) mean spectra. The meanings of the other panels, lines, and histograms are the same as in Figure 2. Panel (c) is the combined Hβ light curve from Lijiang and CAHA.
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 1310−108. 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: Time-series analysis of PG 1351+695. 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: Time-series analysis of PG 1100+772. 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: Time-series analysis of PG 1048+342. The meanings of the panels, lines, and histograms are the same as in Figure 2.
Paper: Likelihood-free Inference with the Mixture Density Network
Authors: Guo-Jian Wang, Cheng Cheng, Yin-Zhe Ma, Jun-Qing Xia
Figure caption: Mean deviations between the MDN results and the fiducial values as a function of the number of hidden layers, the number of training samples, the number of epochs, and the activation function.