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J/MNRAS/342/738 HI Jodrell All Sky Survey (Lang+, 2003)
First results from the HI Jodrell All Sky Survey: inclination-dependent selection effects in a 21-cm blind survey. Lang R.H., Boyce P.J., Kilborn V.A., Minchin R.F., Disney M.J., Jordan C.A., Grossi M., Garcia D.A., Freeman K.C., Phillipps S., Wright A.E. <Mon. Not. R. Astron. Soc. 342, 738 (2003)> =2003MNRAS.342..738L
ADC_Keywords: Surveys ; H I data ; Radial velocities Keywords: surveys - galaxies: distances and redshifts - galaxies: evolution - galaxies: luminosity function, mass function - large-scale structure of Universe Abstract: Details are presented of the H I Jodrell All Sky Survey (HIJASS). HIJASS is a blind neutral hydrogen (H I) survey of the northern sky (δ>22°), being conducted using the multibeam receiver on the Lovell Telescope (full width at half-maximum beamwidth 12-arcmin) at Jodrell Bank. HIJASS covers the velocity range -3500 to 10000 km/s, with a velocity resolution of 18.1km/s and spatial positional accuracy of ∼2.5arcmin. Thus far about 1115 deg2 of sky have been surveyed. The average rms noise during the early part of the survey was around 16mJy/beam Following the first phase of the Lovell Telescope upgrade (in 2001), the rms noise is now around 13mJy/beam. We describe the methods of detecting galaxies within the HIJASS data and of measuring their H I parameters. The properties of the resulting H I-selected sample of galaxies are described. Of the 222 sources so far confirmed, 170 (77 per cent) are clearly associated with a previously catalogued galaxy. A further 23 sources (10 per cent) lie close (within 6 arcmin) to a previously catalogued galaxy for which no previous redshift exists. A further 29 sources (13 per cent) do not appear to be associated with any previously catalogued galaxy. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 103 222 The sample of confirmed HIJASS sources
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 8 A8 --- HIJASS HIJASS source name (JHHMM+DD) 10- 11 I2 h RAh Right ascension (J2000) 13- 14 I2 min RAm Right ascension (J2000) 16- 19 F4.1 s RAs Right ascension (J2000) 21 A1 --- DE- Declination sign (J2000) 22- 23 I2 deg DEd Declination (J2000) 25- 26 I2 arcmin DEm Declination (J2000) 28- 29 I2 arcsec DEs Declination (J2000) 31- 36 F6.2 Jy.km/s Sint Integrated flux density of H I line 38- 41 F4.2 Jy.km/s e_Sint rms uncertainty on Sint 43- 47 I5 mJy Speak 21cm peak flux density 49- 52 F4.1 mJy rms rms noise 54- 57 I4 km/s BRV Barycentric velocity 59- 61 I3 km/s DV20 Velocity width at 20% of the peak flux 63- 65 I3 km/s DV50 Velocity width at 50% of the peak flux 67- 70 A4 --- Class Classificiation (1) 72- 95 A24 --- OName Optical counterpart 96- 99 F4.1 arcmin Offset ? Position offset of the optical counterpart from the H I position 101-103 I3 km/s OffVel ? Velocity offset of the barycentric velocity contained within NED from the barycentric velocity as measured by HIJASS
Note (1): Classification use the following symbols: ASS: object within NED which is spatially coincident with the HIJASS source (i.e. within 6 arcmin) but for which no redshift is listed in NED ASS*: If there is more than one galaxy within 6 arcmin in NED ID: object in NED which matches the HIJASS source in both position and space (defined as being within 6 arcmin and 100km/s) ID*: ID which have been detected in H I for the first time by HIJASS PUG: previously uncatalogued galaxy
History: From electronic version of the journal
(End) James Marcout, Patricia Vannier [CDS] 11-Sep-2003
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