| 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. |
| Auth.: | PHARO J.+ |
| Ref: | =2019ApJ...874..125P |
| by | PHARO 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. | |
| o | Tables 4-6: <FIGS GWN NNNN> N=61 among (GS1 724-GS1 6865). |
| Ref: | =2019MNRAS.486.1358F |
| by | FERRERAS 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. | |
| o | Tables A1-A3: <FIGS GWN NNNN> N=10+14+27 among (Nos GN1 2083-GN1 2590, GN2 411-GN2 1314, GS1 724-GS1 4272). |
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