Dictionary of Nomenclature of Celestial Objects
(Last update: 11-Oct-2019)

Result of query: info cati GPA$

Details on Acronym:   GPA
   GPA (Galactic Plane A survey)= ([LMD2000b]) Write:<<GPA LLL.ll+B.bb>> N: 677 Object:?  (SIMBAD class: Unknown = Object of unknown nature) Stat:is completely incorporated in Simbad Note: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. Ref:=2000AJ....119.2801L byLANGSTON G. , 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/119/2801 Originof the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym:   [LMD2000b]
   [LMD2000b] (Langston+Minter+D'Addario+, 2000) ====>Equivalent to: GPA Originof the Acronym: S = Created by Simbad, the CDS Database

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