Details on Acronym: [PMR2018] | |
| [PMR2018] | (Pharo+Malhotra+Rhoads+, 2018) |
| Write: | <<[PMR2018] GWN-N.N>> |
| N: | 24 |
| Object: | Poss. Overdensity (SIMBAD class: GroupG_Candidate = Group of Galaxies Candidate) |
| Note: | N=24 potential overdensities in the four fields of the Faint Infrared Grism Survey (FIGS). Use of FIGS And CANDELS data. |
| in source: | NAME GOODS North Field |
| in source: | NAME GOODS South Field |
| Ref: | =2018ApJ...856..116P |
| by | PHARO J. , MALHOTRA S., RHOADS J., RYAN R., TILVI V., PIRZKAL N., FINKELSTEIN S., WINDHORST R., GROGIN N., KOEKEMOER A., ZHENG Z., HATHI N., KIM K., JOSHI B., YANG H., CHRISTENSEN L., CIMATTI A., GARDNER J.P., ZAKAMSKA N., FERRERAS I., HIBON P., PASQUALI A. |
| Astrophys. J., 856, 116-116 (2018) | |
| Spectrophotometric redshifts in the Faint Infrared Grism Survey: finding overdensities of faint galaxies. | |
| o | Table 1: Fields GN1, GN2, GS1 and GS2 are not in SIMBAD. |
| o | Tables 6-7: <[PMR2018] GWN-N.N> N=24. Tables 8-9: <FIGS GWN NNNN> N=38. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |