Dictionary of Nomenclature of Celestial Objects (Last update: 17-Feb-2020)
Result of query: info cati GPA$
Details on Acronym: GPA GPA (Galactic Plane A survey)= ([LMD2000b])
Object:? (SIMBAD class: Unknown = Object of unknown nature)
Stat:is completely incorporated in SimbadNote:Galactic Plane A survey: l = -15deg to 255deg, b = -5deg to +5deg, first images of galactic sources, HII regions, SNRs and transients. See also GPB. These observations used the NRAO/NASA Green Bank Earth Station to survey the sky simultaneously at these frequencies. These are the first results from the Galactic Plane (GP) survey observations, a program to monitor the sky at 8.35 and 14.35 GHz. The GP survey series is intended to detect short lived radio-sources. We present four independent observations of the galactic plane, combined to provide a set of reference images of the galactic plane. We compare the relative brightness of Cassiopeia A and Cygnus A and find the rate of decrease of Cassiopeia A is slower than previously reported. The first survey, GPA, covers 0.82 sr (6.5%) of the sky. A source list is presented for all sources brighter than 0.9Jy at 8.35GHz and also for all sources brighter than 2.5 Jy at 14.35 GHz.
, MINTER A., D'ADDARIO L., EBERHARDT K., KOSKI K., ZUBER J.
Astron. J., 119, 2801-2827 (2000)
The first galactic plane survey at 8.35 and 14.35 GHz.
oTable 3: <GPA LLL.ll+B.bb> N=677.
=E=Catalogue in electronic form as J/AJ/119/2801Originof the Acronym: p = Pre-registered to IAU Comm.5 Details on Acronym: [LMD2000b] [LMD2000b] (Langston+Minter+D'Addario+, 2000)
====>Equivalent to: GPAOriginof the Acronym: S = Created by Simbad, the CDS Database