Search Results - "Quintana, Elisa V."

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  1. 1

    Kepler Data Validation II-Transit Model Fitting and Multiple-planet Search by Li, Jie, Tenenbaum, Peter, Twicken, Joseph D., Burke, Christopher J., Jenkins, Jon M., Quintana, Elisa V., Rowe, Jason F., Seader, Shawn E.

    “…This paper discusses the transit model-fitting and multiple-planet search algorithms and performance of the Kepler Science Data Processing Pipeline, developed…”
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    Journal Article
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    Implications of the Interstellar Object 1I/'Oumuamua for Planetary Dynamics and Planetesimal Formation by Raymond, Sean N., Armitage, Philip J., Veras, Dimitri, Quintana, Elisa V., Barclay, Thomas

    “…'Oumuamua, the first bona fide interstellar planetesimal, was discovered passing through our Solar system on a hyperbolic orbit. This object was likely…”
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    THE FREQUENCY OF GIANT IMPACTS ON EARTH-LIKE WORLDS by Quintana, Elisa V., Barclay, Thomas, Borucki, William J., Rowe, Jason F., Chambers, John E.

    Published in The Astrophysical journal (20-04-2016)
    “…ABSTRACT The late stages of terrestrial planet formation are dominated by giant impacts that collectively influence the growth, composition, and habitability…”
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  4. 4

    A CATALOG OF KEPLER HABITABLE ZONE EXOPLANET CANDIDATES by Kane, Stephen R., Hill, Michelle L., Kasting, James F., Kopparapu, Ravi Kumar, Quintana, Elisa V., Barclay, Thomas, Batalha, Natalie M., Borucki, William J., Ciardi, David R., Haghighipour, Nader, Hinkel, Natalie R., Kaltenegger, Lisa, Selsis, Franck, Torres, Guillermo

    Published in The Astrophysical journal (10-10-2016)
    “…ABSTRACT The NASA Kepler mission ha s discovered thousands of new planetary candidates, many of which have been confirmed through follow-up observations. A…”
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  5. 5

    Climate Modeling of a Potential ExoVenus by Kane, Stephen R., Ceja, Alma Y., Way, Michael J., Quintana, Elisa V.

    Published in The Astrophysical journal (10-12-2018)
    “…The planetary mass and radius sensitivity of exoplanet discovery capabilities has reached into the terrestrial regime. The focus of such investigations is to…”
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  6. 6

    Prospects for Cryovolcanic Activity on Cold Ocean Planets by Quick, Lynnae C., Roberge, Aki, Mendoza, Guadalupe Tovar, Quintana, Elisa V., Youngblood, Allison A.

    Published in The Astrophysical journal (01-10-2023)
    “…Abstract We have estimated total internal heating rates and depths to possible subsurface oceans for 17 planets that may be cold ocean planets, low-mass…”
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    A MIRI Search for Planets and Dust around WD 2149+021 by Poulsen, Sabrina, Debes, John, Cracraft, Misty, Mullally, Susan E., Reach, William T., Kilic, Mukremin, Mullally, Fergal, Albert, Loic, Thibault, Katherine, Hermes, J. J., Barclay, Thomas, Quintana, Elisa V.

    Published in The Astronomical journal (01-06-2024)
    “…Abstract The launch of JWST has ushered in a new era of high-precision infrared astronomy, allowing us to probe nearby white dwarfs for cold dust, exoplanets,…”
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    JWST Directly Images Giant Planet Candidates Around Two Metal-polluted White Dwarf Stars by Mullally, Susan E., Debes, John, Cracraft, Misty, Mullally, Fergal, Poulsen, Sabrina, Albert, Loic, Thibault, Katherine, Reach, William T., Hermes, J. J., Barclay, Thomas, Kilic, Mukremin, Quintana, Elisa V.

    Published in Astrophysical journal. Letters (01-02-2024)
    “…Abstract We report the discovery of two directly imaged, giant planet candidates orbiting the metal-rich, hydrogen atmosphere white dwarfs WD 1202−232 and WD…”
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  12. 12

    Atmospheric Escape From Three Terrestrial Planets in the L 98-59 System by Fromont, Emeline F., Ahlers, John P., do Amaral, Laura N. R., Barnes, Rory, Gilbert, Emily A., Quintana, Elisa V., Peacock, Sarah, Barclay, Thomas, Youngblood, Allison

    Published in The Astrophysical journal (01-01-2024)
    “…Abstract A critically important process affecting the climate evolution and potential habitability of an exoplanet is atmospheric escape, in which high-energy…”
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    CONFIRMATION OF HOT JUPITER KEPLER-41b VIA PHASE CURVE ANALYSIS by Quintana, Elisa V, Rowe, Jason F, Barclay, Thomas, Howell, Steve B, Ciardi, David R, Demory, Brice-Olivier, Caldwell, Douglas A, Borucki, William J, Christiansen, Jessie L, Jenkins, Jon M

    Published in The Astrophysical journal (20-04-2013)
    “…We present high precision photometry of Kepler-41, a giant planet in a 1.86 day orbit around a G6V star that was recently confirmed through radial velocity…”
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  17. 17

    The Demographics of Rocky Free-floating Planets and their Detectability by WFIRST by Barclay, Thomas, Quintana, Elisa V., Raymond, Sean N., Penny, Matthew T.

    Published in The Astrophysical journal (01-06-2017)
    “…Planets are thought to form via accretion from a remnant disk of gas and solids around a newly formed star. During this process, material in the disk either…”
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    Habitable Planet Formation around Low-mass Stars: Rapid Accretion, Rapid Debris Removal, and the Essential Contribution of External Giants by Clement, Matthew S., Quintana, Elisa V., Quarles, Billy L.

    Published in The Astrophysical journal (01-03-2022)
    “…Abstract In recent years, a paradigm shift has occurred in exoplanet science, wherein low-mass stars are increasingly viewed as a foundational pillar of the…”
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    RADIAL VELOCITY OBSERVATIONS AND LIGHT CURVE NOISE MODELING CONFIRM THAT KEPLER-91b IS A GIANT PLANET ORBITING A GIANT STAR by Barclay, Thomas, Endl, Michael, Huber, Daniel, eman-Mackey, Daniel, Cochran, William D, MacQueen, Phillip J, Rowe, Jason F, Quintana, Elisa V

    Published in The Astrophysical journal (10-02-2015)
    “…Kepler-91b is a rare example of a transiting hot Jupiter around a red giant star, providing the possibility to study the formation and composition of hot…”
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    FORMATION, TIDAL EVOLUTION, AND HABITABILITY OF THE KEPLER-186 SYSTEM by BOLMONT, EMELINE, Raymond, Sean N, von Paris, Philip, Selsis, Franck, Hersant, Franck, Quintana, Elisa V, Barclay, Thomas

    Published in The Astrophysical journal (20-09-2014)
    “…The Kepler-186 system consists of five planets orbiting an early M dwarf. The planets have physical radii of 1.0-1.50 R sub([+ in circle]) and orbital periods…”
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