J/PASP/113/10       Sub-mJy radio sources complete sample        (Masci+, 2001)

A new complete sample of submilliJansky radio sources: an optical and near-infrared study. Masci F.J., Condon J.J., Barlow T.A., Lonsdale C.J., Xu C., Shupe D.L., Pevunova O., Fang F., Cutri R. <Publ. Astron. Soc. Pac. 113, 10 (2001)> =2001PASP..113...10M 2001PASP..113...10M
ADC_Keywords: Radio sources ; Photometry, infrared Abstract: The Very Large Array has been used in C configuration to map an area ~=0.3deg2 at 1.4GHz with 5σ sensitivities of 0.305, 0.325, 0.380, and 0.450mJy/beam over four equal subareas. Radio properties are presented for 62 detected sources. Deep optical imaging to Gunn r ~=25mag using the Hale 5m telescope covering ~=0.21deg2 is reported for a subset of 43 sources. This optical follow-up is much deeper than that of existing larger area radio surveys of similar radio sensitivity. Archival J-, H-, and K-band photometry from the Two-Micron All Sky Survey is also presented. Using a robust likelihood ratio technique, we optically identified 26 radio sources with probability ≳80%, nine with uncertain/ambiguous detections, and eight with empty fields. Comparisons with a stellar synthesis model that includes radio emission and dust reddening suggest that the near-infrared-optical emission in a small, bright subsample is reddened by "optically thin" dust with absorption AV~=22.5mag, regardless of morphological type. This is consistent with other, more direct determinations of absorption. The radio-optical(-near-infrared) flux ratios of early-type galaxies require significant contamination in the radio by an active galactic nucleus, consistent with the current paradigm. Using our simple modeling approach, we also discuss a potential diagnostic for selecting ultraluminous infrared galaxies to z~=1.6 from microJansky radio surveys. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 113 62 Catalog of radio source data table3.dat 131 43 Complete sample of sub-mJy radio sources -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- [MCB2001] Source name (RAD JHHMMSS+DDMM) 17- 18 A2 --- m_[MCB2001] [C1 C2] Multiplicity index on [MCB2001] 20- 21 I2 h RAh Right ascension (J2000.0) 23- 24 I2 min RAm Right ascension (J2000.0) 26- 31 F6.3 s RAs Right ascension (J2000.0) 33 A1 --- DE- Declination sign (J2000.0) 34- 35 I2 deg DEd Declination (J2000.0) 37- 38 I2 arcmin DEm Declination (J2000.0) 40- 44 F5.2 arcsec DEs Declination (J2000.0) 46- 49 F4.2 arcsec e_RAs rms uncertainty on right ascension 51- 54 F4.2 arcsec e_DEs rms uncertainty on declination 56- 61 F6.3 mJy Sp Peak flux density at 1.4GHz 63- 67 F5.3 mJy e_Sp rms uncertainty on Sp 69- 74 F6.3 mJy ST Total flux density at 1.4GHz 76- 80 F5.3 mJy e_ST rms uncertainty on ST 82- 87 F6.3 arcsec ThetaM FWHM of the major axis (from Gaussian fits) 89- 94 F6.3 arcsec Thetam FWHM of the minor axis (from Gaussian fits) 96- 98 I3 deg PA Position angle 100-104 F5.3 arcsec e_ThetaM rms uncertainty on ThetaM 106-110 F5.3 arcsec e_Thetam rms uncertainty on Thetam 112-113 I2 deg e_PA rms uncertainty on PA -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- [MCB2001] Source name (RAD JHHMMSS+DDMM) 17- 18 A2 --- m_[MCB2001] [C1 C2] Multiplicity index on [MCB2001] 19 A1 --- n_[MCB2001] [d] Note on [MCB2001] (1) 21- 22 I2 h RAh ? Optical right ascension (J2000.0) 24- 25 I2 min RAm ? Optical right ascension (J2000.0) 27- 32 F6.3 s RAs ? Optical right ascension (J2000.0) 34 A1 --- DE- Optical declination sign (J2000.0) 35- 36 I2 deg DEd ? Optical declination (J2000.0) 38- 39 I2 arcmin DEm ? Optical declination (J2000.0) 41- 45 F5.2 arcsec DEs ? Optical declination (J2000.0) 47- 50 F4.2 arcsec DRO ? optical-radio position separation 52- 57 F6.3 --- log(LR) ? logarithm of the likelihood ratio 59- 60 A2 --- l_Rid [∼ <] Limit flag on Rid (2) 61- 65 F5.3 --- Rid ? Reliability of the optical identification (2) 67 A1 --- l_rmag Limit flag on rmag 68- 73 F6.3 --- rmag ? Apparent r-band magnitude 74 A1 --- u_rmag [?] Uncertainty flag on rmag 75 A1 --- l_Jmag Limit flag on J(sigmaJ) (3) 76- 81 F6.3 --- Jmag ? J magnitude 83- 87 F5.3 --- e_Jmag ? rms uncertainty on Jmag 89- 94 F6.3 --- Hmag ? H magnitude 96-100 F5.3 --- e_Hmag ? rms uncertainty on Hmag 102 A1 --- l_KSmag Limit flag on KSmag (3) 103-108 F6.3 --- KSmag ? KS magnitude 110-114 F5.3 --- e_KSmag ? rms uncertainty on KSmag 116-120 F5.3 mag r-H ? r-H colour index 122 A1 --- l_r-K Limit flag on r-K (3) 123-127 F5.3 mag r-K ? r-K colour index 129-131 A3 --- MType Morphology (4) -------------------------------------------------------------------------------- Note (1): Optical identification is uncertain because of either extended radio emission and large offset from radio centroid position or "moderately low" LR value. Note (2): Reliability of the optical identification. Cases with "very low" and "very large" log(LR) are listed with Rid≪1 and Rid∼1, respectively. Note (3): Values with ">" are 2σ upper limits on measured fluxes Note (4): Optical morphology: E, elliptical Irr, irregular or disturbed S, spiral ?, unknown -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 05-Jun-2001
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