The balloon-borne large aperture submillimeter telescope (BLAST)

Mark Devlin; Peter Ade; Itziar Aretxaga; James Bock; Jaspaul Chung; Edward Chapin; Simon Dicker; Matt Griffin; Joshua Gundersen; Mark Halpern; Peter Hargrave; David Hughes; Jeffrey Klein; Gaelen Marsden; Peter Martin; Phillip Mauskopf; Barth Netterfield; Luca Olmi; Enzo Pascale; Marie Rex; Douglas Scott; Christopher Semisch; Matthew Truch; Carole Tucker; Gregory Tucker; Anthony Turner; Donald Weibe

doi:10.1117/12.555258

The balloon-borne large aperture submillimeter telescope (BLAST)

Mark Devlin, Peter Ade, Itziar Aretxaga, James Bock, Jaspaul Chung, Edward Chapin, Simon Dicker, Matt Griffin, Joshua Gundersen, Mark Halpern, Peter Hargrave, David Hughes, Jeffrey Klein, Gaelen Marsden, Peter Martin, Phillip Mauskopf, Barth Netterfield, Luca Olmi, Enzo Pascale, Marie RexDouglas Scott, Christopher Semisch, Matthew Truch, Carole Tucker, Gregory Tucker, Anthony Turner, Donald Weibe

Physics

Research output: Contribution to journal › Conference article › peer-review

12 Scopus citations

Abstract

Advances in bolometric detector technology over the past decade have allowed submillimeter wavelength measurements to contribute important data to some of the most challenging questions in observational cosmology. The availability of large format bolometer arrays will provide observations with unprecedented image fidelity. The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) will be one of the first experiments to make full use of this new capability. The high altitude (≈ 35 km) of the balloon platform allows for high-sensitivity measurements in the 250, 350 and 500 μm bands with a total of 260 detectors.

Original language	English (US)
Article number	05
Pages (from-to)	42-54
Number of pages	13
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	5498
DOIs	https://doi.org/10.1117/12.555258
State	Published - 2004
Event	Millimeter and Submillimeter Detectors for Astronomy II - Glasgow, United Kingdom Duration: Jun 23 2004 → Jun 25 2004

Keywords

Bolometer array
Detectors
Galaxy evolution
High-redshift
Submillimeter

ASJC Scopus subject areas

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

Access to Document

10.1117/12.555258

Fingerprint Dive into the research topics of 'The balloon-borne large aperture submillimeter telescope (BLAST)'. Together they form a unique fingerprint.

Cite this

Devlin, M., Ade, P., Aretxaga, I., Bock, J., Chung, J., Chapin, E., Dicker, S., Griffin, M., Gundersen, J., Halpern, M., Hargrave, P., Hughes, D., Klein, J., Marsden, G., Martin, P., Mauskopf, P., Netterfield, B., Olmi, L., Pascale, E., ... Weibe, D. (2004). The balloon-borne large aperture submillimeter telescope (BLAST). Proceedings of SPIE - The International Society for Optical Engineering, 5498, 42-54. [05]. https://doi.org/10.1117/12.555258

The balloon-borne large aperture submillimeter telescope (BLAST). / Devlin, Mark; Ade, Peter; Aretxaga, Itziar; Bock, James; Chung, Jaspaul; Chapin, Edward; Dicker, Simon; Griffin, Matt; Gundersen, Joshua; Halpern, Mark; Hargrave, Peter; Hughes, David; Klein, Jeffrey; Marsden, Gaelen; Martin, Peter; Mauskopf, Phillip; Netterfield, Barth; Olmi, Luca; Pascale, Enzo; Rex, Marie; Scott, Douglas; Semisch, Christopher; Truch, Matthew; Tucker, Carole; Tucker, Gregory; Turner, Anthony; Weibe, Donald.

In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 5498, 05, 2004, p. 42-54.

Research output: Contribution to journal › Conference article › peer-review

Devlin, M, Ade, P, Aretxaga, I, Bock, J, Chung, J, Chapin, E, Dicker, S, Griffin, M, Gundersen, J, Halpern, M, Hargrave, P, Hughes, D, Klein, J, Marsden, G, Martin, P, Mauskopf, P, Netterfield, B, Olmi, L, Pascale, E, Rex, M, Scott, D, Semisch, C, Truch, M, Tucker, C, Tucker, G, Turner, A & Weibe, D 2004, 'The balloon-borne large aperture submillimeter telescope (BLAST)', Proceedings of SPIE - The International Society for Optical Engineering, vol. 5498, 05, pp. 42-54. https://doi.org/10.1117/12.555258

Devlin, Mark ; Ade, Peter ; Aretxaga, Itziar ; Bock, James ; Chung, Jaspaul ; Chapin, Edward ; Dicker, Simon ; Griffin, Matt ; Gundersen, Joshua ; Halpern, Mark ; Hargrave, Peter ; Hughes, David ; Klein, Jeffrey ; Marsden, Gaelen ; Martin, Peter ; Mauskopf, Phillip ; Netterfield, Barth ; Olmi, Luca ; Pascale, Enzo ; Rex, Marie ; Scott, Douglas ; Semisch, Christopher ; Truch, Matthew ; Tucker, Carole ; Tucker, Gregory ; Turner, Anthony ; Weibe, Donald. / The balloon-borne large aperture submillimeter telescope (BLAST). In: Proceedings of SPIE - The International Society for Optical Engineering. 2004 ; Vol. 5498. pp. 42-54.

@article{2ee583de69024e9a9baeb6b7fcbb355e,

title = "The balloon-borne large aperture submillimeter telescope (BLAST)",

abstract = "Advances in bolometric detector technology over the past decade have allowed submillimeter wavelength measurements to contribute important data to some of the most challenging questions in observational cosmology. The availability of large format bolometer arrays will provide observations with unprecedented image fidelity. The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) will be one of the first experiments to make full use of this new capability. The high altitude (≈ 35 km) of the balloon platform allows for high-sensitivity measurements in the 250, 350 and 500 μm bands with a total of 260 detectors.",

keywords = "Bolometer array, Detectors, Galaxy evolution, High-redshift, Submillimeter",

author = "Mark Devlin and Peter Ade and Itziar Aretxaga and James Bock and Jaspaul Chung and Edward Chapin and Simon Dicker and Matt Griffin and Joshua Gundersen and Mark Halpern and Peter Hargrave and David Hughes and Jeffrey Klein and Gaelen Marsden and Peter Martin and Phillip Mauskopf and Barth Netterfield and Luca Olmi and Enzo Pascale and Marie Rex and Douglas Scott and Christopher Semisch and Matthew Truch and Carole Tucker and Gregory Tucker and Anthony Turner and Donald Weibe",

year = "2004",

doi = "10.1117/12.555258",

language = "English (US)",

volume = "5498",

pages = "42--54",

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

issn = "0277-786X",

publisher = "SPIE",

}

TY - JOUR

T1 - The balloon-borne large aperture submillimeter telescope (BLAST)

AU - Devlin, Mark

AU - Ade, Peter

AU - Aretxaga, Itziar

AU - Bock, James

AU - Chung, Jaspaul

AU - Chapin, Edward

AU - Dicker, Simon

AU - Griffin, Matt

AU - Gundersen, Joshua

AU - Halpern, Mark

AU - Hargrave, Peter

AU - Hughes, David

AU - Klein, Jeffrey

AU - Marsden, Gaelen

AU - Martin, Peter

AU - Mauskopf, Phillip

AU - Netterfield, Barth

AU - Olmi, Luca

AU - Pascale, Enzo

AU - Rex, Marie

AU - Scott, Douglas

AU - Semisch, Christopher

AU - Truch, Matthew

AU - Tucker, Carole

AU - Tucker, Gregory

AU - Turner, Anthony

AU - Weibe, Donald

PY - 2004

Y1 - 2004

N2 - Advances in bolometric detector technology over the past decade have allowed submillimeter wavelength measurements to contribute important data to some of the most challenging questions in observational cosmology. The availability of large format bolometer arrays will provide observations with unprecedented image fidelity. The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) will be one of the first experiments to make full use of this new capability. The high altitude (≈ 35 km) of the balloon platform allows for high-sensitivity measurements in the 250, 350 and 500 μm bands with a total of 260 detectors.

AB - Advances in bolometric detector technology over the past decade have allowed submillimeter wavelength measurements to contribute important data to some of the most challenging questions in observational cosmology. The availability of large format bolometer arrays will provide observations with unprecedented image fidelity. The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) will be one of the first experiments to make full use of this new capability. The high altitude (≈ 35 km) of the balloon platform allows for high-sensitivity measurements in the 250, 350 and 500 μm bands with a total of 260 detectors.

KW - Bolometer array

KW - Detectors

KW - Galaxy evolution

KW - High-redshift

KW - Submillimeter

UR - http://www.scopus.com/inward/record.url?scp=19944431410&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=19944431410&partnerID=8YFLogxK

U2 - 10.1117/12.555258

DO - 10.1117/12.555258

M3 - Conference article

AN - SCOPUS:19944431410

VL - 5498

SP - 42

EP - 54

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

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

SN - 0277-786X

M1 - 05

T2 - Millimeter and Submillimeter Detectors for Astronomy II

Y2 - 23 June 2004 through 25 June 2004

ER -