FF
F. Finet
astro-ph.EPastro-ph.SRastro-ph.COastro-ph.GAastro-ph.HEastro-ph.IM
On Valency
published · living versionsW_grtgmvr3·v1 · currentpublished
Microlensing Discovery of a Population of Very Tight, Very Low-mass Binary Brown Dwarfs
with J. -Y. Choi, C. Han, A. Udalski, T. Sumi +119
1 version
Preprints & journals
32 papers in the corpus · 2009–2019X-ray study of the double source plane gravitational lens system Eye of Horus observed with XMM-Newton1911.04805v1 · Keigo Tanaka, Ayumi Tsuji, Hiroki Akamatsu et al.2019 · 2 citationsarXiv
XXL Survey XXI. The environment and clustering of X-ray AGN in the XXL-South field1712.01872v2 · O. Melnyk, A. Elyiv, V. Smolcic et al.2017 · 11 citationsA&A 620, A6 (2018)
J-GEM observations of an electromagnetic counterpart to the neutron star merger GW1708171710.05848v1 · Yousuke Utsumi, Masaomi Tanaka, Nozomu Tominaga et al.2017 · 229 citationsarXiv
A Challenge to Identify an Optical Counterpart of the Gravitational Wave Event GW151226 with Hyper Suprime-Cam1710.00127v1 · Yousuke Utsumi, Nozomu Tominaga, Masaomi Tanaka et al.2017 · 19 citationsarXiv
The Hyper Suprime-Cam SSP Survey: Overview and Survey Design1704.05858v3 · H. Aihara, N. Arimoto, R. Armstrong et al.2017 · 1,161 citationsPublications of the Astronomical Society of Japan, Volume 70, Issue SP1, S4 (2018)
First Data Release of the Hyper Suprime-Cam Subaru Strategic Program1702.08449v2 · Hiroaki Aihara, Robert Armstrong, Steven Bickerton et al.2017 · 647 citationsarXiv
MiNDSTEp differential photometry of the gravitationally lensed quasars WFI2033-4723 and HE0047-1756: Microlensing and a new time delay1610.03732v1 · E. Giannini, R. W. Schmidt, J. Wambsganß et al.2016 · 15 citationsA&A 597, A49 (2017)
The XXL survey XIV. AAOmega redshifts for the southern XXL field1512.04662v1 · C. Lidman, F. Ardila, M. Owers et al.2015 · 23 citationsarXiv
The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme1512.04317v1 · M. Pierre, F. Pacaud, C. Adami et al.2015 · 271 citationsarXiv
Predicted multiply-imaged X-ray AGNs in the XXL survey1507.00345v1 · F. Finet, A. Elyiv, O. Melnyk et al.2015 · 3 citationsarXiv
Transits and starspots in the WASP-6 planetary system1503.09184v1 · Jeremy Tregloan-Reed, John Southworth, M. Burgdorf et al.2015 · 70 citationsarXiv
High-precision photometry by telescope defocussing. VI. WASP-24, WASP-25 and WASP-261407.6253v1 · John Southworth, T. C. Hinse, M. Burgdorf et al.2014 · 71 citationsarXiv
MOA-2010-BLG-328Lb: a sub-Neptune orbiting very late M dwarf ?1309.7714v2 · K.Furusawa, A.Udalski, T.Sumi et al.2013 · 36 citationsarXiv
Search for gravitational lens candidates in the XMM-LSS/CFHTLS common field1307.2254v1 · A. Elyiv, O. Melnyk, F. Finet et al.2013 · 7 citationsarXiv
Physical properties, transmission and emission spectra of the WASP-19 planetary system from multi-colour photometry1306.6384v2 · L. Mancini, S. Ciceri, G. Chen et al.2013 · 97 citationsMonthly Notices of the Royal Astronomical Society 436, 2-18 (2013)
High-precision photometry by telescope defocussing. V. WASP-15 and WASP-161306.3509v1 · J. Southworth, L. Mancini, P. Browne et al.2013 · 33 citationsarXiv
Microlensing Discovery of a Population of Very Tight, Very Low-mass Binary Brown Dwarfs1302.4169v2 · J.-Y. Choi, C. Han, A. Udalski et al.2013 · 50 citationsarXivon Valency
Flux and color variations of the doubly imaged quasar UM6731302.0766v2 · D. Ricci, A. Elyiv, F. Finet et al.2013 · 8 citations2013A&A...551A.104R
MOA-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf Boundary1211.3782v2 · R. A. Street, J.-Y. Choi, Y. Tsapras et al.2012 · 46 citationsarXiv
MOA-2010-BLG-311: A planetary candidate below the threshold of reliable detection1210.6041v3 · J. C. Yee, L.-W. Hung, I. A. Bond et al.2012 · 19 citationsarXiv
MOA-2010-BLG-523: "Failed Planet" = RS CVn Star1210.6045v2 · A. Gould (OSU), J. C. Yee (OSU), I. A. Bond (Massey U.) et al.2012 · 16 citationsarXiv
The Transiting System GJ1214: High-Precision Defocused Transit Observations and a Search for Evidence of Transit Timing Variation1207.3064v2 · K. B. W. Harpsœ, S. Hardis, T. C. Hinse et al.2012 · 78 citationsarXiv
MOA-2010-BLG-477Lb: constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light1205.6323v1 · E. Bachelet, I.-G. Shin, C. Han et al.2012 · 77 citationsarXiv
Characterizing Lenses and Lensed Stars of High-Magnification Single-lens Gravitational Microlensing Events With Lenses Passing Over Source Stars1111.4032v2 · J.-Y. Choi, I.-G. Shin, S.-Y. Park et al.2011 · 33 citationsarXiv
Microlensing Binaries Discovered through High-Magnification Channel1109.3295v2 · I.-G. Shin, J.-Y. Choi, S.-Y. Park et al.2011 · 14 citationsarXiv
Discovery and Mass Measurements of a Cold, 10-Earth Mass Planet and Its Host Star1106.2160v1 · Y. Muraki, C. Han, D.P. Bennett et al.2011 · 121 citationsarXiv
I. Flux and color variations of the quadruply imaged quasar HE 0435-12231101.3664v3 · D. Ricci, J. Poels, A. Elyiv et al.2011 · 20 citationsarXiv
A much lower density for the transiting extrasolar planet WASP-71012.5181v1 · John Southworth, M. Dominik, U. G. Jorgensen et al.2010 · 22 citationsarXiv
A sub-Saturn Mass Planet, MOA-2009-BLG-319Lb1010.1809v3 · N. Miyake, T. Sumi, Subo Dong et al.2010 · 42 citationsarXiv
OGLE-2009-BLG-092/MOA-2009-BLG-137: A Dramatic Repeating Event With the Second Perturbation Predicted by Real-Time Analysis1009.0338v1 · Y.-H. Ryu, C. Han, K.-H. Hwang et al.2010 · 42 citationsarXiv
High-precision photometry by telescope defocussing. III. The transiting planetary system WASP-21006.4464v1 · John Southworth, L. Mancini, S. Calchi Novati et al.2010 · 57 citationsarXiv
Physical properties of the 0.94-day period transiting planetary system WASP-180910.4875v1 · John Southworth, T. C. Hinse, M. Dominik et al.2009 · 112 citationsAstrophys.J.707:167-172,2009; Erratum-ibid.723:1829,2010
Career total: 94 works. 32 are in this corpus.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.