Allyson Brodzeller
Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument
Brodzeller, Allyson; Dawson, Kyle; Bailey, Stephen; Yu, Jiaxi; Ross, A. J.; Bault, A.; Filbert, S.; Aguilar, J.; Ahlen, S.; Alexander, David M.; Armengaud, E.; Berti, A.; Brooks, D.; Chaussidon, E.; de la Macorra, A.; Doel, P.; Fanning, K.; Fawcett, V. A.; Font-Ribera, A.; A Gontcho, S. Gontcho; Guy, J.; Honscheid, K.; Juneau, S.; Kehoe, R.; Kisner, T.; Kremin, Anthony; Lan, Ting-Wen; Landriau, M.; Levi, Michael E.; Magneville, C.; Martini, Paul; Meisner, Aaron M.; Miquel, R.; Moustakas, J.; Palanque-Delabrouille, N.; Percival, W. J.; Prada, F.; Ravoux, C.; Rossi, Graziano; Saulder, C.; Siudek, M.; Tarlé, Gregory; Weaver, B. A.; Youles, S.; Zheng, Zheng; Zhou, Rongpu; Zhou, Zhimin
Authors
Kyle Dawson
Stephen Bailey
Jiaxi Yu
A. J. Ross
A. Bault
S. Filbert
J. Aguilar
S. Ahlen
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
E. Armengaud
A. Berti
D. Brooks
E. Chaussidon
A. de la Macorra
P. Doel
K. Fanning
V. A. Fawcett
A. Font-Ribera
S. Gontcho A Gontcho
J. Guy
K. Honscheid
S. Juneau
R. Kehoe
T. Kisner
Anthony Kremin
Ting-Wen Lan
M. Landriau
Michael E. Levi
C. Magneville
Paul Martini
Aaron M. Meisner
R. Miquel
J. Moustakas
N. Palanque-Delabrouille
W. J. Percival
F. Prada
C. Ravoux
Graziano Rossi
C. Saulder
M. Siudek
Gregory Tarlé
B. A. Weaver
S. Youles
Zheng Zheng
Rongpu Zhou
Zhimin Zhou
Abstract
Millions of quasar spectra will be collected by the Dark Energy Spectroscopic Instrument (DESI), leading to a fourfold increase in the number of known quasars. High-accuracy quasar classification is essential to tighten constraints on cosmological parameters measured at the highest redshifts DESI observes (z > 2.0). We present spectral templates for identification and redshift estimation of quasars in the DESI Year 1 data release. The quasar templates are comprised of two quasar eigenspectra sets, trained on spectra from the Sloan Digital Sky Survey. The sets are specialized to reconstruct quasar spectral variation observed over separate yet overlapping redshift ranges and, together, are capable of identifying DESI quasars from 0.05 < z < 7.0. The new quasar templates show significant improvement over the previous DESI quasar templates regarding catastrophic failure rates, redshift precision and accuracy, quasar completeness, and the contamination fraction in the final quasar sample.
Citation
Brodzeller, A., Dawson, K., Bailey, S., Yu, J., Ross, A. J., Bault, A., …Zhou, Z. (2023). Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument. Astronomical Journal, 166(2), Article 66. https://doi.org/10.3847/1538-3881/ace35d
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 1, 2023 |
Online Publication Date | Jul 18, 2023 |
Publication Date | Aug 1, 2023 |
Deposit Date | Nov 1, 2023 |
Publicly Available Date | Nov 1, 2023 |
Journal | The Astronomical Journal |
Print ISSN | 0004-6256 |
Electronic ISSN | 1538-3881 |
Publisher | IOP Publishing |
Peer Reviewed | Peer Reviewed |
Volume | 166 |
Issue | 2 |
Article Number | 66 |
DOI | https://doi.org/10.3847/1538-3881/ace35d |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://durham-repository.worktribe.com/output/1873281 |
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Copyright Statement
© 2023. The Author(s). Published by the American Astronomical Society.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
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