Mehdi Rezaie
Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey – I: Catalogue preparation and systematic mitigation
Rezaie, Mehdi; Ross, Ashley J; Seo, Hee-Jong; Mueller, Eva-Maria; Percival, Will J; Merz, Grant; Katebi, Reza; Bunescu, Razvan C; Bautista, Julian; Brownstein, Joel R; Burtin, Etienne; Dawson, Kyle; Gil-Marín, Héctor; Hou, Jiamin; Lyke, Eleanor B; de la Macorra, Axel; Rossi, Graziano; Schneider, Donald P; Zarrouk, Pauline; Zhao, Gong-Bo
Authors
Ashley J Ross
Hee-Jong Seo
Eva-Maria Mueller
Will J Percival
Grant Merz
Reza Katebi
Razvan C Bunescu
Julian Bautista
Joel R Brownstein
Etienne Burtin
Kyle Dawson
Héctor Gil-Marín
Jiamin Hou
Eleanor B Lyke
Axel de la Macorra
Graziano Rossi
Donald P Schneider
Dr Pauline Zarrouk pauline.s.zarrouk@durham.ac.uk
Academic Visitor
Gong-Bo Zhao
Abstract
We investigate the large-scale clustering of the final spectroscopic sample of quasars from the recently completed extended Baryon Oscillation Spectroscopic Survey (eBOSS). The sample contains 343 708 objects in the redshift range 0.8 < z < 2.2 and 72 667 objects with redshifts 2.2 < z < 3.5, covering an effective area of 4699deg2. We develop a neural network-based approach to mitigate spurious fluctuations in the density field caused by spatial variations in the quality of the imaging data used to select targets for follow-up spectroscopy. Simulations are used with the same angular and radial distributions as the real data to estimate covariance matrices, perform error analyses, and assess residual systematic uncertainties. We measure the mean density contrast and cross-correlations of the eBOSS quasars against maps of potential sources of imaging systematics to address algorithm effectiveness, finding that the neural network-based approach outperforms standard linear regression. Stellar density is one of the most important sources of spurious fluctuations, and a new template constructed using data from the Gaia spacecraft provides the best match to the observed quasar clustering. The end-product from this work is a new value-added quasar catalogue with the improved weights to correct for non-linear imaging systematic effects, which will be made public. Our quasar catalogue is used to measure the local-type primordial non-Gaussianity in a companion paper.
Citation
Rezaie, M., Ross, A. J., Seo, H.-J., Mueller, E.-M., Percival, W. J., Merz, G., Katebi, R., Bunescu, R. C., Bautista, J., Brownstein, J. R., Burtin, E., Dawson, K., Gil-Marín, H., Hou, J., Lyke, E. B., de la Macorra, A., Rossi, G., Schneider, D. P., Zarrouk, P., & Zhao, G.-B. (2021). Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey – I: Catalogue preparation and systematic mitigation. Monthly Notices of the Royal Astronomical Society, 506(3), 3439-3454. https://doi.org/10.1093/mnras/stab1730
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 14, 2021 |
Online Publication Date | Jul 18, 2021 |
Publication Date | 2021-09 |
Deposit Date | Nov 16, 2021 |
Publicly Available Date | Nov 16, 2021 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 506 |
Issue | 3 |
Pages | 3439-3454 |
DOI | https://doi.org/10.1093/mnras/stab1730 |
Public URL | https://durham-repository.worktribe.com/output/1221854 |
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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2021 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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