Details on Acronym: [OIK2017] | |
| [OIK2017] | (Ota+Iye+Kashikawa+, 2017) |
| Write: | <<[OIK2017] NB973-SDF-NNNNNN>> <<[OIK2017] {NB973-SXDS}-{S|C}-NNNNN>> |
| N: | 24 |
| Object: | Poss. LAE (SIMBAD class: EmissionG = Emission-line galaxy) |
| Note: | Subaru Suprime-Cam observations of N=24 probable z=7 LAE candidates in the Subaru Deep Field and the Subaru/XMM-Newton Deep Survey field. See also [OIK2010]. |
| in source: | NAME SXDF |
| in source: | NAME SDF |
| Ref: | =2017ApJ...844...85O |
| by | OTA K. , IYE M., KASHIKAWA N., KONNO A., NAKATA F., TOTANI T., KOBAYASHI M.A.R., FUDAMOTO Y., SEKO A., TOSHIKAWA J., ICHIKAWA A., SHIBUYA T., ONOUE M. |
| Astrophys. J., 844, 85-85 (2017) | |
| A new constraint on reionization from the evolution of the Lyα luminosity function at z ~ 6-7 probed by a Deep census of z = 7.0 Lyα emitter candidates to 0.3L*. | |
| o | Table 2: <[OIK2017] NB973-SDF-NNNNNN> N=18 among (Nos 30693-155934), <[OIK2017] NB973-SXDS-A-NNNNN> N=6 among (Nos C-66280 to S-95993). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |