Transition Edge Sensor Arrays for Future FIR Space Missions

Johannes Staguhn; Elmer Sharp; Ari Brown; Archana Devasia; William Doriese; Malcolm Durkin; Dale Fixsen; Suzanne Staggs; Felipe Colazo Petit; Kevin Denis; Mike DiPirro; Shannon Duff; Jason Glenn; Bert Harrop; Stephen Maher; Vilem Mikula; Peter Nagler; Edward Wollack

doi:10.1117/12.3019128

Transition Edge Sensor Arrays for Future FIR Space Missions

Johannes Staguhn, Elmer Sharp, Ari Brown, Archana Devasia, William Doriese, Malcolm Durkin, Dale Fixsen, Suzanne Staggs, Felipe Colazo Petit, Kevin Denis, Mike DiPirro, Shannon Duff, Jason Glenn, Bert Harrop, Stephen Maher, Vilem Mikula, Peter Nagler, Edward Wollack

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

Abstract

We have obtained NASA funding to build and demonstrate Transition Edge Sensor (TES) based kilopixel arrays with the properties that match the requirements for cryogenic far-infrared space missions: the arrays are very closely tileable in one direction and have only a moderate gap in the other direction. This array architecture can meet the sampling- and pixel number requirement of ~ 10⁴ pixels. Many details of the architecture have already been demonstrated individually, and the detector board will be optimized for the use of the latest cryogenic bump bonded NIST 2-D time domain SQUID readout multiplexers with a high density fanout scheme. Additionally, we use flex-lines that are very similar to those developed at Princeton University for the ACT project. We already have a pixel design that exceeds the continuum sensitivity requirements for a cryogenic space mission.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII
Editors	Jonas Zmuidzinas, Jian-Rong Gao, Jian-Rong Gao
Publisher	SPIE
ISBN (Electronic)	9781510675278
DOIs	https://doi.org/10.1117/12.3019128
State	Published - 2024
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII 2024 - Yokohama, Japan Duration: Jun 18 2024 → Jun 22 2024

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	13102
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII 2024
Country/Territory	Japan
City	Yokohama
Period	6/18/24 → 6/22/24

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Keywords

Detector array architectures
Far-infrared
Superconducting detectors
Transition Edge Sensors

Access to Document

10.1117/12.3019128

Cite this

Staguhn, J., Sharp, E., Brown, A., Devasia, A., Doriese, W., Durkin, M., Fixsen, D., Staggs, S., Petit, F. C., Denis, K., DiPirro, M., Duff, S., Glenn, J., Harrop, B., Maher, S., Mikula, V., Nagler, P., & Wollack, E. (2024). Transition Edge Sensor Arrays for Future FIR Space Missions. In J. Zmuidzinas, J.-R. Gao, & J.-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII Article 131020B (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 13102). SPIE. https://doi.org/10.1117/12.3019128

@inproceedings{21c58f1fccd646969ea7e9eb547a239c,

title = "Transition Edge Sensor Arrays for Future FIR Space Missions",

abstract = "We have obtained NASA funding to build and demonstrate Transition Edge Sensor (TES) based kilopixel arrays with the properties that match the requirements for cryogenic far-infrared space missions: the arrays are very closely tileable in one direction and have only a moderate gap in the other direction. This array architecture can meet the sampling- and pixel number requirement of ~ 104 pixels. Many details of the architecture have already been demonstrated individually, and the detector board will be optimized for the use of the latest cryogenic bump bonded NIST 2-D time domain SQUID readout multiplexers with a high density fanout scheme. Additionally, we use flex-lines that are very similar to those developed at Princeton University for the ACT project. We already have a pixel design that exceeds the continuum sensitivity requirements for a cryogenic space mission.",

keywords = "Detector array architectures, Far-infrared, Superconducting detectors, Transition Edge Sensors",

author = "Johannes Staguhn and Elmer Sharp and Ari Brown and Archana Devasia and William Doriese and Malcolm Durkin and Dale Fixsen and Suzanne Staggs and Petit, {Felipe Colazo} and Kevin Denis and Mike DiPirro and Shannon Duff and Jason Glenn and Bert Harrop and Stephen Maher and Vilem Mikula and Peter Nagler and Edward Wollack",

note = "Publisher Copyright: {\textcopyright} 2024 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII 2024 ; Conference date: 18-06-2024 Through 22-06-2024",

year = "2024",

doi = "10.1117/12.3019128",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Jian-Rong Gao and Jian-Rong Gao",

booktitle = "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII",

address = "United States",

}

Staguhn, J, Sharp, E, Brown, A, Devasia, A, Doriese, W, Durkin, M, Fixsen, D, Staggs, S, Petit, FC, Denis, K, DiPirro, M, Duff, S, Glenn, J, Harrop, B, Maher, S, Mikula, V, Nagler, P & Wollack, E 2024, Transition Edge Sensor Arrays for Future FIR Space Missions. in J Zmuidzinas, J-R Gao & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII., 131020B, Proceedings of SPIE - The International Society for Optical Engineering, vol. 13102, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII 2024, Yokohama, Japan, 6/18/24. https://doi.org/10.1117/12.3019128

Transition Edge Sensor Arrays for Future FIR Space Missions. / Staguhn, Johannes; Sharp, Elmer; Brown, Ari et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII. ed. / Jonas Zmuidzinas; Jian-Rong Gao; Jian-Rong Gao. SPIE, 2024. 131020B (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 13102).

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

TY - GEN

T1 - Transition Edge Sensor Arrays for Future FIR Space Missions

AU - Staguhn, Johannes

AU - Sharp, Elmer

AU - Brown, Ari

AU - Devasia, Archana

AU - Doriese, William

AU - Durkin, Malcolm

AU - Fixsen, Dale

AU - Staggs, Suzanne

AU - Petit, Felipe Colazo

AU - Denis, Kevin

AU - DiPirro, Mike

AU - Duff, Shannon

AU - Glenn, Jason

AU - Harrop, Bert

AU - Maher, Stephen

AU - Mikula, Vilem

AU - Nagler, Peter

AU - Wollack, Edward

PY - 2024

Y1 - 2024

N2 - We have obtained NASA funding to build and demonstrate Transition Edge Sensor (TES) based kilopixel arrays with the properties that match the requirements for cryogenic far-infrared space missions: the arrays are very closely tileable in one direction and have only a moderate gap in the other direction. This array architecture can meet the sampling- and pixel number requirement of ~ 104 pixels. Many details of the architecture have already been demonstrated individually, and the detector board will be optimized for the use of the latest cryogenic bump bonded NIST 2-D time domain SQUID readout multiplexers with a high density fanout scheme. Additionally, we use flex-lines that are very similar to those developed at Princeton University for the ACT project. We already have a pixel design that exceeds the continuum sensitivity requirements for a cryogenic space mission.

AB - We have obtained NASA funding to build and demonstrate Transition Edge Sensor (TES) based kilopixel arrays with the properties that match the requirements for cryogenic far-infrared space missions: the arrays are very closely tileable in one direction and have only a moderate gap in the other direction. This array architecture can meet the sampling- and pixel number requirement of ~ 104 pixels. Many details of the architecture have already been demonstrated individually, and the detector board will be optimized for the use of the latest cryogenic bump bonded NIST 2-D time domain SQUID readout multiplexers with a high density fanout scheme. Additionally, we use flex-lines that are very similar to those developed at Princeton University for the ACT project. We already have a pixel design that exceeds the continuum sensitivity requirements for a cryogenic space mission.

KW - Detector array architectures

KW - Far-infrared

KW - Superconducting detectors

KW - Transition Edge Sensors

UR - http://www.scopus.com/inward/record.url?scp=85204693147&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85204693147&partnerID=8YFLogxK

U2 - 10.1117/12.3019128

DO - 10.1117/12.3019128

M3 - Conference contribution

AN - SCOPUS:85204693147

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII

A2 - Zmuidzinas, Jonas

A2 - Gao, Jian-Rong

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII 2024

Y2 - 18 June 2024 through 22 June 2024

ER -

Staguhn J, Sharp E, Brown A, Devasia A, Doriese W, Durkin M et al. Transition Edge Sensor Arrays for Future FIR Space Missions. In Zmuidzinas J, Gao JR, Gao JR, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII. SPIE. 2024. 131020B. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.3019128

Transition Edge Sensor Arrays for Future FIR Space Missions

Abstract

Publication series

Conference

All Science Journal Classification (ASJC) codes

Keywords

Access to Document

Other files and links

Fingerprint

Cite this