2015MNRAS.450.1565L


Query : 2015MNRAS.450.1565L

2015MNRAS.450.1565L - Mon. Not. R. Astron. Soc., 450, 1565-1584 (2015/June-3)

The complete catalogue of light curves in equal-mass binary microlensing.

LIEBIG C., D'AGO G., BOZZA V. and DOMINIK M.

Abstract (from CDS):

The light curves observed in microlensing events due to binary lenses span an extremely wide variety of forms, characterized by U-shaped caustic crossings and/or additional smoother peaks. However, all peaks of the binary-lens light curve can be traced back to features of caustics of the lens system. Moreover, all peaks can be categorized as one of only four types (cusp-grazing, cusp-crossing, fold-crossing or fold-grazing). This enables us to present the first complete map of the parameter space of the equal-mass case by identifying regions in which light curves feature the same number and nature of peaks. We find that the total number of morphologies that can be obtained is 73 out of 232 different regions. The partition of the parameter space so-obtained provides a new key to optimize modelling of observed events through a clever choice of initial conditions for fitting algorithms.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): Gravitational lensing: micro - methods: numerical

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 OGLE-2009-BLG-510 * 18 09 37.65 -26 02 26.7           ~ 7 0

Query : 2015MNRAS.450.1565L

Basic data :
OGLE-2009-BLG-510 -- Star
Other object types:
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* (), Lev (MOA,OGLE)
ICRS coord. (ep=J2000) :
18 09 37.65 -26 02 26.7 [ ] D 2012ApJ...746..127S
FK4 coord. (ep=B1950 eq=1950) :
18 06 31.23 -26 03 02.0 [ ]
Gal coord. (ep=J2000) :
005.17321 -03.15914 [ ]
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MOA 2008-BLG-369 OGLE-2008-BLG-510 OGLE-2009-BLG-510

References (7 between 1850 and 2026) (Total 7)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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