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J/AJ/140/1093   NGC7332/7339 and NGC 1156 HI sources from AGES  (Minchin+, 2010)

The Arecibo Galaxy Environment Survey. III. Observations toward the galaxy pair NGC 7332/7339 and the isolated galaxy NGC 1156. Minchin R.F., Momjian E., Auld R., Davies J.I., Valls-Gabaud D., Karachentsev I.D., Henning P.A., O'Neil K.L., Schneider S., Smith M.W.L., Stage M.D., Taylor R., Van Driel W. <Astron. J., 140, 1093-1118 (2010)> =2010AJ....140.1093M
ADC_Keywords: Surveys ; Clusters, galaxy ; Radio sources ; H I data Keywords: galaxies: individual (NGC 7332, NGC 7339) - radio lines: galaxies - surveys Abstract: Two 5deg2 regions around the NGC 7332/9 galaxy pair and the isolated galaxy NGC 1156 have been mapped in the 21cm line of neutral hydrogen (HI) with the Arecibo L-band Feed Array out to a redshift of ∼0.065 (∼20000km/s) as part of the Arecibo Galaxy Environment Survey. One of the aims of this survey is to investigate the environment of galaxies by identifying dwarf companions and interaction remnants; both of these areas provide the potential for such discoveries. The neutral hydrogen observations were complemented by optical and radio follow-up observations with a number of telescopes. A total of 87 galaxies were found, of which 39 (45%) were previously catalogued and 15 (17%) have prior redshifts. Two dwarf galaxies have been discovered in the NGC 7332 group and a single dwarf galaxy in the vicinity of NGC 1156. A parallel optical search of the area revealed one further possible dwarf galaxy near NGC 7332. Description: The HI survey observations of the NGC 1156 region were carried out using the 305m telescope at Arecibo Observatory between 2005 December and 2006 February and those of the NGC 7332 region between 2006 July and September. Both sets of observations used the Arecibo L-band Feed Array multibeam system and the fixed-azimuth drift observing mode to reach an integration time of around 300s/point. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 96 87 HI properties of the AGES galaxies in the NGC 7332 and NGC 1156 regions table6.dat 104 88 Optical identifications of galaxies in the NGC 1156 and NGC 7332 fields notes.dat 80 35 Individual notes
See also: J/MNRAS/383/1519 : Abell 1367 HI sources from AGES (Cortese+, 2008) J/MNRAS/415/1883 : NGC 7448 HI sources from AGES (Davies+, 2011) : AGES databases Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 4 A4 --- --- [AGES] 6- 19 A14 --- AGES AGES designation (JHHMMSS+DDMMSS) 21- 22 I2 h RAh HI Right ascension (J2000) 24- 25 I2 min RAm HI Right ascension (J2000) 27- 30 F4.1 s RAs HI Right ascension (J2000) 32- 34 F3.1 s e_RAs rms uncertainty on RA 36 A1 --- DE- HI Declination sign (J2000) 37- 38 I2 deg DEd HI Declination (J2000) 40- 41 I2 arcmin DEm HI Declination (J2000) 43- 44 I2 arcsec DEs HI Declination (J2000) 46- 47 I2 arcsec e_DEs rms uncertainty on Declination 49- 53 I5 km/s HV Heliocentric velocity (1) 55- 56 I2 km/s e_HV rms uncertainty on HV 58- 60 I3 km/s W50 Velocity width of the source line profile measured at the 50% level of peak maximum (2) 62- 63 I2 km/s e_W50 rms uncertainty on W50 65- 67 I3 km/s W20 Velocity width of the source line profile measured at the 20% level of peak maximum (2) 69- 70 I2 km/s e_W20 rms uncertainty on W20 72- 76 F5.1 mJy Fpeak Peak flux density at 21cm 78- 81 F4.1 mJy e_Fpeak rms uncertainty on Fpeak 83- 88 F6.3 Ftot Total (integrated) flux at 21cm 90- 94 F5.3 e_Ftot rms uncertainty on Ftot 96 I1 --- Flag [0/3] Detection confidence (0/1=good) (3)
Note (1): Measured as the mid-point of the H i profile at 50% of the peak flux. Note (2): The velocity widths are not corrected for instrumental broadening, turbulent motions, disc inclination or cosmological effects. Note (3): Object flags, defined as follows: 0 = source securely detected in the survey data 1 = source confirmed by follow-up observations 2 = source contaminated by RFI (none of the sources in the regions reported in this paper have this flag) 3 = marks extended sources, measured as described in Section 2.1.
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 14 A14 --- AGES AGES designation (JHHMMSS+DDMMSS) 15 A1 --- n_AGES Note, in notes.dat file 17- 18 I2 h RAh Optical Right ascension (J2000) 20- 21 I2 min RAm Optical Right ascension (J2000) 23- 27 F5.2 s RAs Optical Right ascension (J2000) 29 A1 --- DE- Optical Declination sign (J2000) 30- 31 I2 deg DEd Optical Declination (J2000) 33- 34 I2 arcmin DEm Optical Declination (J2000) 36- 39 F4.1 arcsec DEs Optical Declination (J2000) 41- 45 F5.2 s DRA Offset in right ascension, HI-optical 47- 51 F5.1 arcsec DDE Offset in declination, HI-optical 53- 57 F5.2 mag BJmag ?=- SuperCOSMOS BJ magnitude 59- 63 F5.2 mag Rmag ?=- SuperCOSMOS R magnitude 65- 69 F5.2 Msun/Lsun MHI/LB HI mass to BJ luminosity ratio 71- 74 F4.2 Msun/Lsun e_MHI/LB rms uncertainty on MHI/LB 76- 98 A23 --- Name Literature Name 100-104 I5 km/s RV ? Radial velocity from NED database
Byte-by-byte Description of file: notes.dat
Bytes Format Units Label Explanations
1 A1 --- Note Note code 3- 80 A78 --- Text Text of the note
History: From electronic version of the journal References: Auld et al., Paper I, 2006MNRAS.371.1617A Cortese et al., Paper II, 2008MNRAS.383.1519C, Cat. J/MNRAS/383/1519 Davies et al., Paper IV, 2011MNRAS.415.1883D, Cat. J/MNRAS/415/1883
(End) Patricia Vannier [CDS] 15-Mar-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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