J/A+A/585/A41       EBHIS spectra and HI column density maps    (Winkel+, 2016)

The Effelsberg-Bonn HI Survey: Milky Way gas. First data release. Winkel B., Kerp J., Floeer L., Kalberla P.M.W., Ben Bekhti N., Keller R., Lenz D <Astron. Astrophys. 585, A41 (2016)> =2016A&A...585A..41W 2016A&A...585A..41W (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Milky Way ; Interstellar medium ; H I data ; Spectroscopy Keywords: surveys - ISM: atoms - techniques: spectroscopic Abstract: The Effelsberg-Bonn HI Survey (EBHIS) is a new 21-cm survey performed with the 100-m telescope at Effelsberg. It covers the whole northern sky out to a redshift of z∼0.07 and comprises HI line emission from the Milky Way and the Local Volume. We aim to substitute the northern-hemisphere part of the Leiden/Argentine/Bonn Milky Way HI survey (LAB) with this first EBHIS data release, which presents the HI gas in the Milky Way regime. The use of a seven-beam L-band array made it feasible to perform this all-sky survey with a 100-m class telescope in a reasonable amount of observing time. State-of-the-art fast-Fourier-transform spectrometers provide the necessary data read-out speed, dynamic range, and spectral resolution to apply software radio-frequency interference mitigation. EBHIS is corrected for stray radiation and employs frequency-dependent flux-density calibration and sophisticated baseline-removal techniques to ensure the highest possible data quality. Detailed analyses of the resulting data products show that EBHIS is not only outperforming LAB in terms of sensitivity and angular resolution, but also matches the intensity-scale of LAB extremely well, allowing EBHIS to be used as a drop-in replacement for LAB. Data products are made available to the public in a variety of forms. Most important, we provide a properly gridded Milky Way HI column density map in HEALPix representation. To maximize the usefulness of EBHIS data, we estimate uncertainties in the HI column density and brightness temperature distributions, accounting for systematic effects. Description: The EBHIS 1st data release comprises 21-cm neutral atomic hydrogen data of the Milky Way (-600km/s<vlsr<+600km/s) as observed with the 100-m radio telescope at Effelsberg. EBHIS covers the full northern hemisphere (north of a declination of -5°). Full spectral data is provided in two forms: (1) Standard FITS data cubes, each having a size of about 20x20sq.deg. For convenience, we provide three different map projections, CAR, SIN, and SFL; see world-coordinate-system, WCS, references: Greisen & Calabretta, 2002A&A...395.1061G 2002A&A...395.1061G Calabretta & Greisen, 2002A&A...395.1077C 2002A&A...395.1077C Greisen et al., 2006A&A...446..747G 2006A&A...446..747G Note, size in longitude is 20° in absolute coordinates for CAR projection, and true-angular size for SIN and SFL projections. (2) FITS binary tables containing lists of spectra sampled on a HealPIX grid (nside=1024, Galactic coordinates, Ring indexing scheme, Gorski et al., 2005ApJ...622..759G 2005ApJ...622..759G). To make handling of the data easier, the table is split into smaller files. Each of these contains spectra belonging to one of the 192 base/parent pixels of the nside=4 pixelization. For convenience, the binary tables also contain EQ2000 and Galactic coordinate positions for each individual spectrum, as well as the associated HealPIX index. Furthermore, we provide the full northern-sky HI column density distribution, both, in a (1) HealPIX-grid binary table (nside=1024, Galactic coordinates, Ring indexing scheme) (2) Standard FITS 2D image in ZEA-projection (zenith equal area). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file nhi.dat 60 2 HI column densities fits files list nhi/* . 2 Individual HI column densities fits files cubes.dat 26 232 List of FITS data cubes fits/* . 232 Individual FITS data cubes hpxspec.dat 57 122 List of HPX-grid FITS binary tables hpx/* . 122 Individual HPX-grid FITS binary tables -------------------------------------------------------------------------------- Byte-by-byte Description of file: nhi.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- FileName Name of the fits file in subdirectory nhi 13- 60 A48 --- Title Title of the file -------------------------------------------------------------------------------- Byte-by-byte Description of file: cubes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 F5.1 deg RAdeg Right ascension (J2000) of data cube center 7- 10 F4.1 deg DEdeg Declination (J2000) of data cube center 12- 14 A3 --- WCSproj WCS projection code 16- 26 A11 --- FileName Name of the FITS file in subdirectory fits -------------------------------------------------------------------------------- Byte-by-byte Description of file: hpxspec.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.4 deg GLON Galactic longitude 10- 17 F8.4 deg GLAT Galactic latitude 19- 26 F8.4 deg RAdeg Right ascension (J2000) 28- 35 F8.4 deg DEdeg Declination (J2000) 37- 41 I5 --- NumRows Number of spectra in file 43- 45 I3 --- HPXidx HealPIX index (nside=4, RING scheme,0-based) 47- 57 A11 --- FileName Name of the FITS file in subdirectory hpx -------------------------------------------------------------------------------- Acknowledgements: Benjamin Winkel, bwinkel(at)mpifr.de
(End) Benjamin Winkel [MPIfR], Patricia Vannier [CDS] 18-Nov-2015
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