J/AJ/131/100        The Molonglo Southern 4Jy sample. I         (Burgess+, 2006)

The Molonglo Southern 4Jy sample (MS4). I. Definition. Burgess A.M., Hunstead R.W. <Astron. J., 131, 100-113 (2006)> =2006AJ....131..100B 2006AJ....131..100B
ADC_Keywords: Active gal. nuclei ; Radio continuum Keywords: galaxies: active - radio continuum: galaxies - surveys Abstract: We have defined a complete sample of 228 southern radio sources at 408MHz with integrated flux densities S(408)>4.0Jy, Galactic latitude |b|>10°, and declination -85°<δ←30°. The main finding survey used was the Molonglo Reference Catalogue (Cat. VIII/16). Sources in the sample were imaged at 843MHz with the Molonglo Observatory Synthesis Telescope to obtain positions accurate to about 1", as well as flux densities and angular sizes. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 153 244 List of sources in the MS4 sample table5.dat 147 228 Radio positions, flux densities, angular sizes, and position angles for the MS4 sample refs4.dat 96 125 References for table4.dat refs5.dat 102 47 References for table5.dat -------------------------------------------------------------------------------- See also: J/AJ/131/114 : The Molonglo Southern 4Jy sample. II (Burgess+, 2006) J/ApJS/80/137 : Southern Extragalactic Radio Sources (Jones+, 1992) VIII/15 : Parkes Radio Sources Catalogue (PKSCAT90) (Wright+ 1990) VIII/16 : Molonglo Reference Catalogue of Radio Sources (Large+ 1991) VIII/34 : Parkes Half-Jansky Flat-Spectrum Sample (Drinkwater + 1997) VIII/35 : Radio Sources obs. with Culgoora Circular Array (Slee 1995) VIII/38 : Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996) VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998) J/ApJS/124/285 : VLA Images of Extragalactic Objects (Reid+, 1999) J/ApJS/90/173 : PMN map catalog of radiosources (Gregory+, 1994) Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- MRC The MRC source name 12 A1 --- f_MRC Indicates the source has more than one MRC name 14- 22 A9 --- PKS The PKS source name 24 A1 --- f_PKS Indicates the source has more than one PKS name 26- 31 A6 --- MSH The MSH source name 33- 39 F7.2 Jy S408MHz The 408MHz flux density 41- 46 F6.2 Jy e_S408MHz Error in S408MHz 48-153 A106 --- Ref Reference(s) for radio image(s) (detailed in refs4.dat) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Source name (1) 16 A1 --- f_Name Flag on Name (2) 18- 19 I2 h RAh Hour of Right Ascension (J2000) (3) 21- 22 I2 min RAm Minute of Right Ascension (J2000) (3) 24- 28 F5.2 s RAs Second of Right Ascension (J2000) (3) 30 A1 --- DE- Sign of the Declination (J2000) (3) 31- 32 I2 deg DEd Degree of Declination (J2000) (3) 34- 35 I2 arcmin DEm Arcminute of Declination (J2000) (3) 37- 40 F4.1 arcsec DEs Arcsecond of Declination (J2000) (3) 42- 48 F7.2 Jy S178MHz Estimated 178MHz flux density 49 A1 --- u_S178MHz Uncertainty flag on S178MHz 51 I1 --- n_S178MHz Order of polynomial used to calculate S178MHz 53- 56 I4 Jy S80MHz ? The 80MHz flux density (4) 58 A1 --- f_S80MHz Flag on S80MHz (5) 60- 61 A2 --- r_S80MHz Reference for S80MHz 63- 69 F7.2 Jy S408MHz The 408MHz flux density (4) 71 A1 --- f_S408MHz Flag on S408MHz (5) 73- 74 A2 --- r_S408MHz Reference for S408MHz 76- 82 F7.2 Jy S843MHz The 843MHz flux density (4) 84- 85 A2 --- f_S843MHz Flag on S843MHz (5) 87- 88 A2 --- r_S843MHz Reference for S843MHz 90- 96 F7.2 Jy S1400MHz ? The 1400MHz flux density (4) 98 A1 --- f_S1400MHz Flag on S1400MHz (5) 100-101 A2 --- r_S1400MHz Reference for S1400MHz 103-108 F6.2 Jy S2700MHz ? The 2700MHz flux density (4) 110 A1 --- f_S2700MHz Flag on S2700MHz (5) 112-113 A2 --- r_S2700MHz Reference for S2700 115-121 F7.3 Jy S5000MHz ? The 5000MHz flux density (4) 123 A1 --- f_S5000MHz Flag on S5000MHz (5) 125-126 A2 --- r_S5000MHz Reference for S5000MHz 128-132 F5.2 --- Sp+Index ? Spectral index between 408 & 2700MHz (6) 134 A1 --- f_Sp+Index Flag on Sp+Index (7) 136-137 A2 --- l_LAS [≤] Limit flag on LAS 138-141 I4 arcsec LAS ? Largest angular size at 843MHz (8) 143 A1 --- n_LAS Note on LAS (9) 145-147 I3 deg PA [-90/90]? Position angle at 843MHz (10) -------------------------------------------------------------------------------- Note (1): Taken from the MRC, unless the source has more than one MRC entry, in which case the name is from the original Parkes catalog (Bolton et al. 1964, Cat. VIII/15; Price & Milne 1965, Cat. VIII/15) or Parkes 2700MHz catalog (Bolton et al. 1979, Cat. VIII/15 and references therein). Note (2): Flag on Name, defined as follows: d = The total angular extent is almost 10° (e.g. Cooper et al. 1965AuJPh..18..589C 1965AuJPh..18..589C ), whereas that of the inner lobes is 6.8' (Jones & McAdam, 1992, Cat. J/ApJS/80/137). The position angle of the structure varies at different angular scales: for the inner lobes it is 49° (Jones & McAdam, 1992, Cat. J/ApJS/80/137). e = The position, largest angular extent and position angle are the 408MHz values from McAdam & Schilizzi (1977A&A....55...67M 1977A&A....55...67M). f = The position is that of the core in the MOST image. g = Angular size and position angle were measured from an ATCA contour map (Norris et al. 1990PASAu...8..252N 1990PASAu...8..252N), as the MOST CUTS were affected by MRC B2152-699. Note (3): At 843MHz. The reference for the radio position is the same as for S843MHz. Note (4): See text for a discussion of the various telescopes used for the flux densities measured at different frequencies. Note (5): Flag on the flux density, defined as follows: h = Flux density estimated from the radio spectrum. i = Flux density not used in estimating S178MHz. j = Variable at 843MHz (Gaensler & Hunstead 2000PASA...17...72G 2000PASA...17...72G). Note (6): Defined in the sense Sν∝να. Note (7): Flag on Sp+Index, defined as follows: b = Spectral index defined between 408 and 5000MHz. c = Spectral index defined between 843 and 5000MHz. Note (8): The reference is the same as for the 843MHz flux density, except for a few sources, noted in Section 5.1. We have imaged all sources with LAS<35" with the ATCA at 5GHz (Burgess & Hunstead, 2000, Cat. J/AJ/131/114), with the exception of MRC B0521-365, MRC B0743-673, MRC B1740-517, MRC B1814-519, MRC B2153-699, and MRC B2259-375. Note (9): Note on LAS, defined as follows: d = separation of peaks of a double source; e = largest separation of peaks of a complex source; l = largest size of low-surface-brightness emission in a complex source: the position angle given is that of the central axis; m = deconvolved extent along the axis of a source, as in Jones & McAdam (1992, Cat. J/ApJS/80/137). Note (10): Defined in degrees east of north (modulo 90). The reference is the same as for the 843MHz flux density, except for a few sources which are noted in Section 5.1. -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs4.dat refs5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref Reference number 5- 23 A19 --- Bibcode Bibcode 25- 50 A26 --- Aut Author's name 52-102 A51 --- Com Comment -------------------------------------------------------------------------------- History: From electronic version of the journal References: Burgess & Hunstead, Paper II 2006AJ....131..114B 2006AJ....131..114B, Cat. J/AJ/131/114
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 17-Aug-2006
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