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Browsing by Author "Breivik, Katelyn"

Browsing by Author "Breivik, Katelyn"

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  • A red giant orbiting a black hole 
    El-Badry, Kareem; Rix, Hans-Walter; Cendes, Yvette; Rodriguez, Antonio C.; Conroy, Charlie; Quataert, Eliot; Hawkins, Keith; Zari, Eleonora; Hobson, Melissa; Breivik, Katelyn; Rau, Arne; Berger, Edo; Shahaf, Sahar; Seeburger, Rhys; Burdge, Kevin B.; Latham, David W.; Buchhave, Lars A.; Bieryla, Allyson; Bashi, Dolev; Mazeh, Tsevi; Faigler, Simchon (2023)
    We report spectroscopic and photometric follow-up of a dormant black hole (BH) candidate from Gaia DR3. The system, which we call Gaia BH2, contains a ~1 M<sub>?</sub> red giant and a dark companion with mass $M_2 = 8.9\pm ...
  • A Sun-like star orbiting a black hole 
    El-Badry, Kareem; Rix, Hans-Walter; Quataert, Eliot; Howard, Andrew W.; Isaacson, Howard; Fuller, Jim; Hawkins, Keith; Breivik, Katelyn; Wong, Kaze W. K.; Rodriguez, Antonio C.; Conroy, Charlie; Shahaf, Sahar; Mazeh, Tsevi; Arenou, Frédéric; Burdge, Kevin B.; Bashi, Dolev; Faigler, Simchon; Weisz, Daniel R.; Seeburger, Rhys; Almada Monter, Silvia; Wojno, Jennifer (2023)
    We report discovery of a bright, nearby ($G = 13.8;\, \, d = 480\, \rm pc$) Sun-like star orbiting a dark object. We identified the system as a black hole candidate via its astrometric orbital solution from the Gaia mission. ...
  • TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period-Eccentricity Relation for Giant Planets Transiting Evolved Stars 
    Grunblatt, Samuel K.; Saunders, Nicholas; Chontos, Ashley; Hattori, Soichiro; Veras, Dimitri; Huber, Daniel; Angus, Ruth; Rice, Malena; Breivik, Katelyn; Blunt, Sarah; Giacalone, Steven; Lubin, Jack; Isaacson, Howard; Howard, Andrew W.; Ciardi, David R.; Safonov, Boris S.; Strakhov, Ivan A.; Latham, David W.; Bieryla, Allyson; Ricker, George R.; Jenkins, Jon M.; Tenenbaum, Peter; Shporer, Avi; Morgan, Edward H.; Kostov, Veselin; Osborn, Hugh P.; Dragomir, Diana; Seager, Sara; Vanderspek, Roland K.; Winn, Joshua N. (2023)
    The fate of planets around rapidly evolving stars is not well understood. Previous studies have suggested that, relative to the main-sequence population, planets transiting evolved stars (P <sub> J </sub>, 0.53 ± 0.05 M ...

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