Zobrazeno 1 - 10
of 78
pro vyhledávání: '"Cassata, P."'
Autor:
Burgarella, D., Bogdanoska, J., Nanni, A., Bardelli, S., Béthermin, M., Boquien, M., Buat, V., Faisst, A. L., Dessauges-Zavadsky, M., Fudamoto, Y., Fujimoto, S., Giavalisco, M., Ginolfi, M., Gruppioni, C., Hathi, N. P., Ibar, E., Jones, G. C., Koekemoer, A. M., Kohno, K., Lemaux, B. C., Narayanan, D., Oesch, P., Ouchi, M., Riechers, D. A., Pozzi, F., Romano, M., Schaerer, D., Talia, M., Theulé, P., Vergani, D., Zamorani, G., Zucca, E., Cassata, P.
Publikováno v:
Burgarella, D, Bogdanoska, J, Nanni, A, Bardelli, S, Bethermin, M, Boquien, M, Buat, V, Faisst, A L, Dessauges-Zavadsky, M, Fudamoto, Y, Fujimoto, S, Giavalisco, M, Ginolfi, M, Gruppioni, C, Hathi, N P, Ibar, E, Jones, G C, Koekemoer, A M, Kohno, K, Lemaux, B C, Narayanan, D, Oesch, P, Ouchi, M, Riechers, D A, Pozzi, F, Romano, M, Schaerer, D, Talia, M, Theule, P, Vergani, D, Zamorani, G, Zucca, E, Cassata, P & ALPINE Team 2022, ' The ALMA-ALPINE [CII] survey The star formation history and the dust emission of star-forming galaxies at 4.5 < z < 6.2 ', Astronomy & Astrophysics, vol. 664, A73 . https://doi.org/10.1051/0004-6361/202142554
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 664, pp.A73. ⟨10.1051/0004-6361/202142554⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 664, pp.A73. ⟨10.1051/0004-6361/202142554⟩
Star-forming galaxies are composed of various types of galaxies. However, the luminosity functions at z ≳ 4–5 suggest that most galaxies have a relatively low stellar mass (log Mstar ∼ 10) and a low dust attenuation (AFUV ∼ 1.0). The physical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47e3dde0e04a3710c78b6004449e8301
https://curis.ku.dk/ws/files/317436910/aa42554_21.pdf
https://curis.ku.dk/ws/files/317436910/aa42554_21.pdf
Autor:
Garilli, B., McLure, R., Pentericci, L., Franzetti, P., Gargiulo, A., Carnall, A., Cucciati, O., Iovino, A., Amorin, R., Bolzonella, M., Bongiorno, A., Castellano, M., Cimatti, A., Cirasuolo, M., Cullen, F., Dunlop, J., Elbaz, D., Finkelstein, S., Fontana, A., Fontanot, F., Fumana, M., Guaita, L., Hartley, W., Jarvis, M., Juneau, S., Maccagni, D., McLeod, D., Nandra, K., Pompei, E., Pozzetti, L., Scodeggio, M., Talia, M., Cresci, G., Fynbo, J. P. U., Hathi, N. P., Hibon, P., Koekemoer, A. M., Magliocchetti, M., Salvato, M., Vietri, G., Zamorani, G., Almaini, O., Balestra, I., Bardelli, S., Begley, R., Brammer, G., Bell, E. F., Bowler, R. A. A., Brusa, M., Buitrago, F., Caputi, C., Cassata, P., Charlot, S., Citro, A., Cristiani, S., Curtis-Lake, E., Dickinson, M., Fazio, G., Ferguson, H. C., Fiore, F., Franco, M., Georgakakis, A., Giavalisco, M., Grazian, A., Hamadouche, M., Jung, I., Kim, S., Khusanova, Y., Longhetti, M., Lotz, J., Mannucci, F., Maltby, D., Matsuoka, K., Mendez-Hernandez, H., Mendez-Abreu, J., Mignoli, M., Moresco, M., Nonino, M., Pannella, M., Papovich, C., Popesso, P., Roberts-Borsani, G., Rosario, D. J., Saldana-Lopez, A., Santini, P., Saxena, A., Schaerer, D., Schreiber, C., Stark, D., Tasca, L. A. M., Thomas, R., Vanzella, E., Wild, V., Williams, C., Zucca, E.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::5fa5b85d121b761a7651caa904f19bf0
Autor:
Faisst A. L., Schaerer D., Lemaux B. C., Oesch P. A., Fudamoto Y., Cassata P., Bethermin M., Capak P. L., Fevre O. L., Silverman J. D., Yan L., Ginolfi M., Koekemoer A. M., Morselli L., Amorin R., Bardelli S., Boquien M., Brammer G., Cimatti A., Dessauges-Zavadsky M., Fujimoto S., Gruppioni C., Hathi N. P., Hemmati S., Ibar E., Jones G. C., Khusanova Y., Loiacono F., Pozzi F., Talia M., Tasca L. A. M., Riechers D. A., Rodighiero G., Romano M., Scoville N., Toft S., Vallini L., Vergani D., Zamorani G., Zucca E.
Publikováno v:
The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, 2020, 247, ⟨10.3847/1538-4365/ab7ccd⟩
The Astrophysical Journal Supplement Series, 247(2), 61
The Astrophysical Journal Supplement Series, 2020, 247, ⟨10.3847/1538-4365/ab7ccd⟩
The Astrophysical Journal Supplement Series, 247(2), 61
We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey - the first large multi-wavelength survey which aims at characterizing the gas and dust properti
Autor:
Iani, E., Rodighiero, G., Fritz, J., Cresci, G., Mancini, C., Tozzi, P., Rodríguez-Muñoz, L., Rosati, P., Caminha, G. B., Berta, S., Cassata, P., Concas, A., Enia, A., Fadda, D., Franceschini, A., Liu, A., Mercurio, A., Morselli, L., Pérez-González, P. G., Popesso, P., Sabatini, G., Zanella, A., Boquien, M., Lusso, E., Gruppioni, C., Tissera, P.
Publikováno v:
Challenges in Panchromatic Modelling withNext Generation Facilities: Proceedings, 15, 83-87
Brightest cluster galaxies (BCGs) residing in cool-core clusters are known to be the stage of intricate baryon cycle phenomena (e.g. gas inflows, AGN outflows, star formation feedback). The scenarios describing the observed properties of these galaxi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::918c9d4c6cdcad862a0324ee44575ae0
http://hdl.handle.net/11585/793782
http://hdl.handle.net/11585/793782
Autor:
Lemaux, B. C., Le Floc’h, E., Le Fèvre, O., Ilbert, O., Tresse, L., Lubin, L. M., Zamorani, G., Gal, R. R., Ciliegi, P., Cassata, P., Kocevski, D. D., Mcgrath, E. J., Bardelli, S., Zucca, E., Squires, G. K.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3657::8809ebc2a10d9766765e8f0552ddd9f8
http://hdl.handle.net/11577/3260325
http://hdl.handle.net/11577/3260325
Autor:
Zucca E., Bardelli S., Bolzonella M., Zamorani G., Ilbert O., Pozzetti L., Mignoli M., Kova, #269, Lilly S., Tresse L., Tasca L., Cassata P., Halliday C., Vergani D., Caputi K., Carollo C. M., Contini T., Kneib J. P., Le Fèvre O., Mainieri V., Renzini A., Scodeggio M., Bongiorno A., Coppa G., de La Torre S., de Ravel L., Franzetti P., Garilli B., Iovino A., Kampczyk P., Knobel C., Lamareille F., Le Borgne J. F., Le Brun V., Maier C., Pellò R., Peng Y., Perez Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Abbas U., Bottini D., Cappi A., Guzzo L., Koekemoer A. M., Leauthaud A., Maccagni D., Marinoni C., McCracken H. J., Meme, P., Meneux B., Oesch P., Porciani C., Scaramella R., Arnouts S., Aussel H., Capak P., Kartaltepe J., Salvato M., Sanders D., Scoville N., Taniguchi Y., Thompson D., CUCCIATI, OLGA, CIMATTI, ANDREA, MORESCO, MICHELE ENNIO MARIA
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2009, 508 (3), pp.1217-1234. ⟨10.1051/0004-6361/200912665⟩
Astronomy & astrophysics, 508(3), 1217-1234. EDP Sciences
Astronomy and Astrophysics-A&A, EDP Sciences, 2009, 508 (3), pp.1217-1234. ⟨10.1051/0004-6361/200912665⟩
Astronomy and Astrophysics-A&A, 2009, 508 (3), pp.1217-1234. ⟨10.1051/0004-6361/200912665⟩
Astronomy & astrophysics, 508(3), 1217-1234. EDP Sciences
Astronomy and Astrophysics-A&A, EDP Sciences, 2009, 508 (3), pp.1217-1234. ⟨10.1051/0004-6361/200912665⟩
(Abridged) We studied the evolution in the B band luminosity function to z~1 in the zCOSMOS 10k sample, for which both accurate galaxy classifications and a detailed description of the local density field are available. The global LF exhibits a brigh
Autor:
Tasca, L. A. M., Le Fèvre, O., Hathi, N. P., Schaerer, D., Ilbert, O., Zamorani, G., Lemaux, B. C., Cassata, P., Garilli, B., Le Brun, V., Maccagni, D., Pentericci, L., Thomas, R., Vanzella, E., Zucca, E., Amorin, R., Bardelli, S., Cassarà, L. P., Castellano, M., Cimatti, A., Cucciati, O., Durkalec, A., Fontana, A., Giavalisco, M., Grazian, A., Paltani, S., Ribeiro, B., Scodeggio, M., Sommariva, V., Talia, M., Tresse, L., Vergani, D., Capak, P., Charlot, S., Contini, T., De La Torre, S., Dunlop, J., Fotopoulou, S., Koekemoer, A., López-Sanjuan, C., Mellier, Y., Pforr, J., Salvato, M., Scoville, N., Taniguchi, Y., Wang, P. W.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3657::d075746b11bf9122736c1820367a8bb4
http://hdl.handle.net/11577/3260305
http://hdl.handle.net/11577/3260305
We present the analysis of a large sample of early-type galaxies (ETGs) at 02 are removed from the sample, suggesting an accelerated increase of the typical sizes at z>2, especially for the ETGs with the largest masses. A pure dry merging LambdaCDM m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::948cc4b563945af36e00f7c9e4281f5b
http://hdl.handle.net/11577/3260280
http://hdl.handle.net/11577/3260280
Autor:
Kova, #269, Porciani C., Lilly S. J., Marinoni C., Guzzo L., Zamorani G., Iovino A., Oesch P., Bolzonella M., Peng Y., Meneux B., Zucca E., Bardelli S., Carollo C. M., Contini T., Kneib J. P., Le Fèvre O., Mainieri V., Renzini A., Scodeggio M., Bongiorno A., Caputi K., Coppa G., de la Torre S., de Ravel L., Finoguenov A., Franzetti P., Garilli B., Kampczyk P., Knobel C., Lamareille F., Le Borgne J. F., Le Brun V., Maier C., Mignoli M., Pello R., Perez Montero E., Pozzetti L., Ricciardelli E., Silverman J. D., Tanaka M., Tasca L. A. M., Tresse L., Vergani D., Abbas U., Bottini D., Cappi A., Cassata P., Fumana M., Koekemoer A. M., Leauthaud A., Maccagni D., McCracken H. J., Memeo P., Scaramella R., Scoville N. Z., CUCCIATI, OLGA, CIMATTI, ANDREA
We use the zCOSMOS galaxy overdensity field to study the biasing of galaxies in the COSMOS field. By comparing the probability distribution function of the galaxy density contrast δ g to the lognormal approximation of the mass density contrast δ, w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10ad348b9b74c987f91b79f6626ff5a5
http://hdl.handle.net/11585/110784
http://hdl.handle.net/11585/110784
Autor:
Coppa G., Mignoli M., Zamorani G., Bardelli S., Lilly S. J., Bolzonella M., Scodeggio M., Vergani D., Nair P., Pozzetti L., Zucca E., Carollo C. M., Contini T., Le Fèvre O., Renzini A., Mainieri V., Bongiorno A., Caputi K. I., de la Torre S., de Ravel L., Franzetti P., Garilli B., Memeo P., Iovino A., Kampczyk P., Kneib J. P., Knobel C., Koekemoer A. M., Kova, #269, Lamareille F., Le Borgne J. F., Le Brun V., Maier C., Pellò R., Peng Y., Perez Montero E., Ricciardelli E., Scarlata C., Silverman J. D., Tanaka M., Tasca L., Tresse L., Abbas U., Bottini D., Capak P., Cappi A., Cassata P., Fumana M., Guzzo L., Leauthaud A., Maccagni D., Marinoni C., Meneux B., Oesch P., Porciani C., Scaramella R., Scoville N., CIMATTI, ANDREA, CUCCIATI, OLGA
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2011, 535, pp.10. ⟨10.1051/0004-6361/201016130⟩
Astronomy & astrophysics, 535:A10. EDP Sciences
Astronomy and Astrophysics-A&A, 2011, 535, pp.10. ⟨10.1051/0004-6361/201016130⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2011, 535, pp.10. ⟨10.1051/0004-6361/201016130⟩
Astronomy & astrophysics, 535:A10. EDP Sciences
Astronomy and Astrophysics-A&A, 2011, 535, pp.10. ⟨10.1051/0004-6361/201016130⟩
Our goal is to develop a new and reliable statistical method to classify galaxies from large surveys. We probe the reliability of the method by comparing it with a three-dimensional classification cube, using the same set of spectral, photometric and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb3e2e45bf9190d6444f83e4ec897dd2
http://arxiv.org/abs/1009.0723
http://arxiv.org/abs/1009.0723