Finding the brightest cosmic beacons in the Southern Hemisphere
Calderone G., Boutsia K., Cristiani S., Grazian A., Amorin R.,, D'Odorico V., Cupani G., Fontanot F., Salvato M

TL;DR
This paper introduces a new method using Canonical Correlation Analysis to identify bright high-redshift QSOs in the Southern Hemisphere, significantly increasing the available sample for cosmological studies.
Contribution
The study develops a novel candidate selection technique combining multiple databases, resulting in a high success rate and improved completeness for bright high-z QSOs in the south.
Findings
Identified 1476 QSO candidates over 12,400 sq. degrees.
Confirmed 56 new bright QSOs at z > 2.5 with ~80% success rate.
Achieved an estimated 90% completeness in the candidate sample.
Abstract
The study of absorptions along the lines of sight to bright high- QSOs is an invaluable cosmological tool that provides a wealth of information on the inter-/circum-galactic medium, Dark Matter, primordial elements, reionization, fundamental constants, and General Relativity. Unfortunately, the number of bright ( 18) QSOs at in the Southern hemisphere is much lower than in the North, due to the lack of wide multi-wavelength surveys at declination 0, hampering the effectiveness of observations from southern observatories. In this work we present a new method based on Canonical Correlation Analysis to identify such objects, taking advantage of a number of available databases: Skymapper, Gaia DR2, WISE, 2MASS. Our QSO candidate sample lists 1476 sources with over 12,400 square degrees in the southern hemisphere. With a preliminary…
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