Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
TMT Observatory Corporation, USA
St.Andrews
Thiry Meter Telescope
TMT Observatory Corporation, Pasadena, CA, USA
TMT Observatory Corporation, Pasadena, USA
TMT Observatory Corporation, 2632 E. Washington Blvd., Pasadena, CA 91107, USA
School of Physics and Astronomy, University of St. Andrews, UK
St. Andrews University
Thirty Meter Telescope
School of Physics and Astronomy, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS, UK.
Keele University, Department of Physics, Keele, Staffordshire ST5 5BG; University of Wyoming, Physics and Astronomy Department, Laramie, WY 82071, USA
Department of Physics and Astronomy, University of Wyoming, Wyoming, WY 82071-3985, USA
University of St-Andrews, School of Physics and Astronomy, North Haugh, St Andrews, Fife, KY16-9SS, Scotland; Department of Physics and Astronomy, University of Wyoming, PO Box 3905, Laramie, WY 82071, USA
University of St. Andrews / W.I.R.O.
Univ. St. Andrews
St. Andrews University, Scotland
TMT Observatory Corp., USA
Keele, University
TMT Observatory Corporation, 1200 E. California Blvd, Pasadena, CA, USA
School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS; Department of Physics and Astronomy, University of Wyoming, PO Box 3905, University Station, Laramie, WY 82071, USA
Department of Physics and Astronomy, University of 82071-3985, Wyoming, WY, USA
Thirty Meter Telescope, USA
Keele University, Department of Physics, Keele, Staffordshire ST55BG
Wyoming Infrared Observatory and Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071
Thirty Meter Telescope Project, USA
California Institute of Technology, USA
A Search for Magnetic Activity in Secondary Stars of Late Type CVs
All Sky Camera Observations of Cloud and Light Pollution at Thirty Meter Telescope Candidate Sites
An analysis of light pollution at the Thirty Meter Telescope candidate sites
Analysis of the oscillations in HST observations of the quiescent SU UMa type dwarf nova WZ Sagittae
Can SPH Simulations of CV Accretion Discs Predict the Observed Periodic Signals of WZ Sge?
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