TY - JOUR
T1 - Present performance of a single pixel Ti/Au bilayer TES calorimeter
AU - Ishisaki, Yoshitaka
AU - Morita, Umeyo
AU - Koga, Takeo
AU - Sato, Kosuke
AU - Ohashi, Takaya
AU - Mitsuda, Kazuhisa
AU - Yamasaki, Noriko Y.
AU - Fujimoto, Ryuichi
AU - Iyomoto, Naoko
AU - Oshima, Tai
AU - Futamoto, Kazuo
AU - Takei, Yoh
AU - Ichitsubo, Taro
AU - Fujimori, Tamayuki
AU - Shoji, Shuichi
AU - Kudo, Hiroyuki
AU - Nakamura, Tomoaki
AU - Arakawa, Takahiro
AU - Osaka, Tetsuya
AU - Homma, Takayuki
AU - Sato, Hirotaka
AU - Kobayashi, Hideomi
AU - Mori, Kentaro
AU - Tanaka, Keiichi
AU - Morooka, Toshimitsu
AU - Nakayama, Satoshi
AU - Chinone, Kazuo
AU - Kuroda, Yoshikatsu
AU - Onishi, Mitsunobu
AU - Otake, Kunio
PY - 2002
Y1 - 2002
N2 - We are developing a superconducting transition-edge sensor (TES) calorimeter for future Japanese X-ray astronomy missions (e.g. NeXT mission). The performance of our single pixel TES calorimeter is presented. We fabricated a Ti/Au (40 nm/110 nm) bilayer TES on a thin silicon-nitride membrane, which is adjusted to have a transition temperature of about 100 mK. The size of the TES is 500 μm × 500 μm, and 300 μm × 300 μm gold with a thickness of 300 nm is deposited with sputtering as an X-ray absorber. The TES calorimeter was installed in a dilution refrigerator operated at ∼ 40 mK, with a combination of 400-series SQUID array as an ammeter. Collimated 5.9 keV X-rays (200 μm in diameter) from 55Fe isotope were irradiated and X-ray pulses were obtained. Simultaneously with a fast falling time constant of 74.2 μs, the energy resolution of 6.6 ± 0.4 eV was attained, while the baseline noise was 6.4 eV. The contents of the energy resolution are 5.1 eV of the excess noise, 3.3 eV of the readout noise, 1.6 eV of the pulse by pulse variation, and 1.9 eV of the intrinsic noise. The baseline noise are dominated by an unknown excess noise, which increases roughly in proportion to the inverse of the TES resistance. The pulse height is sensitive to the operating conditions, and the superconducting shield appears to have improved it by a factor of ∼ 2. The calorimeter works fine over six months surviving five thermal cycles, even though it is kept in air.
AB - We are developing a superconducting transition-edge sensor (TES) calorimeter for future Japanese X-ray astronomy missions (e.g. NeXT mission). The performance of our single pixel TES calorimeter is presented. We fabricated a Ti/Au (40 nm/110 nm) bilayer TES on a thin silicon-nitride membrane, which is adjusted to have a transition temperature of about 100 mK. The size of the TES is 500 μm × 500 μm, and 300 μm × 300 μm gold with a thickness of 300 nm is deposited with sputtering as an X-ray absorber. The TES calorimeter was installed in a dilution refrigerator operated at ∼ 40 mK, with a combination of 400-series SQUID array as an ammeter. Collimated 5.9 keV X-rays (200 μm in diameter) from 55Fe isotope were irradiated and X-ray pulses were obtained. Simultaneously with a fast falling time constant of 74.2 μs, the energy resolution of 6.6 ± 0.4 eV was attained, while the baseline noise was 6.4 eV. The contents of the energy resolution are 5.1 eV of the excess noise, 3.3 eV of the readout noise, 1.6 eV of the pulse by pulse variation, and 1.9 eV of the intrinsic noise. The baseline noise are dominated by an unknown excess noise, which increases roughly in proportion to the inverse of the TES resistance. The pulse height is sensitive to the operating conditions, and the superconducting shield appears to have improved it by a factor of ∼ 2. The calorimeter works fine over six months surviving five thermal cycles, even though it is kept in air.
KW - Microcalorimeter
KW - TES
KW - Transition edge sensor
KW - X-ray
UR - http://www.scopus.com/inward/record.url?scp=0037957263&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0037957263&partnerID=8YFLogxK
U2 - 10.1117/12.461336
DO - 10.1117/12.461336
M3 - Conference article
AN - SCOPUS:0037957263
SN - 0277-786X
VL - 4851
SP - 831
EP - 841
JO - Proceedings of SPIE - The International Society for Optical Engineering
JF - Proceedings of SPIE - The International Society for Optical Engineering
IS - 2
T2 - X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy
Y2 - 24 August 2002 through 28 August 2002
ER -