Zobrazeno 1 - 10
of 150
pro vyhledávání: '"LeFevrè, O."'
Autor:
Faisst, A. L., Yan, L., Béthermin, M., Cassata, P., Dessauges-Zavadsky, M., Fudamoto, Y., Ginolfi, M., Gruppioni, C., Jones, G., Khusanova, Y., LeFèvre, O., Pozzi, F., Romano, M., Schaerer, D., Silverman, J., Vanderhoof, B.
Publikováno v:
Universe 2022, 8(6), 314
A multiwavelength study of galaxies is important to understand their formation and evolution. Only in the recent past, thanks to the Atacama Large (Sub) Millimeter Array (ALMA), were we able to study the far-infrared (IR) properties of galaxies at hi
Externí odkaz:
http://arxiv.org/abs/2206.03510
Autor:
Schinnerer, E., Groves, B., Sargent, M. T., Karim, A., Oesch, P. A., Magnelli, B., LeFevre, O., Tasca, L., Civano, F., Cassata, P., Smolcic, V.
The observed evolution of the gas fraction and its associated depletion time in main sequence (MS) galaxies provides insights on how star formation proceeds over cosmic time. We report ALMA detections of the rest-frame $\sim$300$\mu$m continuum obser
Externí odkaz:
http://arxiv.org/abs/1610.03656
Autor:
Capak, P. L., Carilli, C., Jones, G., Casey, C. M., Riechers, D., Sheth, K., Carollo, C. M., Ilbert, O., Karim, A., LeFevre, O., Lilly, S., Scoville, N., Smolcic, V., Yan, L.
Evolution in the measured rest frame ultraviolet spectral slope and ultraviolet to optical flux ratios indicate a rapid evolution in the dust obscuration of galaxies during the first 3 billion years of cosmic time (z>4). This evolution implies a chan
Externí odkaz:
http://arxiv.org/abs/1503.07596
Autor:
Mauduit, J. -C., Lacy, M., Farrah, D., Surace, J. A., Jarvis, M., Oliver, S., Maraston, C., Vaccari, M., Marchetti, L., Zeimann, G., Gonzalez-Solares, E. A., Pforr, J., Petric, A. O., Henriques, B., Thomas, P. A., Afonso, J., Rettura, A., Wilson, G., Falder, J. T., Geach, J. E., Huynh, M., Norris, R. P., Seymour, N., Richards, G. T., Stanford, S. A., Alexander, D. M., Becker, R. H., Best, P. N., Bizzocchi, L., Bonfield, D., Castro, N., Cava, A., Chapman, S., Christopher, N., Clements, D. L., Covone, G., Dubois, N., Dunlop, J. S., Dyke, E., Edge, A., Ferguson, H. C., Foucaud, S., Franceschini, A., Gal, R. R., Grant, J. K., Grossi, M., Hatziminaoglou, E., Hickey, S., Hodge, J. A., Huang, J. -S., Ivison, R. J., Kim, M., LeFevre, O., Lehnert, M., Lonsdale, C. J., Lubin, L. M., McLure, R. J., Messias, H., Martinez-Sansigre, A., Mortier, A. M. J., Nielsen, D. M., Ouchi, M., Parish, G., Perez-Fournon, I., Pierre, M., Rawlings, S., Readhead, A., Ridgway, S. E., Rigopoulou, D., Romer, A. K., Rosebloom, I. G., Rottgering, H. J. A., Rowan-Robinson, M., Sajina, A., Simpson, C. J., Smail, I., Squires, G. K., Stevens, J. A., Taylor, R., Trichas, M., Urrutia, T., van Kampen, E., Verma, A., Xu, C. K.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2012, Volume 124, issue 917, pp.714-736
We present the Spitzer Extragalactic Representative Volume Survey (SERVS), an 18 square degrees medium-deep survey at 3.6 and 4.5 microns with the post-cryogenic Spitzer Space Telescope to ~2 microJy (AB=23.1) depth of five highly observed astronomic
Externí odkaz:
http://arxiv.org/abs/1206.4060
Autor:
Domínguez, H., Mignoli, M., Pozzi, F., Calura, F., Cimatti, A., Gruppioni, C., Cepa, J., Sánchez-Portal, M., Zamorani, G., Berta, S., Elbaz, D., LeFloc'h, E., Granato, G. L., Lutz, D., Maiolino, R., Mateucci, F., Nair, P., Nordon, R., Pozzetti, L., Silva, L., Silverman, J., Wuyts, S., Carollo, C. M., Contini, T., Kneib, J. -P., LeFevrè, O., Lilly, S. J., Mainieri, V., Renzini, A., Scodeggio, M., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de la Torre, S., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Kovac, K., Lamareille, F., Borgne, J. -F. Le, Maier, V. le Brun. C., Magnelli, B., Pellò, R., Peng, Y., Pérez-Montero, E., Riccardelli, E., Riguccini, L., Tanaka, M., Tasca, L. A. M., Tresse, L., Vergani, D., Zucca, E.
We empirically test the relation between the SFR(LIR) derived from the infrared luminosity, LIR, and the SFR(Ha) derived from the Ha emission line luminosity using simple conversion relations. We use a sample of 474 galaxies at z = 0.06 - 0.46 with b
Externí odkaz:
http://arxiv.org/abs/1205.4573
Autor:
Adami, C., Mazure, A., Pierre, M., Sprimont, P. G., Libbrecht, C., Pacaud, F., Clerc, N., Sadibekova, T., Surdej, J., Altieri, B., Duc, P. A., Galaz, G., Gueguen, A., Guennou, L., Hertling, G., Ilbert, O., LeFèvre, J. P., Quintana, H., Valtchanov, I., Willis, J. P., Akiyama, M., Aussel, H., Chiappetti, L., Detal, A., Garilli, B., LeBrun, V., LeFèvre, O., Maccagni, D., Melin, J. B., Ponman, T. J., Ricci, D., Tresse, L.
XMM and Chandra opened a new area for the study of clusters of galaxies. Not only for cluster physics but also, for the detection of faint and distant clusters that were inaccessible with previous missions. This article presents 66 spectroscopically
Externí odkaz:
http://arxiv.org/abs/1010.6195
Autor:
Bardelli, S., Schinnerer, E., Smolcic, V., Zamorani, G., Zucca, E., Mignoli, M., Halliday, C., Kovac, K., Ciliegi, P., Caputi, K., Koekemoer, A. M., Bongiorno, A., Bondi, M., Bolzonella, M., Vergani, D., Pozzetti, L., Carollo, C. M., Contini, T., Kneib, J. -P., LeFevre, O., Lilly, S., Mainieri, V., Renzini, A., Scodeggio, M., Coppa, G., Cucciati, O., delaTorre, S., deRavel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Lamareille, F., LeBorgne, J. -F., LeBrun, V., Maier, C., Pello`, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J. D., Tanaka, M., Tasca, L., Tresse, L., Abbas, U., Bottini, D., Cappi, A., Cassata, P., Cimatti, A., Guzzo, L., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Meneux, B., Oesch, P., Porciani, C., Scaramella, R., Capak, P., Sanders, D., Scoville, N., Taniguchi, Y., Jahnke, K.
We investigate the properties and the environment of radio sources with optical counterpart from the combined VLA-COSMOS and zCOSMOS samples. The advantage of this sample is the availability of optical spectroscopic information, high quality redshift
Externí odkaz:
http://arxiv.org/abs/0911.0523
Autor:
Adami, C., Durret, F., Benoist, C., Coupon, J., Mazure, A., Meneux, B., Ilbert, O., Blaizot, J., Arnouts, C., Cappi, A., Garilli, B., Guennou, L., LeBrun, V., LeFevre, O., Maurogordato, S., McCracken, H. J., Mellier, Y., Slezak, E., Tresse, L., Ulmer, M. P.
In order to enlarge publicly available optical cluster catalogs, in particular at high redshift, we have performed a systematic search for clusters of galaxies in the CFHTLS. We used the Le Phare photometric redshifts for the galaxies detected with m
Externí odkaz:
http://arxiv.org/abs/0910.3827
Autor:
Zucca, E., Bardelli, S., Bolzonella, M., Zamorani, G., Ilbert, O., Pozzetti, L., Mignoli, M., Kovac, K., Lilly, S., Tresse, L., Tasca, L., Cassata, P., Halliday, C., Vergani, D., Caputi, K., Carollo, C. M., Contini, T., Kneib, J. P., LeFevre, O., Mainieri, V., Renzini, A., Scodeggio, M., Bongiorno, A., Coppa, G., Cucciati, O., delaTorre, S., deRavel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Lamareille, F., LeBorgne, J. F., LeBrun, V., Maier, C., Pello`, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J. D., Tanaka, M., Abbas, U., Bottini, D., Cappi, A., Cimatti, A., Guzzo, L., Koekemoer, A. M., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Meneux, B., Moresco, M., Oesch, P., Porciani, C., Scaramella, R., Arnouts, S., Aussel, H., Capak, P., Kartaltepe, J., Salvato, M., Sanders, D., Scoville, N., Taniguchi, Y., Thompson, D.
(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
Externí odkaz:
http://arxiv.org/abs/0909.4674
Autor:
Shioya, Y., Taniguchi, Y., Sasaki, S. S., Nagao, T., Murayama, T., Saito, T., Ideue, Y., Nakajima, A., Matsuoka, K. L., Trump, J., Scoville, N. Z., Sanders, D. B., Mobasher, B., Aussel, H., Capak, P., Kartaltepe, J., Koekemoer, A., Carilli, C., Ellis, R. S., Garilli, B., Giavalisco, M., Kitzbichler, M. G., Impey, C., LeFevre, O., Schinnerer, E., Smolcic, V.
Publikováno v:
Astrophys.J.696:546-561,2009
We present results of a survey for Ly alpha emitters at z=4.86 based on optical narrowband (lambda_c=7126 angstrom, Delta lambda=73 angstrom) and broadband (B, V, r', i', and z') observations of the Cosmic Evolution Survey (COSMOS) field using Suprim
Externí odkaz:
http://arxiv.org/abs/0901.4627