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Identification and photometric classification of extragalactic transients in the Vera C. Rubin Observatory's Data Preview 1

Published 30 Jul 2025 in astro-ph.HE and astro-ph.IM | (2507.22864v1)

Abstract: The Vera C. Rubin Observatory will soon survey the southern sky, delivering a depth and sky coverage that is unprecedented in time domain astronomy. As part of commissioning, Data Preview 1 (DP1) has been released. It comprises a ComCam observing campaign between November and December 2024 with multi-band imaging of seven fields, covering roughly 0.4 square degree each, provides a first glimpse into the data products that will become available once the Legacy Survey of Space and Time begins. In this work, we search three fields for extragalactic transients. We identify six new extragalactic transients, and three known ones from a sample of 369,644 difference image analysis objects. Photometric classification using \texttt{Superphot+} indicates that this sample likely comprises six type Ia, two type II, two type Ibc and one type IIn supernovae. Our findings are in slight tension with supernova detection rate predictions from the literature of $12\pm3$ SN Ia and $3\pm1$ core-collapse supernovae likely due to the lack of suitable templates. Nevertheless, this work demonstrates the quality of the data products delivered in DP1 and indicates that Rubin Observatory Legacy Survey and Space and Time (LSST) is well placed to fulfill its discovery potential in time domain astronomy.

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