J/ApJS/105/369                   Galactic H I column densities (Murphy+ 1996)

Galactic H I column densities toward quasars and active galactic nuclei Murphy E.M., Lockman F.J., Laor A., Elvis M. <Astrophys. J. Suppl. Ser. 105, 369 (1996)> =1996ApJS..105..369M 1996ApJS..105..369M
ADC_Keywords: QSOs ; Active gal. nuclei ; H I data Keywords: Galaxy: structure - radio lines: ISM - X-rays: general Abstract: We have determined accurate values of the Galactic neutral hydrogen column density, NH, toward 220 quasars and active galactic nuclei from 21cm H I measurements made on the 130 Foot Telescope (42.7m). Accurate values of NH have now been obtained for the whole PG bright quasar sample and most quasars that have been observed by ROSAT and the Hubble Space Telescope through mid-1993. The spectra were corrected for stray 21cm radiation yielding values of NH with a typical uncertainty of 1x1019cm-2 for high Galactic latitude directions. The H I column densities will be useful for correcting for interstellar opacity at UV and soft X-ray wavelengths, and for estimating the reddening and extinction toward these objects. Description: The file data.fit contains the data for all 220 objects as FITS IMAGE extensions. The spectrum for each object is written as an image extension in the same order as printed in table 1 (and the FITS table in the first file). The data are written as 1-dimensional spectra and are in units of brightness temperature in Kelvins. In the header, the LSR velocity (CRVAL1), the reference pixel (CRPIX1), and the velocity increment (CRPIX1) can by used to calculate the LSR velocity of a given pixel. Note that the data are linear in frequency, not velocity, and this must be taken into account when calculating the velocity of a given pixel. The FITS files were written using the CFITSIO package written by Dr. William Pence at the GSFC. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 66 220 Summary of 21 cm H I observations data.fit 2880 441 FITS IMAGE Extension file of spectra -------------------------------------------------------------------------------- Byte-per-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Object Object name 18- 24 F7.3 deg RAdeg Right ascension, 1950 26- 32 F7.3 deg DEdeg Declination, 1950 34- 40 F7.3 deg GLon Galactic longitude 42- 48 F7.3 deg GLat Galactic latitude 50- 54 F5.1 cm-2 NH_Thin Optically thin H I column density 56- 60 F5.1 cm-2 NH_TS150 Uniform temp 150 K H I column density 62 I1 --- Comment *Comment number 64- 66 I3 --- Image *Image extension number -------------------------------------------------------------------------------- Note on Comment: 1) Data not corrected for stray radiation 2) The listed value of NH includes emission only between LSR velocities -60km/s and +28km/s. The H I in NGC 247 itself appears in the spectrum at V_LSR>+28km/s. Note on Image: The image extension number of the data for each object in the data file, data.fit. -------------------------------------------------------------------------------- Origin: AAS CD-ROM series, Volume 7, 1996 Lee Brotzman [ADS] 22-Oct-96
(End) [CDS] 03-Feb-1997
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