Details on Acronym: [CSR2018] | |
[CSR2018] | (Cava A.+Schaerer D.+Richard+, 2018) |
Write: | <<[CSR2018] Cosmic Snake>> <<[CSR2018] Counterimage>> <<[CSR2018] Source Galaxy>> <<[CSR2018] MACS J1206.2-0847 A.N>> <<[CSR2018] MACS J1206.2-0847 GN>> <<[CSR2018] MACS J1206.2-0847 BCG>> |
N: | 1+1+16+1+4+1 |
Object: | Grav. lensed image of a G + G + G in ClG + Brightest Cluster Galaxy (SIMBAD class: Unknown = Object of Unknown Nature) |
Note: | N=1+1+16 gravitationally lensed images of N=1 background galaxy, lensed by the galaxy cluster MCS J1206.2-0847. N=4 cluster members and N=1 brightest cluster galaxy (BCG). Use of HST CLASH data. |
Ref: | =2018NatAs...2...76C |
by | CAVA A. , SCHAERER D., RICHARD J., PEREZ-GONZALEZ P.G., DESSAUGES-ZAVADSKY M., MAYER L., TAMBURELLO V. |
NatAs, 2, 76-82 (2018) | |
The nature of giant clumps in distant galaxies probed by the anatomy of the Cosmic Snake. | |
o | <[CSR2018] Cosmic Snake> N=1. <[CSR2018] Counterimage> N=1. <[CSR2018] Source Galaxy> N=1. Fig. 8, Table 4: <[CSR2018] MACS J1206.2-0847 A.N> N=16. Fig. 8, Table 5: <[CSR2018] MACS J1206.2-0847 GN> (Nos G1-G4), <[CSR2018] MACS J1206.2-0847 BCG> N=1. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |