Search Results - "McCracken, H."

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    Revealing galaxy candidates out to z ∼ 16 with JWST observations of the lensing cluster SMACS0723 by Atek, Hakim, Shuntov, Marko, Furtak, Lukas J, Richard, Johan, Kneib, Jean-Paul, Mahler, Guillaume, Zitrin, Adi, McCracken, H J, Charlot, Stéphane, Chevallard, Jacopo, Chemerynska, Iryna

    “…ABSTRACT One of the main goals of the JWST is to study the first galaxies in the Universe. We present a systematic photometric analysis of very distant…”
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    Journal Article
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    A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10 by Bowler, R A A, Jarvis, M J, Dunlop, J S, McLure, R J, McLeod, D J, Adams, N J, Milvang-Jensen, B, McCracken, H J

    “…ABSTRACT We utilize deep near-infrared survey data from the UltraVISTA fourth data release (DR4) and the VIDEO survey, in combination with overlapping optical…”
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    Journal Article
  4. 4

    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.

    Published in The Astrophysical journal (10-03-2017)
    “…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…”
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    Journal Article
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    COSMOS2015 photometric redshifts probe the impact of filaments on galaxy properties by Laigle, C, Pichon, C, Arnouts, S, McCracken, H J, Dubois, Y, Devriendt, J, Slyz, A, Le Borgne, D, Benoit-Lévy, A, Hwang, Ho Seong, Ilbert, O, Kraljic, K, Malavasi, N, Park, Changbom, Vibert, D

    “…Abstract The variation of galaxy stellar masses and colour types with the distance to projected cosmic filaments are quantified using the precise photometric…”
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    The bright end of the galaxy luminosity function at z≃7: before the onset of mass quenching? by Bowler, R. A. A., Dunlop, J. S., McLure, R. J., Rogers, A. B., McCracken, H. J., Milvang-Jensen, B., Furusawa, H., Fynbo, J. P. U., Taniguchi, Y., Afonso, J., Bremer, M. N., Le Fèvre, O.

    “…We present the results of a new search for bright star-forming galaxies at redshift z ... 7 within the UltraVISTA second data release (DR2) and UKIDSS (UKIRT…”
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    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…”
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    Galaxy Stellar Mass Assembly Between 0.2 < z < 2 from the S-COSMOS Survey by Ilbert, O, Salvato, M, Le Floc'h, E, Aussel, H, Capak, P, McCracken, H. J, Mobasher, B, Kartaltepe, J, Scoville, N, Sanders, D. B, Arnouts, S, Bundy, K, Cassata, P, Kneib, J.-P, Koekemoer, A, Le Fèvre, O, Lilly, S, Surace, J, Taniguchi, Y, Tasca, L, Thompson, D, Tresse, L, Zamojski, M, Zamorani, G, Zucca, E

    Published in Analytica chimica acta (01-02-2010)
    “…We follow the galaxy stellar mass assembly by morphological and spectral type in the COSMOS 2 deg2 field. We derive the stellar mass functions and stellar mass…”
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    The galaxy luminosity function at z ≃ 6 and evidence for rapid evolution in the bright end from z ≃ 7 to 5 by Bowler, R. A. A., Dunlop, J. S., McLure, R. J., McCracken, H. J., Milvang-Jensen, B., Furusawa, H., Taniguchi, Y., Le Fèvre, O., Fynbo, J. P. U., Jarvis, M. J., Häußler, B.

    “…We present the results of a search for bright (−22.7 ≤ M UV ≤ −20.5) Lyman-break galaxies at z ≃ 6 within a total of 1.65 deg2 of imaging in the…”
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    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…”
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    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.

    Published in The Astrophysical journal (20-04-2017)
    “…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…”
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    Journal Article
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    SPITZER BRIGHT, ULTRAVISTA FAINT SOURCES IN COSMOS: THE CONTRIBUTION TO THE OVERALL POPULATION OF MASSIVE GALAXIES AT z = 3-7 by Caputi, K. I., Ilbert, O., Laigle, C., McCracken, H. J., Le Fèvre, O., Fynbo, J., Milvang-Jensen, B., Capak, P., Salvato, M., Taniguchi, Y.

    Published in The Astrophysical journal (01-09-2015)
    “…ABSTRACT We have analyzed a sample of 574 Spitzer 4.5 m selected galaxies with and (AB) over the UltraVISTA ultradeep COSMOS field. Our aim is to investigate…”
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    Journal Article