[
    {
        "id": "authors:xx10x-e3y20",
        "collection": "authors",
        "collection_id": "xx10x-e3y20",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20191126-091657483",
        "type": "publication_whitepaper",
        "title": "Comparing key compositional indicators in Jupiter with those in extra-solar giant planets",
        "author": [
            {
                "family_name": "Lunine",
                "given_name": "Jonathan I.",
                "orcid": "0000-0003-2279-4131",
                "clpid": "Lunine-Jonathan-Irving"
            },
            {
                "family_name": "Greene",
                "given_name": "Tom",
                "orcid": "0000-0002-8963-8056",
                "clpid": "Greene-Thomas-P"
            },
            {
                "family_name": "Beichman",
                "given_name": "Charles",
                "orcid": "0000-0002-5627-5471",
                "clpid": "Beichman-C-A"
            },
            {
                "family_name": "Bean",
                "given_name": "Jacob",
                "orcid": "0000-0003-4733-6532",
                "clpid": "Bean-J-L"
            },
            {
                "family_name": "Hammel",
                "given_name": "Heidi B.",
                "orcid": "0000-0001-8751-3463",
                "clpid": "Hammel-H-B"
            },
            {
                "family_name": "Marley",
                "given_name": "Mark S.",
                "orcid": "0000-0002-5251-2943",
                "clpid": "Marley-M-S"
            }
        ],
        "abstract": "Spectroscopic transiting observations of the atmospheres of hot Jupiters around other stars, first with Hubble Space Telescope and then Spitzer, opened the door to compositional studies of exoplanets. The James Webb Space Telescope will provide such a profound improvement in signal-to-noise ratio that it will enable detailed analysis of molecular abundances, including but not limited to determining abundances of all the major carbon- and oxygen-bearing species in hot Jupiter atmospheres. This will allow determination of the carbon-to-oxygen ratio, an essential number for planet formation models and a motivating goal of the Juno mission currently around Jupiter.",
        "doi": "10.48550/arXiv.1904.00054",
        "publisher": "arXiv",
        "publication_date": "2019-03-29"
    },
    {
        "id": "authors:4zp4w-5b844",
        "collection": "authors",
        "collection_id": "4zp4w-5b844",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190619-110958838",
        "type": "publication_whitepaper",
        "title": "Imaging Cool Giant Planets in Reflected Light: Science Investigations and Synergy with Habitable Planets",
        "author": [
            {
                "family_name": "Marley",
                "given_name": "Mark",
                "orcid": "0000-0002-5251-2943",
                "clpid": "Marley-M-S"
            },
            {
                "family_name": "Lewis",
                "given_name": "Nikole",
                "orcid": "0000-0002-8507-1304",
                "clpid": "Lewis-N-K"
            },
            {
                "family_name": "Arney",
                "given_name": "Giada"
            },
            {
                "family_name": "Bailey",
                "given_name": "Vanessa",
                "orcid": "0000-0002-5407-2806",
                "clpid": "Bailey-V-P"
            },
            {
                "family_name": "Batalha",
                "given_name": "Natasha"
            },
            {
                "family_name": "Beichman",
                "given_name": "Charles",
                "orcid": "0000-0002-5627-5471",
                "clpid": "Beichman-C-A"
            },
            {
                "family_name": "Benneke",
                "given_name": "Bj\u00f6rn"
            },
            {
                "family_name": "Blecic",
                "given_name": "Jasmina"
            },
            {
                "family_name": "Cahoy",
                "given_name": "Kerri"
            },
            {
                "family_name": "Chilcote",
                "given_name": "Jeffrey"
            },
            {
                "family_name": "Domagal-Goldman",
                "given_name": "Shawn"
            },
            {
                "family_name": "Dressing",
                "given_name": "Courtney"
            },
            {
                "family_name": "Fitzgerald",
                "given_name": "Michael"
            },
            {
                "family_name": "Fortney",
                "given_name": "Jonathan"
            },
            {
                "family_name": "Freedman",
                "given_name": "Richard"
            },
            {
                "family_name": "Gelino",
                "given_name": "Dawn"
            },
            {
                "family_name": "Gizis",
                "given_name": "John"
            },
            {
                "family_name": "Guyon",
                "given_name": "Olivier"
            },
            {
                "family_name": "Greene",
                "given_name": "Thomas",
                "orcid": "0000-0002-8963-8056",
                "clpid": "Greene-Thomas-P"
            },
            {
                "family_name": "Hammel",
                "given_name": "Heidi"
            },
            {
                "family_name": "Hasegawa",
                "given_name": "Yasuhiro"
            },
            {
                "family_name": "Jovanovic",
                "given_name": "Nemanja",
                "clpid": "Jovanovic-N"
            },
            {
                "family_name": "Konopacky",
                "given_name": "Quinn"
            },
            {
                "family_name": "Kopparapu",
                "given_name": "Ravi"
            },
            {
                "family_name": "Liu",
                "given_name": "Michael"
            },
            {
                "family_name": "Lopez",
                "given_name": "Eric"
            },
            {
                "family_name": "Lunine",
                "given_name": "Jonathan"
            },
            {
                "family_name": "Lupu",
                "given_name": "Roxana"
            },
            {
                "family_name": "Macintosh",
                "given_name": "Bruce"
            },
            {
                "family_name": "Mandt",
                "given_name": "Kathleen"
            },
            {
                "family_name": "Marois",
                "given_name": "Christian"
            },
            {
                "family_name": "Mawet",
                "given_name": "Dimitri",
                "orcid": "0000-0002-8895-4735",
                "clpid": "Mawet-D"
            },
            {
                "family_name": "Mayorga",
                "given_name": "Laura"
            },
            {
                "family_name": "Morley",
                "given_name": "Caroline"
            },
            {
                "family_name": "Nielsen",
                "given_name": "Eric"
            },
            {
                "family_name": "Roberge",
                "given_name": "Aki"
            },
            {
                "family_name": "Serabyn",
                "given_name": "Eugene"
            },
            {
                "family_name": "Skemer",
                "given_name": "Andrew"
            },
            {
                "family_name": "Stapelfeldt",
                "given_name": "Karl"
            },
            {
                "family_name": "Visscher",
                "given_name": "Channon"
            },
            {
                "family_name": "Wang",
                "given_name": "Jason",
                "orcid": "0000-0003-0774-6502",
                "clpid": "Wang-Jason-J"
            }
        ],
        "abstract": "Planned astronomical observatories of the 2020s will be capable of obtaining reflected light photometry and spectroscopy of cool extrasolar giant planets. Here we explain that such data are valuable both for understanding the origin and evolution of giant planets as a whole and for preparing for the interpretation of similar datasets from potentially habitable extrasolar terrestrial planets in the decades to follow.",
        "doi": "10.48550/arXiv.1903.09322",
        "publisher": "arXiv",
        "publication_date": "2019-03-22"
    }
]