| > %o GrG) | Details on Acronym: [DRV2022] | |
| [DRV2022] | ||
| Write: | <<[DRV2022] FVX-LAB>> <<[DRV2022] RO-HHMM>> | |
| N: | 1+2 | |
| Object: | Group of G (SIMBAD class: GroupG = Group of Galaxies) | |
| Stat: | is completely incorporated in Simbad | |
| Note: | Keck KCWI observations of N=1 Lymanα blob (LAB) and N=2 radio overdensities (RO). | |
| Ref: | =2022ApJ...926L..21D | |
| by | DADDI E. , RICH R.M., VALENTINO F., JIN S., DELVECCHIO I., LIU D., STRAZZULLO V., NEILL J., GOBAT R., FINOGUENOV A., BOURNAUD F., ELBAZ D., KALITA B.S., O'SULLIVAN D., WANG T. | |
| Astrophys. J., 926L, 21-21 (2022) | ||
| Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3. | ||
| o | Fig. 1, Table 1: <[DRV2022] FXV-LAB> N=1, <[DRV2022] RO-HHMM> (Nos RO-0958, RO-0959). | |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database | |