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The variable radio counterpart and possible large-scale jet of the new Z-source XTE J1701-462

(2007)

Authors:

RP Fender, M Dahlem, J Homan, S Corbel, R Sault, TM Belloni
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The variability plane of accreting compact objects

(2007)

Authors:

EG Koerding, S Migliari, R Fender, T Belloni, C Knigge, I McHardy
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The high energy emission of GRO J1655-40 as revealed with INTEGRAL spectroscopy of the 2005 outburst

(2007)

Authors:

MD Caballero-Garcia, JM Miller, E Kuulkers, M Diaz Trigo, J Homan, WHG Lewin, P Kretschmar, A Domingo, JM Mas-Hesse, R Wijnands, AC Fabian, RP Fender, M van der Klis
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The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197

ArXiv 0705.4095 (2007)

Authors:

F Camilo, SM Ransom, J Penalver, A Karastergiou, MH van Kerkwijk, M Durant, JP Halpern, J Reynolds, C Thum, DJ Helfand, N Zimmerman, I Cognard

Abstract:

We have observed the 5.54s anomalous X-ray pulsar XTE J1810-197 at radio, millimeter, and infrared (IR) wavelengths, with the aim of learning about its broad-band spectrum. At the IRAM 30m telescope, we have detected the magnetar at 88 and 144GHz, the highest radio-frequency emission ever seen from a pulsar. At 88GHz we detected numerous individual pulses, with typical widths ~2ms and peak flux densities up to 45Jy. Together with nearly contemporaneous observations with the Parkes, Nancay, and Green Bank telescopes, we find that in late 2006 July the spectral index of the pulsar was -0.5
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Evidence for a jet contribution to the optical/infrared light of neutron star X-ray binaries

(2007)

Authors:

DM Russell, RP Fender, PG Jonker
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