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Journal article

Identifying Transient Hosts in LSST’s Deep Drilling Fields with Galaxy Catalogs

Abstract:
The upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will enable astronomers to discover rare and distant astrophysical transients. Host-galaxy association is crucial for selecting the most scientifically interesting transients for follow-up. LSST deep drilling field (DDF) observations will detect distant transients occurring in galaxies below the detection limits of most all-sky catalogs. Here, we investigate the use of preexisting, field-specific catalogs for host identification in the DDFs and a ranking of their usefulness. We have compiled a database of 70 deep catalogs that overlap with the Rubin DDFs and constructed thin catalogs to be homogenized and combined for transient-host matching. A systematic ranking of their utility is discussed and applied based on the inclusion of information such as spectroscopic redshifts and morphological information. Utilizing this data against a Dark Energy Survey sample of supernovae with pre-identified hosts in the XMM-Large Scale Structure and the Extended Chandra Deep Field-South fields, we evaluate different methods for transient-host association in terms of both accuracy and processing speed. We also apply light data-cleaning techniques to identify and remove contaminants within our associations, such as diffraction spikes and blended galaxies where the correct host cannot be determined with confidence. We use a lightweight machine learning approach in the form of extreme gradient boosting to generate confidence scores in our contaminant selections and associated metrics. Finally, we discuss the computational expense of implementation within the LSST transient alert brokers, which will require efficient, fast-paced processing to handle the large stream of survey data.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4357/ae4e1a

Authors

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Role:
Author
ORCID:
0009-0002-9460-9900
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Role:
Author
ORCID:
0000-0002-1229-2499
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
ORCID:
0000-0002-8229-1731
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Role:
Author
ORCID:
0000-0002-2555-3192
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
ORCID:
0000-0001-7039-9078


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
1000
Issue:
2
Pages:
289
Article number:
289
Publication date:
2026-03-30
Acceptance date:
2026-03-04
DOI:
EISSN:
1538-4357
ISSN:
0004637X, 0004-637X


Language:
English
Keywords:
Source identifiers:
3898726
Deposit date:
2026-03-30
ARK identifier:
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