Other
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..188c&link_type=abstract
XMM-Newton Proposal ID #03058201
Other
White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Xte J1814-338, Xmm-Newton Proposal 03058201
Scientific paper
XTE J1814-338 is the 5th transient millisecond X-ray pulsar (TMXP) discovered. In outburst and in quiescence TMXP are peculiar, showing faint outbursts, weaker quiescent luminosities and (when detected) lack of the soft component usually observed in other quiescent transients. Here we propose to observe for the first time XTE J1814-338 in quiescence. In the last few years a good sample of quiescent transients have been observed providing spectral information with some details and allowing to study the sample of quiescent transients statistically. Only one source has too few counts (22) to asses its quiescent spectrum: XTE J2123-058. Here we ask to observe this source to complement existing data and to disentangle the soft and hard components in its spectrum.
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