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most citedThe MACHO Project: Microlensing Results from 5.7 Years of LMC Observations

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astro-ph2000★ 1 cited

VLT Deep I-band Surface Brightness Fluctuations of IC 4296

S. Mei, D. R. Silva, P. J. Quinn

From theoretical predictions, the introduction of 8-m class telescopes permits one to extend Surface Brightness Fluctuations measurements from the ground to ~7000 km/s, with a prec…

astro-ph2000★ 15 cited

Anomalous Surface Brightness Fluctuations in NGC 4489

S. Mei, D. R. Silva, P. J. Quinn

Anomalously high K-band surface brightness fluctuations (SBF) have been reported in NGC 4489 by Pahre & Mould (1994), Jensen et al. (1996) and Jensen et al. (1998). However, these…

astro-ph2000★ 36 cited

A 421 d Activity Cycle in the BeX Recurrent Transient A0538-66 from MACHO monitoring

C. Alcock, R. A. Allsman, D. R. Alves +23

We present a ~ 5-yr optical light curve of the recurrent Be/X-ray transient A0538-66 obtained as a by-product of the MACHO Project. These data reveal both a long-term modulation at…

astro-ph2000★ 44 cited

The MACHO Project Hubble Space Telescope Follow-Up: Preliminary Results on the Location of the Large Magellanic Cloud Microlensing Source Stars

C. Alcock, R. A. Allsman, D. R. Alves +21

We attempt to determine whether the MACHO microlensing source stars are drawn from the average population of the LMC or from a population behind the LMC by examining the HST color-…

astro-ph2000★ 1 cited

Galactic Bulge Microlensing Events with Clump Giants as Sources

P. Popowski, C. Alcock, R. A. Allsman +21

We present preliminary results of the analysis of 5 years of MACHO data on the Galactic bulge microlensing events with clump giants as sources. In particular, we discuss: 1) the se…

astro-ph2000★ 5 cited

Searching for periodicities in the MACHO light curve of LMC X-2

C. Alcock, R. A. Allsman, D. R. Alves +23

Using the exceptional long-term monitoring capabilities of the MACHO project, we present here the optical history of LMC X-2 for a continuous 6-yr period. These data were used to i…