Zobrazeno 1 - 5
of 5
pro vyhledávání: '"C. K. Stahle"'
Autor:
S. Deiker, Wilton T. Sanders, Wei Cui, E. Apodaca, R. Almy, Jian-Fu Zhang, Massimiliano Galeazzi, Frederick S. Porter, Enectali Figueroa-Feliciano, Jeffrey P. Morgenthaler, Andrew E. Szymkowiak, Michael Juda, Tatehiro Mihara, W. Bergmann Tiest, Richard Mushotzky, C. K. Stahle, A. Lesser, Dan McCammon, S. H. Moseley, Richard L. Kelley
Publikováno v:
The Astrophysical Journal. 576:188-203
A high spectral resolution observation of the diffuse X-ray background in the 60 - 1000 eV energy range has been made using an array of thirty-six 1 mm^2 micro-calorimeters flown on a sounding rocket. Detector energy resolution ranged from 5-12 eV FW
Publikováno v:
AIP Conference Proceedings.
In order to optimize the design of microcalorimeters and bolometers, it is necessary to be able to predict the resolution of any given configuration. For detectors using ion-implanted silicon thermistors, we have sufficient engineering data on their
Publikováno v:
AIP Conference Proceedings.
One major problem with TES micro-calorimeters is the very narrow temperature range in which they work. To detect high energy events the heat capacity of the detector must be sufficiently large to keep the sensor running in its sensitive region. The l
Autor:
C. K. Stahle, Enectali Figueroa-Feliciano, F. M. Finkbeiner, Jay Chervenak, Regis P. Brekosky, Nilesh Tralshawala, Mary J. Li, M. A. Lindeman
Publikováno v:
AIP Conference Proceedings.
We are developing superconducting transition-edge sensor (TES) microcalorimeters for astronomical x-ray spectroscopy. We have obtained very high energy resolution (2.4 eV at 1.5 keV and 3.7 eV at 3.3 keV) in large, isolated TES pixels using Mo/Au pro
Autor:
Regis P. Brekosky, F. M. Finkbeiner, Mary J. Li, C. K. Stahle, C. M. Stahle, Jay Chervenak, Nilesh Tralshawala, M. A. Lindeman, Enectali Figueroa-Feliciano
Publikováno v:
AIP Conference Proceedings.
We present an overview of our efforts in fabricating Transition-Edge Sensor (TES) microcalorimeter arrays for use in astronomical x-ray spectroscopy. Two distinct types of array schemes are currently pursued: 5×5 single pixel TES array where each pi