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 |
by | LANGSTON 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. | |
o | Table 3: <GPA LLL.ll+B.bb> N=677. |
=E= | Catalogue in electronic form as J/AJ/119/2801 |
Origin | of the Acronym: p = Pre-registered to IAU Comm.5 |
Details on Acronym: [LMD2000b] | |
[LMD2000b] | (Langston+Minter+D'Addario+, 2000) |
====> | Equivalent to: GPA |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |