Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver

Ian Lowe; Peter A.R. Ade; Peter C. Ashton; Jason E. Austermann; Gabriele Coppi; Erin G. Cox; Mark J. Devlin; Bradley J. Dober; Valentina Fanfani; Laura M. Fissel; Nicholas Galitzki; Jiansong Gao; Samuel Gordon; Christopher E. Groppi; Gene C. Hilton; Johannes Hubmayr; Jeffrey Klein; Dale Li; Nathan P. Lourie; Hamdi Mani; Philip Mauskopf; Christopher McKenney; Federico Nati; Giles Novak; Giampaolo Pisano; Javier Romualdez; Juan D. Soler; Adrian Sinclair; Carole Tucker; Joel Ullom; Michael Vissers; Caleb Wheeler; Paul A. Williams

doi:10.1117/12.2560854

Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver

Ian Lowe, Peter A.R. Ade, Peter C. Ashton, Jason E. Austermann, Gabriele Coppi, Erin G. Cox, Mark J. Devlin, Bradley J. Dober, Valentina Fanfani, Laura M. Fissel, Nicholas Galitzki, Jiansong Gao, Samuel Gordon, Christopher E. Groppi, Gene C. Hilton, Johannes Hubmayr, Jeffrey Klein, Dale Li, Nathan P. Lourie, Hamdi ManiPhilip Mauskopf, Christopher McKenney, Federico Nati, Giles Novak, Giampaolo Pisano, Javier Romualdez, Juan D. Soler, Adrian Sinclair, Carole Tucker, Joel Ullom, Michael Vissers, Caleb Wheeler, Paul A. Williams

Earth and Space Exploration, School of (SESE)

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

7 Scopus citations

Abstract

The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter polarimeter designed to map interstellar dust and galactic foregrounds at 250, 350, and 500 microns during a 24-day Antarctic flight. The BLAST-TNG detector arrays are comprised of 918, 469, and 272 MKID pixels, respectively. The pixels are formed from two orthogonally oriented, crossed, linear-polarization sensitive MKID antennae. The arrays are cooled to sub 300 mK temperatures and stabilized via a closed cycle 3He sorption fridge in combination with a 4He vacuum pot. The detectors are read out through a combination of the second-generation Reconfigurable Open Architecture Computing Hardware (ROACH2) and custom RF electronics designed for BLAST-TNG. The firmware and software designed to readout and characterize these detectors was built from scratch by the BLAST team around these detectors, and has been adapted for use by other MKID instruments such as TolTEC and OLIMPO.1 We present an overview of these systems as well as in-depth methodology of the ground-based characterization and the measured in-flight performance.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
Editors	Jonas Zmuidzinas, Jian-Rong Gao
Publisher	SPIE
ISBN (Electronic)	9781510636934
DOIs	https://doi.org/10.1117/12.2560854
State	Published - 2020
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020 - Virtual, Online, United States Duration: Dec 14 2020 → Dec 22 2020

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11453
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020
Country/Territory	United States
City	Virtual, Online
Period	12/14/20 → 12/22/20

ASJC Scopus subject areas

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

Access to Document

10.1117/12.2560854

Cite this

Lowe, I., Ade, P. A. R., Ashton, P. C., Austermann, J. E., Coppi, G., Cox, E. G., Devlin, M. J., Dober, B. J., Fanfani, V., Fissel, L. M., Galitzki, N., Gao, J., Gordon, S., Groppi, C. E., Hilton, G. C., Hubmayr, J., Klein, J., Li, D., Lourie, N. P., ... Williams, P. A. (2020). Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver. In J. Zmuidzinas, & J.-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X Article 1145304 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11453). SPIE. https://doi.org/10.1117/12.2560854

Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver. / Lowe, Ian; Ade, Peter A.R.; Ashton, Peter C. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. ed. / Jonas Zmuidzinas; Jian-Rong Gao. SPIE, 2020. 1145304 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11453).

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

Lowe, I, Ade, PAR, Ashton, PC, Austermann, JE, Coppi, G, Cox, EG, Devlin, MJ, Dober, BJ, Fanfani, V, Fissel, LM, Galitzki, N, Gao, J, Gordon, S, Groppi, CE, Hilton, GC, Hubmayr, J, Klein, J, Li, D, Lourie, NP, Mani, H, Mauskopf, P, McKenney, C, Nati, F, Novak, G, Pisano, G, Romualdez, J, Soler, JD, Sinclair, A, Tucker, C, Ullom, J, Vissers, M, Wheeler, C & Williams, PA 2020, Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver. in J Zmuidzinas & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X., 1145304, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11453, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020, Virtual, Online, United States, 12/14/20. https://doi.org/10.1117/12.2560854

Lowe I, Ade PAR, Ashton PC, Austermann JE, Coppi G, Cox EG et al. Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver. In Zmuidzinas J, Gao JR, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. SPIE. 2020. 1145304. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2560854

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title = "Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver",

abstract = "The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter polarimeter designed to map interstellar dust and galactic foregrounds at 250, 350, and 500 microns during a 24-day Antarctic flight. The BLAST-TNG detector arrays are comprised of 918, 469, and 272 MKID pixels, respectively. The pixels are formed from two orthogonally oriented, crossed, linear-polarization sensitive MKID antennae. The arrays are cooled to sub 300 mK temperatures and stabilized via a closed cycle 3He sorption fridge in combination with a 4He vacuum pot. The detectors are read out through a combination of the second-generation Reconfigurable Open Architecture Computing Hardware (ROACH2) and custom RF electronics designed for BLAST-TNG. The firmware and software designed to readout and characterize these detectors was built from scratch by the BLAST team around these detectors, and has been adapted for use by other MKID instruments such as TolTEC and OLIMPO.1 We present an overview of these systems as well as in-depth methodology of the ground-based characterization and the measured in-flight performance.",

author = "Ian Lowe and Ade, {Peter A.R.} and Ashton, {Peter C.} and Austermann, {Jason E.} and Gabriele Coppi and Cox, {Erin G.} and Devlin, {Mark J.} and Dober, {Bradley J.} and Valentina Fanfani and Fissel, {Laura M.} and Nicholas Galitzki and Jiansong Gao and Samuel Gordon and Groppi, {Christopher E.} and Hilton, {Gene C.} and Johannes Hubmayr and Jeffrey Klein and Dale Li and Lourie, {Nathan P.} and Hamdi Mani and Philip Mauskopf and Christopher McKenney and Federico Nati and Giles Novak and Giampaolo Pisano and Javier Romualdez and Soler, {Juan D.} and Adrian Sinclair and Carole Tucker and Joel Ullom and Michael Vissers and Caleb Wheeler and Williams, {Paul A.}",

note = "Publisher Copyright: {\textcopyright} COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020 ; Conference date: 14-12-2020 Through 22-12-2020",

year = "2020",

doi = "10.1117/12.2560854",

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

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AU - Austermann, Jason E.

AU - Coppi, Gabriele

AU - Cox, Erin G.

AU - Devlin, Mark J.

AU - Dober, Bradley J.

AU - Fanfani, Valentina

AU - Fissel, Laura M.

AU - Galitzki, Nicholas

AU - Gao, Jiansong

AU - Gordon, Samuel

AU - Groppi, Christopher E.

AU - Hilton, Gene C.

AU - Hubmayr, Johannes

AU - Klein, Jeffrey

AU - Li, Dale

AU - Lourie, Nathan P.

AU - Mani, Hamdi

AU - Mauskopf, Philip

AU - McKenney, Christopher

AU - Nati, Federico

AU - Novak, Giles

AU - Pisano, Giampaolo

AU - Romualdez, Javier

AU - Soler, Juan D.

AU - Sinclair, Adrian

AU - Tucker, Carole

AU - Ullom, Joel

AU - Vissers, Michael

AU - Wheeler, Caleb

AU - Williams, Paul A.

PY - 2020

Y1 - 2020

N2 - The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter polarimeter designed to map interstellar dust and galactic foregrounds at 250, 350, and 500 microns during a 24-day Antarctic flight. The BLAST-TNG detector arrays are comprised of 918, 469, and 272 MKID pixels, respectively. The pixels are formed from two orthogonally oriented, crossed, linear-polarization sensitive MKID antennae. The arrays are cooled to sub 300 mK temperatures and stabilized via a closed cycle 3He sorption fridge in combination with a 4He vacuum pot. The detectors are read out through a combination of the second-generation Reconfigurable Open Architecture Computing Hardware (ROACH2) and custom RF electronics designed for BLAST-TNG. The firmware and software designed to readout and characterize these detectors was built from scratch by the BLAST team around these detectors, and has been adapted for use by other MKID instruments such as TolTEC and OLIMPO.1 We present an overview of these systems as well as in-depth methodology of the ground-based characterization and the measured in-flight performance.

AB - The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter polarimeter designed to map interstellar dust and galactic foregrounds at 250, 350, and 500 microns during a 24-day Antarctic flight. The BLAST-TNG detector arrays are comprised of 918, 469, and 272 MKID pixels, respectively. The pixels are formed from two orthogonally oriented, crossed, linear-polarization sensitive MKID antennae. The arrays are cooled to sub 300 mK temperatures and stabilized via a closed cycle 3He sorption fridge in combination with a 4He vacuum pot. The detectors are read out through a combination of the second-generation Reconfigurable Open Architecture Computing Hardware (ROACH2) and custom RF electronics designed for BLAST-TNG. The firmware and software designed to readout and characterize these detectors was built from scratch by the BLAST team around these detectors, and has been adapted for use by other MKID instruments such as TolTEC and OLIMPO.1 We present an overview of these systems as well as in-depth methodology of the ground-based characterization and the measured in-flight performance.

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

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

A2 - Zmuidzinas, Jonas

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PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020

Y2 - 14 December 2020 through 22 December 2020

ER -

Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver

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