FISICA APLICADA
Departamento
University of Crete
Heraklion, GreciaPublicaciones en colaboración con investigadores/as de University of Crete (26)
2019
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Advances in Understanding High-Mass X-ray Binaries with INTEGRALand Future Directions
New Astronomy Reviews, Vol. 86
2016
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The LOFT mission concept - A status update
Proceedings of SPIE - The International Society for Optical Engineering
2014
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The large observatory for x-ray timing
Proceedings of SPIE - The International Society for Optical Engineering
2009
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Discovery of slow X-ray pulsations in the high-mass X-ray binary 4U 2206+54
Astronomy and Astrophysics, Vol. 494, Núm. 3, pp. 1073-1082
2008
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INTEGRAL long-term monitoring of the supergiant fast X-ray transient XTE J1739-302
Astronomy and Astrophysics, Vol. 489, Núm. 2, pp. 669-676
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Supergiant Fast X-ray Transients and other wind accretors
POPULATION EXPLOSION: THE NATURE AND EVOLUTION OF X-RAY BINARIES IN DIVERSE ENVIRONMENTS
2007
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4U 2206+54, a multiwavelength approach
6TH INTEGRAL WORKSHOP: THE OBSCURED UNIVERSE
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Sax J2103.5+4545: Bright and faint states characterized with INTEGRAL
6TH INTEGRAL WORKSHOP: THE OBSCURED UNIVERSE
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Supergiant fast X-ray transients: A common behaviour or a class of objects?
6TH INTEGRAL WORKSHOP: THE OBSCURED UNIVERSE
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The Be/X-ray transient 4U 0115+63/V635 Cassiopeiae III. Quasi-cyclic variability
Astronomy and Astrophysics, Vol. 462, Núm. 3, pp. 1081-1089
2006
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4U 2206+54, A multiwavelength approach
European Space Agency, (Special Publication) ESA SP
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Multiwavelength monitoring of BD +53°2790, the optical counterpart to 4U 2206+54
Astronomy and Astrophysics, Vol. 446, Núm. 3, pp. 1095-1105
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SAX J2103.5+4545, the closest Be plus neutron star galactic system.
PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2
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SAX J2103.5+4545, the closest be+neutron star galactic system
European Space Agency, (Special Publication) ESA SP
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SAX J2103.5+4545: Bright and faint states characterized with integral
European Space Agency, (Special Publication) ESA SP
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Supergiant fast X-ray transients: A new class of high mass X-ray binaries unveiled by integral
PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2
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Wind accretion in the massive X-ray binary 4U 2206+54: Abnormally slow wind and a moderately eccentric orbit
Astronomy and Astrophysics, Vol. 449, Núm. 2, pp. 687-698
2005
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Further evidence for the presence of a neutron star in 4U 2206+54. INTEGRAL and VLA observations
Astronomy and Astrophysics, Vol. 438, Núm. 3, pp. 963-972
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Identification of the optical counterparts of high-mass X-ray binaries through optical photometry and spectroscopy
Astronomy and Astrophysics, Vol. 440, Núm. 2, pp. 637-646
2004
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Discovery of the optical counterpart to the X-ray pulsar SAX J2103.5+4545
Astronomy and Astrophysics, Vol. 421, Núm. 2, pp. 673-680