Search Results - "Koekemoer, Anton M."

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    A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16 by Harikane, Yuichi, Inoue, Akio K., Mawatari, Ken, Hashimoto, Takuya, Yamanaka, Satoshi, Fudamoto, Yoshinobu, Matsuo, Hiroshi, Tamura, Yoichi, Dayal, Pratika, Yung, L. Y. Aaron, Hutter, Anne, Pacucci, Fabio, Sugahara, Yuma, Koekemoer, Anton M.

    Published in The Astrophysical journal (01-04-2022)
    “…We present two bright galaxy candidates at z ∼ 12–13 identified in our H-dropout Lyman break selection with 2.3 deg(exp 2) near-infrared deep imaging data…”
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    Journal Article
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    COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at 0 < z < 5 Revealed by X-Ray and Radio Stacking by Ito, Kei, Tanaka, Masayuki, Miyaji, Takamitsu, Ilbert, Olivier, Kauffmann, Olivier B., Koekemoer, Anton M., Marchesi, Stefano, Shuntov, Marko, Toft, Sune, Valentino, Francesco, Weaver, John R.

    Published in The Astrophysical journal (01-04-2022)
    “…Abstract We characterize the average X-ray and radio properties of quiescent galaxies (QGs) with log ( M ⋆ / M ⊙ ) > 10 at 0 < z < 5. QGs are photometrically…”
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    Journal Article
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    The SFR-M Correlation Extends to Low Mass at High Redshift by Iyer, Kartheik, Gawiser, Eric, Davé, Romeel, Davis, Philip, Finkelstein, Steven L., Kodra, Dritan, Koekemoer, Anton M., Kurczynski, Peter, Newman, Jeffery A., Pacifici, Camilla, Somerville, Rachel S.

    Published in The Astrophysical journal (20-10-2018)
    “…To achieve a fuller understanding of galaxy evolution, SED fitting can be used to recover quantities beyond stellar masses (M*) and star formation rates…”
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    Journal Article
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    Physical Properties of Sub-galactic Clumps at 0.5 ≤ Z ≤ 1.5 in the UVUDF by Soto, Emmaris, Mello, Duilia F. de, Rafelski, Marc, Gardner, Jonathan P., Teplitz, Harry I., Koekemoer, Anton M., Ravindranath, Swara, Grogin, Norman A., Scarlata, Claudia, Kurczynski, Peter, Gawiser, Eric

    Published in The Astrophysical journal (01-03-2017)
    “…We present an investigation of clumpy galaxies in the Hubble Ultra Deep Field at in the rest-frame far-ultraviolet (FUV) using Hubble Space Telescope Wide…”
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    Journal Article
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