Loading…
Galactic Bulge microlensing optical depth from EROS-2
Aims.We present a new EROS-2 measurement of the microlensing optical depth toward the Galactic Bulge. Methods.Light curves of $5.6\times 10^{6}$ clump-giant stars distributed over $66\,\rm deg^2$ of the Bulge were monitored during seven Bulge seasons. 120 events were found with apparent amplificatio...
Saved in:
Published in: | Astronomy and astrophysics (Berlin) 2006-07, Vol.454 (1), p.185-199 |
---|---|
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | Aims.We present a new EROS-2 measurement of the microlensing optical depth toward the Galactic Bulge. Methods.Light curves of $5.6\times 10^{6}$ clump-giant stars distributed over $66\,\rm deg^2$ of the Bulge were monitored during seven Bulge seasons. 120 events were found with apparent amplifications greater than 1.6 and Einstein radius crossing times in the range $5\,{\rm d} |
---|---|
ISSN: | 0004-6361 1432-0746 1432-0756 |
DOI: | 10.1051/0004-6361:20064893 |