adsabs/AstroCLIMB huggingface dataset:
Paper: Physical Parameters and Chromospheric Activity of Eclipsing Binaries Observed by the LAMOST DR10 Survey
Authors: Ansong Shi, Li-yun Zhang, Tianhao Su, Yinpeng Wang, Qi An, Xianming L. Han, Prabhakar Misra, Linyan Jiang, Rui Guo, Qingfeng Pi
Figure caption: The left and right panels show the flare amplitude as a function of Teff and stellar mass, respectively, for EA, EB, and EW subtypes. Power-law fits suggest a declining flare contrast with increasing Teff and mass.
Paper: Physical Parameters and Chromospheric Activity of Eclipsing Binaries Observed by the LAMOST DR10 Survey
Authors: Ansong Shi, Li-yun Zhang, Tianhao Su, Yinpeng Wang, Qi An, Xianming L. Han, Prabhakar Misra, Linyan Jiang, Rui Guo, Qingfeng Pi
Figure caption: Left panel: flare duration vs. bolometric flare energy. Right panel: flare energy vs. amplitude. The EA, EB, and EW types are shown separately. Longer flares tend to be more energetic, and higher amplitude events generally release more energy.
Paper: Physical Parameters and Chromospheric Activity of Eclipsing Binaries Observed by the LAMOST DR10 Survey
Authors: Ansong Shi, Li-yun Zhang, Tianhao Su, Yinpeng Wang, Qi An, Xianming L. Han, Prabhakar Misra, Linyan Jiang, Rui Guo, Qingfeng Pi
Figure caption: The position distribution for EA (left), EB (middle), and EW (right) systems in the future LAMOST survey, where the color represents the number density of the corresponding eclipsing binaries.
Paper: Proper Motion of Dense Circumstellar Knots in the Supernova Remnant Cassiopeia A
Authors: Bon-Chul Koo, Sang Bum Ko, Christopher F. McKee, Carl Heiles, Robert A. Fesen, Ji Yeon Seok, Hyun-Jeong Kim, Sung-Chul Yoon
Figure caption: (Left) A deep [Fe II]+[Si I] 1.64 μm image of Cas A (B.-C. Koo et al. 2018). QSFs with optical counterparts are highlighted with magenta contours. The filled red star symbol indicates the explosion center at (α, δ)J2000 = (23h23m27.77s, +58◦48′49.4) (J. R. Thorstensen et al. 2001), while the yellow contour marks the outer boundary of the SNR in radio in September 2000 (T. A. DeLaney 2004). North is up, and east is to the left. The white boxes represent 11 fields used for measuring proper motion of QSFs (see Section 2). (Right) An Hα image of Cas A, taken with GMOS on the Gemini North telescope in 2019. The white contours show the location of the main ejecta shell in the deep [Fe II]+[Si I] image.
Paper: Proper Motion of Dense Circumstellar Knots in the Supernova Remnant Cassiopeia A
Authors: Bon-Chul Koo, Sang Bum Ko, Christopher F. McKee, Carl Heiles, Robert A. Fesen, Ji Yeon Seok, Hyun-Jeong Kim, Sung-Chul Yoon
Figure caption: Sample QSFs illustrating typical proper-motion results: Knots 1 and 2, 21, 24, 46, and 102 from top to bottom. For each QSF, three frames are presented: (Left) A 2004 HST F625W image of the QSF with proper-motion vectors overlaid in cyan. The red contours indicate the boundary of the QSF. (Middle) A 2019 HST F625W image with the red contours from the 2004 image overlaid. The red arrow indicates the radial direction from the explosion center. (Right) A Gemini Hα image of the QSF with red contours from the 2004 image overlaid. The image was obtained in 2019 with an angular resolution of 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩6 and has been regridded to match the HST images. In each frame, north is up, and east is to the left. At the distance of Cas A (3.4 kpc), 2″ corresponds to 0.033 pc. A full set of proper-motion maps of 36 QSFs is listed in Figure 11.
Paper: AllBRICQS: The Discovery of Luminous Quasars in the Northern Hemisphere
Authors: Yunyi Choi, Yuming Fu, Myungshin Im, Xue-Bing Wu, Christopher A. Onken, Christian Wolf, Seo-Won Chang, Hyeonho Choi, Mankeun Jeong, Yongjung Kim, Gu Lim, Yuxuan Pang, Taewan Kim, Jubee Sohn, Dohyeong Kim, Ji Hoon Kim, Eunhee Ko, Gregory S. H. Paek, Sungho Jung
Figure caption: Distributions of key properties of the spectroscopically observed 75 sources in this study. The histograms, displayed from left to right, show Gaia RP magnitude, W1 − W2 color, measured redshift, and Galactic latitude. The W1 − W2 color cut at 0.2 is indicated by a black dashed line. The color values are primarily sourced from the CatWISE catalog (P. R. M. Eisenhardt et al. 2020; F. Marocco et al. 2021) and supplemented with AllWISE (https://wise2.ipac.caltech.edu/docs/release/allwise/expsup/index.html) when CatWISE values are unavailable. Although the original AllBRICQS selection used AllWISE magnitudes, the color values shown here are based on CatWISE to reflect the intended selection methodology. As a result, a few objects appear below the 0.2 cut, since they were selected using AllWISE but would not have satisfied the cut under CatWISE photometry. With the exception of redshift, all other properties are derived from Gaia DR3 (Gaia Collaboration et al. 2016, 2021).
Paper: AllBRICQS: The Discovery of Luminous Quasars in the Northern Hemisphere
Authors: Yunyi Choi, Yuming Fu, Myungshin Im, Xue-Bing Wu, Christopher A. Onken, Christian Wolf, Seo-Won Chang, Hyeonho Choi, Mankeun Jeong, Yongjung Kim, Gu Lim, Yuxuan Pang, Taewan Kim, Jubee Sohn, Dohyeong Kim, Ji Hoon Kim, Eunhee Ko, Gregory S. H. Paek, Sungho Jung
Figure caption: Distribution of RP − W1 and W1 − W2 colors as a function of redshift. The shaded regions along the central dashed lines represent the mean color trends and the 1σ scatter within redshift bins of width 0.2. The red shaded region corresponds to our newly discovered 62 quasars, while the black shaded region corresponds to 319 SDSS DR16Q quasars (B. W. Lyke et al. 2020) that satisfy our bright selection criteria (BP < 16.5 or RP < 16.0 mag). Redshift bins in the SDSS sample containing only a single data point within z < 2.0 were excluded. Red pentagons denote the 18 quasars located within the SDSS footprint.
Paper: AllBRICQS: The Discovery of Luminous Quasars in the Northern Hemisphere
Authors: Yunyi Choi, Yuming Fu, Myungshin Im, Xue-Bing Wu, Christopher A. Onken, Christian Wolf, Seo-Won Chang, Hyeonho Choi, Mankeun Jeong, Yongjung Kim, Gu Lim, Yuxuan Pang, Taewan Kim, Jubee Sohn, Dohyeong Kim, Ji Hoon Kim, Eunhee Ko, Gregory S. H. Paek, Sungho Jung
Figure caption: Distribution of the 75 observed sources in the AllBRICQS sample, with all astrometric properties derived from Gaia DR3 (Gaia Collaboration et al. 2016, 2021). (Left) Histogram of the parallax-to-error ratio, ϖ/σϖ. Quasars (red) do not exceed a value of 2.0, with many exhibiting negative values, which correspond to near-zero parallaxes in reality (see Section 5.2 and Figure 6 of L. Lindegren et al. 2018). Stars (navy) all have ϖ/σϖ > 1.5. (Right) Scatter plot of proper motion  μ vs. parallax-to-error ratio. The dashed lines indicate the newly proposed stringent criteria for quasar selection.
Paper: AllBRICQS: The Discovery of Luminous Quasars in the Northern Hemisphere
Authors: Yunyi Choi, Yuming Fu, Myungshin Im, Xue-Bing Wu, Christopher A. Onken, Christian Wolf, Seo-Won Chang, Hyeonho Choi, Mankeun Jeong, Yongjung Kim, Gu Lim, Yuxuan Pang, Taewan Kim, Jubee Sohn, Dohyeong Kim, Ji Hoon Kim, Eunhee Ko, Gregory S. H. Paek, Sungho Jung
Figure caption: Distribution of redshift and bolometric luminosity for AllBRICQS quasars in this work (Northern Hemisphere; filled red circles) and from C. A. Onken et al. (2023) (Southern Hemisphere; open blue triangles), in comparison to SDSS DR16Q (B. W. Lyke et al. 2020), shown as gray contours. The AllBRICQS quasars occupy the bright end of the quasar luminosity distribution, exhibiting significantly higher luminosities than the bulk of the SDSS DR16Q sample. The gray contours correspond to a two-dimensional histogram constructed using 10,000 bins (100 bins per axis), effectively illustrating the density distribution of the SDSS quasars.
Paper: AllBRICQS: The Discovery of Luminous Quasars in the Northern Hemisphere
Authors: Yunyi Choi, Yuming Fu, Myungshin Im, Xue-Bing Wu, Christopher A. Onken, Christian Wolf, Seo-Won Chang, Hyeonho Choi, Mankeun Jeong, Yongjung Kim, Gu Lim, Yuxuan Pang, Taewan Kim, Jubee Sohn, Dohyeong Kim, Ji Hoon Kim, Eunhee Ko, Gregory S. H. Paek, Sungho Jung
Figure caption: Comparison of redshift measurements between AllBRICQS spectroscopic values and Quaia photometric estimates. The x-axis represents the spectroscopic redshifts obtained from AllBRICQS observations, while the y-axis shows the corresponding photometric redshift estimates from the Quaia catalog.
Paper: AllBRICQS: The Discovery of Luminous Quasars in the Northern Hemisphere
Authors: Yunyi Choi, Yuming Fu, Myungshin Im, Xue-Bing Wu, Christopher A. Onken, Christian Wolf, Seo-Won Chang, Hyeonho Choi, Mankeun Jeong, Yongjung Kim, Gu Lim, Yuxuan Pang, Taewan Kim, Jubee Sohn, Dohyeong Kim, Ji Hoon Kim, Eunhee Ko, Gregory S. H. Paek, Sungho Jung
Figure caption: The sky positions of the 75 observed targets are overplotted on the SDSS footprint. Red points with yellow outlines indicate the observed sources. The red and blue dashed lines represent Galactic latitudes of b = 0° and b = ±10°, respectively.
Paper: Comprehensive Analysis of NGC 6134: Structure, Dynamics, and Blue Straggler Star Candidates
Authors: Dexin Zeng, Ying Mei, Huanbin Chi, Hui Deng, Feng Wang
Figure caption: Three-dimensional Galactic orbit of the open cluster NGC 6134, integrated backward for 1.20954 Gyr using the MWPotential2014 potential from galpy. The red point labeled now marks the present-day position of the cluster, while the green point labeled birth indicates its inferred birthplace corresponding to the cluster’s age of log(age/yr) = 9.1683. This visualization helps assess the cluster’s origin and vertical oscillation through the Galactic disk.
Paper: Comprehensive Analysis of NGC 6134: Structure, Dynamics, and Blue Straggler Star Candidates
Authors: Dexin Zeng, Ying Mei, Huanbin Chi, Hui Deng, Feng Wang
Figure caption: Present-day mass function (PDMF) of NGC 6134 for the sample including all stellar populations. The PDMF shows a break at ﹩{\mathrm{log}}\,(M/{M}_{\odot })=-0.02\pm 0.02﹩, with slopes αA = −1.61 ± 0.31 (low-mass regime, ﹩{\mathrm{log}}\,(M/{M}_{\odot })\lt -0.05﹩) and αB = 2.09 ± 0.12 (high-mass regime). A drop at ﹩{\mathrm{log}}\,(M/{M}_{\odot })\approx -0.2﹩ may be due to completeness biases (see text).
Paper: Comprehensive Analysis of NGC 6134: Structure, Dynamics, and Blue Straggler Star Candidates
Authors: Dexin Zeng, Ying Mei, Huanbin Chi, Hui Deng, Feng Wang
Figure caption: Left: isochrone fit for NGC 6134, with black points representing member stars, the red isochrone corresponding to the mean of the posterior distribution, and the blue and green isochrones indicating the lower and upper limits of parameter uncertainties, respectively. Right: marginalized posterior distributions and associated uncertainties of model parameters from the PARSEC fit for NGC 6134 cluster members, derived from MCMC analysis.
Paper: Comprehensive Analysis of NGC 6134: Structure, Dynamics, and Blue Straggler Star Candidates
Authors: Dexin Zeng, Ying Mei, Huanbin Chi, Hui Deng, Feng Wang
Figure caption: Density profile of NGC 6134. Points with error bars represent the observed stellar density profile. The black solid line indicates the best-fitting King profile 1. The dashed vertical lines are the rc and rt values.
Paper: Comprehensive Analysis of NGC 6134: Structure, Dynamics, and Blue Straggler Star Candidates
Authors: Dexin Zeng, Ying Mei, Huanbin Chi, Hui Deng, Feng Wang
Figure caption: Mass-segregation ratio (ΛMSR) of NGC 6134 as a function of the number of massive stars considered. A value of ΛMSR = 1.71 ± 0.26 for the 20 most-massive stars indicates significant mass segregation.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Comparison of eccentricity, orbital period, and minimum mass measurements from the literature and those from our orbit refits. Warm Jupiters in single-planet systems are denoted by blue circles, and those in multiplanet systems are represented by orange stars. Literature solutions were selected from the original fits in the discovery papers, with updated fits from follow-up papers utilized when available. References to earlier work used in this figure are reported in Table 3.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Example summary plot of the known warm Jupiters 14 And b and 24 Boo b using RadVel. Left: panel showing the RV time-series plot combined with the residuals to the model and the phase-folded orbit of the planet. Right: corner plot with the joint posterior distributions and a histogram of the eccentricity posterior distribution of the planet.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Distribution of eccentricities, orbital periods, minimum masses, and number of RVs per target for all planets in our analysis. Eccentricities, orbital periods, and minimum masses are derived from the final fits using RadVel.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters BD-08 2823 c and CoRoT-10 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters BD+45 564 b and BD+55 362 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters BD+15 2375 b and BD+15 2940 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters 91 Aqr b and BD+14 4559 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters 70 Vir b and 8 UMi b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters 4 UMa b and 55 Cnc b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 145457 b and HD 147018 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 147873 b and HD 148164 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 12661 b and HD 128356 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 130322 b and HD 134987 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 12484 b and HD 12648 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 148427 b and HD 154672 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 141399 b and HD 141399 c.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 142 b and HD 145377 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 13908 b and HD 1397 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 224693 b and HD 231701 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 180053 b and HD 191939 e.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 220842 b and HD 221416 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 208897 b and HD 210702 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 211403 b and HD 216536 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 192263 b and HD 192699 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 207832 b and HD 208487 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 216770 b and HD 219139 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 195019 b and HD 205739 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 37605 b and HD 38283 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 43691 b and HD 45364 c.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 33283 b and HD 35759 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 38529 b and HD 40979 b.
Paper: Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Figure caption: Summary of results for the warm Jupiters HD 233604 b and HD 27894 b.