| R.M. | |
| by | 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). |
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