Published April 30, 2026
| Version 1.0.0
Dataset
Open
The data for "Worlds Next Door. IV. Mapping the Late Stages of Giant Planet Evolution with a Precise Dynamical Mass and Luminosity for eInd Ab"
Authors/Creators
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Sanghi, Aniket
(Contact person)1
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Thompson, William R.2
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Mang, James3
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Xuan, Jerry W.4
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Mawet, Dimitri1
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Ruffio, Jean-Baptiste5
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Zhang, Yapeng1
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Wang, Jason J.6
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Morley, Caroline V.3
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Nielsen, Eric7
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Roberson, William7
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Matthews, Elisabeth8
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Carter, Aarynn L.9
- Crossfield, Ian10
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Mâlin, Mathilde9
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Benneke, Björn4
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Bidot, Alexis9
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Gaspar, Andras11
- He, Carrie4
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Horstman, Katelyn1
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Madurowicz, Alexander9
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Marois, Christian2
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Oppenheimer, Rebecca12
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Perrin, Marshall9
- 1. Cahill Center for Astronomy and Astrophysics, California Institute of Technology, 1200 E. California Boulevard, MC 249-17, Pasadena, CA 91125, USA
- 2. NRC Herzberg Astronomy and Astrophysics, 5071 West Saanich Road, Victoria, BC, V9E 2E7, Canada
- 3. Department of Astronomy, University of Texas at Austin, Austin, TX 78712, USA
- 4. Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095, USA
- 5. Department of Astronomy \& Astrophysics, University of California, San Diego, La Jolla, CA 92093, USA
- 6. Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University, 1800 Sherman Avenue, Evanston, IL, 60201, USA
- 7. Department of Astronomy, New Mexico State University, 1320 Frenger Mall, Las Cruces, NM 88003, USA
- 8. Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
- 9. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
- 10. Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
- 11. Steward Observatory, University of Arizona, Tucson, AZ 85721, USA
- 12. American Museum of Natural History, New York, NY, USA
Description
This repository provides the orbital parameter posteriors for all models discussed in Section 3.5 in "Worlds Next Door. IV. Mapping the Late Stages of Giant Planet Evolution with a Precise Dynamical Mass and Luminosity for eInd Ab" by Sanghi et al. (2026). A sample notebook demonstrates how to access the posterior samples from the individual fits files.
Below is the correspondence between the filename and the orbit model. By default, all orbit models use observable-based priors for the relative astrometry and include a GP in the RV model, unless otherwise specified.
- epsInd_astro-post.fits – Relative astrometry only
- epsInd_astro_HGCA-post.fits – Relative astrometry + HGCA
- epsInd_astro_RV-post.fits – Relative astrometry + RV
- epsInd_NoNIRCam-post.fits – Relative astrometry (No JWST/NIRCam) + HGCA + RV
- No File. Model did not converge – Relative astrometry + HGCA + RV (No GP)
- epsInd_allData_noGP_noUVES-post.fits – Relative astrometry + HGCA + RV (No UVES and No GP)
- epsInd_allData_unipri-post.fits – Relative astrometry (Uniform Priors) + HGCA + RV
- epsInd_allData_obspri-post.fits – Relative astrometry + HGCA + RV
Files
read_orbit_posterior.ipynb
Files
(125.5 MB)
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md5:25065bd9c7780aeecfbfd525154c1883
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24.1 MB | Download |
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md5:09203a0d7c138d8449023b66ea620ea1
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22.3 MB | Download |
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md5:93775caa150a392ed16638c9c31ddd33
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22.3 MB | Download |
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md5:a0b648a54b32c2ad2e27cde0c725846a
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5.8 MB | Download |
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md5:3a8981ab4c8cdb95acd91910a2927423
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6.3 MB | Download |
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md5:f9e707f3bebc2e2ab046e999bcbee90a
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22.3 MB | Download |
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md5:9ec03a3a786dae450edc2e6240d6cdd3
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22.3 MB | Download |
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27.8 kB | Preview Download |