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Detailed Description of VIII/76
VIII/76     Leiden/Argentine/Bonn (LAB) Survey of Galactic HI  (Kalberla+ 2005)
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Leiden/Argentine/Bonn (LAB) Survey of Galactic HI
     Kalberla P.M.W., Burton W.B., Hartmann D., Arnal E.M., Bajaja E.,
     Morras R., Poeppel W.G.L.
    <Astron. Astrophys., 440, 775 (2005) >
    =2005A&A...440..775K
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ADC_Keywords: H I data ; Interstellar medium; Surveys; Radio sources; Atlases

Keywords: surveys - ISM: general - Galaxy: general - radio lines: ISM -
          ISM: clouds

Description:

    The LAB survey contains the final data release of observations of
    21-cm emission from Galactic neutral hydrogen over the entire sky,
    merging the Leiden/Dwingeloo Survey (LDS: Hartmann & Burton 1997,
    Cat. VIII/54) of the sky north of -30° with the Instituto
    Argentino de Radioastronomia Survey (IAR: Arnal et al.
    2000A&AS..142...35A and Bajaja et al. 2005, Cat. VIII/75) of the sky
    south of -25°. The angular resolution of the combined material is
    HPBW ~ 0.6°. The LSR velocity coverage spans the interval -450
    km/s to +400 km/s, at a resolution of 1.3km/s. The data were corrected
    for stray radiation at the Institute for Radioastronomy of the
    University of Bonn, refining the original correction applied to the
    LDS. The rms brightness-temperature noise of the merged database is
    0.07-0.09 K. Residual errors in the profile wings due to defects in
    the correction for stray radiation are for most of the data below a
    level of 20-40 mK. It would be necessary to construct a telescope with
    a main beam efficiency of {eta}MB>99% to achieve the same accuracy.
    The merged and refined material entering the LAB Survey of Galactic
    H I is intended to be a general resource useful to a wide range of
    studies of the physical and structural characteristices of the
    Galactic interstellar environment. The LAB Survey is the most
    sensitive Milky Way H I survey to date, with the most extensive
    coverage both spatially and kinematically.

    The Survey is available as 3-D maps, with or without Hanning smoothing,
    covering the whole ±458km/s or limited to ±250km/s range.
    The resolution of the 3-D maps is 0.5° in galactic longitude
    and latitude, and up to 1km/s in velocity.

    The survey exists also as (b,v) maps at longitude intervals
    stepped by 0.5° -- these files supersedes the FITS files
    given in the Hartmann and Burton Atlas (Cat. VIII/54)

File Summary:

FileName Lrecl Records Explanations
ReadMe 80 . This file lab.fit 2880 161052 The LAB Survey (full velocity range, 1km/s resolution) labh.fit 2880 161052 The LAB Survey (full velocity range, Hanning smoothed, 1km/s resolution) lab2.fit 2880 80438 The LAB Survey (full velocity range, 2km/s resolution) lab250.fit 2880 87668 The LAB Survey (±250km/s range, 1km/s resolution) lab250h.fit 2880 87668 The LAB Survey (±250km/s range, Hanning smoothed, 1km/s resolution) lab250hs.fit 2880 87668 The LAB Survey (±250km/s range, Hanning smoothed, including stray radiation) bvmaps.dat 16 721 List of the 721 (v,b) maps in "bvmaps" subdirectory bvmaps/* 0 721 HI Maps for constant Galactic Longitude
See also: http://www.astro.uni-bonn.de/~webrai/german/tools_labsurvey.php : the LAB Home Page Byte-by-byte Description of file: bvmaps.dat
Bytes Format Units Label Explanations
1- 5 F5.1 deg GLON Galactic longitude of the map 7- 16 A10 --- FITSfile Name of fits file in "bvmaps" subdirectory, made of 893x361 points (±450km/s velocity range, ±90° galactic latitude range)
Acknowledgements: Peter Kalberla, Bonn University ================================================================================ (End) Francois Ochsenbein [CDS] 18-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

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