J/MNRAS/479/807     Catalogue of faint local radio AGN        (Lofthouse+, 2018)

A catalogue of faint local radio AGN and the properties of their host galaxies. Lofthouse E.K., Kaviraj S., Smith D.J.B., Hardcastle M.J. <Mon. Not. R. Astron. Soc. 479, 807 (2018)> =2018MNRAS.479..807L 2018MNRAS.479..807L (SIMBAD/NED BibCode)
ADC_Keywords: Active gal. nuclei; Radio sources; Radio continuum Keywords: active galaxies; luminosity function; radio continuum Abstract: We present a catalogue of 2210 local (z<0.1) galaxies that contain faint active galactic nuclei (AGN). We select these objects by identifying galaxies that exhibit a significant excess in their radio luminosities, compared to what is expected from the observed levels of star formation activity in these systems. This is achieved by comparing the optical (spectroscopic) star formation rate (SFR) to the 1.4GHz luminosity measured from the Faint Images of the Radio Sky at Twenty centimeters survey. The majority of the AGN identified in this study are fainter than those in previous work, such as in the Best and Heckman (2012, Cat. J/MNRAS/421/1569) catalogue. We show that these faint AGN make a non-negligible contribution to the radio luminosity function at low luminosities (below 1022.5W/Hz), and host ∼13 per cent of the local radio luminosity budget. Their host galaxies are predominantly high stellar-mass systems (with a median stellar mass of 1011 M), are found across a range of environments (but typically in denser environments than star-forming galaxies) and have early-type morphologies. This study demonstrates a general technique to identify AGN in galaxy populations where reliable optical SFRs can be extracted using spectro-photometry and where radio data are also available so that a radio excess can be measured. Our results also demonstrate that it is unsafe to infer SFRs from radio emission alone, even if bright AGN have been excluded from a sample, since there is a significant population of faint radio AGN that may contaminate the radio-derived SFRs. Description: We present a catalogue of 2210 local (z<0.1) galaxies that contain faint active galactic nuclei (AGN). We select these objects by identifying galaxies that exhibit a significant excess in their radio luminosities, compared to what is expected from the observed levels of star formation activity in these systems. This is achieved by comparing the optical (spectroscopic) star formation rate (SFR) to the 1.4 GHz luminosity measured from the Faint Images of the Radio Sky at Twenty centimeters survey. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 104 2210 Catalogue of faint local radio AGN -------------------------------------------------------------------------------- See also: VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015) J/MNRAS/421/1569 : Properties of 18286 SDSS radio galaxies (Best+, 2012) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.5 deg RAdeg Right Ascension (J2000) 11- 19 F9.5 deg DEdeg Declination (J2000) 21- 27 F7.5 --- z Redshift 29- 50 E22.17 W/Hz LFIRST FIRST Luminosity 52- 59 F8.5 [Msun/yr] logSFRF Logarithm of star formation rate derived from FIRST luminosity 61- 68 F8.5 [Msun/yr] logSFRM Logarithm of star formation rate from SDSS MPA-JHU catalogue 70- 77 F8.5 [Msun] logM* Logarithm of stellar mass 79- 90 F12.7 --- BT ?=-999 Bulge-to-total light ratio 92-101 F10.5 [Msun] logMhalo ?=-999 Logarithm of halo mass 103-104 I2 --- BPT [-1/5] BPT classification (1) -------------------------------------------------------------------------------- Note (1): BPT classification code as follows: -1 = Unclassified 1 = star forming 2 = low S/N star forming 3 = Composite 4 = AGN (Non-LINER) 5 = LINER -------------------------------------------------------------------------------- Acknowledgements: Emma Lofthouse, e.k.lofthouse(at)gmail.com History: * 24-Aug-2018: on-line version * 13-Jun-2019: complete catalog ...
(End) E. Lofthouse [Univ. of Hertfordshire], P. Vannier [CDS] 23-Aug-2018
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