Near-infrared spectroscopy of extreme BAL QSOs from the QUBRICS bright quasar survey
| Autor: | Guido Cupani, Giorgio Calderone, Pierluigi Selvelli, Stefano Cristiani, Konstantina Boutsia, Andrea Grazian, Fabio Fontanot, Francesco Guarneri, Valentina D’Odorico, Emanuele Giallongo, Nicola Menci |
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| Jazyk: | angličtina |
| Rok vydání: | 2021 |
| Předmět: |
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) FOS: Physical sciences Astronomy and Astrophysics Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) Astrophysics - Astrophysics of Galaxies Astrophysics - Cosmology and Nongalactic Astrophysics |
| Popis: | 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 $z\simeq 2.1$. 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 FeLoBAL QSOs). The detection of such a large fraction of rare objects (which are estimated to account for less than one percent of the general QSO population) is interpreted as an unexpected (yet favourable) consequence of the particular candidate selection procedure adopted within the QUBRICS survey. The measured properties of FeLoBAL QSOs observed so far provide no evidence that they are a manifestation of a particular stage in AGN evolution. In this paper we present an explorative analysis of the individual QSOs, to serve as a basis for a further, more detailed investigation. 20 pages, 7 figures. This is a pre-copyedited, author-produced PDF of an article accepted for publication in MNRAS following peer review. Associated data and procedures available at https://www.ict.inaf.it/index.php/31-doi/137-ds-2021-03 |
| Databáze: | OpenAIRE |
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