The Star Formation History of Mass-selected Galaxies in the COSMOS Field von Karim, A, Schinnerer, E, Martínez-Sansigre, A, Sargent, M. T, van der Wel, A, Rix, H.-W, Ilbert, O, Smolčić, V, Carilli, C, Pannella, M, Koekemoer, A. M, Bell, E. F, Salvato, M

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Galaxies at redshifts 5 to 6 with systematically low dust content and high [C ii] emission von 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.

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Dust Properties of C ii Detected z ∼ 5.5 Galaxies: New HST/WFC3 Near-IR Observations von Barisic, I., Faisst, A. L., Capak, P. L., Pavesi, R., Riechers, D. A., Scoville, N. Z., Cooke, K., Kartaltepe, J. S., Casey, C. M., Smolcic, V.

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The faint radio sky: VLBA observations of the COSMOS field von Herrera Ruiz, N., Middelberg, E., Deller, A., Norris, R. P., Best, P. N., Brisken, W., Schinnerer, E., Smolčić, V., Delvecchio, I., Momjian, E., Bomans, D., Scoville, N. Z., Carilli, C.

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The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population von Smolčić, V., Delvecchio, I., Zamorani, G., Baran, N., Novak, M., Delhaize, J., Schinnerer, E., Berta, S., Bondi, M., Ciliegi, P., Capak, P., Civano, F., Karim, A., Le Fevre, O., Ilbert, O., Laigle, C., Marchesi, S., McCracken, H. J., Tasca, L., Salvato, M., Vardoulaki, E.

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Active galactic nuclei: what’s in a name? von Padovani, P., Alexander, D. M., Assef, R. J., De Marco, B., Giommi, P., Hickox, R. C., Richards, G. T., Smolčić, V., Hatziminaoglou, E., Mainieri, V., Salvato, M.

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The VLA-COSMOS Survey. IV. Deep Data and Joint Catalog von Schinnerer, E, Sargent, M. T, Bondi, M, Smolčić, V, Datta, A, Carilli, C. L, Bertoldi, F, Blain, A, Ciliegi, P, Koekemoer, A, Scoville, N. Z

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The VLA-COSMOS Survey. II. Source Catalog of the Large Project von Schinnerer, E, Smolčić, V, Carilli, C. L, Bondi, M, Ciliegi, P, Jahnke, K, Scoville, N. Z, Aussel, H, Bertoldi, F, Blain, A. W, Impey, C. D, Koekemoer, A. M, Le Fevre, O, Urry, C. M

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The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field von Hale, C L, Jarvis, M J, Delvecchio, I, Hatfield, P W, Novak, M, Smolčić, V, Zamorani, G

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A Multiwavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population von Algera, H. S. B., van der Vlugt, D., Hodge, J. A., Smail, I. R., Novak, M., Radcliffe, J. F., Riechers, D. A., Röttgering, H., Smol i, V., Walter, F.

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THE CHANDRA COSMOS LEGACY SURVEY: OPTICAL/IR IDENTIFICATIONS von Marchesi, S., Civano, F., Elvis, M., Salvato, M., Brusa, M., Comastri, A., Gilli, R., Hasinger, G., Lanzuisi, G., Miyaji, T., Treister, E., Urry, C. M., Vignali, C., Zamorani, G., Allevato, V., Cappelluti, N., Cardamone, C., Finoguenov, A., Griffiths, R. E., Karim, A., Laigle, C., LaMassa, S. M., Jahnke, K., Ranalli, P., Schawinski, K., Schinnerer, E., Silverman, J. D., Smolcic, V., Suh, H., Trakhtenbrot, B.

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The infrared-radio correlation of star-forming galaxies is strongly M☆-dependent but nearly redshift-invariant since z ∼ 4 von Delvecchio, I., Daddi, E., Sargent, M. T., Jarvis, M. J., Elbaz, D., Jin, S., Liu, D., Whittam, I. H., Algera, H., Carraro, R., D'Eugenio, C., Delhaize, J., Kalita, B. S., Leslie, S., Molnar, D. Cs, Novak, M., Prandoni, I., Smolcic, V., Ao, Y., Aravena, M., Bournaud, F., Collier, J. D., Randriamampandry, S. M., Randriamanakoto, Z., Rodighiero, G., Schober, J., White, S. V., Zamorani, G.

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THE CHANDRA COSMOS LEGACY SURVEY: OVERVIEW AND POINT SOURCE CATALOG von Civano, F., Marchesi, S., Comastri, A., Urry, M. C., Elvis, M., Cappelluti, N., Puccetti, S., Brusa, M., Zamorani, G., Hasinger, G., Aldcroft, T., Alexander, D. M., Allevato, V., Brunner, H., Capak, P., Finoguenov, A., Fiore, F., Fruscione, A., Gilli, R., Glotfelty, K., Griffiths, R. E., Hao, H., Harrison, F. A., Jahnke, K., Kartaltepe, J., Karim, A., LaMassa, S. M., Lanzuisi, G., Miyaji, T., Ranalli, P., Salvato, M., Sargent, M., Scoville, N. J., Schawinski, K., Schinnerer, E., Silverman, J., Smolcic, V., Stern, D., Toft, S., Trakhenbrot, B., Treister, E., Vignali, C.

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Star Formation and Dust Obscuration at z 2: Galaxies at the Dawn of Downsizing von Pannella, M, Carilli, C. L, Daddi, E, McCracken, H. J, Owen, F. N, Renzini, A, Strazzullo, V, Civano, F, Koekemoer, A. M, Schinnerer, E, Scoville, N, Smolčić, V, Taniguchi, Y, Aussel, H, Kneib, J. P, Ilbert, O, Mellier, Y, Salvato, M, Thompson, D, Willott, C. J

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The Radio AGN Population Dichotomy: Green Valley Seyferts Versus Red Sequence Low-Excitation Active Galactic Nuclei von Smolcic, V

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The VLA-COSMOS Survey. III. Further Catalog Analysis and the Radio Source Counts von Bondi, M, Ciliegi, P, Schinnerer, E, Smolčić, V, Jahnke, K, Carilli, C, Zamorani, G

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Photometric Redshift and Classification for the XMM-COSMOS Sources von Salvato, M, Hasinger, G, Ilbert, O, Zamorani, G, Brusa, M, Scoville, N. Z, Rau, A, Capak, P, Arnouts, S, Aussel, H, Bolzonella, M, Buongiorno, A, Cappelluti, N, Caputi, K, Civano, F, Cook, R, Elvis, M, Gilli, R, Jahnke, K, Kartaltepe, J. S, Impey, C. D, Lamareille, F, Le Floch, E, Lilly, S, Mainieri, V, McCarthy, P, McCracken, H, Mignoli, M, Mobasher, B, Murayama, T, Sasaki, S, Sanders, D. B, Schiminovich, D, Shioya, Y, Shopbell, P, Silverman, J, Smolčić, V, Surace, J, Taniguchi, Y, Thompson, D, Trump, J. R, Urry, M, Zamojski, M

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DISCLOSING THE RADIO LOUDNESS DISTRIBUTION DICHOTOMY IN QUASARS: AN UNBIASED MONTE CARLO APPROACH APPLIED TO THE SDSS-FIRST QUASAR SAMPLE von BALOKOVIC, M, Smolcic, V, Ivezic, Z, Zamorani, G, Schinnerer, E, Kelly, B C

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An Ultradeep Multiband VLA Survey of the Faint Radio Sky (COSMOS-XS): Source Catalog and Number Counts von van der Vlugt, D., Algera, H. S. B., Hodge, J. A., Novak, M., Radcliffe, J. F., Riechers, D. A., Röttgering, H., Smolčić, V., Walter, F.

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An Ultradeep Multiband Very Large Array Survey of the Faint Radio Sky (COSMOS-XS): New Constraints on the Optically Dark Population von van der Vlugt, D., Hodge, J. A., Jin, S., Algera, H. S. B., Leslie, S. K., Riechers, D. A., Röttgering, H., Smolčić, V., Walter, F.

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