Spectroscopic characterisation of microlensing events - Towards a new interpretation of OGLE-2011-BLG-0417
暂无分享,去创建一个
J. Beaulieu | D. James | D. Bennett | A. Santerne | J. Almenara | I. Boisse | R. D'iaz | N. Santos | P. Figueira | J. Lillo-Box | S. Sousa | E. Schlawin | T. Herter | J. Marquette | V. Batista | C. Ranc | B. R. Ayala
[1] A. Santerne,et al. WASP-121 b: a hot Jupiter close to tidal disruption transiting an active F star , 2015, 1506.02471.
[2] D. Bennett,et al. A New Nonplanetary Interpretation of the Microlensing Event OGLE-2013-BLG-0723 , 2016, 1604.06533.
[3] A. Bhattacharya,et al. CONFIRMATION OF THE OGLE-2005-BLG-169 PLANET SIGNATURE AND ITS CHARACTERISTICS WITH LENS–SOURCE PROPER MOTION DETECTION , 2015, 1507.08914.
[4] R. Pfeifle,et al. CONFIRMATION OF THE PLANETARY MICROLENSING SIGNAL AND STAR AND PLANET MASS DETERMINATIONS FOR EVENT OGLE-2005-BLG-169 , 2015, 1507.08661.
[5] K. Ulaczyk,et al. OGLE-2012-BLG-0563Lb: A SATURN-MASS PLANET AROUND AN M DWARF WITH THE MASS CONSTRAINED BY SUBARU AO IMAGING , 2015, 1506.08850.
[6] J. Beaulieu,et al. The first radial velocity measurements of a microlensing event: no evidence for the predicted binary , 2015, 1506.02019.
[7] A. Santerne,et al. PASTIS: Bayesian extrasolar planet validation II. Constraining exoplanet blend scenarios using spectroscopic diagnoses , 2015, 1505.02663.
[8] David J Armstrong,et al. One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c , 2015, Astronomy & Astrophysics.
[9] C. Moutou,et al. CoRoT-22 b: a validated 4.9 R⊕ exoplanet in 10-d orbit , 2014, 1408.2576.
[10] S. Sousa. ARES + MOOG: A Practical Overview of an Equivalent Width (EW) Method to Derive Stellar Parameters , 2014, 1407.5817.
[11] T. L. Herter,et al. Design updates and status of the fourth generation TripleSpec spectrograph , 2014, Astronomical Telescopes and Instrumentation.
[12] R. Roy,et al. SOPHIE velocimetry of Kepler transit candidates - XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet , 2014, 1406.6172.
[13] J. Lillo-Box,et al. High-resolution imaging of Kepler planet host candidates - A comprehensive comparison of different techniques , 2014, 1405.3120.
[14] France,et al. PASTIS: Bayesian extrasolar planet validation. I. General framework, models, and performance , 2014, 1403.6725.
[15] C. H. Ling,et al. MOA-2011-BLG-262Lb: A SUB-EARTH-MASS MOON ORBITING A GAS GIANT PRIMARY OR A HIGH VELOCITY PLANETARY SYSTEM IN THE GALACTIC BULGE , 2013, 1312.3951.
[16] W. Freudling,et al. Automated data reduction workflows for astronomy , 2013, 1311.5411.
[17] C. H. Ling,et al. INTERPRETATION OF A SHORT-TERM ANOMALY IN THE GRAVITATIONAL MICROLENSING EVENT MOA-2012-BLG-486 , 2013, 1308.5762.
[18] R. Poleski,et al. OGLE-2002-BLG-360: from a gravitational microlensing candidate to an overlooked red transient , 2013, 1304.1694.
[19] A. Gould,et al. OGLE-2011-BLG-0417: A RADIAL VELOCITY TESTBED FOR MICROLENSING , 2013, 1302.0841.
[20] C. H. Ling,et al. CHARACTERIZING LOW-MASS BINARIES FROM OBSERVATION OF LONG-TIMESCALE CAUSTIC-CROSSING GRAVITATIONAL MICROLENSING EVENTS , 2012, 1204.2869.
[21] J. B. Marquette,et al. A frozen super-Earth orbiting a star at the bottom of the main sequence , 2010, 1009.5665.
[22] R. Manuputy,et al. X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope , 2011, 1110.1944.
[23] K. Ulaczyk,et al. BINARY MICROLENSING EVENT OGLE-2009-BLG-020 GIVES VERIFIABLE MASS, DISTANCE, AND ORBIT PREDICTIONS , 2011, 1101.3312.
[24] R. de Grijs,et al. VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way , 2009, 0912.1056.
[25] Frantz Martinache,et al. The performance of TripleSpec at Palomar , 2008, Astronomical Telescopes + Instrumentation.
[26] N. Santos,et al. New constraints from the Hα line for the temperature of the transiting planet host star OGLE‐TR‐10 , 2008 .
[27] Darko Jevremovic,et al. The Dartmouth Stellar Evolution Database , 2008, 0804.4473.
[28] Hiroyuki Mito,et al. The IRSA 2MASS all-sky point source catalog , 2008 .
[29] J. Beaulieu,et al. Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing , 2006, Nature.
[30] James Howard,et al. Mass producing an efficient NIR spectrograph , 2004, SPIE Astronomical Telescopes + Instrumentation.
[31] John T. Rayner,et al. Spextool: A Spectral Extraction Package for SpeX, a 0.8–5.5 Micron Cross‐Dispersed Spectrograph , 2004 .
[32] J. Lépine,et al. Models for Interstellar Extinction in the Galaxy , 2005 .
[33] H Germany,et al. A Method of Correcting Near‐Infrared Spectra for Telluric Absorption , 2002, astro-ph/0211255.
[34] P. Kroupa. On the variation of the initial mass function , 2000, astro-ph/0009005.
[35] Bernard Delabre,et al. Design, construction, and performance of UVES, the echelle spectrograph for the UT2 Kueyen Telescope at the ESO Paranal Observatory , 2000, Astronomical Telescopes and Instrumentation.
[36] Andrew Gould,et al. A Natural Formalism for Microlensing , 2000, astro-ph/0001421.
[37] Edward L. Fitzpatrick,et al. Correcting for the Effects of Interstellar Extinction , 1998, astro-ph/9809387.
[38] M. Dworetsky,et al. Peculiar versus Normal Phenomena in A-type and Related Stars , 1993 .
[39] J. B. Oke. Absolute spectral energy distributions for white dwarfs , 1974 .