Karl Gordon
1971
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country of citizenship: United States of America
languages spoken, written or signed: English
educated at: University of Toledo
occupation: researcher
Articles 215
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PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars
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The JWST Early Release Observations
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SpeX Near-infrared Spectroscopic Extinction Curves in the Milky Way
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Relations between Mid-infrared Dust Emission and UV Extinction
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A Census of Thermally Pulsing AGB Stars in the Andromeda Galaxy and a First Estimate of Their Contribution to the Global Dust Budget
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METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. II. Variations of Interstellar Depletions and Dust-to-gas Ratio within the LMC
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The Quest for the Missing Dust. I. Restoring Large-scale Emission in Herschel Maps of Local Group Galaxies
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DirtyGrid II: An Analysis of the Dust and Stellar Properties in Nearby Star-forming Galaxies
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METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. I. Overview and Initial Results
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Multiple incursion pathways for Helicoverpa armigera in Brazil show its genetic diversity spreading in a connected world
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Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxies
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Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies
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The Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE): The Dust Extinction Curve from Red Clump Stars
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The Panchromatic Hubble Andromeda Treasury. XV. The BEAST: Bayesian Extinction and Stellar Tool
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The mid-infrared instrument for the James Webb Space Telescope: performance and operation of the Low-Resolution Spectrometer
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Hubble Tarantula Treasury Project. III. Photometric catalog and resulting constraints on the progression of star formation in the 30 Doradus region
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A new method for deriving the stellar birth function of resolved stellar populations
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Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC
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ERRATUM: “THE HERSCHEL INVENTORY OF THE AGENTS OF GALAXY EVOLUTION (HERITAGE) IN THE MAGELLANIC CLOUDS, A HERSCHEL OPEN TIME KEY PROGRAM” (2013, AJ, 146, 62)
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The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20-600 {mu}m wavelengths
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An infrared census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). II. Discovery of metal-poor dusty AGB stars
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Benchmarking the calculation of stochastic heating and emissivity of dust grains in the context of radiative transfer simulations
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Cool dust heating and temperature mixing in nearby star-forming galaxies
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The panchromatic Hubble Andromeda treasury. VIII. A wide-area, high-resolution map of dust extinction in M31
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Panchromatic Hubble Andromeda Treasury. IX. A photometric survey of planetary nebulae in M31
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Dissecting the origin of the submillimetre emission in nearby galaxies with Herschel and LABOCA
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Untangling the nature of spatial variations of cold dust properties in star forming galaxies
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The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation Across Space and Time in M 31
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An infrared census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). I. Overview
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Dust and gas in the Magellanic Clouds from the HERITAGE Herschel key project. II. Gas-to-dust ratio variations across interstellar medium phases
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Molecular hydrogen emission in the interstellar medium of the Large Magellanic Cloud
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The Panchromatic Hubble Andromeda Treasury. X. Ultraviolet to infrared photometry of 117 million equidistant stars
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