@Article{HendersonPSUGTHGBABBBFFFIKLMMMNORSSSSTTWYYYSKPSSKPUWPABCCDDFHJJKLMMMNNPSSTTYABBDHHJKSSSCCCC:2014:CaGrMi,
author = "Henderson, C. B. and Park, H. and Sumi, T. and Udalski, A. and
Gould, A. and Tsapras, Y. and Han, C. and Gaudi, B. S. and Bozza,
V. and Abe, F. and Bennett, D. P. and Bond, I. A. and Botzler, C.
S. and Freeman, M. and Fukui, A. and Fukunaga, D. and Itow, Y. and
Koshimoto, N. and Ling, C. H. and Masuda, K. and Matsubara, Y. and
Muraki, Y. and Namba, S. and Ohnishi, K. and Rattenbury, N. J. and
Saito, To and Sullivan, D. J. and Suzuki, D. and Sweatman, W. L.
and Tristram, P. J. and Tsurumi, N. and Wada, K. and Yamai, N. and
Yock, P. C. M. and Yonehara, A. and Szymanski, M. K. and Kubiak,
M. and Pietrzynski, G. and Soszynski, I. and Skowron, J. and
Kozlowski, S. and Poleski, R. and Ulaczyk, K. and Wyrzykowski, L.
and Pietrukowicz, P. and Almeida, Leonardo A. and Bos, M. and
Choi, J. -Y. and Christie, G. W. and Depoy, D. L. and Dong, S. and
Friedmann, M. and Hwang, K. -H. and Jablonski, F. and Jung, Y. K.
and Kaspi, S. and Lee, C. -U. and Maoz, D. and McCormick, J. and
Moorhouse, D. and Natusch, T. and Ngan, H. and Pogge, R. W. and
Shin, I. -G. and Shvartzvald, Y. and Tan, T. -G. and Thornley, G.
and Yee, J. C. and Allan, A. and Bramich, D. M. and Browne, P. and
Dominik, M. and Horne, K. and Hundertmark, M. and Jaimes, R.
Figuera and Kains, N. and Snodgrass, C. and Steele, I. A. and
Street, R. A. and Collaboration, MOA and Collaboration, OGLE and
Collaboration, FUN and Collaboration, RoboNet",
affiliation = "{Ohio State University} and {Chungbuk National University} and
{Osaka University} and {Warsaw University Observatory} and {Ohio
State University} and {Las Cumbres Observatory Global Telescope
Network} and {Chungbuk National University} and {Ohio State
University} and {University of Salerno} and {Nagoya University}
and Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA. and
Massey Univ, Inst Informat \& Math Sci, North Shore Mail Ctr,
Auckland 0745, New Zealand. and Univ Auckland, Dept Phys, Auckland
1001, New Zealand. and Univ Auckland, Dept Phys, Auckland 1001,
New Zealand. and Victoria Univ, Sch Chem \& Phys Sci, Wellington
6140, New Zealand. and Nagoya Univ, Solar Terr Environm Lab,
Nagoya, Aichi 4648601, Japan. and Nagoya Univ, Solar Terr Environm
Lab, Nagoya, Aichi 4648601, Japan. and Osaka Univ, Dept Earth \&
Space Sci, Osaka 5600043, Japan. and Massey Univ, Inst Informat
\& Math Sci, North Shore Mail Ctr, Auckland 0745, New Zealand.
and Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601,
Japan. and Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi
4648601, Japan. and Nagoya Univ, Solar Terr Environm Lab, Nagoya,
Aichi 4648601, Japan. and Osaka Univ, Dept Earth \& Space Sci,
Osaka 5600043, Japan. and Natl Astron Observ Japan, Okayama
Astrophys Observ, Okayama 7190232, Japan. and Univ Auckland, Dept
Phys, Auckland 1001, New Zealand. and Nagano Natl Coll Technol,
Nagano 3818550, Japan. and Tokyo Metropolitan Coll Aeronaut, Tokyo
1168523, Japan. and Osaka Univ, Dept Earth \& Space Sci, Osaka
5600043, Japan. and Massey Univ, Inst Informat \& Math Sci, North
Shore Mail Ctr, Auckland 0745, New Zealand. and Mt John Univ
Observ, Lake Tekapo 8770, New Zealand. and Nagoya Univ, Solar Terr
Environm Lab, Nagoya, Aichi 4648601, Japan. and Osaka Univ, Dept
Earth \& Space Sci, Osaka 5600043, Japan. and Kyoto Sangyo Univ,
Fac Sci, Dept Phys, Kyoto 6038555, Japan. and Univ Auckland, Dept
Phys, Auckland 1001, New Zealand. and Kyoto Sangyo Univ, Fac Sci,
Dept Phys, Kyoto 6038555, Japan. and Univ Warsaw Observ, PL-00478
Warsaw, Poland. and Univ Warsaw Observ, PL-00478 Warsaw, Poland.
and Univ Warsaw Observ, PL-00478 Warsaw, Poland.; Univ Concepcion,
Dept Astron, Concepcion, Chile. and Univ Warsaw Observ, PL-00478
Warsaw, Poland. and Univ Warsaw Observ, PL-00478 Warsaw, Poland.
and Univ Warsaw Observ, PL-00478 Warsaw, Poland. and Ohio State
Univ, Dept Astron, Columbus, OH 43210 USA.; Univ Warsaw Observ,
PL-00478 Warsaw, Poland. and Univ Warsaw Observ, PL-00478 Warsaw,
Poland. and Univ Warsaw Observ, PL-00478 Warsaw, Poland.; Univ
Cambridge, Inst Astron, Cambridge CB3 0HA, England. and Univ
Warsaw Observ, PL-00478 Warsaw, Poland. and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and Molehill Astron Observ, North
Shore, New Zealand. and Chungbuk Natl Univ, Inst Astrophys, Dept
Phys, Cheongju 371763, South Korea. and Auckland Observ, Auckland,
New Zealand. and Texas A\&M Univ, Dept Phys \& Astron, College
Stn, TX 77843 USA. and Peking Univ, Kavli Inst Astron \&
Astrophys, Beijing 100871, Peoples R China. and Tel Aviv Univ, Sch
Phys \& Astron, IL-69978 Tel Aviv, Israel. and Chungbuk Natl
Univ, Inst Astrophys, Dept Phys, Cheongju 371763, South Korea. and
Obsev Pico dos Dias, Brazopolis, MG, Brazil. and Chungbuk Natl
Univ, Inst Astrophys, Dept Phys, Cheongju 371763, South Korea. and
Tel Aviv Univ, Sch Phys \& Astron, IL-69978 Tel Aviv, Israel. and
Korea Astron \& Space Sci Inst, Taejon 305348, South Korea. and
Tel Aviv Univ, Sch Phys \& Astron, IL-69978 Tel Aviv, Israel. and
Farm Cove Observ, Ctr Backyard Astrophys, Auckland, New Zealand.
and Kumeu Observ, Kumeu, New Zealand. and Auckland Observ,
Auckland, New Zealand.; AUT Univ, Inst Radiophys \& Space Res,
Auckland, New Zealand. and Auckland Observ, Auckland, New Zealand.
and Ohio State Univ, Dept Astron, Columbus, OH 43210 USA. and
Chungbuk Natl Univ, Inst Astrophys, Dept Phys, Cheongju 371763,
South Korea. and Tel Aviv Univ, Sch Phys \& Astron, IL-69978 Tel
Aviv, Israel. and Perth Exoplanet Survey Telescope, Perth, WA,
Australia. and Kumeu Observ, Kumeu, New Zealand. and Ohio State
Univ, Dept Astron, Columbus, OH 43210 USA.; Harvard Smithsonian
Ctr Astrophys, Cambridge, MA 02138 USA. and Univ Exeter, Sch Phys,
Exeter EX4 4QL, Devon, England. and Qatar Fdn, Qatar Environm \&
Energy Res Inst, Doha, Qatar. and Univ St Andrews, SUPA, Sch Phys
\& Astron, St Andrews KY16 9SS, Fife, Scotland. and Univ St
Andrews, SUPA, Sch Phys \& Astron, St Andrews KY16 9SS, Fife,
Scotland. and Univ St Andrews, SUPA, Sch Phys \& Astron, St
Andrews KY16 9SS, Fife, Scotland. and Univ St Andrews, SUPA, Sch
Phys \& Astron, St Andrews KY16 9SS, Fife, Scotland. and Univ St
Andrews, SUPA, Sch Phys \& Astron, St Andrews KY16 9SS, Fife,
Scotland.; European So Observ, D-85748 Garching, Germany. and
European So Observ, D-85748 Garching, Germany. and Max Planck Inst
Solar Syst Res, D-37191 Katlenburg Lindau, Germany. and Liverpool
John Moores Univ, Astrophys Res Inst, Wirral CH41 1LD, Merseyside,
England. and Cumbres Observ Global Telescope Network, Goleta, CA
93117 USA.",
title = "Candidaie gravitational microlensing events for future direct lens
imaging",
journal = "Astrophysical Journal",
year = "2014",
volume = "794",
number = "1",
month = "Oct.",
keywords = "binaries: general, gravitational lensing: micro.",
abstract = "The mass of the lenses giving rise to Galactic microlensing events
can be constrained by measuring the relative lenssource proper
motion and lens flux. The flux of the lens can be separated from
that of the source, companions to the source, and unrelated nearby
stars with high-resolution images taken when the lens and source
are spatially resolved. For typical ground-based adaptive optics
(AO) or space-based observations, this requires either
inordinately long time baselines or high relative proper motions.
We provide a list of microlensing events toward the Galactic bulge
with high relative lens-source proper motion that are therefore
good candidates for constraining the lens mass with future
high-resolution imaging. We investigate all events from 2004 to
2013 that display detectable finite-source effects, a feature that
allows us to measure the proper motion. In total, we present 20
events with mu >= 8 mas yr(-1). Of these, 14 were culled from
previous analyses while 6 are new, including OGLE-2004-BLG-368,
MOA-2005-BLG-36, OGLE-2012-BLG-0211, OGLE-2012-BLG-0456,
MOA-2012-BLG-532, and MOA-2013-BLG-029. In <= 12 yr from the time
of each event the lens and source of each event will be
sufficiently separated for ground-based telescopes with AO systems
or space telescopes to resolve each component and further
characterize the lens system. Furthermore, for the most recent
events, comparison of the lens flux estimates from images taken
immediately to those estimated from images taken when the lens and
source are resolved can be used to empirically check the
robustness of the single-epoch method currently being used to
estimate lens masses for many events.",
doi = "10.1088/0004-637X/794/1/71",
url = "http://dx.doi.org/10.1088/0004-637X/794/1/71",
issn = "0004-637X and 1538-4357",
label = "isi 2014-11
HendersonPSUGTHGBABBBFFFIKLMMMNORSSSSTTWYYYSKPSSKPUWPABCCDDFHJJKLMMMNNPSSTTYABBDHHJKSSSCCCC:2014:CAGRMI",
language = "en",
targetfile = "Henderson_candidate.pdf",
urlaccessdate = "27 abr. 2024"
}