Search Results - "Quadri, R. F."

The Dead Sequence: A Clear Bimodality in Galaxy Colors from z = 0 to z = 2.5 by Brammer, G. B, Whitaker, K. E, van Dokkum, P. G, Marchesini, D, Labbé, I, Franx, M, Kriek, M, Quadri, R. F, Illingworth, G, Lee, K.-S, Muzzin, A, Rudnick, G

“…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 approx< 2.5. The…”
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HerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFT by Viero, M P, MONCELSI, L, Quadri, R F, Arumugam, V, Assef, R J, BETHERMIN, M, Bock, J, Bridge, C, Casey, C M, Conley, A

“…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…”
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Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z  = 2.25 by Rees, G A, Spitler, L R, Norris, R P, Cowley, M J, Papovich, C, Glazebrook, K, Quadri, R F, Straatman, C MS, 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…”
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DISCOVERY OF LYMAN BREAK GALAXIES AT z ∼ 7 FROM THE zFourGE SURVEY by 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

“…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…”
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The Number Density and Mass Density of Star-forming and Quiescent Galaxies at 0.4 ≤ z ≤ 2.2 by Brammer, Gabriel B, Whitaker, K. E, van Dokkum, P. G, Marchesini, D, Franx, M, Kriek, M, Labbé, I, Lee, K.-S, Muzzin, A, Quadri, R. F, Rudnick, G, Williams, R

“…We study the buildup of the bimodal galaxy population using the NEWFIRM Medium-Band Survey, which provides excellent redshifts and well-sampled spectral energy…”
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Decoupled black hole accretion and quenching: the relationship between BHAR, SFR and quenching in Milky Way- and Andromeda-mass progenitors since z = 2.5 by Cowley, M. J., Spitler, L. R., Quadri, R. F., Goulding, A. D., Papovich, C., Tran, K. V. H., Labbé, I., Alcorn, L., Allen, R. J., Forrest, B., Glazebrook, K., Kacprzak, G. G., Morrison, G., Nanayakkara, T., Straatman, C. M. S., Tomczak, A. R.

“…Abstract We investigate the relationship between the black hole accretion rate (BHAR) and star formation rate (SFR) for Milky Way (MW) and Andromeda (M31)-mass…”
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THE ROLE OF BULGE FORMATION IN THE HOMOGENIZATION OF STELLAR POPULATIONS AT Z ∼ 2 AS REVEALED BY INTERNAL COLOR DISPERSION IN CANDELS by 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.

“…ABSTRACT We use data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey to study how the spatial variation in the stellar populations of…”
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Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25 by 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…”
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HerMES: Current Cosmic Infrared Background Estimates Can be Explained by Known Galaxies and their Faint Companions at z < 4 by 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…”
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HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift by 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…”
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Discovery of Lyman Break Galaxies at z~7 from the ZFOURGE Survey by 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…”
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THE NUMBER DENSITY AND MASS DENSITY OF STAR-FORMING AND QUIESCENT GALAXIES AT 0.4 {<=} z {<=} 2.2 by Brammer, Gabriel B., Whitaker, K. E., Van Dokkum, P. G., Lee, K.-S., Muzzin, A., Marchesini, D., Franx, M., Kriek, M., Labbe, I., Quadri, R. F., Williams, R., Rudnick, G.

“…We study the buildup of the bimodal galaxy population using the NEWFIRM Medium-Band Survey, which provides excellent redshifts and well-sampled spectral energy…”
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The Age Spread of Quiescent Galaxies with the NEWFIRM Medium-band Survey: Identification of the Oldest Galaxies out to z~2 by 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…”
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The Dead Sequence: A Clear Bimodality in Galaxy Colors from z=0 to z=2.5 by 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

“…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…”
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The Role of Bulge Formation in the Homogenization of Stellar Populations at $z\sim2$ as revealed by Internal Color Dispersion in CANDELS by 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…”
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