Details on Acronym: [CWF2012] | |
| [CWF2012] | (Connelly+Wilman+Finoguenov+, 2012) |
| Write: | <<[CWF2012] DDD.dddddd+DD.dddddd>> <<[CWF2012] XRHHhNN>> <<[CWF2012] OPHHhNNN>> |
| N: | 4702+67+38 |
| Object: | G + Group of G (SIMBAD class: Unknown = Object of Unknown Nature) |
| Note: | Two samples of galaxy groups (in two CNOC2 fields, RA14h and RA21h), containing N=67 high-quality X-ray-selected systems and N=38 optically (spectroscopically) selected systems. VLT FORS2, Magellan IMACS, and Gemini GMOS follow-up spectroscopy of N=4704 sources. |
| Ref: | =2012ApJ...756..139C |
| by | CONNELLY J.L. , WILMAN D.J., FINOGUENOV A., HOU A., MULCHAEY J.S., McGEE S.L., BALOGH M.L., PARKER L.C., SAGLIA R., HENDERSON R.D.E., BOWER R.G. |
| Astrophys. J., 756, 139 (2012) | |
| Exploring the diversity of groups at 0.1 < z < 0.8 with X-ray and optically selected samples. | |
| o | Table 2: <[CWF2012] DDD.dddddd+DD.dddddd> N=4702. Tables 3-4+7: <[CWF2012] XRHHhNN> N=67 among (Nos XR14h01-XR14h47, XR21h06-XR21h69). Tables 5-6+8: <[CWF2012] OPHHhNNN> N=38 among (Nos OP14h01-OP14h40, OP21h101-OP21h140). |
| =E= | Catalogue in electronic form as <J/ApJ/756/139/> |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |