2005A&A...442..501A


Query : 2005A&A...442..501A

2005A&A...442..501A - Astronomy and Astrophysics, volume 442, 501-505 (2005/11-1)

Source blending effects on microlensing time-histograms and optical depth determination.

ALIBERT Y., CHABRIER G. and MASSACRIER G.

Abstract (from CDS):

Source blending in microlensing experiments is known to modify the Einstein time of the observed events. In this paper, we have conducted Monte-Carlo calculations, using analytical relationships to quantify the effect of blending on the observed event time distribution and optical depth. We show that short events are affected significantly by source blending and that, for moderately blended sources, the optical depth τ is globally overestimated, because of an underestimation of the exposure. For high blending situations, on the other hand, blending leads to an underestimation of the optical depth. Our results are in agreement with the most recent optical depth determinations toward the Galactic Center of the MACHO and OGLE-II collaborations that use clump giants (less affected by the blending effect) as sources. The blending-corrected, lower optical depth toward the Galactic Bulge is now in good agreement with the value inferred from galactic models, reconciling theoretical and observational determinations.

Abstract Copyright:

Journal keyword(s): Galaxy: stellar content - galaxies: structure - gravitational lensing

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 NAME Galactic Center gam 17 45 39.60213 -29 00 22.0000           ~ 12299 0
2 NAME Galactic Bulge reg ~ ~           ~ 3622 0

    Equat.    Gal    SGal    Ecl

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2021.07.24-05:28:24

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