Dictionary of Nomenclature of Celestial Objects
(Last update: 19-Apr-2024)

Result of query: info cati FIGS GS1$


Details on Acronym:   FIGS
   FIGS (Faint Infrared Grism Survey) Write:<<FIGS GWN NNNN>> N: 8645 Object:G  (SIMBAD class: Galaxy) Note:The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR slitless spectroscopic survey of four deep fields. Two fields are located in the Great Observatories Origins Deep Survey-North (GOODS-N) area and two fields are located in the Great Observatories Origins Deep Survey-South (GOODS-S) area. One of the southern fields selected is the Hubble Ultra Deep Field.
Only the first references citing FIGS sources are listed here. in source:NAME GOODS North Field in source:NAME GOODS South Field Ref:=2018ApJ...856..116P byPHARO 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. oTable 1: Fields GN1, GN2, GS1 and GS2 are not in SIMBAD. oTables 6-7: <[PMR2018] GWN-N.N> N=24. Tables 8-9: <FIGS GWN NNNN> N=38. Ref:=2019ApJ...874..125P byPHARO J. , MALHOTRA S., RHOADS J., CHRISTENSEN L., FINKELSTEIN S.L., GROGIN N., HARISH S., JIANG T., KIM K., KOEKEMOER A., PIRZKAL N., SMITH M., YANG H., CIMATTI A., FERRERAS I., HATHI N., HIBON P., MEURER G., OESTLIN G., PASQUALI A., RYAN R., STRAUGHN A., WINDHORST R. Astrophys. J., 874, 125-125 (2019) Emission-line metallicities from the Faint Infrared Grism Survey and VLT/MUSE. oTables 4-6: <FIGS GWN NNNN> N=61 among (GS1 724-GS1 6865). Ref:=2019MNRAS.486.1358F byFERRERAS I. , PASQUALI A., PIRZKAL N., PHARO J., MALHOTRA S., RHOADS J., HATHI N., WINDHORST R., CIMATTI A., CHRISTENSEN L., FINKELSTEIN S.L., GROGIN N., JOSHI B., KIM K., KOEKEMOER A., O'CONNELL R., OSTLIN G., ROTHBERG B., RYAN R. Mon. Not. R. Astron. Soc., 486, 1358-1376 (2019) FIGS: spectral fitting constraints on the star formation history of massive galaxies since the cosmic noon. oTables A1-A3: <FIGS GWN NNNN> N=10+14+27 among (Nos GN1 2083-GN1 2590, GN2 411-GN2 1314, GS1 724-GS1 4272). Originof the Acronym: A = Assigned by the author(s)