47 Tuc in Rubin Data Preview 1: Exploring Early LSST Data and Science Potential

Fuente: arXiv
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Autores principales: Choi, Yumi, Olsen, Knut A. G., Carlin, Jeffrey L., Yuankun, Wang, Moolekamp, Fred, Saha, Abhijit, Sullivan, Ian, Slater, Colin T., Tucker, Douglas L., Adair, Christina L., Ferguson, Peter S., Kang, Yijung, Ramírez, Karla Peña, Rabus, Markus
Formato: Preprint
Publicado: 2025
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author Choi, Yumi
Olsen, Knut A. G.
Carlin, Jeffrey L.
Yuankun
Wang
Moolekamp, Fred
Saha, Abhijit
Sullivan, Ian
Slater, Colin T.
Tucker, Douglas L.
Adair, Christina L.
Ferguson, Peter S.
Kang, Yijung
Ramírez, Karla Peña
Rabus, Markus
author_facet Choi, Yumi
Olsen, Knut A. G.
Carlin, Jeffrey L.
Yuankun
Wang
Moolekamp, Fred
Saha, Abhijit
Sullivan, Ian
Slater, Colin T.
Tucker, Douglas L.
Adair, Christina L.
Ferguson, Peter S.
Kang, Yijung
Ramírez, Karla Peña
Rabus, Markus
contents We present analyses of the early data from Rubin Observatory's Data Preview 1 (DP1) for the globular cluster 47 Tuc field. The DP1 dataset for 47 Tuc includes four nights of observations from the Rubin Commissioning Camera (LSSTComCam), covering multiple bands ($ugriy$). We address challenges of crowding in the inner region of the cluster and toward the SMC in DP1, and demonstrate improved star-galaxy separation by fitting fifth-degree polynomials to the stellar loci in color-color diagrams and applying multi-dimensional sigma clipping. We compile a catalog of 3,576 probable 47 Tuc member stars selected via a combination of isochrone, Gaia proper-motion, and color-color space matched filtering. We explore the sources of photometric scatter in the 47 Tuc color-color sequence, evaluating contributions from various potential sources, including differential extinction within the cluster. Finally, of the 72 well-characterized variables in the field, we recover five known variable stars, including three RR Lyrae and two eclipsing binaries, in the coadd-based object catalog, and identify 62 in the difference image-based object catalog. Although the DP1 lightcurves have sparse temporal sampling, they appear to follow the patterns of densely-sampled literature lightcurves well. Despite some data limitations for crowded-field stellar analysis, DP1 demonstrates the promising scientific potential for future LSST data releases.
format Preprint
id arxiv_https___arxiv_org_abs_2507_01343
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle 47 Tuc in Rubin Data Preview 1: Exploring Early LSST Data and Science Potential
Choi, Yumi
Olsen, Knut A. G.
Carlin, Jeffrey L.
Yuankun
Wang
Moolekamp, Fred
Saha, Abhijit
Sullivan, Ian
Slater, Colin T.
Tucker, Douglas L.
Adair, Christina L.
Ferguson, Peter S.
Kang, Yijung
Ramírez, Karla Peña
Rabus, Markus
Solar and Stellar Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
We present analyses of the early data from Rubin Observatory's Data Preview 1 (DP1) for the globular cluster 47 Tuc field. The DP1 dataset for 47 Tuc includes four nights of observations from the Rubin Commissioning Camera (LSSTComCam), covering multiple bands ($ugriy$). We address challenges of crowding in the inner region of the cluster and toward the SMC in DP1, and demonstrate improved star-galaxy separation by fitting fifth-degree polynomials to the stellar loci in color-color diagrams and applying multi-dimensional sigma clipping. We compile a catalog of 3,576 probable 47 Tuc member stars selected via a combination of isochrone, Gaia proper-motion, and color-color space matched filtering. We explore the sources of photometric scatter in the 47 Tuc color-color sequence, evaluating contributions from various potential sources, including differential extinction within the cluster. Finally, of the 72 well-characterized variables in the field, we recover five known variable stars, including three RR Lyrae and two eclipsing binaries, in the coadd-based object catalog, and identify 62 in the difference image-based object catalog. Although the DP1 lightcurves have sparse temporal sampling, they appear to follow the patterns of densely-sampled literature lightcurves well. Despite some data limitations for crowded-field stellar analysis, DP1 demonstrates the promising scientific potential for future LSST data releases.
title 47 Tuc in Rubin Data Preview 1: Exploring Early LSST Data and Science Potential
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2507.01343