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@article{https://resolver.caltech.edu/CaltechAUTHORS:20180329-132609534,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20170828-074937096,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20170623-141442582,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20170331-143835493,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20170127-143159985,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20160427-105744845,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20160205-114722704,
    title = "The Phase Space of z \textasciitilde\ 1.2 SpARCS Clusters: Using Herschel to Probe Dust Temperature as a Function of Environment and Accretion History",
    journal = "Astrophysical Journal",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20151105-132712181,
    title = "Learning from FITS: Limitations in use in modern astronomical research",
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    title = "SPIRE point source photometry: within the Herschel interactive processing environment (HIPE)",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20140131-080059273,
    title = "HerMES: Candidate High-redshift Galaxies Discovered with Herschel/SPIRE",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20130904-083919768,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20130815-100959854,
    title = "HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-forming Galaxies",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20130730-104305133,
    title = "The Herschel PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4",
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    url = "https://resolver.caltech.edu/CaltechAUTHORS:20130730-104305133",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20130709-110259992,
    title = "HerMES: A Deficit in the Surface Brightness of the Cosmic Infrared Background due to Galaxy Cluster Gravitational Lensing",
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    title = "The Herschel census of infrared SEDs through cosmic time",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20130205-093943506,
    title = "HerMES: Candidate Gravitationally Lensed Galaxies and Lensing Statistics at Submillimeter Wavelengths",
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    title = "HerMES: deep number counts at 250 μm, 350 μm and 500 μm
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    year = "2010",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20101201-111403706,
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    year = "2010",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20101117-104045678,
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20101122-111936760,
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    year = "2010",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20101122-111936760",
    id = "record",
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    volume = "518"
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20101124-111407085,
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    year = "2010",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20101124-111407085",
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@article{https://resolver.caltech.edu/CaltechAUTHORS:20101203-082006802,
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