Search Results - "CAPAK, P"

ISM MASSES AND THE STAR FORMATION LAW AT Z = 1 TO 6: ALMA OBSERVATIONS OF DUST CONTINUUM IN 145 GALAXIES IN THE COSMOS SURVEY FIELD by Scoville, N., Sheth, K., Aussel, H., Bout, P. Vanden, Capak, P., Bongiorno, A., Casey, C. M., Murchikova, L., Koda, J., Álvarez-Márquez, J., Lee, N., Laigle, C., McCracken, H. J., Ilbert, O., Pope, A., Sanders, D., Chu, J., Toft, S., Ivison, R. J., Manohar, S.

“…ABSTRACT ALMA Cycle 2 observations of long-wavelength dust emission in 145 star-forming galaxies are used to probe the evolution of the star-forming…”
Get full text

The DEIMOS 10K Spectroscopic Survey Catalog of the COSMOS Field by Hasinger, G., Capak, P., Salvato, M., Barger, A. J., Cowie, L. L., Faisst, A., Hemmati, S., Kakazu, Y., Kartaltepe, J., Masters, D., Mobasher, B., Nayyeri, H., Sanders, D., Scoville, N. Z., Suh, H., Steinhardt, C., Yang, Fengwei

“…Abstract We present a catalog of 10,718 objects in the COSMOS field, observed through multi-slit spectroscopy with the Deep Imaging Multi-Object Spectrograph…”
Get full text

Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift by Scoville, N., Lee, N., Bout, P. Vanden, Diaz-Santos, T., Sanders, D., Darvish, B., Bongiorno, A., Casey, C. M., Murchikova, L., Koda, J., Capak, P., Vlahakis, Catherine, Ilbert, O., Sheth, K., Morokuma-Matsui, K., Ivison, R. J., Aussel, H., Laigle, C., McCracken, H. J., Armus, L., Pope, A., Toft, S., Masters, D.

“…ALMA observations of the long wavelength dust continuum are used to estimate the interstellar medium (ISM) masses in a sample of 708 galaxies at z = 0.3 to 4.5…”
Get full text

ISM EXCITATION AND METALLICITY OF STAR-FORMING GALAXIES AT Z 3.3 FROM NEAR-IR SPECTROSCOPY by Onodera, M., Carollo, C. M., Lilly, S., Renzini, A., Arimoto, N., Capak, P., Daddi, E., Scoville, N., Tacchella, S., Tatehora, S., Zamorani, G.

“…ABSTRACT We study the relationship between stellar mass, star formation rate (SFR), ionization state, and gas-phase metallicity for a sample of 41 normal…”
Get full text

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

“…Measurements of [C ii ] emission and dust emission from nine typical star-forming galaxies about one billion years after the Big Bang show that galaxies of…”
Get full text

NEWLY QUENCHED GALAXIES AS THE CAUSE FOR THE APPARENT EVOLUTION IN AVERAGE SIZE OF THE POPULATION by Carollo, C M, BSCHORR, T J, Renzini, A, Lilly, S J, CAPAK, P, Cibinel, A, Ilbert, O, Onodera, M, Scoville, N, Cameron, E, Mobasher, B, Sanders, D, Taniguchi, Y

“…We use the large COSMOS sample of galaxies to study in an internally self-consistent way the change in the number densities of quenched early-type galaxies…”
Get full text

Horizon-AGN virtual observatory – 1. SED-fitting performance and forecasts for future imaging surveys by Laigle, C, Davidzon, I, Ilbert, O, Devriendt, J, Kashino, D, Pichon, C, Capak, P, Arnouts, S, de la Torre, S, Dubois, Y, Gozaliasl, G, Le Borgne, D, Lilly, S, McCracken, H J, Salvato, M, Slyz, A

“…Abstract Using the light-cone from the cosmological hydrodynamical simulation horizon-AGN, we produced a photometric catalogue over 0 < z < 4 with apparent…”
Get full text

The ALPINE-ALMA [C ii] Survey: kinematic diversity and rotation in massive star-forming galaxies at z ~ 4.4–5.9 by Jones, G C, Vergani, D, Romano, M, Ginolfi, M, Fudamoto, Y, Béthermin, M, Fujimoto, S, Lemaux, B C, Morselli, L, Capak, P, Cassata, P, Faisst, A, Le Fèvre, O, Schaerer, D, Silverman, J D, Yan, Lin, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Ibar, E, Maiolino, R, Rizzo, F, Talia, M, Zamorani, G

“…ABSTRACT While the kinematics of galaxies up to z ∼ 3 have been characterized in detail, only a handful of galaxies at high redshift (z > 4) have been examined…”
Get full text

THE EVOLUTION OF INTERSTELLAR MEDIUM MASS PROBED BY DUST EMISSION: ALMA OBSERVATIONS AT z = 0.3-2 by Scoville, N, Aussel, H, Sheth, K, Scott, K S, Sanders, D, Ivison, R, Pope, A, CAPAK, P, Vanden Bout, P, Manohar, S, KARTALTEPE, J, Robertson, B, Lilly, S

“…The use of submillimeter dust continuum emission to probe the mass of interstellar dust and gas in galaxies is empirically calibrated using samples of local…”
Get full text

Dust Properties of C ii Detected z ∼ 5.5 Galaxies: New HST/WFC3 Near-IR Observations by 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.

“…We examine the rest-frame ultraviolet (UV) properties of 10 [C ii]λ158 m-detected galaxies at z ∼ 5.5 in COSMOS using new Hubble Space Telescope/Wide Field…”
Get full text

Dynamical Characterization of Galaxies at z ∼ 4-6 via Tilted Ring Fitting to ALMA [C ii] Observations by Jones, G. C., Carilli, C. L., Shao, Y., Wang, R., Capak, P. L., Pavesi, R., Riechers, D. A., Karim, A., Neeleman, M., Walter, F.

“…Until recently, determining the rotational properties of galaxies in the early universe ( , universe age Gyr) was impractical, with the exception of a few…”
Get full text

horizon-AGN virtual observatory – 2. Template-free estimates of galaxy properties from colours by Davidzon, I, Laigle, C, Capak, P L, Ilbert, O, Masters, D C, Hemmati, S, Apostolakos, N, Coupon, J, de la Torre, S, Devriendt, J, Dubois, Y, Kashino, D, Paltani, S, Pichon, C

“…ABSTRACT Using the horizon-AGN hydrodynamical simulation and self-organizing maps (SOMs), we show how to compress the complex, high-dimensional data structure…”
Get full text

The Frontier Fields: Survey Design and Initial Results by Lotz, J. M., Koekemoer, A., Coe, D., Grogin, N., Capak, P., Mack, J., Anderson, J., Avila, R., Barker, E. A., Borncamp, D., Brammer, G., Durbin, M., Gunning, H., Hilbert, B., Jenkner, H., Khandrika, H., Levay, Z., Lucas, R. A., MacKenty, J., Ogaz, S., Porterfield, B., Reid, N., Robberto, M., Royle, P., Smith, L. J., Storrie-Lombardi, L. J., Sunnquist, B., Surace, J., Taylor, D. C., Williams, R., Bullock, J., Dickinson, M., Finkelstein, S., Natarajan, P., Richard, J., Robertson, B., Tumlinson, J., Zitrin, A., Flanagan, K., Sembach, K., Soifer, B. T., Mountain, M.

“…What are the faintest distant galaxies we can see with the Hubble Space Telescope (HST) now, before the launch of the James Webb Space Telescope? This is the…”
Get full text

The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z ∼ 5 by Legrand, L, McCracken, H J, Davidzon, I, Ilbert, O, Coupon, J, Aghanim, N, Douspis, M, Capak, P L, Le Fèvre, O, Milvang-Jensen, B

“…Abstract Using precise galaxy stellar mass function measurements in the COSMOS field we determine the stellar-to-halo mass relationship (SHMR) using a…”
Get full text

Constraints on Quenching of Z 2 Massive Galaxies from the Evolution of the Average Sizes of Star-forming and Quenched Populations in COSMOS by Faisst, A. L., Carollo, C. M., Capak, P. L., Tacchella, S., Renzini, A., Ilbert, O., McCracken, H. J., Scoville, N. Z.

“…We use >9400 quiescent and star-forming galaxies at z 2 in COSMOS/UltraVISTA to study the average size evolution of these systems, with focus on the rare…”
Get full text

SpecPro: An Interactive IDL Program for Viewing and Analyzing Astronomical Spectra by Masters, D., Capak, P.

“…We present an interactive IDL program for viewing and analyzing astronomical spectra in the context of modern imaging surveys. SpecPro’s interactive design…”
Get full text

THE CHANDRA COSMOS LEGACY SURVEY: OVERVIEW AND POINT SOURCE CATALOG by 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.

“…ABSTRACT The COSMOS-Legacy survey is a 4.6 Ms Chandra program that has imaged 2.2 deg2 of the COSMOS field with an effective exposure of ks over the central…”
Get full text

ARE DUSTY GALAXIES BLUE? INSIGHTS ON UV ATTENUATION FROM DUST-SELECTED GALAXIES by Casey, C M, Scoville, N Z, Sanders, D B, Lee, N, Cooray, A, Finkelstein, S L, CAPAK, P, Conley, A, DE ZOTTI, G, Farrah, D, FU, H, Le Floc'h, E, Ilbert, O, Ivison, R J, Takeuchi, T T

“…Galaxies' rest-frame ultraviolet (UV) properties are often used to directly infer the degree to which dust obscuration affects the measurement of star…”
Get full text

An Atlas of z = 5.7 and z = 6.5 Lyα Emitters by Hu, E. M, Cowie, L. L, Barger, A. J, Capak, P, Kakazu, Y, Trouille, L

Get full text

REST-UV ABSORPTION LINES AS METALLICITY ESTIMATOR: THE METAL CONTENT OF STAR-FORMING GALAXIES AT z ∼ 5 by Faisst, A. L., Capak, P. L., Davidzon, I., Salvato, M., Laigle, C., Ilbert, O., Onodera, M., Hasinger, G., Kakazu, Y., Masters, D., McCracken, H. J., Mobasher, B., Sanders, D., Silverman, J. D., Yan, L., Scoville, N. Z.

“…ABSTRACT We measure a relation between the depth of four prominent rest-UV absorption complexes and metallicity for local galaxies and verify it up to . We…”
Get full text