Publikationen in Zusammenarbeit mit Forschern von University of Crete (33)

2018

  1. NuSTAR rules out a cyclotron line in the accreting magnetar candidate 4U2206+54

    Monthly Notices of the Royal Astronomical Society, Vol. 479, Núm. 3, pp. 3366-3372

2016

  1. The LOFT mission concept - A status update

    Proceedings of SPIE - The International Society for Optical Engineering

2014

  1. The large observatory for x-ray timing

    Proceedings of SPIE - The International Society for Optical Engineering

2012

  1. Accreting magnetars: A new type of high-mass X-ray binaries?

    Monthly Notices of the Royal Astronomical Society, Vol. 425, Núm. 1, pp. 595-604

  2. LOFT - The large observatory for x-ray timing

    Proceedings of SPIE - The International Society for Optical Engineering, Vol. 8443

2010

  1. BeX systems, an INTEGRAL view

    Proceedings of Science

2009

  1. 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

  1. BeX systems as seen by INTEGRAL

    Proceedings of Science

  2. INTEGRAL long-term monitoring of the supergiant fast X-ray transient XTE J1739-302

    Astronomy and Astrophysics, Vol. 489, Núm. 2, pp. 669-676

  3. Supergiant Fast X-ray Transients and other wind accretors

    POPULATION EXPLOSION: THE NATURE AND EVOLUTION OF X-RAY BINARIES IN DIVERSE ENVIRONMENTS

2007

  1. 4U 2206+54, a multiwavelength approach

    6TH INTEGRAL WORKSHOP: THE OBSCURED UNIVERSE

  2. Sax J2103.5+4545: Bright and faint states characterized with INTEGRAL

    6TH INTEGRAL WORKSHOP: THE OBSCURED UNIVERSE

  3. Supergiant fast X-ray transients: A common behaviour or a class of objects?

    6TH INTEGRAL WORKSHOP: THE OBSCURED UNIVERSE

  4. 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

  1. 4U 2206+54, A multiwavelength approach

    European Space Agency, (Special Publication) ESA SP

  2. Multiwavelength monitoring of BD +53°2790, the optical counterpart to 4U 2206+54

    Astronomy and Astrophysics, Vol. 446, Núm. 3, pp. 1095-1105

  3. SAX J2103.5+4545, the closest Be plus neutron star galactic system.

    PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2