The relationship between stellar and black hole mass in submillimetergalaxies
(2005)
Journal Article
Borys, C., Smail, I., Chapman, S., Blain, A., Alexander, D., & Ivison, R. (2005). The relationship between stellar and black hole mass in submillimetergalaxies. Astrophysical Journal, 635(2), 853-863. https://doi.org/10.1086/491617
Outputs (10)
The Extended Chandra Deep Field-South Survey: Chandra Point-Source Catalogs (2005)
Journal Article
Lehmer, B., Brandt, W., Alexander, D., Bauer, F., Schneider, D., Tozzi, P., …Vignali, C. (2005). The Extended Chandra Deep Field-South Survey: Chandra Point-Source Catalogs. Astrophysical Journal Supplement, 161(1), 21-40. https://doi.org/10.1086/444590We present Chandra point‐source catalogs for the Extended Chandra Deep Field–South (E‐CDF‐S) survey. The E‐CDF‐S consists of four contiguous 250 ks Chandra observations covering an approximately square region of total solid angle ≈0.3 deg2, which fla... Read More about The Extended Chandra Deep Field-South Survey: Chandra Point-Source Catalogs.
The X-ray spectral properties of scuba galaxies (2005)
Journal Article
Alexander, D., Bauer, F., Chapman, S., Smail, I., Blain, A., Brandt, W., & Ivison, R. (2005). The X-ray spectral properties of scuba galaxies. Astrophysical Journal, 632(2), 736-750. https://doi.org/10.1086/444342Deep SCUBA surveys have uncovered a large population of massive submillimeter-emitting galaxies (SMGs; f850m 4 mJy) at z 1. Although it is generally believed that these galaxies host intense star formation activity, there is growing evidence that a s... Read More about The X-ray spectral properties of scuba galaxies.
The population of BzK-selected ulirgs at z similar to 2 (2005)
Journal Article
Daddi, E., Dickinson, M., Chary, R., Pope, A., Morrison, G., Alexander, D., …Renzini, A. (2005). The population of BzK-selected ulirgs at z similar to 2. Astrophysical Journal, 631(1), L13-L16. https://doi.org/10.1086/496918
The Chandra deep field South/GOODS survey - Optically faint X-raysources (2005)
Journal Article
Mainieri, V., Rosati, P., Tozzi, P., Bergeron, J., Gilli, R., Hasinger, G., …Zheng, W. (2005). The Chandra deep field South/GOODS survey - Optically faint X-raysources. Astronomy & Astrophysics, 437(3), 805-821. https://doi.org/10.1051/0004-6361%3A20041212
AGN host galaxies at z similar to 0.4-1.3: Bulge-dominated and lackingmerger-AGN connection (2005)
Journal Article
Grogin, N., Conselice, C., Chatzichristou, E., Alexander, D., Bauer, F., Hornschemeier, A., …Urry, C. (2005). AGN host galaxies at z similar to 0.4-1.3: Bulge-dominated and lackingmerger-AGN connection. Astrophysical Journal, 627(2), L97-L100. https://doi.org/10.1086/432256
Correlations between bright submillimetre sources and low-redshiftgalaxies (2005)
Journal Article
Almaini, O., Dunlop, J., Willott, C., Alexander, D., Bauer, F., & Liu, C. (2005). Correlations between bright submillimetre sources and low-redshiftgalaxies. Monthly Notices of the Royal Astronomical Society, 358(3), 875-882
Rapid growth of black holes in massive star-forming galaxies (2005)
Journal Article
Alexander, D., Smail, I., Bauer, F., Chapman, S., Blain, A., Brandt, W., & Ivison, R. (2005). Rapid growth of black holes in massive star-forming galaxies. Nature, 434(7034), 738-740. https://doi.org/10.1038/nature03473
The unresolved hard X-ray background: the missing source populationimplied by the Chandra and XMM-Newton deep fields (2005)
Journal Article
Worsley, M., Fabian, A., Bauer, F., Alexander, D., Hasinger, G., Mateos, S., …Schneider, D. (2005). The unresolved hard X-ray background: the missing source populationimplied by the Chandra and XMM-Newton deep fields. Monthly Notices of the Royal Astronomical Society, 357(4), 1281-1287
A Chandra observation of the z = 2.285 galaxy FSC 10214+4724: evidencefor a Compton-thick quasar? (2005)
Journal Article
Alexander, D., Chartas, G., Bauer, F., Brandt, W., Simpson, C., & Vignali, C. (2005). A Chandra observation of the z = 2.285 galaxy FSC 10214+4724: evidencefor a Compton-thick quasar?. Monthly Notices of the Royal Astronomical Society, 357(1), L16-L20