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II/114 UV Interstellar Extinction (Savage+ 1985)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
catalog
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/114
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A Catalogue of UV Interstellar Extinction Excesses for 1415 stars
Savage B.D., Massa D., Meade M., Wesselius P.R.
<Astrophys. J. Suppl. 59, 397 (1985)>
=1985ApJS...59..397S (SIMBAD/NED BibCode)
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ADC_Keywords: Interstellar medium ; Photometry, ultraviolet ; Extinction
Description:
The documentation is mostly adapted from the "Documentation for the
Machine-Readable Version of A catalog of Ultraviolet Interstellar
Extinction Excesses for 1415 Stars" by Wayne H. Warren Jr., May 1986,
National Space Science Data Center NSSDC/WDC-A-R&S 86-05
This document describes the machine-readable version of the catalog as
it is currently being distributed from the Astronomical Data Centers.
It is intended to enable users to read and process the data without
problems and guesswork, but it is not intended to replace the original
published paper, which users should study before processing the data.
The format described below is very similar to that given on page 431
of the source reference, but some modifications were made at the ADC
(with the consent of the authors) to effect uniformity.
Introduction:
"A Catalog of Ultraviolet Interstellar Extinction Excesses for 1415
Stars" contains interstellar extinction excesses in the ultraviolet
region derived from five-channel UV photometry carried out with the
ANS spacecraft. Filters centered at approximately 155, 180, 220, 250
and 330 nm were used for the observations and excesses were derived
for each UV wavelength with reference to the V magnitude of the UBV
system. The photometric data used to derive the UV excesses are taken
from the "ANS Ultraviolet Photometry Catalogue of Point Sources
(Wesselius et al. 1982), also available in machine-readable form from
the international network of astronomical data centers (catalog II/97;
Warren 1984). For additional information concerning the source data,
object selection, extinction parameters, and relations among the color
excesses themselves and with the excess extinction in the 220-nm bump,
the source reference should be consulted.