DeepDISC-photoz: Deep Learning-Based Photometric Redshift Estimation for Rubin LSST
Photometric redshift
DOI:
10.33232/001c.136809
Publication Date:
2025-04-16T07:59:36Z
AUTHORS (14)
ABSTRACT
Photometric redshifts will be a key data product for the Rubin Observatory Legacy Survey of Space and Time (LSST) as well future ground space-based surveys. The need photometric redshifts, or photo-zs, arises from sparse spectroscopic coverage observed galaxies. LSST is expected to observe billions objects, making it crucial have photo-z estimator that accurate efficient. To end, we present DeepDISC photo-z, an extension framework. base network simultaneously detects, segments, classifies objects in multi-band coadded images. We introduce capabilities by adding redshift estimation Region Interest head, which produces probability distribution function each detected object. On simulated images, outperforms traditional catalog-based estimators, both point estimate probabilistic metrics. validate examining dependencies on systematics including galactic extinction, blending PSF effects. also examine impact quality size training set model. find biggest factor signal-to-noise imaging data, see reduction scatter approximately proportional image signal-to-noise. Our code fully public integrated RAIL package ease use comparison other codes at https://github.com/LSSTDESC/rail_deepdisc
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