J/MNRAS/446/3199    24um fluxes of GOODS-S AGN          (Garcia-Gonzalez+, 2015)

Selection of AGN candidates in the GOODS-South Field through Spitzer/MIPS 24 µm variability. Garcia-Gonzalez J., Alonso-Herrero A., Perez-Gonzalez P.G., Hernan-Caballero A., Sarajedini V.L., Villar V. <Mon. Not. R. Astron. Soc., 446, 3199-3223 (2015)> =2015MNRAS.446.3199G 2015MNRAS.446.3199G (SIMBAD/NED BibCode)
ADC_Keywords: Active gal. nuclei ; Galaxies, IR ; Photometry, infrared Keywords: galaxies: active - infrared: galaxies Abstract: We present a study of galaxies showing mid-infrared variability in data taken in the deepest Spitzer/MIPS 24µm surveys in the Great Observatory Origins Deep Survey South field. We divide the data set in epochs and subepochs to study the long-term (months-years) and the short-term (days) variability. We use a χ2-statistics method to select active galactic nucleus (AGN) candidates with a probability ≤1% that the observed variability is due to statistical errors alone. We find 39 (1.7% of the parent sample) sources that show long-term variability and 55 (2.2% of the parent sample) showing short-term variability. That is, 0.03sources/arcmin2 for both, long-term and short-term variable sources. After removing the expected number of false positives inherent to the method, the estimated percentages are 1.0 and 1.4% of the parent sample for the long term and short term, respectively. We compare our candidates with AGN selected in the X-ray and radio bands, and AGN candidates selected by their IR emission. Approximately, 50% of the MIPS (Multiband Imaging Photometer for Spitzer) 24µm variable sources would be identified as AGN with these other methods. Therefore, MIPS 24µm variability is a new method to identify AGN candidates, possibly dust obscured and low-luminosity AGN, that might be missed by other methods. However, the contribution of the MIPS 24µm variable identified AGN to the general AGN population is small (≤13%) in GOODS-South. Description: We compiled all the data taken around the GOODS South field with the MIPS instrument at 24µm by querying the Spitzer Heritage Archive.1 This field was observed by Spitzer during several campaigns from 2004 January to 2007 March. We focused our study on a region around RA=03:32:36 (J2000) and DE=-27:48:39 (J2000). These data correspond to different observing proposals from different PI, including the Guaranteed Time Observations programme (GTO, PI: G. Rieke) and the GOODS programme (PI: M. Dickinson). We have obtained 151 AORs (Astronomical Observation Request) but only downloaded 127 because the others were from the SWIRE (Spitzer Wide-area InfraRed Extragalactic) survey and were not sufficiently deep. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tabled1.dat 106 39 Catalogue of the long-term variable candidates tablee1.dat 99 55 Catalogue of the short-term variable candidates -------------------------------------------------------------------------------- See also: J/A+A/428/1043 : Redshifts from VIMOS VLT Deep Survey (Le Fevre+, 2004) J/A+A/437/883 : K20 survey: spectroscopic catalogue (Mignoli+, 2005) J/A+A/449/951 : GOODS-MUSIC sample: multicolour catalog (Grazian+, 2006) J/ApJS/179/95 : VLA survey of CDF-S. II. (Mainieri+, 2008) J/A+A/512/A12 : VLT/VIMOS spectroscopy in GOODS-South field (Balestra+, 2010) Byte-by-byte Description of file: tabled1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- ID Identification number 6 A1 --- f_ID [*] *: in the E-CDFS 7- 9 A3 --- n_ID [a,b ] Note (G1) 12- 21 F10.7 deg RAdeg Right ascension (J2000) 23- 33 F11.7 deg DEdeg Declination (J2000) 35- 37 I3 uJy Flux1 Spitzer/MIPS 24um Flux [epoch 1] 39- 40 I2 uJy e_Flux1 rms uncertainty on Flux1 42- 44 I3 uJy Flux3 Spitzer/MIPS 24um Flux [epoch 3] 46- 47 I2 uJy e_Flux3 rms uncertainty on Flux3 49- 51 I3 uJy Flux6 Spitzer/MIPS 24um Flux [epoch 6] 53- 54 I2 uJy e_Flux6 rms uncertainty on Flux6 56- 58 I3 uJy Flux7 Spitzer/MIPS 24um Flux [epoch 7] 60- 61 I2 uJy e_Flux7 rms uncertainty on Flux7 63- 65 I3 uJy <Flux> Mean 24um flux 67- 71 F5.2 --- chi2 Chi2 value 73- 76 F4.1 % Var Measure of the variability (Var=[(Fmax-Fmin)/]*100) 78- 81 F4.2 --- Rmax Maximum to minimum flux ratio (Dmax/Fmin) 83- 86 F4.2 --- zph ? Photometric redshift 88- 92 F5.3 --- zsp ? Spectrocopic redshift (G2) 94- 98 F5.2 --- R ?=- COMBO-17 R magnitude 100-102 A3 --- Xray? [YES NO] Detected in X-ray ? 104-106 A3 --- Radio? [YES NO] Detected in radio ? -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablee1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- ID Identification number 6 A1 --- f_ID [*] *: in the E-CDFS 7- 9 A3 --- n_ID [a,b ] Note (G1) 12- 21 F10.7 deg RAdeg Right ascension (J2000) 23- 33 F11.7 deg DEdeg Declination (J2000) 35- 37 I3 uJy Flux7a Spitzer/MIPS 24um Flux [epoch 7a] 39- 40 I2 uJy e_Flux7a rms uncertainty on Flux7a 42- 44 I3 uJy Flux7b Spitzer/MIPS 24um Flux [epoch 7b] 46- 47 I2 uJy e_Flux7b rms uncertainty on Flux7b 49- 51 I3 uJy Flux7 Spitzer/MIPS 24um Flux [epoch 7] 53- 54 I2 uJy e_Flux7 rms uncertainty on Flux7 56- 58 I3 uJy <Flux> Mean 24um flux 60- 64 F5.2 --- chi2 Chi2 value 66- 69 F4.1 % Var Measure of the variability (Var=[(Fmax-Fmin)/]*100) 71- 74 F4.2 --- Rmax Maximum to minimum flux ratio (Dmax/Fmin) 76- 79 F4.2 --- zph ? Photometric redshift 81- 85 F5.3 --- zsp ? Spectrocopic redshift (G2) 87- 91 F5.2 --- R ?=- COMBO-17 R magnitude 93- 95 A3 --- Xray? [YES NO] Detected in X-ray ? 97- 99 A3 --- Radio? [YES NO] Detected in radio ? -------------------------------------------------------------------------------- Globasl notes: Note (G1): Notes as follows: a = in COMBO-17 catalogue and only one counterpart in 2.5" in Rainbow catalogue b = only one counterpart in 2.5" in COMBO-17 catalogue Note (G2): References for spectroscopic redshifts: ID 5080 : Grazian et al. (2006A&A...449..951G 2006A&A...449..951G, Cat. J/A+A/449/951) ID 5109, 4501 : Mignoli et al. (2005A&A...437..883M 2005A&A...437..883M, Cat. J/A+A/437/883) ID 7742, 10015, 14779, 2324, 4648, 2847 : Le Fevre et al. (2004A&A...428.1043L 2004A&A...428.1043L, Cat. J/A+A/428/1043) ID 2226, 718, 7513 : Balestra et al. (2010A&A...512A..12B 2010A&A...512A..12B, Cat. J/A+A/512/A12) ID 13601, 7761 : Mainieri et al. (2008ApJS..179...95M 2008ApJS..179...95M, Cat. J/ApJS/179/95) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 26-Jun-2015
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