Fe emission and ionized excess absorption in the luminous quasar 3C 109 with XMM–Newton |
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| Authors: | G Miniutti D R Ballantyne S W Allen A C Fabian R R Ross |
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| Institution: | Osservatorio Astronomico di Cagliari, Loc. Poggio dei Pini, Strada 54, 09012 Capoterra (CA), Italy;National Centre for Radio Astrophysics, PO Bag 3, Ganeshkhind, Pune 411007, India;Universitàdegli Studi di Cagliari, Dipartimento di Fisica, SP Monserrato-Sestu km 0.7, 09042 Monserrato, Italy;Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL;Australia Telescope National Facility –CSIRO, PO Box 76, Epping, NSW 1710, Australia;Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA;National Astronomy and Ionosphere Center, Arecibo Observatory, HC3 Box 53995, PR 00612, USA |
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| Abstract: | The Parkes High-Latitude pulsar survey covers a region of the sky enclosed by Galactic longitudes 220° < l < 260° and Galactic latitudes | b | < 60°. The observations have been performed using the 20-cm multibeam receiver on the Parkes 64-m radio telescope. A total of 6456 pointings of 265 s each have been collected. The system adopted provided a sensitivity limit, for long-period pulsars with 5 per cent duty cycles, of ～0.5 mJy. Data analysis resulted in the detection of 42 pulsars of which 18 were new discoveries. Four of these belong to the class of the millisecond – or recycled – pulsars; three of these four are in binary systems. The double pulsar system J0737?3039 is among those and has been presented elsewhere. Here, we discuss the other discoveries and provide timing parameters for the objects for which we have a phase-connected solution. |
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| Keywords: | methods: observational pulsars: general |
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