Search Results - "Larson, Rebecca L."

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    Spectral Templates Optimal for Selecting Galaxies at z > 8 with the JWST by Larson, Rebecca L., Hutchison, Taylor A., Bagley, Micaela, Finkelstein, Steven L., Yung, L. Y. Aaron, Somerville, Rachel S., Hirschmann, Michaela, Brammer, Gabriel, Holwerda, Benne W., Papovich, Casey, Morales, Alexa M., Wilkins, Stephen M.

    Published in The Astrophysical journal (01-12-2023)
    “…Abstract The selection of high-redshift galaxies often involves spectral energy distribution (SED) fitting to photometric data, an expectation for…”
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    A Mixture of LBG Overdensities in the Fields of Three 6 < z < 7 Quasars: Implications for the Robustness of Photometric Selection by Champagne, Jaclyn B., Casey, Caitlin M., Finkelstein, Steven L., Bagley, Micaela, Cooper, Olivia R., Larson, Rebecca L., Long, Arianna S., Wang, Feige

    Published in The Astrophysical journal (01-08-2023)
    “…Abstract The most luminous quasars at z > 6 are suspected to be both highly clustered and to reside in the most massive dark matter halos in the early…”
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    Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13 by Kokorev, Vasily, Chisholm, John, Endsley, Ryan, Finkelstein, Steven L., Greene, Jenny E., Akins, Hollis B., Bromm, Volker, Casey, Caitlin M., Fujimoto, Seiji, Labbé, Ivo, Larson, Rebecca L.

    Published in The Astrophysical journal (01-11-2024)
    “…Abstract The James Webb Space Telescope (JWST) has uncovered a ubiquitous population of dust-obscured compact sources at z ≳ 4. Many of these objects exhibit…”
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    Texas Spectroscopic Search for Lyα  Emission at the End of Reionization I. Constraining the Lyα Equivalent-width Distribution at 6.0 < z < 7.0 by Jung, Intae, Finkelstein, Steven L., Livermore, Rachael C., Dickinson, Mark, Larson, Rebecca L., Papovich, Casey, Song, Mimi, Tilvi, Vithal, Wold, Isak

    Published in The Astrophysical journal (10-09-2018)
    “…Abstract The distribution of Ly α emission is a presently accessible method for studying the state of the intergalactic medium (IGM) into the reionization era…”
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