Zobrazeno 1 - 10
of 226
pro vyhledávání: '"Quadri, R. A."'
Autor:
Rees, G. A., Spitler, L. R., Norris, R. P., Cowley, M. J., Papovich, C., Glazebrook, K., Quadri, R. F., Straatman, C. M. S., Allen, R., Kacprzak, G. G., Labbe, I., Nanayakkara, T., Tomczak, A. R., Tran, K. -V.
In order to reproduce the high-mass end of the galaxy mass-distribution, some process must be responsible for the suppression of star-formation in the most massive of galaxies. Commonly Active Galactic Nuclei (AGN) are invoked to fulfil this role, bu
Externí odkaz:
http://arxiv.org/abs/1511.01988
Autor:
Viero, M. P., Moncelsi, L., Quadri, R. F., Béthermin, M., Bock, J. J., Burgarella, D., Chapman, S. C., Clements, D. L., Conley, A., Conversi, L., Duivenvoorden, S., Dunlop, J. S., Farrah, D., Franceschini, A., Halpern, M., Ivison, R. J., Lagache, G., Magdis, G., Marchetti, L., Álvarez-Márquez, J., Marsden, G., Oliver, S. J., Page, M. J., Pérez-Fournon, I., Schulz, B., Scott, Douglas, Valtchanov, I., Vieira, J. D., Wang, L., Wardlow, J., Zemcov, M.
We report contributions to cosmic infrared background (CIB) intensities originating from known galaxies and their faint companions at submillimeter wavelengths. Using the publicly-available UltraVISTA catalog, and maps at 250, 350, and 500 {\mu}m fro
Externí odkaz:
http://arxiv.org/abs/1505.06242
Autor:
Boada, Steven, Tilvi, V., Papovich, C., Quadri, R. F., Hilton, M., Finkelstein, S., Guo, Yicheng, Bond, N., Conselice, C., Dekel, A., Ferguson, H., Giavalisco, M., Grogin, N. A., Kocevski, D. D., Koekemoer, A. M., Koo, D. C.
We use data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey to study how the spatial variation in the stellar populations of galaxies relate to the formation of galaxies at $1.5 < z < 3.5$. We use the Internal Color Dispersion
Externí odkaz:
http://arxiv.org/abs/1503.00722
Autor:
Papovich, Casey, Labbé, I., Quadri, R., Tilvi, V., Behroozi, P., Bell, E. F., Glazebrook, K., Spitler, L., Straatman, C. M. S., Tran, K. -V., Cowley, M., Davé, R., Dekel, A., Dickinson, M., Ferguson, H., Finkelstein, S. L., Gawiser, E., Inami, H., Faber, S. M., Kacprzak, G. G., Kawinwanchakij, L., Kocevski, D., Koekemoer, A., Koo, D. C., Kurczynski, P., Lotz, J. M., Lu, Y., Lucas, R. A., McIntosh, D., Mehrtens, N., Mobasher, B., Monson, A., Morrison, G., Nanayakkara, T., Perrson, S. E., Salmon, B., Simons, R., Tomczak, A., van Dokkum, P., Weiner, B., Willner, S. P.
Galaxies with stellar masses near M* contain the majority of stellar mass in the universe, and are therefore of special interest in the study of galaxy evolution. The Milky Way (MW) and Andromeda (M31) have present day stellar masses near M*, at 5x10
Externí odkaz:
http://arxiv.org/abs/1412.3806
Autor:
Viero, M. P., Asboth, V., Roseboom, I. G., Moncelsi, L., Marsden, G., Cooper, E. Mentuch, Zemcov, M., Addison, G., Baker, A. J., Beelen, A., Bock, J., Bridge, C., Conley, A., Devlin, M. J., Doré, O., Farrah, D., Finkelstein, S., Font-Ribera, A., Geach, J. E., Gebhardt, K., Gill, A., Glenn, J., Hajian, A., Halpern, M., Jogee, S., Kurczynski, P., Lapi, A., Negrello, M., Oliver, S. J., Papovich, C., Quadri, R., Ross, N., Scott, D., Schulz, B., Somerville, R., Spergel, D. N., Vieira, J. D., Wang, L., Wechsler, R.
We present the first set of maps and band-merged catalog from the Herschel Stripe 82 Survey (HerS). Observations at 250, 350, and 500 micron were taken with the Spectral and Photometric Imaging Receiver (SPIRE) instrument aboard the Herschel Space Ob
Externí odkaz:
http://arxiv.org/abs/1308.4399
Autor:
Tilvi, V., Papovich, C., Tran, K. -V. H., Labbe, I., Spitler, L. R., Straatman, C. M. S., Persson, S. E., Monson, A., Glazebrook, K., Quadri, R. F., van Dokkum, P., Ashby, M. L. N., Faber, S. M., Fazio, G. G., Finkelstein, S. L., Ferguson, H. C., Grogin, N. A., Kacprzak, G. G., Kelson, D. D., Koekemoer, A. M., Murphy, D., McCarthy, P. J., Newman, J. A., Salmon, B., Willner, S. P.
Star-forming galaxies at redshifts z>6 are likely responsible for the reionization of the universe, and it is important to study the nature of these galaxies. We present three candidates for z~7 Lyman-break galaxies (LBGs) from a 155 arcmin^2 area in
Externí odkaz:
http://arxiv.org/abs/1304.4227
Autor:
Viero, M. P., Moncelsi, L., Quadri, R. F., Arumugam, V., Assef, R. J., Bethermin, M., Bock, J., Bridge, C., Conley, A., Cooray, A., Farrah, D., Heinis, S., Ikarashi, S., Ivison, R. J., Kohno, K., Marsden, G., Oliver, S. J., Roseboom, I. G., Schulz, B., Scott, D., Serra, P., Vaccari, M., Vieira, J. D., Wang, L., Wardlow, J., Williams, R. J., Wilson, G. W., Yun, M. S., Zemcov, M.
We quantify the fraction of the cosmic infrared background (CIB) that originates from galaxies identified in the UV/optical/near-infrared by stacking 81,250 (~35.7 arcmin^2) K-selected sources (K_AB < 24.0), split according to their rest-frame U - V
Externí odkaz:
http://arxiv.org/abs/1304.0446
Autor:
Whitaker, K. E., van Dokkum, P. G., Brammer, G., Kriek, M., Franx, M., Labbe, I., Marchesini, D., Quadri, R. F., Bezanson, R., Illingworth, G. D., Lee, K. -S., Muzzin, A., Rudnick, G., Wake, D. A.
With a complete, mass-selected sample of quiescent galaxies from the NEWFIRM Medium-Band Survey (NMBS), we study the stellar populations of the oldest and most massive galaxies (>10^11 Msun) to high redshift. The sample includes 570 quiescent galaxie
Externí odkaz:
http://arxiv.org/abs/1006.5453
Autor:
Brammer, G. B., Whitaker, K. E., van Dokkum, P. G., Marchesini, D., Labbe, I., Franx, M., Kriek, M., Quadri, R. F., Illingworth, G., Lee, K. -S., Muzzin, A., Rudnick, G.
Publikováno v:
Astrophys.J.706:L173-L177,2009
We select 25,000 galaxies from the NEWFIRM Medium Band Survey (NMBS) to study the rest-frame U-V color distribution of galaxies at 0 < z < 2.5. The five unique NIR filters of the NMBS enable the precise measurement of photometric redshifts and rest-f
Externí odkaz:
http://arxiv.org/abs/0910.2227
Autor:
van Dokkum, P., Quadri, R., Marchesini, D., Rudnick, G., Franx, M., Gawiser, E., Herrera, D., Wuyts, S., Lira, P., Labbe, I., Maza, J., Illingworth, G., Schreiber, N. Forster, Kriek, M., Rix, H. -W., Taylor, E., Toft, S., Webb, T., Yi, S.
Using the deep multi-wavelength MUSYC, GOODS, and FIRES surveys we construct a stellar mass-limited sample of galaxies at 210^11 Solar masses distributed over four independent fields with a total area of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601113