Search Results - "Mckinney, Jed"

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    Neutral Gas Properties and Lyα Escape in Extreme Green Pea Galaxies by McKinney, Jed H., Jaskot, Anne E., Oey, M. S., Yun, Min S., Dowd, Tara, Lowenthal, James D.

    Published in The Astrophysical journal (20-03-2019)
    “…Mechanisms regulating the escape of Ly α photons and ionizing radiation remain poorly understood. To study these processes, we analyze Very Large Array 21 cm…”
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    Journal Article
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    Dust-enshrouded AGNs Can Dominate Host-galaxy-scale Cold Dust Emission by McKinney, Jed, Hayward, Christopher C., Rosenthal, Lee J., Martínez-Galarza, Juan Rafael, Pope, Alexandra, Sajina, Anna, Smith, Howard A.

    Published in The Astrophysical journal (01-11-2021)
    “…It is widely assumed that long-wavelength infrared (IR) emission from cold dust ( T ∼ 20–40 K) is a reliable tracer of star formation even in the presence of a…”
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    First Constraints on the Interstellar Medium Conditions of a Low-mass, Highly Obscured z = 4.27 Main-sequence Galaxy by Mizener, Andrew, Pope, Alexandra, McKinney, Jed, Kamieneski, Patrick, Whitaker, Katherine E., Battisti, Andrew, Murphy, Eric

    Published in The Astrophysical journal (01-07-2024)
    “…We present the molecular gas content and interstellar medium conditions of MACS J0717_Az9, a strong gravitationally lensed z = 4.273, M * ≃ 2 × 10 9 M ⊙…”
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    Measuring Star Formation and Black Hole Accretion Rates in Tandem Using Mid-infrared Spectra of Local Infrared Luminous Galaxies by Stone, Meredith, Pope, Alexandra, McKinney, Jed, Armus, Lee, Díaz-Santos, Tanio, Inami, Hanae, Kirkpatrick, Allison, Stierwalt, Sabrina

    Published in The Astrophysical journal (01-07-2022)
    “…We present the results of a stacking analysis performed on Spitzer/Infrared Spectrograph high-resolution mid-infrared (mid-IR) spectra of luminous infrared…”
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    Measuring the Total Ultraviolet Light from Galaxy Clusters at z = 0.5–1.6: The Balance of Obscured and Unobscured Star Formation by McKinney, Jed, Ramakrishnan, Vandana, Lee, Kyoung-Soo, Pope, Alexandra, Alberts, Stacey, Chiang, Yi-Kuan, Popescu, Roxana

    Published in The Astrophysical journal (01-03-2022)
    “…Combined observations from UV to IR wavelengths are necessary to fully account for the star formation in galaxy clusters. Low-mass galaxies with log ( M ∗ / M…”
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    The IR Compactness of Dusty Galaxies Sets Star Formation and Dust Properties at z ∼ 0–2 by McKinney, Jed, Pope, Alexandra, Kirkpatrick, Allison, Armus, Lee, Díaz-Santos, Tanio, Gómez-Guijarro, Carlos, Franco, Maximilien, Elbaz, David, Hayward, Christopher C., Inami, Hanae, Popping, Gergö, Xiao, Mengyuan

    Published in The Astrophysical journal (01-10-2023)
    “…The surface densities of gas, dust, and stars provide a window into the physics of star formation that, until the advent of high-resolution…”
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    Tracing the Total Stellar Mass and Star Formation of High-redshift Protoclusters by Popescu, Roxana, Pope, Alexandra, Lee, Kyoung-Soo, Alberts, Stacey, Chiang, Yi-Kuan, Lee, Sowon, Brodwin, Mark, McKinney, Jed, Ramakrishnan, Vandana

    Published in The Astrophysical journal (01-11-2023)
    “…As the progenitors of present-day galaxy clusters, protoclusters are excellent laboratories to study galaxy evolution. Since existing observations of…”
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    Measuring the Heating and Cooling of the Interstellar Medium at High Redshift: PAH and [C ii] Observations of the Same Star-forming Galaxies at z ∼ 2 by McKinney, Jed, Pope, Alexandra, Armus, Lee, Chary, Ranga-Ram, Díaz-Santos, Tanio, Dickinson, Mark E., Kirkpatrick, Allison

    Published in The Astrophysical journal (01-04-2020)
    “…Star formation depends critically on cooling mechanisms in the interstellar medium (ISM); however, thermal properties of gas in galaxies at the peak epoch of…”
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    Dust in Little Red Dots by Casey, Caitlin M., Akins, Hollis B., Kokorev, Vasily, McKinney, Jed, Cooper, Olivia R., Long, Arianna S., Franco, Maximilien, Manning, Sinclaire M.

    Published in Astrophysical journal. Letters (01-11-2024)
    “…JWST has revealed a ubiquitous population of “little red dots” (LRDs) at z ≳ 4, selected via their red rest-frame optical emission and compact morphologies…”
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