The SDSS-IV eBOSS: Emission line galaxy catalogues at z ≈ 0.8 and study of systematic errors in the angular clustering

DOI: 
10.1093/mnras/stw274
Publication date: 
25/07/2017
Main author: 
Delubac T.
IAA authors: 
Prada, F.
Authors: 
Delubac T., Raichoor A., Comparat J., Jouvel S., Kneib J.-P., Yèche C., Zou H., Brownstein J.R., Abdalla F.B., Dawson K., Jullo E., Myers A.D., Newman J.A., Percival W.J., Prada F., Ross A.J., Schneider D.P., Zhou X., Zhou Z., Zhu G.
Journal: 
Monthly Notices of the Royal Astronomical Society
Publication type: 
Article
Volume: 
465
Pages: 
1831-1846
Abstract: 

We present two wide-field catalogues of photometrically selected emission line galaxies (ELGs) at z ≈ 0.8 covering about 2800 deg2over the south galactic cap. The catalogues were obtained using a Fisher discriminant technique described in a companion paper. The two catalogues differ by the imaging used to define the Fisher discriminant: the first catalogue includes imaging from the Sloan Digital Sky Survey and the Wide-field Infrared Survey Explorer, the second also includes information from the South Galactic Cap U-band Sky Survey. Containing respectively 560 045 and 615 601 objects, they represent the largest ELG catalogues available today and were designed for the ELG programme of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). We study potential sources of systematic variation in the angular distribution of the selected ELGs due to fluctuations of the observational parameters. We model the influence of the observational parameters using a multivariate regression and implement a weighting scheme which allows effective removal of all of the systematic errors induced by the observational parameters. We show that fluctuations in the imaging zero-points of the photometric bands have minor impact on the angular distribution of objects in our catalogues. We compute the angular clustering of both catalogues and show that our weighting procedure effectively removes spurious clustering on large scales. We fit a model to the small-scale angular clustering, showing that the selections have similar biases of 1.35/Da(z) and 1.28/Da(z). Both catalogues are publicly available. © 2016 The Authors.

Database: 
SCOPUS
URL: 
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85022223963&doi=10.1093%2fmnras%2fstw274&partnerID=40&md5=c85dd517cda5e9c2a243f1b8f5618b80
Keywords: 
Catalogues; Cosmology: observations; galaxies: distances and redshifts; Galaxies: general; Galaxies: photometry; methods: data analysis