Details on Acronym: HDF | |
HDF | (Hubble Deep Field) |
***** | Avoid the usage of HDF, prefer [PGG97] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [PGG97] | |
[PGG97] | (Phillips+Guzman+Gallego+, 1997)= (HDF) |
Write: | <<[PGG97] aaN-xxxx-yyyy>> |
N: | 120 |
Object: | G (SIMBAD class: Galaxy) |
Note: | HST HDF observations In the format 'aaN-xxxx-yyyy', 'aa' stands for HDF field, 'N' stands for the WFPC2 chip number, 'xxxx' and 'yyyy' give the pixel coordinates of the object See also [LKG97], [MS98b] |
in source: | NAME HDFN |
Ref: | =1997ApJ...489..543P |
by | PHILLIPS A.C. , GUZMAN R., GALLEGO J., KOO D.C., LOWENTHAL J.D., VOGT N.P., FABER S.M., ILLINGWORTH G.D. |
Astrophys. J., 489, 543-558 (1997) | |
The nature of compact galaxies in the Hubble Deep Field. I. Global properties. | |
o | in ref list: Kormendy 1985ApJ.295.73 instead of 733 |
o | Table 1: <[PGG97] aaN-xxxx-yyyy> N=71. |
Ref: | =1997ApJ...489..559G |
by | GUZMAN R. , GALLEGO J., KOO D.C., PHILLIPS A.C., LOWENTHAL J.D., FABER S.M., ILLINGWORTH G.D., VOGT N.P. |
Astrophys. J., 489, 559-572 (1997) | |
The nature of compact galaxies in the Hubble Deep Field. II. Spectroscopic properties and implications for the evolution of the star formation rate density of the universe. | |
o | Table 1: '[PGG97] aaN-xxxx-yyyy' in SIMBAD |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |