activity
19952003
most citedRecent Microlensing Results from the MACHO Project

1 citations · 2 across the 2 of their papers we have counts for

collaborators

16 papers

astro-ph20031 cited

Recent Microlensing Results from the MACHO Project

P. Popowski, C. A. Nelson, D. P. Bennett +19

We describe a few recent microlensing results from the MACHO Collaboration. The aim of the MACHO Project was the identification and quantitative description of dark and luminous ma…

astro-ph20021 cited

Statistical Methods for Detecting Stellar Occultations by Kuiper Belt Objects: the Taiwanese-American Occultation Survey

Chyng-Lan Liang, John A. Rice, Imke de Pater +3

The Taiwanese-American Occultation Survey (TAOS) will detect objects in the Kuiper Belt, by measuring the rate of occultations of stars by these objects, using an array of three to…

astro-ph2002

MACHO Project Analysis of the Galactic Bulge Microlensing Events with Clump Giants as Sources

P. Popowski, T. Vandehei, K. Griest +19

We present preliminary results of the analysis of 5 years of MACHO data on the Galactic bulge microlensing events with clump giants as sources. This class of events allows one to o…

astro-ph2000

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-ph1999

Cepheid Variables in the LMC and SMC

The MACHO Collaboration, D. L. Welch, C. Alcock +20

In this paper, we will review major new results regarding classical Cepheids, in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). Specifically, we discuss recent…

astro-ph1997

Pulsating Variable Stars in the MACHO Bulge database: The Semiregular Variables

D. Minniti, C. Alcock, R. A. Allsman +17

We review the pulsating stars contained in the top 24 fields of the MACHO bulge database, with special emphasis on the red semiregular stars. Based on period, amplitude and color c…