Search Results - "Tomaney, A. B"
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The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud Observations
Published in The Astrophysical journal (10-10-2000)Get full text
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MACHO Project Limits on Black Hole Dark Matter in the 1-30 M Range
Published in The Astrophysical journal (01-04-2001)Get full text
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Direct detection of a microlens in the Milky Way
Published in Nature (London) (06-12-2001)“…The nature of dark matter remains mysterious, with luminous material accounting for at most ∼25 per cent of the baryons in the Universe. We accordingly…”
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The MACHO Project: Microlensing Optical Depth toward the Galactic Bulge from Difference Image Analysis
Published in The Astrophysical journal (01-10-2000)Get full text
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Gravitational Microlensing Events Due to Stellar-Mass Black Holes
Published in The Astrophysical journal (10-11-2002)Get full text
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Calibration of the MACHO Photometry Database
Published in Publications of the Astronomical Society of the Pacific (01-12-1999)“…The MACHO Project is a microlensing survey that monitors the brightnesses of ∼60 million stars in the Large Magellanic Cloud (LMC), Small Magellanic Cloud, and…”
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MACHO 96-LMC-2: Lensing of a Binary Source in the Large Magellanic Cloud and Constraints on the Lensing Object
Published in The Astrophysical journal (01-05-2001)Get full text
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First Detection of a Gravitational Microlensing Candidate toward the Small Magellanic Cloud
Published in The Astrophysical journal (10-12-1997)Get full text
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Is the Large Magellanic Cloud Microlensing Due to an Intervening Dwarf Galaxy?
Published in The Astrophysical journal (20-11-1997)Get full text
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Mass-losing Semiregular Variable Stars in Baade's Windows
Published in The Astrophysical journal (01-05-2001)“…By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been…”
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DO LEONIS: A NEW ECLIPSING CATACLYSMIC VARIABLE
Published in Publications of the Astronomical Society of the Pacific (01-05-1990)“…Photometric and spectroscopic observations of DO Leo have been obtained using the McDonald Observatory high-speed CCD photometer and a conventional two-channel…”
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A 421-d activity cycle in the BeX recurrent transient A0538-66 from MACHO monitoring
Published in Monthly notices of the Royal Astronomical Society (11-03-2001)“…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…”
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The MACHO Project: Microlensing Optical Depth toward the Galactic Bulge from Difference Image Analysis
Published in The Astrophysical journal (20-08-2001)Get full text
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Searching for periodicities in the MACHO light curve of LMC X-2
Published in Monthly notices of the Royal Astronomical Society (21-08-2000)“…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…”
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Results from a Survey of Gravitational Microlensing toward M31
Published in The Astrophysical journal (20-12-1996)Get full text
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Searching for periodicities in the MACHO light curve of LMC X-2
Published in Monthly notices of the Royal Astronomical Society (01-08-2000)Get full text
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The MACHO Project HST Follow-Up: The Large Magellanic Cloud Microlensing Source Stars
Published 12-02-2009“…We present Hubble Space Telescope (HST) WFPC2 photometry of 13 microlensed source stars from the 5.7 year Large Magellanic Cloud (LMC) survey conducted by the…”
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Variability-Selected Quasars in MACHO Project Magellanic Cloud Fields
Published 24-09-2002“…Astron.J. 125 (2003) 1 We present 47 spectroscopically-confirmed quasars discovered behind the Magellanic Clouds identified via photometric variability in the…”
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