Computer Science
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005noao.prop..466o&link_type=abstract
NOAO Proposal ID #2005B-0466
Computer Science
Scientific paper
Searches for the transient brightening of LMC stars due to the gravitational lensing by foreground MACHOs have produced a peculiar result: while the event rate indicates that MACHOs comprise at most ~20% of the dark matter halo, it also far exceeds that expected from known stellar populations. The possible explanations range from the presence of previously undetected tidally stripped LMC material to halo dark matter in the form of compact stellar-mass objects. The SuperMACHO program aims to determine the nature of the lenses by collecting 10× more events than previous searches. However, critical complementary evidence must come from study of the LMC stellar populations themselves. In 2004B, the NOAO TAC awarded 6 half-nights on the CTIO 4-m and 7 nights of 1.0-m time to cover the SuperMACHO fields in B and I. Because the 2004B observing season was plagued by poor seeing, telescope problems, and the unavailability of the expected 4K imager on the CTIO 1.0-m, we are proposing for an additional 2 half- nights of CTIO 4-m time and 7 nights of CTIO 1.0-m time to complete this project. These observations will allow us to (1) reveal whether a significant fraction of events prefer a particular LMC stellar population, and (2) measure the structure of the inner LMC Bar and disk, which may help to reveal tidal debris.
Becker Andrew C.
Clocchiatti Alejandro
Cook Kem
Garg Arti
Miceli Antonino
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