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J/A+A/505/1049   Parkes HI observations behind Milky Way II   (Schroeder+, 2009)

Parkes HI observations of galaxies behind the southern Milky Way. II. The Crux and Great Attractor regions (l∼289° to 338°). Schroeder A.C., Kraan-Korteweg R.C., Henning P.A. <Astron. Astrophys. 505, 1049 (2009)> =2009A&A...505.1049S
ADC_Keywords: Galaxy catalogs ; Galaxies, radio ; Radio lines ; Radial velocities ; Morphology Keywords: catalogs - surveys - ISM: dust, extinction - galaxies: fundamental parameters - Radio lines: galaxies - cosmology: large-scale structure of the Universe Abstract: As part of our programme to map the large-scale distribution of galaxies behind the southern Milky Way, we observed 314 optically-selected, partially-obscured galaxies in the Zone of Avoidance (ZOA) in the Crux and Great Attractor (GA) regions. An additional 29 galaxies were observed in the Vela ZOA survey region (because of the small numbers they are not discussed any further). The observations were conducted with the Parkes 64m (210 ft) radio telescope, in a single-pixel pointed mode, reaching an rms noise level of typically 2-6mJy over the velocity search range of 400<v<10500km/s. A total of 162 galaxies were detected (plus 14 galaxies in the Vela region). The detection rate is slightly higher than for the Hydra/Antlia region (52% versus 45%) observed in the same way. Description: The Parkes 64m radio telescope1 was used over four observing periods of about 10-14 days each (June 1993, April 1994, July 1995 and September 1996). Here, we report on the observations that cover the Crux and Great Attractor Zone of Avoidance regions. A detailed description of the observational set-up is given in Paper I (Kraan-Korteweg et al. 2002, Cat. J/A+A/391/887). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 150 162 HI-detections in the Crux and Great Attractor region
See also: B/denis : The DENIS database (DENIS Consortium, 2005) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) J/A+A/391/887 : Redshifts in the Hydra/Antlia Extension (Kraan-Korteweg+, 2002) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Name Source name (WKKNNNN, ICNNNN or YNNN-N) 9- 11 A3 --- f_Name Uncertain identification flag (1) 13- 25 A13 --- OName Other name 27- 28 A2 --- IR [MID ] Identification in the infrared (IR) and near-infrared (NIR) (2) 30- 31 I2 h RAh ? Right ascension (J2000) 33- 34 I2 min RAm ? Right ascension (J2000) 36- 39 F4.1 s RAs ? Right ascension (J2000) 41 A1 --- DE- Declination sign (J2000) 42- 43 I2 deg DEd ? Declination (J2000) 45- 46 I2 arcmin DEm ? Declination (J2000) 48- 49 I2 arcsec DEs ? Declination (J2000) 50 A1 --- u_DEs Uncertainty flag on Position 52- 57 F6.2 deg GLON ? Galactic longitude 59- 64 F6.2 deg GLAT ? Galactic latitude 66- 70 A5 --- MType Morphological type 72- 74 I3 arcsec D ? Major axis diameter 75 A1 --- --- [x] 76- 78 I3 arcsec d ? Minor axis diameter 80- 83 F4.1 mag Bj ? Apparent BJ magnitude 84 A1 --- n_Bj [NR] Unexplained meaning 86- 89 F4.2 mag E(B-V) Galactic reddening at the position of the galaxy 91 A1 --- l_HRV Limit flag on HRV 92- 96 I5 km/s HRV Heliocentric HI radial velocity (3) 97 A1 --- u_HRV Uncertainty flag on HRV 99-102 I4 km/s DV50 ? Velocity width of the HI profile measured at the 50% level of the peak intensity 103 A1 --- u_DV50 Uncertainty flag on DV50 105-107 I3 km/s DV20 ? Velocity width of the HI profile measured at the 20% level of the peak intensity 108 A1 --- u_DV20 Uncertainty flag on DV20 110-115 F6.2 Jy.km/s Sint ? Integrated HI flux density uncorrected for finite beam size 116 A1 --- u_Sint Uncertainty flag on integrated HI flux 118-120 F3.1 --- rms ? rms noise level 122 A1 --- hann [n] n for no Hanning-smoothing (4) 124 A1 --- n_Name [*] * indicates a note (5) 126-129 F4.1 arcmin Dist ? Angular distance of the detected galaxy from the centre of the beam in arcminutes 131-135 F5.1 Jy.km/s Sc ? Corrected flux density for off-centre detection 137-150 A14 --- RFI Excised RFI (radio frequency interference) on or near the detected HI profile
Note (1): Note as follows: ? = uncertain identification of the HI signal + = more than one signal was found in the pointing or in the associated OFF-observation Note (2): Flag as follows: I = indicates an entry in the IRAS Point Source Catalog (II/125) according to the precepts explained in Woudt & Kraan-Korteweg (2001, Cat. J/A+A/380/441) M = an entry in the 2MASS Extended Objects Catalogue (2MASS, 2003, Cat. VII/233) D = indicates an entry in the DENIS catalogue by Vauglin et al. (2002, Cat. J/A+A/387/1 Note (3): Heliocentric HI radial velocity taken at the midpoint of the HI profile at the 20% level. Note (4): Most spectra have been Hanning-smoothed, except when the line width was smaller than 100km/s or for other reasons (see below), which is indicated with an 'n' for 'no Hanning-smoothing'. Note (5): Notes on individual sources are: WKK0969 = see plot of WKK1117 WKK2576 = the signal is blended with WKK2595 and WKK2597 (cf. text), the width and velocity of the narrow peak are given here WKK2597 = see plot of WKK2595 WKK2863 = see plot of WKK2844 WKK4016 = the signal is blended with WKK4022, the velocity measurements refer to the narrow peak at v∼4640km/s only WKK5299 = the parameters are uncertain due to an RFI at the edge of the profile at v∼4500km/s WKK5616 = see plot of WKK5659 WKK5636 = Hanning-smoothed once despite the narrow line, due to ringing in the spectrum WKK5829 = not Hanning-smoothed due to an RFI close to the profile at v=4550km/s WKK5993 = the profile of WKK5999 (see separate pointing) has been excluded from the profile measurement WKK6680 = once Hanning-smoothed for the plot
History: * 16-Oct-2009: From electronic version of the journal * 19-Nov-2014: Corrected table1 with input from author (Anja Schroeder) which concerns the optical name of WKK2542, WKK2597, WKK5760, and WKK7149; the HI flux was also added to WKK3278. References: Kraan-Korteweg et al., Paper I 2002A&A...391..887K, Cat. J/A+A/391/887
(End) Patricia Vannier [CDS] 15-Oct-2009
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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