SIMBAD references

2003ApJ...595..794V - Astrophys. J., 595, 794-802 (2003/October-1)

Using optical and near-infrared photometry to test MACHO lens candidates.

VON HIPPEL T., SARAJEDINI A. and RUIZ M.T.

Abstract (from CDS):

We obtained new VLT/ISAAC H-band observations for five MACHO LMC source stars and adjacent LMC field regions. After combining our near-IR photometry with Hubble Space Telescope/PC BVRI optical photometry, we compared the MACHO objects to the adjacent field stars in a variety of color-magnitude and color-color diagrams. These diagnostic diagrams were chosen to be sensitive to our hypothesis that at least some of the MACHO lenses were foreground Galactic disk or thick-disk M dwarfs. For the five lensed objects we studied, our hypothesis could be ruled out for main-sequence lens masses ≳0.1 Mfor distances out to 4 kpc. On the other hand, the fact that LMC MACHO 5, an object not in our study, has been recently found to have just such a foreground lens highlights that the remainder of the LMC MACHO objects should be searched for the signature of their lenses using our photometric technique or via near-IR spectroscopy. We also constructed diagnostic color-color diagrams sensitive to determining reddening for the individual MACHO source stars and found that these five objects did not show evidence for significant additional reddening. At least these five MACHO objects are thus also inconsistent with the LMC self-lensing hypothesis.

Abstract Copyright:

Journal keyword(s): Cosmology: Gravitational Lensing

CDS comments: Parag. 3.5 : The ref. Alcock et al. 2000a is a misprint for Alcock et al. 2000b (2000ApJ.542.281A)

Simbad objects: 15

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2003ApJ...595..794V and select 'bookmark this link' or equivalent in the popup menu


2021.05.11-09:53:20

© Université de Strasbourg/CNRS

    • Contact