OGLE-2014-BLG-1186: gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source?

Research output: Contribution to journalJournal articleResearchpeer-review

Documents

  • stz306

    Final published version, 6.38 MB, PDF document

  • M. Dominik
  • E. Bachelet
  • V. Bozza
  • R. A. Street
  • C. Han
  • M. Hundertmark
  • A. Udalski
  • D. M. Bramich
  • K. A. Alsubai
  • S. Calchi Novati
  • S. Ciceri
  • G. D'Ago
  • R. Figuera Jaimes
  • T. C. Hinse
  • K. Horne
  • D. Juncher
  • N. Kains
  • H. Korhonen
  • L. Mancini
  • J. Menzies
  • A. Popovas
  • M. Rabus
  • S. Rahvar
  • G. Scarpetta
  • R. Schmidt
  • J. Skottfelt
  • C. Snodgrass
  • J. Southworth
  • D. Starkey
  • I. A. Steele
  • J. Surdej
  • Y. Tsapras
  • J. Wambsganss
  • O. Wertz
  • P. Pietrukowicz
  • M. K. Szymanski
  • P. Mroz
  • J. Skowron
  • I. Soszynski
  • K. Ulaczyk
  • R. Poleski
  • L. Wyrzykowski
  • S. Kozlowski
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume484
Issue number4
Pages (from-to)5608-5632
Number of pages25
ISSN0035-8711
DOIs
Publication statusPublished - Apr 2019

    Research areas

  • gravitational lensing: micro, methods: data analysis, methods: statistical, planets and satellites: detection, (stars:) binaries: eclipsing, Galaxy: kinematics and dynamics

Links

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