The J1030 deep survey
Creators
-
Gilli, Roberto1
- Mignoli, M.
- Nanni, R.
- Balmaverde, B.
- Brusa, M.
- Calura, F.
- Caminha, G. B.
- Cappelluti, N.
- Cappi, M.
- Chiaberge, M.
- Comastri, A.
- Costa, T.
- D'Amato, Q.
- Decarli, R.
- Iwasawa, K.
- Lanzuisi, G.
- Liuzzo, E.
- Norman, C.
- Paolillo, M.
- Peca, A.
- Prandoni, I.
- Risaliti, G.
- Rosati, P.
- Sani, E.
- Tozzi, P.
- Vanzella, E.
- Vignali, C.
- Vito, F.
- Zamorani, G.
- 1. Osservatorio di Astrofisica e Scienza dello Spazio di Bologna
Description
We report on the status of on-going, deep multi-band observations in the field around the z=6.31 QSO SDSS J1030+0524, where an overdensity of candidate Lyman Break Galaxies at the QSO redshift was found. The observations include a large program with Chandra, deep JVLA observations, and a strategic LBT program for optical spectroscopy. Additional imaging and spectroscopic coverage is provided, among others, by HST, VLT/MUSE, Keck and Spitzer data.
The J1030 field is currently the 4th deepest X-ray survey, one of the few radio fields observed at microJy depth, and the only deep multi-band survey in a highly biased region of the early Universe.
We are collecting and organizing all multi-band data in a public database that can be effectively exploited by the AGN community.
Examples of preliminary results from these data include: i) the first spectroscopic confirmation of a few galaxies at the redshift of SDSS J1030+0524, and ii) the discovery of a proto-cluster at z=1.7 around a Compton-thick FRII radio-galaxy.
Files
Gilli-AGN13_talk.pdf
Files
(5.9 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:3d72bf7bf988f9dcb86b4c52140e34fa
|
5.9 MB | Preview Download |