Published May 2, 2024
| Version v1
Dataset
Open
Data products from "oMEGACat II - Photometry and proper motions for 1.4 million stars in Omega Centauri and its rotation in the plane of the sky"
Creators
-
Häberle, Maximilian
(Contact person)1
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Neumayer, Nadine1
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Bellini, Andrea2
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Libralato, Mattia3
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Clontz, Callie1, 4
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Seth, Anil4
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Nitschai, Maria-Selina1
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Kamann, Sebastian5
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Alfaro-Cuello, Mayte6
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Anderson, Jay2
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Dreizler, Stefan7
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Feldmeier-Krause, Anja1, 8
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Kacharov, Nikolay9
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Latour, Marilyn7
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Milone, Antonino10
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Pechetti, Renuka5
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van de Ven, Glenn8
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Voggel, Karina11
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1.
Max Planck Institute for Astronomy
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2.
Space Telescope Science Institute
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3.
National Institute for Astrophysics
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4.
University of Utah
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5.
Liverpool John Moores University
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6.
Universidad Central de Chile
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7.
University of Göttingen
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8.
University of Vienna
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9.
Leibniz Institute for Astrophysics Potsdam
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10.
University of Padua
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11.
Observatoire astronomique de Strasbourg
Description
This repository contains the data products of the publication:
Häberle et al (2024): "oMEGACat II - Photometry and proper motions for 1.4 million stars in Omega Centauri and its rotation in the plane of the sky"
A detailed description of the data products and their creation is given in the accompanying paper.
The data products include:
- The astrometric catalog with position and proper motion information for around 1.4 million sources within the half-light radius of Omega Centauri. We provide the catalog in both the .fits and .mrt format.
- The 7 photometric catalogs (for the 7 different used Hubble Space Telescope filters), both in .fits and .mrt format.
- The 7 deep, stacked image mosaics (one for each filter) in .fits format
- In addition, we include an IPython Notebook with basic usage examples for all these files.
Please cite the catalog paper Häberle et al. (2024) when using this work.
In case of any questions, feel free to contact us using haeberle@mpia.de
Files
omegacat_ii_use_cases_and_examples.ipynb
Files
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md5:3df8a5ee4fedc66b2237e1c416394fe2
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Additional details
Related works
- Is supplement to
- Preprint: arXiv:2404.03722 (arXiv)