Magellan/FIRE quasar [OIII] spectra

DOI

Understanding the links between different phases of outflows from active galactic nuclei is a key goal in extragalactic astrophysics. Here, we compare [OIII] {lambda}{lambda} 4960, 5008 outflow signatures in quasars with and without broad absorption lines (BALs), aiming to test how the broad absorption troughs seen in the rest-frame ultraviolet are linked to the narrow line region outflows seen in the rest-frame optical. We present new near-infrared spectra from Magellan/FIRE that cover [OIII] in 12 quasars with 2.1

Identifier
DOI http://doi.org/10.26093/cds/vizier.75320424
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/532/424
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/532/424
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/532/424
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/532/424
Provenance
Creator Temple M.J.; Rankine A.L.; Banerji M.; Hennawi J.F.; Hewett P.C.,Matthews J.H.; Nanni R.; Ricci C.; Richards G.T.
Publisher CDS
Publication Year 2024
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; High Energy Astrophysics; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy