Physics
Scientific paper
Feb 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..21050369m&link_type=abstract
VizieR On-line Data Catalog: J/ApJS/105/369. Originally published in: 1996ApJS..105..369M
Physics
Qsos, Active Gal. Nuclei, H I Data
Scientific paper
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. (1 data file).
Elvis Martin
Laor Ari
Lockman Felix J.
Murphy Eamonn M.
No associations
LandOfFree
Galactic H I column densities (Murphy+ 1996) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Galactic H I column densities (Murphy+ 1996), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galactic H I column densities (Murphy+ 1996) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1608159