Access to Astronomical Catalogues

← Click to display the menu
J/AJ/129/220    HI Parkes Zone of Avoidance Survey               (Donley+, 2005)

The H I Parkes zone of avoidance survey: the northern extension. Donley J.L., Staveley-Smith L., Kraan-Korteweg R.C., Islas-Islas J.M., Schroeder A., Henning P.A., Koribalski B., Mader S., Stewart I. <Astron. J., 129, 220-238 (2005)> =2005AJ....129..220D
ADC_Keywords: H I data ; Surveys ; Radial velocities Keywords: galaxies: distances and redshifts - galaxies: fundamental parameters - large-scale structure of universe - surveys Abstract: We present the results of the Northern extension of the HI Parkes Zone of Avoidance Survey, a blind HI survey utilizing the multibeam receiver on the Parkes 64m telescope. In the two regions studied here, l=36°-52° and l=196°-212°, |b|≤5°, we have detected 77 HI galaxies, 20 of which have been previously detected in HI. The survey has a median rms noise of 6.0mJy/beam and is complete to a mean flux density of 22mJy. We have searched for multiwavelength counterparts to the 77 galaxies detected here: 19, 27, and 11 have a likely optical, 2MASS (Cat. VII/233), and IRAS (Cat. II/125) cataloged counterpart, respectively. Description: The observations for the Northern extension of the HI Parkes ZOA survey began in 2000 October and were completed in 2002 May. The data were taken at the Parkes 64m telescope using the 21cm multibeam receiver. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 86 77 HI and derived properties table2.dat 123 42 Multiwavelength counterparts
See also: J/AJ/113/905 : HI observations of galaxies (Pantoja+ 1997) J/A+AS/117/1 : Galaxies in the "zone of avoidance". II. (Seeberger+, 1996) J/A+AS/117/369 : Galaxies in the "zone of avoidance". III. (Lercher+, 1996) VIII/73 : HI Parkes All Sky Survey Catalogue (HIPASS) (Meyer+, 2004) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- HIZOA Galaxy name (JHHMM+DDA) 11- 12 I2 h RAh Hour of Right Ascension (J2000) 14- 15 I2 min RAm Minute of Right Ascension (J2000) 17- 18 I2 s RAs [0,60] Second of Right Ascension (J2000) 19 A1 --- DE- Sign of the Declination (J2000) 20- 21 I2 deg DEd Degree of Declination (J2000) 23- 24 I2 arcmin DEm Arcminute of Declination (J2000) 26- 27 I2 arcsec DEs [0,60] Arcsecond of Declination (J2000) 29- 34 F6.2 deg GLON Galactic longitude 36- 40 F5.2 deg GLAT Galactic latitude 42 A1 --- f_F(HI) Flag on F(HI) (1) 44- 48 F5.2 Jy.km/s F(HI) Integrated HI flux density 50- 53 F4.2 Jy.km/s e_F(HI) Error on F(HI) (2) 55- 58 I4 km/s cz Velocity 60- 61 I2 km/s e_cz Error on cz 63- 65 I3 km/s V(50%) 50% velocity width 67- 68 I2 km/s e_V(50%) Error on V(50%) 70 A1 --- f_V(20%) Flag on V(20%) (3) 72- 74 I3 km/s V(20%) ? 20% velocity width 76- 77 I2 km/s e_V(20%) ? Error on V(20%) 79- 81 I3 Mpc Dist Distance to each galaxy (4) 83- 86 F4.1 [solMass] logMHI Log of the HI mass
Note (1): The flux was calculated over a smaller region to isolate the galaxy emission from that arising from a nearby galaxy. This may have led to an underestimation of the total flux. Note (2): The error we estimate for the integrated flux does not take into account the uncertainty due to baseline subtraction or the uncertainty in calibration; the total error on the integrated flux is likely to be ∼10%-15%. Note (3): The 20% velocity width could not be accurately measured. Note (4): The distance to each galaxy, Dist=vLG/H0, was calculated using its velocity in the Local Group standard of rest, vLG=vhel+300sin(l)cos(b).
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 9 A9 --- HIZOA Galaxy name 11 A1 --- n_HIZOA Individual notes (1) 13- 17 F5.2 deg GLAT ? Galactic latitude 19- 22 F4.1 --- E(B-V) ? From DIRBE/IRAS 100µm extinction maps (Schlegel et al., 1998ApJ...500..525S) 25- 47 A23 --- CName Name of the counterpart (2) 49- 51 F3.1 arcmin Sep1 ? Separation between HIZOA and CName 53- 58 F6.1 km/s Delta(v) ? Δv=v(CName)-v(HIZOA) 61- 78 A18 --- OName Optical counterpart name (2) 80 A1 --- n_OName Individual note on OName (1) 82- 84 F3.1 arcmin Sep2 ? Separation between HIZOA and OName 86-102 A17 --- 2MASX 2MASS counterpart (Cat. <VII/233>) (2) 104 A1 --- n_2MASX Individual note on 2MASX (1) 106-108 F3.1 arcmin Sep3 ? Separation between HIZOA and 2MASX 110-119 A10 --- IRAS IRAS counterpart (Cat. II/125) 121-123 F3.1 arcmin Sep4 ? Separation between HIZOA and IRAS
Note (1): Flags, defined as follows: d = There are two possible counterparts to this source, 2MASS J06254183+0346338 at a separation of 2.3' and a DSS galaxy at RA=06 25 45.1, DE=03 47 55 (separation = 1.4'). We do not have enough information to decide between the two. e = We note that there is another possible 2MASS counterpart, J06303033+0240026, at a separation of 2.7'. This candidate appears to be of earlier type than that chosen above, but cannot be excluded. f = Our HI detection was resolved into two galaxies separated by 4' by the ADBS (Cat. J/ApJS/130/177). We are unable to say to which HI galaxy the counterpart belongs. g = In addition to the counterpart listed here, we see another DSS galaxy at 06:59:38.1+06:25:19 as well as two 2MASS candidates: J06595034+0623322 (separation = 4.3') and J06595034+0623322 (separation = 4.4'). From morphology and separation arguments, we believe the candidate we have chosen is the most likely, but we can not rule out those listed here. Note (2): The references for counterparts are: ADBS = Rosenberg & Schneider, 2000, Cat. J/ApJS/130/177 CAP = Pantoja et al., 1997, Cat. J/AJ/113/905 Dw = Henning et al., 1998AJ....115..584H Rivers, 2000 (Ph.D. thesis, Univ. New Mexico) HIZSS = Henning et al. 2000AJ....119.2686H PGC = http://leda.univ-lyon1.fr, Cat. VII/237 UGC = Nilson, 1973, Cat. VII/26 WEIN = Weinberger, 1980A&AS...40..123W ZOAG = Seeberger et al., 1996, Cat. J/A+AS/117/1 2MASX J19061820+1256195 = Jarrett et al., 2000AJ....120..298J
History: From electronic version of the journal
(End) Marianne Brouty [CDS] 22-Jul-2005
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

catalogue service

© UDS/CNRS

Contact