J/ApJ/923/31    CHILES VERDES: COSMOS radio variability    (Sarbadhicary+, 2021)

CHILES VERDES: radio variability at an unprecedented depth and cadence in the COSMOS field. Sarbadhicary S.K., Tremou E., Stewart A.J., Chomiuk L., Peters C., Hales C., Strader J., Momjian E., Fender R., Wilcots E.M. <Astrophys. J., 923, 31 (2021)> =2021ApJ...923...31S 2021ApJ...923...31S
ADC_Keywords: Radio continuum; Active gal. nuclei; Surveys; Redshifts; X-ray sources Keywords: Radio continuum emission ; Radio active galactic nuclei ; Time domain astronomy ; Time series analysis Abstract: Although it is well established that some extragalactic radio sources are time-variable, the properties of this radio variability, and its connection with host galaxy properties, remain to be explored-particularly for faint sources. Here we present an analysis of radio variable sources from the CHILES Variable and Explosive Radio Dynamic Evolution Survey (CHILES VERDES)-a partner project of the 1.4GHz COSMOS HI Large Extragalactic Survey. CHILES VERDES provides an unprecedented combination of survey depth, duration, and cadence, with 960hr of 1-2GHz continuum VLA data obtained over 209 epochs between 2013 and 2019 in a 0.44deg2 section of the well-studied extragalactic deep field, COSMOS. We identified 18 moderate-variability sources (showing 10%-30% flux density variation) and 40 lower-variability sources (2%-10% flux density variation). They are mainly active galactic nuclei (AGNs) with radio luminosities in the range of 1022-1027W/Hz, based on cross-matching with COSMOS multiwavelength catalogs. The moderate-variability sources span redshifts z=0.22-1.56, have mostly flat radio spectra (α>-0.5), and vary on timescales ranging from days to years. The lower-variability sources have similar properties, but generally have higher radio luminosities than the moderate-variability sources, extending to z=2.8, and have steeper radio spectra (α<-0.5). No star-forming galaxy showed statistically significant variability in our analysis. The observed variability likely originates from scintillation on short (∼week) timescales, and Doppler-boosted intrinsic AGN variability on long (month-year) timescales. Description: The COSMOS HI Legacy Extragalactic Survey (CHILES) Variable and Explosive Radio Dynamic Evolution Survey (VERDES), designed to look for variable phenomena within a single VLA pointing observed at L-band (1-2GHz), using nearly 1000hr of observations obtained between 2013 and 2019. The data were taken as part of the CHILES, a survey of neutral hydrogen traced by the 21cm emission line in the COSMOS field out to an unprecedented depth of z∼0.5. The CHILES pointing was chosen to be in the COSMOS field where it can enjoy significant multiwavelength supporting data. The single L-band pointing yields a field of view 0.5° in diameter (half-power beamwidth) at 1.5GHz. The data were obtained in the VLA's B-configuration, which yields a resolution of 4.3" at 1.5GHz. See Section 2. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 90 18 Multi-band and multi-wavelength properties of our 18 CHILES VERDES moderate-variability sources table3.dat 90 40 Multi-band and multi-wavelength properties of our 40 CHILES VERDES low-variability sources fig8.dat 38 3096 Light curves for sources designated "moderate-variability" fig9.dat 38 6880 Light curves of the 40 low-variability sources -------------------------------------------------------------------------------- See also: II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007) VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998) VIII/87 : The Allen Telescope Array 20cm Survey (ATATS). I. (Croft+ 2010) VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012) VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012) J/AJ/127/2565 : Faint FIRST variable radio sources (De Vries+, 2004) J/ApJS/155/271 : CDF-South: Optical spectroscopy (Szokoly+, 2004) J/MNRAS/385/2225 : AzTEC millimetre survey of COSMOS field (Scott+, 2008) J/ApJ/690/20 : Models of AGN & black hole populations (Shankar+, 2009) J/ApJ/699/L43 : FIRST-NVSS-SDSS AGN sample catalog (Smolcic+, 2009) J/ApJS/188/384 : The VLA-COSMOS survey. IV. (Schinnerer+, 2010) J/MNRAS/415/3831 : AzTEC/ASTE source catalogue (Aretxaga+, 2011) J/ApJ/739/76 : Pi GHz Sky Survey (PiGSS). II. (Bower+, 2011) J/ApJ/740/65 : VLA search for 5GHz radio transients (Ofek+, 2011) J/ApJ/742/49 : Var. & transient radio sources in FIRST (Thyagarajan+, 2011) J/MNRAS/436/1919 : SCUBA observations of COSMOS galaxies (Casey+, 2013) J/ApJ/762/93 : PiGSS. III. ELAIS-N1, Coma & Lockman fields (Croft+, 2013) J/ApJ/769/125 : 1.4GHz radio var. in FIRST & SDSS Stripe 82 (Hodge+, 2013) J/AJ/147/143 : MOJAVE. XI. Spectral distributions (Hovatta+, 2014) J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016) J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016) J/ApJ/817/34 : C-COSMOS Legacy multiwavelength cat. (Marchesi+, 2016) J/ApJ/818/105 : CNSS pilot survey (Mooley+, 2016) J/A+A/607/A132 : VLBA observations of the COSMOS field (Herrera Ruiz+, 2017) J/ApJS/230/7 : Spectral flux densities from 50MHz to 50GHz (Perley+, 2017) J/A+A/602/A2 : VLA-COSMOS 3 GHz Large Project. II. (Smolcic+, 2017) J/A+A/602/A1 : VLA-COSMOS 3 GHz Large Project (Smolcic+, 2017) J/MNRAS/474/4396 : MASIV Survey. IV. Radio AGNs variability (Koay+, 2018) J/ApJ/874/13 : 24yr of radio observations of V404 Cygni (Plotkin+, 2019) Byte-by-byte Description of file: table[23].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- ID CHILES VERDES identifier 6- 12 A7 --- TRAP Internal ID used by TraP algorithm for source 14- 22 F9.5 deg RAdeg [149.9/150.7] Right Ascension (J2000) 24- 30 F7.5 deg DEdeg [2/2.7] Declination (J2000) 32- 36 F5.2 mJy Flux [0.09/10.4] Median integrated flux density 38- 42 F5.3 --- Var [0.01/0.3] Coefficient of variability 44- 50 F7.3 --- eta [1/804] Reduced chi-squared statistic 52- 56 F5.2 [W/Hz] logL1.4 [22.17/26.4]? Log 1.4GHz luminosity (1) 58 A1 --- l_logLx Limit flag on logLx 59- 63 F5.2 [10-7W] logLx [41/44.5]? Log 0.5-8keV X-ray luminosity from Marchesi+ 2016, J/AJ/817/34 ; in units of erg/s 65- 70 F6.3 --- alpha [-1.9/1]? The 1-4GHz spectral index 72- 77 F6.3 --- e_alpha [0.07/0.6]? Uncertainty in alpha 79- 84 F6.3 --- zbest [0.12/2.7]? Best available redshift measurement from Marchesi+ 2016, J/AJ/817/34 86- 90 A5 --- Class Classification (2) -------------------------------------------------------------------------------- Note (1): From Smolcic+ 2017, J/A+A/602/A1 Note (2): From Marchesi+ 2016, J/AJ/817/34 -- Code as follows: HLAGN = high-to-moderate luminosity AGN MLAGN = moderate-to-low luminosity AGN See Section 5. -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig[89].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- ID CHILES VERDES identifier 6- 13 E8.2 Jy Flux [6.5e-6/0.013] Integrated flux density 16- 23 E8.2 Jy e_Flux [1.4e-5/0.01] Uncertainty in Flux 26- 38 F13.5 d JD Julian Date -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 15-May-2023
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