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Brown dwarfs with well-determined ages, luminosities, and masses provide rare but valuable tests of low-temperature atmospheric and evolutionary models. We present the discovery and dynamical mass measurement of a substellar companion to HD…

We report the first astrometrically determined mass of an extrasolar planet, a companion previously detected by Doppler spectroscopy. Radial velocities first provided an ephemeris with which to schedule a significant fraction of the {\it…

We present radial velocity measurements of two stars observed as part of the Lick Subgiants Planet Search and the Keck N2K survey. Variations in the radial velocities of both stars reveal the presence of Jupiter-mass exoplanets in highly…

Statistical analyses from exoplanet surveys around low-mass stars indicate that super-Earth and Neptune-mass planets are more frequent than gas giants around such stars, in agreement with core accretion theory of planet formation. Using…

地球与行星天体物理 · 物理学 2019-10-16 J. C. Morales , A. J. Mustill , I. Ribas , M. B. Davies , A. Reiners , F. F. Bauer , D. Kossakowski , E. Herrero , E. Rodríguez , M. J. López-González , C. Rodríguez-López , V. J. S. Béjar , L. González-Cuesta , R. Luque , E. Pallé , M. Perger , D. Baroch , A. Johansen , H. Klahr , C. Mordasini , G. Anglada-Escudé , J. A. Caballero , M. Cortés-Contreras , S. Dreizler , M. Lafarga , E. Nagel , V. M. Passegger , S. Reffert , A. Rosich , A. Schweitzer , L. Tal-Or , T. Trifonov , M. Zechmeister , A. Quirrenbach , P. J. Amado , E. W. Guenther , H. -J. Hagen , T. Henning , S. V. Jeffers , A. Kaminski , M. Kürster , D. Montes , W. Seifert , F. J. Abellán , M. Abril , J. Aceituno , F. J. Aceituno , F. J. Alonso-Floriano , M. Ammler-von Eiff , R. Antona , B. Arroyo-Torres , M. Azzaro , D. Barrado , S. Becerril-Jarque , D. Benítez , Z. M. Berdiñas , G. Bergond , M. Brinkmöller , C. del Burgo , R. Burn , R. Calvo-Ortega , J. Cano , M. C. Cárdenas , C. Cardona Guillén , J. Carro , E. Casal , V. Casanova , N. Casasayas-Barris , P. Chaturvedi , C. Cifuentes , A. Claret , J. Colomé , S. Czesla , E. Díez-Alonso , R. Dorda , A. Emsenhuber , M. Fernández , A. Fernández-Martín , I. M. Ferro , B. Fuhrmeister , D. Galadí-Enríquez , I. Gallardo Cava , M. L. García Vargas , A. Garcia-Piquer , L. Gesa , E. González-Álvarez , J. I. González Hernández , R. González-Peinado , J. Guàrdia , A. Guijarro , E. de Guindos , A. P. Hatzes , P. H. Hauschildt , R. P. Hedrosa , I. Hermelo , R. Hernández Arabi , F. Hernández Otero , D. Hintz , G. Holgado , A. Huber , P. Huke , E. N. Johnson , E. de Juan , M. Kehr , J. Kemmer , M. Kim , J. Klüter , A. Klutsch , F. Labarga , N. Labiche , S. Lalitha , M. Lampón , L. M. Lara , R. Launhardt , F. J. Lázaro , J. -L. Lizon , M. Llamas , N. Lodieu , M. López del Fresno , J. F. López Salas , J. López-Santiago , H. Magán Madinabeitia , U. Mall , L. Mancini , H. Mandel , E. Marfil , J. A. Marín Molina , E. L. Martín , P. Martín-Fernández , S. Martín-Ruiz , H. Martínez-Rodríguez , C. J. Marvin , E. Mirabet , A. Moya , V. Naranjo , R. P. Nelson , L. Nortmann , G. Nowak , A. Ofir , J. Pascual , A. Pavlov , S. Pedraz , D. Pérez Medialdea , A. Pérez-Calpena , M. A. C. Perryman , O. Rabaza , A. Ramón Ballesta , R. Rebolo , P. Redondo , H. -W. Rix , F. Rodler , A. Rodríguez Trinidad , S. Sabotta , S. Sadegi , M. Salz , E. Sánchez-Blanco , M. A. Sánchez Carrasco , A. Sánchez-López , J. Sanz-Forcada , P. Sarkis , L. F. Sarmiento , S. Schäfer , M. Schlecker , J. H. M. M. Schmitt , P. Schöfer , E. Solano , A. Sota , O. Stahl , S. Stock , T. Stuber , J. Stürmer , J. C. Suárez , H. M. Tabernero , S. M. Tulloch , G. Veredas , J. I. Vico-Linares , F. Vilardell , K. Wagner , J. Winkler , V. Wolthoff , F. Yan , M. R. Zapatero Osorio

We have searched for planetary companions around 800 pulsars monitored at the Jodrell Bank Observatory, with both circular and eccentric orbits of periods between $20$ days and $17$ years and inclination-dependent planetary masses from…

地球与行星天体物理 · 物理学 2022-03-14 Iuliana C. Niţu , Michael J. Keith , Ben W. Stappers , Andrew G. Lyne , Mitchell B. Mickaliger

The substellar companion HD206893b has recently been discovered by direct imaging of its disc-bearing host star with the SPHERE instrument. We investigate the atypical properties of the companion, which has the reddest near-infrared colours…

Young intermediate-mass stars have become high-priority targets for direct-imaging planet searches following the recent discoveries of planets orbiting e.g. HR 8799 and Beta Pictoris. Close stellar companions to these stars can affect the…

太阳与恒星天体物理 · 物理学 2014-08-26 Kevin Gullikson , Adam Kraus , Sarah Dodson-Robinson

We present the current status of and new results from our search for exoplanets in a sample of solar-mass, evolved stars observed with the HARPS-N and the 3.6-m Telescopio Nazionale Galileo (TNG), and the High Resolution Spectrograph (HRS)…

地球与行星天体物理 · 物理学 2021-04-14 Andrzej T. Niedzielski , Eva Villaver , Monika Adamów , Kacper Kowalik , Aleksander Wolszczan , Gracjan Maciejewski

We report precise Doppler measurements of the stars HD 216437, HD 196050 and HD 160691 obtained with the Anglo-Australian Telescope using the UCLES spectrometer together with an iodine cell as part of the Anglo-Australian Planet Search. Our…

The planet-hosting and Sirius-type binary system epsilon Reticulum (HD 27442) is examined from the perspective of its more evolved white dwarf secondary. The stellar parameters are determined from a combination of Balmer line spectroscopy,…

太阳与恒星天体物理 · 物理学 2012-06-06 J. Farihi , M. R. Burleigh , J. B. Holberg , S. L. Casewell , M. A. Barstow

Transiting planets around young stars are key benchmarks for our understanding of planetary systems. One of such candidates was identified around the K dwarf HD 18599 by TESS, labeled as TOI-179. We present the confirmation of the…

Recent observations from B-star Exoplanet Abundance Study (BEAST) have illustrated the existence of sub-stellar companions around very massive stars. In this paper, we present the detection of two lower mass companions to a relatively…

We present the discovery of a low-mass companion located at $\rho$ $\sim$ 0\farcs{}85 ($r_{\rm proj} \approx 62~au$) from the early-type 1.2 Gyr-old star HIP 53005 using direct imaging data from the Subaru and Keck Telescopes and astrometry…

Various mechanisms have been proposed to explain the inflated size of HD 209458b after it became clear that it has no companions capable of producing a stellar reflex velocity greater than around 5 m/s. Had there been such a companion, the…

天体物理学 · 物理学 2007-10-03 Rosemary A. Mardling

We report the detection of 3 new extrasolar planets from the precise Doppler survey of G and K giants at Okayama Astrophysical Observatory. The host stars, namely, 18 Del (G6 III), xi Aql (K0 III) and HD 81688 (K0 III-IV), are located at…

We present the discovery of a white dwarf companion to the G1 V star 12 Psc found as part of a Keck adaptive optics imaging survey of long-term accelerating stars from the McDonald Observatory Planet Search Program. Twenty years of precise…

We report the discovery of a several-Jupiter mass planetary companion to the primary lens star in microlensing event OGLE-2005-BLG-071. Precise (<1%) photometry at the peak of the event yields an extremely high signal-to-noise ratio…

We report precise Doppler measurements of seven subgiants from Keck Observatory. All seven stars show variability in their radial velocities consistent with planet-mass companions in Keplerian orbits. The host stars have masses ranging from…

We report the detection of the lowest mass extra-solar planet yet found around a Sun-like star - a planet with an \msini of only 14.21 $\pm$ 2.91 Earth masses in an extremely short period orbit (P=2.808 days) around $\rho^{1}$ Cancri, a…