The Dead Sequence: A Clear Bimodality in Galaxy Colors from z = 0 to z = 2.5 von 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

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HerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFT von Viero, M P, MONCELSI, L, Quadri, R F, Arumugam, V, Assef, R J, BETHERMIN, M, Bock, J, Bridge, C, Casey, C M, Conley, A

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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 von 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

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DISCOVERY OF LYMAN BREAK GALAXIES AT z ∼ 7 FROM THE zFourGE SURVEY von 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

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The Number Density and Mass Density of Star-forming and Quiescent Galaxies at 0.4 ≤ z ≤ 2.2 von 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

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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 von 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.

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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 von 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.

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HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z < 4 von Viero, M. P., Moncelsi, L., Quadri, R. F., Béthermin, M., Bock, 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.

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Changing Roles of Libraries and Academic Librarians in a Knowledge Society von Quadri, R. F

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HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z \textless 4 von Viero, M. P., Moncelsi, L., Quadri, R. F., Bethermin, M., Bock, 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, Guilaine, Magdis, G., Marchetti, L., Alvarez-Marquez, 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.

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THE NUMBER DENSITY AND MASS DENSITY OF STAR-FORMING AND QUIESCENT GALAXIES AT 0.4 {<=} z {<=} 2.2 von 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.

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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 von 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, K -V Tran

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HerMES: Current Cosmic Infrared Background Estimates Can be Explained by Known Galaxies and their Faint Companions at z < 4 von 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

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Hermes: current cosmic infrared background estimates can be explained by known galaxies and their faint companions at z<4 von Viero, MP, Moncelsi, L, Quadri, RF, Bethermin, M, Bock, J, Burgarella, D, Chapman, SC, Clements, DL, Conley, A, Conversi, L, Duivenvoorden, S, Dunlop, JS, Farrah, D, Franceschini, A, Halpern, M, Ivison, RJ, Lagache, G, Magdis, G, Marchetti, L, Alvarez-Marquez, J, Marsden, G, Oliver, SJ, Page, MJ, Perez-Fournon, I, Schulz, B, Scott, D, Valtchanov, I, Vieira, JD, Wang, L, Wardlow, J, Zemcov, M

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HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift von 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

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Discovery of Lyman Break Galaxies at z~7 from the ZFOURGE Survey von 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, P van Dokkum, 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

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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 von 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, K -S Lee, Muzzin, A, Rudnick, G, Wake, D A

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

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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 von Finkelstein, S, Quadri, R. F, Grogin, N. A, Ferguson, H, Giavalisco, M, Kocevski, Dale D, Dekel, A, Guo, Yicheng, Bond, N, Tilvi, V, Boada, Steven, Conselice, C, Koekemoer, A. M, Hilton, M, Koo, D. C

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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 von 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

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