Details on Acronym: FLS | |
| FLS | (First Look Survey) |
| ***** | Avoid the usage of FLS, prefer [MWL2008] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [MWL2008] | |
| [MWL2008] | (Muzzin+Wilson+Lacy+, 2008)= (FLS) |
| Write: | <<[MWL2008] NN>> <<[MWL2008] FLS JHHMMSS+DDMM.m>> |
| N: | 99 |
| Object: | Cluster of G (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate) |
| Stat: | is completely incorporated in Simbad |
| Note: | Catalog of 99 candidate clusters and groups of galaxies discovered in the Spitzer First Look Survey. |
| Ref: | =2008ApJ...686..966M |
| by | MUZZIN A. , WILSON G., LACY M., YEE H.K.C., STANFORD S.A. |
| Astrophys. J., 686, 966-994 (2008) | |
| The evolution of dusty star formation and stellar mass assembly in clusters: results from the IRAC 3.6, 4.5, 5.8, and 8.0 µm cluster luminosity functions. | |
| o | Table 1: <[MWL2008] NN> (Nos 0-98) = <[MWL2008] FLS JHHMMSS+DDMM.m> N=99. |
| =E= | Catalogue in electronic form as <J/ApJ/686/966/> |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |