Academia Sinica
Taiwan, Province of China
Matthew J. Lehner mainly investigates Astrophysics, Astronomy, Gravitational microlensing, Dark matter and Milky Way. His Astrophysics study focuses mostly on Large Magellanic Cloud, Stars, Massive compact halo object, Dark matter halo and Small Magellanic Cloud. Matthew J. Lehner focuses mostly in the field of Dark matter halo, narrowing it down to matters related to Galactic halo and, in some cases, Light dark matter and Baryonic dark matter.
His specific area of interest is Astronomy, where Matthew J. Lehner studies Light curve. The study incorporates disciplines such as Bulge, Halo, Black hole and Gravitational lens in addition to Gravitational microlensing. His study in Dark matter is interdisciplinary in nature, drawing from both Nuclear physics, Recoil and Pulse shape analysis.
Matthew J. Lehner spends much of his time researching Astrophysics, Astronomy, Stars, Occultation and Solar System. The Gravitational microlensing, Large Magellanic Cloud, Light curve and Variable star research Matthew J. Lehner does as part of his general Astrophysics study is frequently linked to other disciplines of science, such as Population, therefore creating a link between diverse domains of science. His biological study spans a wide range of topics, including Massive compact halo object, Dark matter halo, Milky Way, Dark matter and Gravitational lens.
Many of his research projects under Stars are closely connected to Cadence with Cadence, tying the diverse disciplines of science together. His Occultation research includes themes of Eclipse, Observatory, Remote sensing and Sky. Matthew J. Lehner interconnects Centaur and Asteroid in the investigation of issues within Solar System.
His primary areas of investigation include Solar System, Astronomy, Astrophysics, Population and Trans-Neptunian object. His research integrates issues of Telescope, Photometry, Photometry and Asteroid in his study of Solar System. His research investigates the connection between Telescope and topics such as Stars that intersect with issues in High-energy astronomy.
His biological study spans a wide range of topics, including Resonance scattering and Astrobiology. Matthew J. Lehner combines subjects such as Amplitude, Excited state and Surface with his study of Astrophysics. His study in Amplitude is interdisciplinary in nature, drawing from both Accretion, Orbital inclination, Light curve, Black hole and Large Synoptic Survey Telescope.
His primary areas of study are Solar System, Astrophysics, Population, Astronomy and Planetesimal. The concepts of his Solar System study are interwoven with issues in Telescope and Photometry. His Telescope study which covers Jupiter that intersects with Stars.
Astrophysics and Excited state are commonly linked in his work. When carried out as part of a general Astronomy research project, his work on Neptune and Trans-Neptunian object is frequently linked to work in Science and engineering and Research council, therefore connecting diverse disciplines of study. His study focuses on the intersection of Planetesimal and fields such as Asteroid with connections in the field of Object.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud Observations
Charles Alcock;Charles Alcock;Robyn Allsman;David R Alves;Tim Axelrod.
The Astrophysical Journal (2000)
The MACHO Project Large Magellanic Cloud Microlensing Results from the First Two Years and the Nature of the Galactic Dark Halo
C. Alcock;C. Alcock;R. A. Allsman;D. Alves;D. Alves;T. S. Axelrod.
The Astrophysical Journal (1997)
The Macho Project: 45 Candidate Microlensing Events from the First Year Galactic Bulge Data
C. Alcock;C. Alcock;R. A. Allsman;D. Alves;T. S. Axelrod;T. S. Axelrod.
The Astrophysical Journal (1997)
The MACHO Project: 45 Candidate Microlensing Events from the First Year Galactic Bulge Data
C. Alcock;R. A. Allsman;T. S. Axelrod;D. P. Bennett.
arXiv: Astrophysics (1995)
First Observation of Parallax in a Gravitational Microlensing Event
C. Alcock;C. Alcock;R. A. Allsman;D. Alves;D. Alves;T. S. Axelrod;T. S. Axelrod.
The Astrophysical Journal (1995)
EROS and MACHO combined limits on planetary-mass dark matter in the galactic halo
C Alcock;C Alcock;RA Allsman;D Alves;D Alves;R Ansari.
The Astrophysical Journal (1998)
The MACHO Project: Microlensing Optical Depth Toward the Galactic Bulge from Difference Image Analysis
Charles Alcock;Charles Alcock;Robyn Allsman;David R Alves;Tim Axelrod.
The Astrophysical Journal (2000)
The macho project first-year large magellanic cloud results: The microlensing rate and the nature of the galactic dark halo
C. Alcock;R. A. Allsman;T. S. Axelrod;D. P. Bennett.
The Astrophysical Journal (1996)
Calibration of the MACHO Photometry Database
C. Alcock;R. A. Allsman;D. R. Alves;T. S. Axelrod.
arXiv: Astrophysics (1999)
MACHO Project Limits on Black Hole Dark Matter in the 1-30 M☉ Range
Charles Alcock;Charles Alcock;Robyn Allsman;David R Alves;Tim Axelrod.
The Astrophysical Journal (2001)
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