Search Results - "Dickinson, Mark"
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Cosmic Star-Formation History
Published in Annual review of astronomy and astrophysics (01-01-2014)“…Over the past two decades, an avalanche of new data from multiwavelength imaging and spectroscopic surveys has revolutionized our view of galaxy formation and…”
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2
A Survey of Atomic Carbon [C i] in High-redshift Main-sequence Galaxies
Published in The Astrophysical journal (10-12-2018)“…We present the first results of an Atacama Large Millimeter Array survey of the lower fine-structure line of atomic carbon [C i] in far-infrared-selected…”
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"Super-deblended" Dust Emission in Galaxies. I. The GOODS-North Catalog and the Cosmic Star Formation Rate Density out to Redshift 6
Published in The Astrophysical journal (01-02-2018)“…We present a new technique to measure multi-wavelength "super-deblended" photometry from highly confused images, which we apply to Herschel and ground-based…”
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On the Stellar Populations of Galaxies at z = 9–11: The Growth of Metals and Stellar Mass at Early Times
Published in The Astrophysical journal (01-03-2022)“…We present a detailed stellar population analysis of 11 bright (H < 26.6) galaxies at z=9−11 (three spectroscopically confirmed) to constrain the chemical…”
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"Super-deblended" Dust Emission in Galaxies. II. Far-IR to (Sub)millimeter Photometry and High-redshift Galaxy Candidates in the Full COSMOS Field
Published in The Astrophysical journal (01-09-2018)“…We present a "super-deblended" far-infrared (FIR) to (sub)millimeter photometric catalog in the Cosmic Evolution Survey (COSMOS), prepared with the method…”
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COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe
Published in The Astrophysical journal (10-02-2019)“…We report the first detailed measurement of the shape of the CO luminosity function at high redshift, based on >320 hr of the NSF's Karl G. Jansky Very Large…”
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The Star Formation Main Sequence in the Hubble Space Telescope Frontier Fields
Published in The Astrophysical journal (20-09-2017)“…We investigate the relation between star formation rate (SFR) and stellar mass (M), i.e., the main sequence (MS) relation of star-forming galaxies, at in the…”
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THE EVOLUTION OF THE GALAXY REST-FRAME ULTRAVIOLET LUMINOSITY FUNCTION OVER THE FIRST TWO BILLION YEARS
Published in The Astrophysical journal (01-09-2015)“…ABSTRACT We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity functions at z = 4-8. We use deep Hubble Space Telescope…”
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A First Look at the Abundance Pattern—O/H, C/O, and Ne/O—in z > 7 Galaxies with JWST/NIRSpec
Published in Astrophysical journal. Letters (01-11-2022)“…Abstract We analyze the rest-frame near-UV and optical nebular spectra of three z > 7 galaxies from the Early Release Observations taken with the Near-Infrared…”
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THE SFR–M RELATION AND EMPIRICAL STAR FORMATION HISTORIES FROM ZFOURGE AT 0.5 < z < 4
Published in The Astrophysical journal (01-02-2016)“…ABSTRACT We explore star formation histories (SFHs) of galaxies based on the evolution of the star formation rate stellar mass relation (SFR– M * ). Using data…”
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COLDz: A High Space Density of Massive Dusty Starburst Galaxies ∼1 Billion Years after the Big Bang
Published in The Astrophysical journal (01-06-2020)“…We report the detection of CO(J = 2 → 1) emission from three massive dusty starburst galaxies at z > 5 through molecular line scans in the NSF's Karl G. Jansky…”
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A CRITICAL LOOK AT THE MASS-METALLICITY-STAR FORMATION RATE RELATION IN THE LOCAL UNIVERSE. I. AN IMPROVED ANALYSIS FRAMEWORK AND CONFOUNDING SYSTEMATICS
Published in The Astrophysical journal (20-12-2014)“…It has been proposed that the (stellar) mass-(gas) metallicity relation of galaxies exhibits a secondary dependence on star formation rate (SFR), and that the…”
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13
Star formation rates and masses of z∼ 2 galaxies from multicolour photometry
Published in Monthly notices of the Royal Astronomical Society (2010)“…Fitting synthetic spectral energy distributions (SEDs) to the multiband photometry of galaxies to derive their star formation rates (SFRs), stellar masses,…”
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14
Size Evolution of the Most Massive Galaxies at 1.7 < z < 3 from GOODS NICMOS Survey Imaging
Published in The Astrophysical journal (10-11-2008)“…We measure the sizes of 82 massive galaxies at [image] utilizing deep HST NICMOS data taken in the GOODS North and South fields. Our sample is almost an order…”
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Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-deep Field
Published in The Astrophysical journal (01-02-2022)“…Abstract In the next decade, deep galaxy surveys from telescopes such as the James Webb Space Telescope and Roman Space Telescope will provide transformational…”
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Improved GALEX UV Photometry for 700,000 SDSS Galaxies
Published in The Astrophysical journal. Supplement series (01-09-2023)“…Abstract The Galaxy Evolution Explorer (GALEX) satellite performed the first and only large-area UV survey, which in tandem with the Sloan Digital Sky Survey…”
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HOW DO STAR-FORMING GALAXIES AT z > 3 ASSEMBLE THEIR MASSES?
Published in The Astrophysical journal (10-06-2012)“…We investigate how star-forming galaxies typically assemble their masses at high redshift. Taking advantage of the deep multi-wavelength coverage of the GOODS…”
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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
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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Near-infrared Spectroscopy of Galaxies During Reionization: Measuring C iii] in a Galaxy at z = 7.5
Published in The Astrophysical journal (10-07-2019)“…We present Keck/MOSFIRE H-band spectroscopy targeting C iii] λ1907, 1909 in a z = 7.5056 galaxy previously identified via Ly emission. We detect strong line…”
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Selection of Massive Evolved Galaxies at 3 ≤ z ≤ 4.5 in the CANDELS Fields
Published in The Astrophysical journal (01-07-2020)“…Using the CANDELS photometric catalogs for the Hubble Space Telescope/ACS and WFC3, we identified massive evolved galaxies at 3 < z < 4.5 employing three…”
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