Value Added Catalogs

In addition to the primary SDSS photometry and spectroscopy, there are a few extra catalogs created by our collaborators that are distributed through the SAS. These Value-Added Catalogs (VACs) are listed below, and include catalogs that were released in earlier data releases.

Updated redshifts and classifications of Fermi-detected sources within SDSS-V

Scientific Analysis Catalog
BHM
QSO
CAS
DR20

Multi-component optical spectroscopic classifications, redshifts, and jet fractions estimation for 707 Fermi blazar candidates identified in SDSS-V DR20

Mohammed Iddrisu Nlowie, James Aird, Eli Kasai, Amy Rankine, Xinyu Dai, Catarina Aydar, Donald P. Schneider, William Nielsen Brandt, Anton M. Koekemoer, Scott F. Anderson, Mara Salvato, Andrea Merloni, Lorena Hernández-Garcíaz

Catalog Data

DR20
This dataset appears in SkyServer and CasJobs in the following tables:

Abstract

This Value-Added Catalogue (VAC) provides multi-component spectral fitting results for 707 confirmed Fermi blazar candidates identified by cross-matching the Fermi/4FGL-DR4 catalogue (Ballet et al. 2023) with the SDSS-V Data Release 20 spectroscopic database. A physically motivated pipeline decomposes each optical spectrum into a non-thermal power-law jet continuum combined with elliptical galaxy (Polletta et al. 2007) , synthetic QSO (Temple et al. 2021) or emission-line templates, enabling jet-aware classifications that are not provided by the SDSS automated pipeline. For each source the catalogue provides: (1) best-fit spectral model and blazar subclass (BL Lac or FSRQ candidate); (2) spectroscopic redshift with 1σ uncertainty; (3) reduced χ² for the multi-component model fit; (4) optical jet flux fraction (f_jet); (5) power-law slope parameters α and δ describing the jet continuum shape; and (6) observation MJD. Redshifts are validated against the Third Catalog of Hard Fermi-LAT Sources (Ajello et al. 2017), achieving a 10.4% reduction in the catastrophic outlier fraction relative to the SDSS automated pipeline. Independent validation using WISE infrared photometry (Wright et al. 2010) confirms that 96.6% of SDSS-misclassified stellar sources occupy the canonical blazar region of the infrared colour-colour diagram (Massaro et al. 2011) . The catalogue is accompanied by blazarkit, an open-source Python package for streaming, visualising, and analysing individual source spectra and multi-component fits (Nlowie et al., submitted). There is a Python notebook tutorial available for this VAC, which you can find on GitHub here.

Catalog last modified: 2026-07-30 12:12:10

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