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We present results from the archival Chandra observations of the 0.3 s X-ray pulsar PSR J1846−0258 associated with the supernova remnant (SNR) Kes 75. The pulsar has the highest spin-down luminosity (˙ E=8.3×10 36 erg s −1) among all the high magnetic field pulsars (HBPs) and has been classified as a Crab-like pul-sar despite its magnetic field (5×10 13 G)(More)
BACKGROUND Antibodies to M-type phospholipase A2 receptor (PLA2R) correlate with clinical activity of primary membranous nephropathy (PMN). Risk alleles in PLA2R1 and HLA-DQA1 genes are associated with PMN. Whether these alleles are associated with the development of anti-PLA2R is unknown. In this prospective study we evaluated anti-PLA2R, enhanced(More)
PSR J1119−6127 is a high magnetic field (B=4.1×10 13 Gauss), young (≤1,700 year old), and slow (P=408 ms) radio pulsar associated with the supernova remnant (SNR) G292.2−0.5. In 2003, Chandra allowed the detection of the X-ray counterpart of the radio pulsar, and provided the first evidence for a compact and faint pulsar wind nebula (PWN). We here present(More)
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