VIII/68             Huchtmeier-Richter HI catalog          (Huchtmeier+ 1989)

A General Catalog of HI Observations of Galaxies I. The Reference Huchtmeier W.K., Richter O.-G., Bohnenstengel H.D., Hauschildt M. <Springer-Verlag (1989)> =1989H&RHI.C......0H 1989H&RHI.C......0H
ADC_Keywords: Galaxies, radio ; H I data ; Rotational velocities Description: The catalog contains all published HI observations (21cm) of external galaxies published until the middle of 1988. It contains almost 20,000 entries for over 10,000 galaxies based on more than 570 references. The HI data are basically just as they were originally published -- no numerical conversions were made and no error correction was attempted. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 136 19976 General Catalog of HI Observations of Galaxies refs.dat 137 715 List of H I References, ordered by sequence number -------------------------------------------------------------------------------- See also: VIII/77 : HI spectral properties of galaxies (Springob+, 2005) J/A+A/286/17 : 21cm obs. of galaxies in Psc-Per Supercl. (Seeberger+ 1994) J/A+A/465/71 : 21cm observations of 452 galaxies (Theureau+, 2007) J/AJ/117/2039 : Sc galaxies photometry, 21cm data (Haynes+, 1999) http://w0.sao.ru/cats/ : the CATS database home page Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Name Galaxy Name 16- 17 I2 h RAh ? Right Ascension B1950 (hours) 19- 20 I2 min RAm ? Right Ascension B1950 (minutes) 22- 25 F4.1 s RAs ? Right Ascension B1950 (seconds) 27 A1 --- DE- Declination B1950 (sign) 28- 29 I2 deg DEd ? Declination B1950 (degrees) 31- 32 I2 arcmin DEm ? Declination B1950 (minutes) 34- 35 I2 arcsec DEs [0,60]? Declination B1950 (seconds) 37- 41 A5 --- MType Morphological type 42 A1 --- p [p] 'p' for peculiar morphological type 44- 45 I2 deg i ? inclination used by the authors (0=face-on) 47- 51 F5.2 [solMass] Mtot ? Total HI mass (or an upper limit) 53- 56 A4 --- Param [FH Int LogM MHI Smax] Flux type (1) 57 A1 --- l_value Limit flag on value 58- 67 F10.4 --- value ? Value of parameter (1) 69- 76 F8.3 --- e_value ? Mean error on value (1) 79 I1 --- n_RV ? Frame of radial velocity (2) 81- 85 I5 km/s RV ? Radial velocity in various frames (see n_RV) 86 A1 --- f_RV [-] indicates a range of RV searched (3) 87- 91 I5 km/s e_RV ? Mean error on RV, or upper limit of velocity range (3) 93- 95 I3 km/s W50 ? HI line width measured at 50% peak intensity 97- 99 I3 km/s W ? Line width at another level (4) 101 I1 --- n_W ? Level of width (4) 103-109 F7.3 Mpc D ? distance D used by the authors 110-115 F6.2 arcmin a ? Major axis 116-121 F6.2 arcmin b ? Minor axis 123-125 I3 km/s Vmax ? maximum rotational velocity 127-129 I3 deg PA [-30,360[? Dynamical position angle 131-133 I3 --- Ref Reference, detailed in refs.dat 135 A1 --- Tel Code of telescope used (5) 136 A1 --- n_Ref [x] reference contains additional material (6) -------------------------------------------------------------------------------- Note (1): Different parameters may occur in that column, depending on Param: Int = integrated flux = ∫(S.dv) in Jy.km/s FH = reduced HI mass FH in 10+6solMass/Mpc2 MHI = total H1 mass in 10+9solMass LogM = log of total HI mass in [solMass] S = upper limit for the peak flux in mJy Note (2): the Velocity frame is numbered as follows: 0 = Heliocentric velocity (HI radial velocity) 1 = RC2 system (HI radial velocity) 2 = Local Group velocity (HI radial velocity) 3 = LSR Velocity (HI radial velocity) 5 = Heliocentric velocity (optical radial velocity) 6 = RC2 system (optical radial velocity) 7 = Local Group velocity (optical radial velocity) 8 = LSR Velocity (optical radial velocity) Note (3): A range of searched velocities is provided when the HI line could not be found -- indicated by a minus (-) in column f_RV Note (4): the code used for the width definition is as follows: 1, 2 = 0% 3 = 50% of average flux (used only by some Arecibo observers) 4, 6 = 20% of peak flux 5, 7 = 25% of peak flux 8 = Rectangle model (used by some Nancay observers) 9 = Triangle model (used by some Nancay observers) Note (5): the telescope used is coded as follows: A = Arecibo 1000 ft, "circular" feed a = Arecibo 1000 ft, "flat" feed B = NRAO Green Bank 140 ft C = Cambridge 1/2 mile, 1 mile, or 5 km D = Dwingelo 25m E = Effelsberg 100m F = Dominion Radio Astrophysical Observatory 25m G = NRAO Green Bank 300 ft H = Agassiz Harvard 60 ft I = I.A.R. 30m J = Jodrell Bank 250 ft K = Jodrell Bank Mark II L = Potts Hill 36 ft M = Hat Creek 85 ft N = Nancay 30-300m O = Owens Valley P = Parkes 64m Q = Murraybank 21 ft R = RATAN 600m S = Ohio State 260 ft V = NRAO Very Large Array (VLA, 27x25m) W = Westerbork S.R.T. (15x25m) X = NRAO Green Bank Interferometer (3x85ft) Note (6): some graphical representation of the observations (e.g. a profile) and/or a photograph of this object is given in the reference, -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref Reference number 4 A1 --- m_Ref [a-h] Multiple reference 6- 24 A19 --- BibCode BibCode 26- 67 A42 --- Aut Author's name 69-138 A70 --- Com Comments -------------------------------------------------------------------------------- History: * 16-Jul-2001: The catalog was acquired from the CATS database (http://w0.sao.ru/cats/) * 06-Dec-2012: Fixed the equinox of the positions (was originally annotated as J2000 positions)
(End) Francois Ochsenbein [CDS] 16-Jul-2001
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