@article{https://resolver.caltech.edu/CaltechAUTHORS:20220531-844238000,
    title = "When Do Stars Go Boom?",
    journal = "Astrophysical Journal Letters",
    year = "2022",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20220531-844238000",
    id = "record",
    issn = "2041-8205",
    doi = "10.3847/2041-8213/ac6585",
    volume = "931"
}


@other{https://resolver.caltech.edu/CaltechAUTHORS:20190726-093513125,
    title = "The Chaotic Nature of TRAPPIST-1 Planetary Spin States",
    year = "2019",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190726-093513125",
    id = "record",
    doi = "10.48550/arXiv.1905.11419"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20190725-125944308,
    title = "Accounting for multiplicity in calculating eta Earth",
    journal = "Monthly Notices of the Royal Astronomical Society",
    year = "2019",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190725-125944308",
    id = "record",
    issn = "0035-8711",
    doi = "10.1093/mnras/stz1246",
    volume = "487"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20190415-130416951,
    title = "Accounting for incompleteness due to transit multiplicity in Kepler planet occurrence rates",
    journal = "Monthly Notices of the Royal Astronomical Society",
    year = "2019",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190415-130416951",
    id = "record",
    issn = "0035-8711",
    doi = "10.1093/mnras/sty3463",
    volume = "483"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20190124-122559376,
    title = "Spitzer transit follow-up of planet candidates from the K2 mission",
    journal = "Astronomical Journal",
    year = "2019",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190124-122559376",
    id = "record",
    issn = "1538-3881",
    doi = "10.3847/1538-3881/aaff69",
    volume = "157"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20170601-135603463,
    title = "K2-66b and K2-106b: Two Extremely Hot Sub-Neptune-size Planets with High Densities",
    journal = "Astronomical Journal",
    year = "2017",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20170601-135603463",
    id = "record",
    issn = "1538-3881",
    doi = "10.3847/1538-3881/aa725f",
    volume = "153"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20170120-132220743,
    title = "Mass Constraints of the WASP-47 Planetary System from Radial Velocities",
    journal = "Astronomical Journal",
    year = "2017",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20170120-132220743",
    id = "record",
    issn = "1538-3881",
    doi = "10.3847/1538-3881/153/2/70",
    volume = "153"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20160707-153537679,
    title = "Friends of Hot Jupiters. IV. Stellar companions beyond 50 AU might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration",
    journal = "Astrophysical Journal",
    year = "2016",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20160707-153537679",
    id = "record",
    issn = "0004-637X",
    doi = "10.3847/0004-637X/827/1/8",
    volume = "827"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20160810-152533844,
    title = "Eleven Multiplanet Systems from K2 Campaigns 1 and 2 and the Masses of Two Hot Super-Earths",
    journal = "Astrophysical Journal",
    year = "2016",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20160810-152533844",
    id = "record",
    issn = "0004-637X",
    doi = "10.3847/0004-637X/827/1/78",
    volume = "827"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20160311-123435885,
    title = "Two Transiting Low Density Sub-Saturns from K2",
    journal = "Astrophysical Journal",
    year = "2016",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20160311-123435885",
    id = "record",
    issn = "0004-637X",
    doi = "10.3847/0004-637X/818/1/36",
    volume = "818"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20170623-154020107,
    title = "Warm ice giant GJ 3470b. I. A flat transmission spectrum indicates a hazy, low-methane, and/or metal-rich atmosphere",
    journal = "Astronomy and Astrophysics",
    year = "2013",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20170623-154020107",
    id = "record",
    issn = "0004-6361",
    doi = "10.1051/0004-6361/201322278",
    volume = "559"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20170408-172900790,
    title = "Cool White Dwarfs Revisited: New Spectroscopy and Photometry",
    journal = "Astrophysical Journal",
    year = "2004",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20170408-172900790",
    id = "record",
    issn = "0004-637X",
    doi = "10.1086/380581",
    volume = "601"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100054,
    title = "Stellar forensics — II. Millisecond pulsar binaries",
    journal = "Monthly Notices of the Royal Astronomical Society",
    year = "1998",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100054",
    id = "record",
    issn = "0035-8711",
    doi = "10.1111/j.1365-8711.1998.01233.x",
    volume = "294"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100141,
    title = "Stellar forensics — I. Cooling curves",
    journal = "Monthly Notices of the Royal Astronomical Society",
    year = "1998",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100141",
    id = "record",
    issn = "0035-8711",
    doi = "10.1111/j.1365-8711.1998.01232.x",
    volume = "294"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100363,
    title = "The pulsar kick velocity distribution",
    journal = "Monthly Notices of the Royal Astronomical Society",
    year = "1997",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100363",
    id = "record",
    issn = "0035-8711",
    doi = "10.1093/mnras/291.3.569",
    volume = "291"
}