Phase-resolved Crab studies with a cryogenic transition-edge sensor spectrophotometer

被引:60
|
作者
Romani, RW [1 ]
Miller, AJ
Cabrera, B
Nam, SW
Martinis, JM
机构
[1] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[2] Natl Inst Stand & Technol, Boulder, CO 80305 USA
[3] CSIRO, Australia Telescope Natl Facil, Epping, NSW 2121, Australia
来源
ASTROPHYSICAL JOURNAL | 2001年 / 563卷 / 01期
关键词
instrumentation : detectors; pulsars : individual (PSR B0531+21);
D O I
10.1086/323874
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We are developing time- and energy-resolved near-IR/optical/UV photon detectors based on sharp superconducting-normal transition edges in thin films. We report observations of the Crab pulsar made during prototype testing at the McDonald 2.7 m with a fiber-coupled transition-edge sensor (TES) system. These data show substantial (delta alpha similar to 0.3), rapid variations in the spectral index through the pulse profile, with a strong phase-varying IR break across our energy band. These variations correlate with X-ray spectral variations, but no single synchrotron population can account for the full spectral energy distribution. We also describe test spectrophotopolarimetry observations probing the energy dependence of the polarization sweep; this may provide a new key to understanding the radiating particle population.
引用
收藏
页码:221 / 228
页数:8
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