Near-infrared spectroscopy of extreme BAL QSOs from the QUBRICS bright quasar survey
Guido Cupani, Giorgio Calderone, Pierluigi Selvelli, Stefano, Cristiani, Konstantina Boutsia, Andrea Grazian, Fabio Fontanot, Francesco, Guarneri, Valentina D'Odorico, Emanuele Giallongo, Nicola Menci

TL;DR
This study confirms 18 bright QSOs from the QUBRICS survey as BAL QSOs, many with rare FeLoBAL features, using near-infrared spectroscopy, revealing a higher-than-expected occurrence of these objects among bright quasars.
Contribution
First near-infrared spectroscopic confirmation of a large sample of BAL QSOs from the QUBRICS survey, highlighting the high fraction of rare FeLoBAL objects.
Findings
Majority are BAL QSOs with strong Fe II absorption.
High fraction of FeLoBAL QSOs among bright QSOs.
No evidence linking FeLoBAL features to specific AGN evolutionary stages.
Abstract
We report on the spectral confirmation of 18 QSO candidates from the "QUasars as BRIght beacons for Cosmology in the Southern hemisphere'' survey (QUBRICS), previously observed in the optical band, for which we acquired new spectroscopic data in the near-infrared band with the Folded-port InfraRed Echellette spectrograph (FIRE) at the Magellan Baade telescope. In most cases, further observations were prompted by the peculiar nature of the targets, whose optical spectra displayed unexpected absorption features. All candidates have been confirmed as bona fide QSOs, with average emission redshift . The analysis of the emission and absorption features in the spectra, performed with Astrocook and QSFit, reveals that the large majority of these objects are broad-absorption line (BAL) QSOs, with almost half of them displaying strong Fe II absorption (typical of the so-called…
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