Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
University of Toronto
IoA
Utrecht Univ.
Palomar Observatory, Caltech
Univ. of Toronto
Utrecht University
U. Toronto
Caltech, Toronto
Utrecht University;
Utrecht Univ. / Astron. Inst
Dept. of Astronomy, Caltech
Univ. of Amsterdam, Caltech
U. Amsterdam, Caltech
U. of Toronto
University of Toronto, Canada
Amsterdam, Universiteit, Netherlands
IoA / Cambridge
Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4, Canada of Astronomy, California Institute of Technology, Pasadena, CA 91125, USA
Astronomical Institute, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
Amsterdam, University; Centre for High Energy Astrophysics, Netherlands; California, University, Santa Barbara
Department of Astronomy, California Institute of Technology, 105-24, Pasadena, CA 91125, USA
Astronomical Institute, Utrecht University, PO Box 80000, 3508 TA Utrecht, The Netherlands
California Institute of Technology, California
Amsterdam Univ; Centre for High Energy Astrophysics, Netherlands
Astronomical Institute "Anton Pannekoek", University of Amsterdam and Center for High Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands; Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
University of Western Ontario, London.
Astronomical Institute, Utrecht University, P.O. Box 80000, 3508 TA Utrecht, The Netherlands
Amsterdam Univ; Center for High Energy Astrophysics, Netherlands
Universities Space Research Association
UofT
Uni. of Toronto
Department of Astronomy & Astrophysics, University of Toronto
Caltech
KIAA / PKU
University of Toronto, Department of Astronomy and Astrophysics, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
Department of Astronomy & Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON
A 1500-MHz survey for pulsars near the Galactic Centre
A 59 M photometric period in the dwarf nova V 485 Centauri
A Coherent Timing Solution for the Nearby Isolated Neutron Star RX J0720.4-3125
A Coherent Timing Solution for the Nearby Isolated Neutron Star RX J1308.6+2127/RBS 1223
A Coherent Timing Solution for the Nearby, Thermally Emitting Isolated Neutron Star RX J0420.0-5022
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