Paper
25 November 1999 Wideband observation of the Crab pulsar using a superconducting transition-edge sensor
Aaron J. Miller, Blas Cabrera, Roger W. Romani, R. M. Clarke, Enectali Figueroa-Feliciano, Sae Woo Nam
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Abstract
Our detectors are superconducting transition edge sensors (TESs) optimized for the wide band detection of individual photons from the mid infrared, through the optical, and into the near ultraviolet. We typically achieve an energy resolution of 0.15 eV FWHM over this range with timing resolution of 100 ns. We have measured photon events with sub- microsecond rise times and 3 microsecond fall times allowing count rates as high as 30 kHz without significant degradation in energy resolution. Such characteristics along with the predicted high quantum efficiency (10% in IR to 50% in optical-UV) make our TES detectors very appealing for low-flux applications which have energy and timing requirements, such as fast spectrophotometry for observational astronomy. We present results from our recent observation of the Crab Pulsar (PSR BO531 + 21) which demonstrate the ability of our sensors to extract wide band phase-resolved spectroscopic information of the pulsar using the student-class 24 inch telescope on the campus of Stanford University. We present a description of the optical system and an analysis of the single pixel energy response.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Aaron J. Miller, Blas Cabrera, Roger W. Romani, R. M. Clarke, Enectali Figueroa-Feliciano, and Sae Woo Nam "Wideband observation of the Crab pulsar using a superconducting transition-edge sensor", Proc. SPIE 3764, Ultraviolet and X-Ray Detection, Spectroscopy, and Polarimetry III, (25 November 1999); https://doi.org/10.1117/12.371082
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Cited by 2 scholarly publications.
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KEYWORDS
Sensors

Photons

Tungsten

Superconductors

Infrared sensors

Spectrophotometry

Quantum efficiency

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