Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Silvermann, J."'
Autor:
Salvato, M., Ilbert, O., Hasinger, G., Rau, A., Civano, F., Zamorani, G., Brusa, M., Elvis, M., Vignali, C., Aussel, H., Comastri, A., Fiore, F., Floc'h, E. Le, Mainieri, V., Bardelli, S., Bolzonella, M., Bongiorno, A., Capak, P., Caputi, K., Cappelluti, N., Carollo, C. M., Contini, T., Garilli, B., Iovino, A., Fotopoulou, S., Fruscione, A., Gilli, R., Halliday, C., Kneib, J-P., Kakazu, Y., Kartaltepe, J. S., Koekemoer, A. M., Kovac, K., Ideue, Y., Ikeda, H., Impey, C. D., Fevre, O. Le, Lamareille, F., Lanzuisi, G., Borgne, J-F. Le, Brun, V. Le, Lilly, S. J., Maier, C., Manohar, S., Masters, D., McCracken, H., Messias, H., Mignoli, M., Mobasher, B., Nagao, T., Pello, R., Puccetti, S., Renzini, E. Perez Montero A., Sargent, M., Sanders, D. B., Scodeggio, M., Scoville, N., Shopbell, P., Silvermann, J., Taniguchi, Y., Tasca, L., Tresse, L., Trump, J. R., Zucca, E.
With this paper, we release accurate photometric redshifts for 1692 counterparts to Chandra sources in the central square degree of the COSMOS field. The availability of a large training set of spectroscopic redshifts that extends to faint magnitudes
Externí odkaz:
http://arxiv.org/abs/1108.6061
Autor:
Salvato, M., Hasinger, G., Ilbert, O., Zamorani, G., Brusa, M., Scoville, N., Rau, A., Capak, P., Arnouts, S., Aussel, H., Bolzonella, M., Buongiorno, A., Cappelluti, N., Caputi, K., Civano, F., Cook, R., Elvis, M., Gilli, R., Jahnke, K., Kartaltepe, J. S., Impey, C. D., Lamareille, F., Floch, E. Le, Lilly, S., Mainieri, V., McCarthy, P., McCracken, H., Mignoli, M., Mobasher, B., Murayama, T., Sasaki, S., Sanders, D. B., Schiminovich, D., Shioya, Y., Shopbell, P., Silvermann, J., Smolcic, V., Surace, J., Taniguchi, Y., Thompson, D., Trump, J. R., Urry, M., Zamojski, M.
Publikováno v:
Astrophys.J.690:1250-1263,2009
We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in the COSMOS field. Our template fitting classifies 46 sources as stars and 464 as non-active
Externí odkaz:
http://arxiv.org/abs/0809.2098
Autor:
Schaerer, D., Ginolfi, M., Béthermin, M., Fudamoto, Y., Oesch, P. A., Le Fèvre, Olivier, Faisst, A., Capak, P., Cassata, P., Silvermann, J., Yan, Lin, Jones, G.C., Amorín, R., Bardelli, S., Boquien, M., Cimatti, A., Dessauges-Zavadsky, M., Giavalisco, M., Hathi, N. P., Fujimoto, S., Ibar, E., Koekemoer, A., Lagache, Guilaine, Lemaux, B.C., Loiacono, F., Maiolino, R., Riechers, D., Talia, M., Toft, S., Vallini, L., Vergani, D., Zamorani, G., Zucca, E.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 643 (A3)
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643 (A3)
Astronomy and Astrophysics-A&A, 2020, 643 (A3)
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643 (A3)
International audience; The [C ii] 158 µm line is one of the strongest IR emission lines, which has been shown to trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z ∼ 2. Whether this is also the case at higher reds
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::945cc5d69678ee0d2f3e40151b1cc1b6
https://hal-amu.archives-ouvertes.fr/hal-03027619/document
https://hal-amu.archives-ouvertes.fr/hal-03027619/document
Akademický článek
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Autor:
M. Salvato, O. Ilbert, G. Hasinger, A. Rau, F. Civano, G. Zamorani, M. Brusa, M. Elvis, C. Vignali, H. Aussel, A. Comastri, F. Fiore, E. Le Floc'h, V. Mainieri, S. Bardelli, M. Bolzonella, A. Bongiorno, P. Capak, K. Caputi, N. Cappelluti, C. M. Carollo, T. Contini, B. Garilli, A. Iovino, S. Fotopoulou, A. Fruscione, R. Gilli, C. Halliday, J.-P. Kneib, Y. Kakazu, J. S. Kartaltepe, A. M. Koekemoer, K. Kovac, Y. Ideue, H. Ikeda, C. D. Impey, O. Le Fevre, F. Lamareille, G. Lanzuisi, J.-F. Le Borgne, V. Le Brun, S. Lilly, C. Maier, S. Manohar, D. Masters, H. McCracken, H. Messias, M. Mignoli, B. Mobasher, T. Nagao, R. Pello, S. Puccetti, E. Perez-Montero, A. Renzini, M. Sargent, D. B. Sanders, M. Scodeggio, N. Scoville, P. Shopbell, J. Silvermann, Y. Taniguchi, L. Tasca, L. Tresse, J. R. Trump, E. Zucca
Publikováno v:
The Astrophysical Journal, 742(2):61. IOP PUBLISHING LTD
apj
apj, 2011, 742, pp.61. ⟨10.1088/0004-637X/742/2/61⟩
apj
apj, 2011, 742, pp.61. ⟨10.1088/0004-637X/742/2/61⟩
With this paper, we release accurate photometric redshifts for 1692 counterparts to Chandra sources in the central square degree of the COSMOS field. The availability of a large training set of spectroscopic redshifts that extends to faint magnitudes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7eb94afa8debfc7d12b99aa9698e9250
https://research.rug.nl/en/publications/ceea7b58-ac78-41c3-8bbe-6858ab83f248
https://research.rug.nl/en/publications/ceea7b58-ac78-41c3-8bbe-6858ab83f248
Publikováno v:
Science (New York, N.Y.) [Science] 1970 Nov 27; Vol. 170 (3961), pp. 998-1000.