Zobrazeno 1 - 10
of 587
pro vyhledávání: '"Foucaud, S."'
We derive the stellar-to-halo mass relations, SHMR, of local blue and red central galaxies separately, as well as the fraction of halos hosting blue/red central galaxies. We find that: 1) the SHMR of central galaxies is segregated by color, with blue
Externí odkaz:
http://arxiv.org/abs/1408.5407
Autor:
Keenan, R. C., Foucaud, S., De Propris, R., Hsieh, B. C., Lin, L., Chou, R. C. Y., Huang, S., Lin, J. H., Chang, K. H.
We present a study of the largest available sample of near-infrared selected (i.e., stellar mass selected) dynamically close pairs of galaxies at low redshifts ($z<0.3$). We combine this sample with new estimates of the major-merger pair fraction for
Externí odkaz:
http://arxiv.org/abs/1408.3468
Autor:
Fevre, O. Le, Cassata, P., Cucciati, O., Garilli, B., Ilbert, O., Brun, V. Le, Maccagni, D., Moreau, C., Scodeggio, M., Tresse, L., Zamorani, G., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Bondi, M., Bongiorno, A., Bottini, D., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., de la Torre, S., Foucaud, S., Franzetti, P., Gavignaud, I., Guzzo, L., Iovino, A., Lemaux, B., McCracken, H. J., Marano, B., Marinoni, C., Mazure, A., Mellier, Y., Merighi, R., Merluzzi, P., Paltani, S., Pello, R., Pollo, A., Pozzetti, L., Scaramella, R., Vergani, D., Vettolani, G., Zanichelli, A., Zucca, E.
Publikováno v:
2013, Astronomy and Astrophysics, 559, 14
We describe the completed VIMOS VLT Deep Survey, and the final data release of 35016 galaxies and type-I AGN with measured spectroscopic redshifts up to redshift z~6.7, in areas 0.142 to 8.7 square degrees, and volumes from 0.5x10^6 to 2x10^7h^-3Mpc^
Externí odkaz:
http://arxiv.org/abs/1307.0545
Autor:
Bradshaw, E. J., Almaini, O., Hartley, W. G., Smith, K. T., Conselice, C. J., Dunlop, J. S., Simpson, C., Chuter, R. W., Cirasuolo, M., Foucaud, S., McLure, R. J., Mortlock, A., Pearce, H.
We investigate galactic-scale outflows in the redshift range 0.71 < z < 1.63, using 413 K-band selected galaxies observed in the spectroscopic follow-up of the UKIDSS Ultra-Deep Survey (UDSz). The galaxies have an average stellar mass of ~10^9.5 sola
Externí odkaz:
http://arxiv.org/abs/1304.7276
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:
McLure, R. J., Pearce, H. J., Dunlop, J. S., Cirasuolo, M., Curtis-Lake, E., Bruce, V. A., Caputi, K., Almaini, O., Bonfield, D. G., Bradshaw, E. J., Buitrago, F., Chuter, R., Foucaud, S., Hartley, W. G., Jarvis, M. J.
We report the results of a comprehensive study of the relationship between galaxy size, stellar mass and specific star-formation rate (sSFR) at redshifts 1.3= 6x10^10 Msun), spectroscopic sample from the UKID
Externí odkaz:
http://arxiv.org/abs/1205.4058
Autor:
Moresco, M., Cimatti, A., Jimenez, Raul, Pozzetti, L., Zamorani, G., Bolzonella, M., Dunlop, J., Lamareille, F., Mignoli, M., Pearce, H., Rosati, P., Stern, D., Verde, L., Zucca, E., Carollo, C. M., Contini, T., Kneib, J. -P., Fevre, O. Le, Lilly, S. J., Mainieri, V., Renzini, A., Scodeggio, M., Balestra, I., Gobat, R., McLure, R., Bardelli, S., Bongiorno, A., Caputi, K., Cucciati, O., de la Torre, S., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Kovac, K., Borgne, J. -F. Le, Brun, V. Le, Maier, C., Pelló, R., Peng, Y., Perez-Montero, E., Presotto, V., Silverman, J. D., Tanaka, M., Tasca, L. A. M., Tresse, L., Vergani, D., Almaini, O., Barnes, L., Bordoloi, R., Bradshaw, E., Cappi, A., Chuter, R., Cirasuolo, M., Coppa, G., Diener, C., Foucaud, S., Hartley, W., Kamionkowski, M., Koekemoer, A. M., López-Sanjuan, C., McCracken, H. J., Nair, P., Oesch, P., Stanford, A., Welikala, N.
We present new improved constraints on the Hubble parameter H(z) in the redshift range 0.15 < z < 1.1, obtained from the differential spectroscopic evolution of early-type galaxies as a function of redshift. We extract a large sample of early-type ga
Externí odkaz:
http://arxiv.org/abs/1201.3609
Autor:
Curtis-Lake, E., McLure, R. J., Pearce, H. J., Dunlop, J. S., Cirasuolo, M., Stark, D. P., Almaini, O., Bradshaw, E. J., Chuter, R., Foucaud, S., Hartley, W. G.
We present spectroscopic confirmation of ten highly luminous (L >= 2L*) Lyman alpha emitters in the redshift range 6.01= 6 Lyman break galaxies (LBGs) selected fro
Externí odkaz:
http://arxiv.org/abs/1110.1722
Autor:
Chuter, R. W., Almaini, O., Hartley, W. G., McLure, R. J., Dunlop, J. S., Foucaud, S., Conselice, C. J., Simpson, C., Cirasuolo, M., Bradshaw, E. J.
We present a study of galaxy environments to z~2, based on a sample of over 33,000 K-band selected galaxies detected in the UKIDSS Ultra Deep Survey (UDS). The combination of infrared depth and area in the UDS allows us to extend previous studies of
Externí odkaz:
http://arxiv.org/abs/1101.0849
Autor:
de la Torre, S., Meneux, B., De Lucia, G., Blaizot, J., Fèvre, O. Le, Garilli, B., Cucciati, O., Mellier, Y., Pollo, A., Bottini, D., Brun, V. Le, Maccagni, D., Scodeggio, M., Tresse, L., Vettolani, G., Zanichelli, A., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marinoni, C., Mazure, A., Merighi, R., Paltani, S., Pelló, R., Pozzetti, L., Vergani, D., Zamorani, G., Zucca, E.
This paper presents a detailed comparison between high-redshift observations from the VIMOS-VLT Deep Survey (VVDS) and predictions from the Munich semi-analytical model of galaxy formation. In particular, we focus this analysis on the magnitude, reds
Externí odkaz:
http://arxiv.org/abs/1010.0360