Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8347
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dc.contributor.authorPaliya, Vaidehi S-
dc.contributor.authorStalin, C. S-
dc.contributor.authorDominguez, Alberto-
dc.contributor.authorSaikia, D. J-
dc.date.accessioned2024-01-25T06:14:24Z-
dc.date.available2024-01-25T06:14:24Z-
dc.date.issued2024-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 527, No. 3, pp. 7055–7069en_US
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/8347-
dc.descriptionOpen Accessen_US
dc.descriptionThis is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium,provided the original work is properly cited.-
dc.description.abstractNarrow-line Seyfert 1 (NLSy1) galaxies are an enigmatic class of active galactic nuclei (AGN) that exhibit peculiar multiwavelength properties across the electromagnetic spectrum. For example, these sources have allowed us to explore the innermost regions of the central engine of AGN using X-ray observations and have also provided clues about the origin of relativistic jets considering radio and gamma-ray bands. Keeping in mind the ongoing and upcoming wide-field, multifrequency sky surveys, we present a new catalogue of NLSy1 galaxies. This was done by carrying out a detailed decomposition of >2 million optical spectra of quasars and galaxies from the Sloan Digital Sky Survey Data Release 17 (SDSS-DR17) using the publicly available software ‘Bayesian AGN Decomposition Analysis for SDSS Spectra’. The catalogue contains 22656 NLSy1 galaxies which is more than twice the size of the previously identified NLSy1s based on SDSS-DR12. As a corollary, we also release a new catalogue of 52273 broad-line Seyfert 1 (BLSy1) galaxies. The estimated optical spectral parameters and derived quantities confirm the previously known finding of NLSy1 galaxies being AGN powered by highly accreting, low-mass black holes. We conclude that this enlarged sample of NLSy1 and BLSy1 galaxies will enable us to explore the low-luminosity end of the AGN population by effectively utilizing the sensitive, high-quality observations delivered by ongoing/upcoming wide-field sky surveys. The catalogue has been made public at https://www.ucm.es/blazars/seyfert.en_US
dc.language.isoenen_US
dc.publisherOxford University Press on behalf of Royal Astronomical Societyen_US
dc.relation.urihttps://doi.org/10.1093/mnras/stad3650-
dc.rights© 2023 The Author(s)-
dc.subjecttechniques: spectroscopicen_US
dc.subjectgalaxies: activeen_US
dc.subjectgalaxies: Seyferten_US
dc.titleNarrow-line Seyfert 1 galaxies in Sloan Digital Sky Survey: a new optical spectroscopic catalogueen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications



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