Details on Acronym: [GSF2010] | |
[GSF2010] | (Giodini+Smolcic+Finoguenov+, 2010) |
Write: | <<[GSF2010] NNNa>> |
N: | 16+7+15+11 |
Object: | Group of G (SIMBAD class: GroupG = Group of Galaxies) |
Note: | Observations of galaxy groups from the GEEC (Group Environment Evolution Collaboration) spectroscopic survey. More information available at http://quixote.uwaterloo.ca/~mbalogh/research/GEEC/ |
Ref: | =2010ApJ...714..218G |
by | GIODINI S. , SMOLCIC V., FINOGUENOV A., BOEHRINGER H., BIRZAN L., ZAMORANI G., OKLOPCIC A., PIERINI D., PRATT G.W., SCHINNERER E., MASSEY R., KOEKEMOER A.M., SALVATO M., SANDERS D.B., KARTALTEPE J.S., THOMPSON D. |
Astrophys. J., 714, 218-228 (2010) | |
Radio galaxy feedback in x-ray-selected groups from COSMOS: the effect on the intracluster medium. | |
o | Table 1: <[GSF2010] NNN> N=16 among (Nos 6-311). |
Ref: | =2011MNRAS.412.2303B |
by | BALOGH M.L. , McGEE S.L., WILMAN D.J., FINOGUENOV A., PARKER L.C., CONNELLY J.L., MULCHAEY J.S., BOWER R.G., TANAKA M., GIODINI S. |
Mon. Not. R. Astron. Soc., 412, 2303-2317 (2011) | |
Direct observational evidence for a large transient galaxy population in groups at 0.85 < z < 1. | |
o | Table 1: <[GSF2010] NNNa> N=7 among (Nos 40-213a). |
Ref: | =2012MNRAS.421.3594H |
by | HOU A. , PARKER L.C., WILMAN D.J., McGEE S.L., HARRIS W.E., CONNELLY J.L., BALOGH M.L., MULCHAEY J.S., BOWER R.G. |
Mon. Not. R. Astron. Soc., 421, 3594-3611 (2012) | |
Substructure in the most massive GEEC groups: field-like populations in dynamically active groups. | |
o | Tables 2-3:<[GSF2010] NNNa> N=4+11 among (Nos 4-362). |
Ref: | =2013MNRAS.431.1090M |
by | MOK A. , BALOGH M.L., McGEE S.L., WILMAN D.J., FINOGUENOV A., TANAKA M., GIODINI S., BOWER R.G., CONNELLY J.L., HOU A., MULCHAEY J.S., PARKER L.C. |
Mon. Not. R. Astron. Soc., 431, 1090-1106 (2013) | |
Efficient satellite quenching at z ~ 1 from the GEEC2 spectroscopic survey of galaxy groups. | |
o | Table 1: <[GSF2010] NNNa> N=11 among (Nos 40-213a). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |