Large arrays of TES X-ray microcalorimeters for dark baryon search

Yuichiro Ezoe; Hiroshi Yoshitake; Kumi Ishikawa; Yoshitaka Ishisaki; Hiroki Akamatsu; Takaya Ohashi; Noriko Y. Yamasaki; Kazuhisa Mitsuda; Takayuki Takano; Ryutaro Maeda

doi:10.1063/1.3292416

Large arrays of TES X-ray microcalorimeters for dark baryon search

Yuichiro Ezoe
, Hiroshi Yoshitake
, Kumi Ishikawa
, Yoshitaka Ishisaki
, Hiroki Akamatsu
, Takaya Ohashi
, Noriko Y. Yamasaki
, Kazuhisa Mitsuda
, Takayuki Takano
, Ryutaro Maeda

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

9 Scopus citations

Abstract

Arrays of transition edge sensor (TES) X-ray microcalorimeters can provide a high energy resolution and a large area necessary for future dark baryon search missions such as DIOS (Diffuse Intergalactic Oxygen Surveyor). In the current design, the energy resolution of 2 eV at 0.3-1.5 keV and the geometrical area of 1 cm² are required for DIOS. As an R&D study, we fabricated a 16×x16 Ti/Au bilayer TES array without an absorber, and achieved the energy resolution of 4.4±0.2 eV at 5.9 keV. Considering the recent experimental results on so-called excess noise, we investigated a detailed design of the TES array for DIOS. We concluded that we need a at least 20×20 pixel array consisting of 250 μm-square TESs and 500 |.im-square mushroom-type Bi/Au absorbers. We discussed technical issues to manufacture such a large format array.

Original language	English
Title of host publication	Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop
Pages	60-63
Number of pages	4
DOIs	https://doi.org/10.1063/1.3292416
State	Published - 2009
Externally published	Yes
Event	13th International Workshop on Low Temperature Detectors, LTD-13 - Stanford, CA, United States Duration: 20 Jul 2009 → 24 Jul 2009

Publication series

Name	AIP Conference Proceedings
Volume	1185
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	13th International Workshop on Low Temperature Detectors, LTD-13
Country/Territory	United States
City	Stanford, CA
Period	20/07/09 → 24/07/09

Keywords

Array
TES
X-ray microcalorimeter

Access to Document

10.1063/1.3292416

Cite this

Ezoe, Y., Yoshitake, H., Ishikawa, K., Ishisaki, Y., Akamatsu, H., Ohashi, T., Yamasaki, N. Y., Mitsuda, K., Takano, T., & Maeda, R. (2009). Large arrays of TES X-ray microcalorimeters for dark baryon search. In Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop (pp. 60-63). (AIP Conference Proceedings; Vol. 1185). https://doi.org/10.1063/1.3292416

@inproceedings{8c76b25afe0042c68b8f8b70dc5d6716,

title = "Large arrays of TES X-ray microcalorimeters for dark baryon search",

abstract = "Arrays of transition edge sensor (TES) X-ray microcalorimeters can provide a high energy resolution and a large area necessary for future dark baryon search missions such as DIOS (Diffuse Intergalactic Oxygen Surveyor). In the current design, the energy resolution of 2 eV at 0.3-1.5 keV and the geometrical area of 1 cm2 are required for DIOS. As an R\&D study, we fabricated a 16×x16 Ti/Au bilayer TES array without an absorber, and achieved the energy resolution of 4.4±0.2 eV at 5.9 keV. Considering the recent experimental results on so-called excess noise, we investigated a detailed design of the TES array for DIOS. We concluded that we need a at least 20×20 pixel array consisting of 250 μm-square TESs and 500 |.im-square mushroom-type Bi/Au absorbers. We discussed technical issues to manufacture such a large format array.",

keywords = "Array, TES, X-ray microcalorimeter",

author = "Yuichiro Ezoe and Hiroshi Yoshitake and Kumi Ishikawa and Yoshitaka Ishisaki and Hiroki Akamatsu and Takaya Ohashi and Yamasaki, \{Noriko Y.\} and Kazuhisa Mitsuda and Takayuki Takano and Ryutaro Maeda",

year = "2009",

doi = "10.1063/1.3292416",

language = "英语",

isbn = "9780735407510",

series = "AIP Conference Proceedings",

pages = "60--63",

booktitle = "Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop",

note = "13th International Workshop on Low Temperature Detectors, LTD-13 ; Conference date: 20-07-2009 Through 24-07-2009",

}

Ezoe, Y, Yoshitake, H, Ishikawa, K, Ishisaki, Y, Akamatsu, H, Ohashi, T, Yamasaki, NY, Mitsuda, K, Takano, T & Maeda, R 2009, Large arrays of TES X-ray microcalorimeters for dark baryon search. in Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop. AIP Conference Proceedings, vol. 1185, pp. 60-63, 13th International Workshop on Low Temperature Detectors, LTD-13, Stanford, CA, United States, 20/07/09. https://doi.org/10.1063/1.3292416

Large arrays of TES X-ray microcalorimeters for dark baryon search. / Ezoe, Yuichiro; Yoshitake, Hiroshi; Ishikawa, Kumi et al.
Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop. 2009. p. 60-63 (AIP Conference Proceedings; Vol. 1185).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Large arrays of TES X-ray microcalorimeters for dark baryon search

AU - Ezoe, Yuichiro

AU - Yoshitake, Hiroshi

AU - Ishikawa, Kumi

AU - Ishisaki, Yoshitaka

AU - Akamatsu, Hiroki

AU - Ohashi, Takaya

AU - Yamasaki, Noriko Y.

AU - Mitsuda, Kazuhisa

AU - Takano, Takayuki

AU - Maeda, Ryutaro

PY - 2009

Y1 - 2009

N2 - Arrays of transition edge sensor (TES) X-ray microcalorimeters can provide a high energy resolution and a large area necessary for future dark baryon search missions such as DIOS (Diffuse Intergalactic Oxygen Surveyor). In the current design, the energy resolution of 2 eV at 0.3-1.5 keV and the geometrical area of 1 cm2 are required for DIOS. As an R&D study, we fabricated a 16×x16 Ti/Au bilayer TES array without an absorber, and achieved the energy resolution of 4.4±0.2 eV at 5.9 keV. Considering the recent experimental results on so-called excess noise, we investigated a detailed design of the TES array for DIOS. We concluded that we need a at least 20×20 pixel array consisting of 250 μm-square TESs and 500 |.im-square mushroom-type Bi/Au absorbers. We discussed technical issues to manufacture such a large format array.

AB - Arrays of transition edge sensor (TES) X-ray microcalorimeters can provide a high energy resolution and a large area necessary for future dark baryon search missions such as DIOS (Diffuse Intergalactic Oxygen Surveyor). In the current design, the energy resolution of 2 eV at 0.3-1.5 keV and the geometrical area of 1 cm2 are required for DIOS. As an R&D study, we fabricated a 16×x16 Ti/Au bilayer TES array without an absorber, and achieved the energy resolution of 4.4±0.2 eV at 5.9 keV. Considering the recent experimental results on so-called excess noise, we investigated a detailed design of the TES array for DIOS. We concluded that we need a at least 20×20 pixel array consisting of 250 μm-square TESs and 500 |.im-square mushroom-type Bi/Au absorbers. We discussed technical issues to manufacture such a large format array.

KW - Array

KW - TES

KW - X-ray microcalorimeter

UR - https://www.scopus.com/pages/publications/74349086578

U2 - 10.1063/1.3292416

DO - 10.1063/1.3292416

M3 - 会议稿件

AN - SCOPUS:74349086578

SN - 9780735407510

T3 - AIP Conference Proceedings

SP - 60

EP - 63

BT - Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop

T2 - 13th International Workshop on Low Temperature Detectors, LTD-13

Y2 - 20 July 2009 through 24 July 2009

ER -

Large arrays of TES X-ray microcalorimeters for dark baryon search

Abstract

Publication series

Conference

Keywords

Access to Document

Other files and links

Fingerprint

Cite this