The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol

International audience The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) is a sub-orbital experiment designed to study the process of star formation in local galaxies (including the Milky Way) and in galaxies at cosmological distances. Using a 2m Cassegrain telescope, BLAST images the...

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Published in:SPIE Proceedings, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
Main Authors: Marsden, G., Ade, P.A.R., Benton, S., Bock, J. J., Chapin, E. L., Chung, J., Devlin, M. J., Dicker, S., Fissel, L., Griffin, M., Gundersen, J. O., Halpern, M., Hargrave, P. C., Hughes, D. H., Klein, J., Korotkov, A., Mactavish, C. J., Martin, P. G., Martin, T. G., Matthews, T. G., Mauskopf, P., Moncelsi, L., Netterfield, C. B., Novak, G., Pascale, E., Olmi, L., Patanchon, G., Rex, M., Savini, G., Scott, D., Semisch, C., Thomas, N., Truch, M. D. P., Tucker, C., Tucker, G. S., Viero, M. P., Ward-Thompson, D., Wiebe, D. V.
Other Authors: APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), William D. Duncan, Wayne S. Holland, Stafford Withington, Jonas Zmuidzinas
Format: Conference Object
Language:English
Published: HAL CCSD 2008
Subjects:
Online Access:https://hal.in2p3.fr/in2p3-00330537
https://doi.org/10.1117/12.788413
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institution Open Polar
collection Université de Nantes: HAL-UNIV-NANTES
op_collection_id ftunivnantes
language English
topic [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
spellingShingle [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
Marsden, G.
Ade, P.A.R.
Benton, S.
Bock, J. J.
Chapin, E. L.
Chung, J.
Devlin, M. J.
Dicker, S.
Fissel, L.
Griffin, M.
Gundersen, J. O.
Halpern, M.
Hargrave, P. C.
Hughes, D. H.
Klein, J.
Korotkov, A.
Mactavish, C. J.
Martin, P. G.
Martin, T. G.
Matthews, T. G.
Mauskopf, P.
Moncelsi, L.
Netterfield, C. B.
Novak, G.
Pascale, E.
Olmi, L.
Patanchon, G.
Rex, M.
Savini, G.
Scott, D.
Semisch, C.
Thomas, N.
Truch, M. D. P.
Tucker, C.
Tucker, G. S.
Viero, M. P.
Ward-Thompson, D.
Wiebe, D. V.
The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol
topic_facet [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
description International audience The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) is a sub-orbital experiment designed to study the process of star formation in local galaxies (including the Milky Way) and in galaxies at cosmological distances. Using a 2m Cassegrain telescope, BLAST images the sky onto a focal plane, which consists of 270 bolometric detectors split between three arrays, observing simultaneously in 30% wide bands, centered at 250, 350, and 500 ?m. The diffraction-limited optical system provides a resolution of 30" at 250 ?m. The pointing system enables raster-like scans with a positional accuracy of ~30", reconstructed to better than 5" rms in postflight analysis. BLAST had two successful flights, from the Arctic in 2005, and from Antarctica in 2006, which provided the first high-resolution and large-area (~0.8-200 deg2) submillimeter surveys at these wavelengths. As a pathfinder for the SPIRE instrument on Herschel, BLAST shares with the ESA satellite similar focal plane technology and scientific motivation. A third flight in 2009 will see the instrument modified to be polarization-sensitive (BLAST-pol). With its unprecedented mapping speed and resolution, BLAST-pol will provide insights into Galactic star-forming nurseries, and give the necessary link between the larger, coarse resolution surveys and the narrow, resolved observations of star-forming structures from space and ground based instruments being commissioned in the next 5 years.
author2 APC - Cosmologie
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
William D. Duncan
Wayne S. Holland
Stafford Withington
Jonas Zmuidzinas
format Conference Object
author Marsden, G.
Ade, P.A.R.
Benton, S.
Bock, J. J.
Chapin, E. L.
Chung, J.
Devlin, M. J.
Dicker, S.
Fissel, L.
Griffin, M.
Gundersen, J. O.
Halpern, M.
Hargrave, P. C.
Hughes, D. H.
Klein, J.
Korotkov, A.
Mactavish, C. J.
Martin, P. G.
Martin, T. G.
Matthews, T. G.
Mauskopf, P.
Moncelsi, L.
Netterfield, C. B.
Novak, G.
Pascale, E.
Olmi, L.
Patanchon, G.
Rex, M.
Savini, G.
Scott, D.
Semisch, C.
Thomas, N.
Truch, M. D. P.
Tucker, C.
Tucker, G. S.
Viero, M. P.
Ward-Thompson, D.
Wiebe, D. V.
author_facet Marsden, G.
Ade, P.A.R.
Benton, S.
Bock, J. J.
Chapin, E. L.
Chung, J.
Devlin, M. J.
Dicker, S.
Fissel, L.
Griffin, M.
Gundersen, J. O.
Halpern, M.
Hargrave, P. C.
Hughes, D. H.
Klein, J.
Korotkov, A.
Mactavish, C. J.
Martin, P. G.
Martin, T. G.
Matthews, T. G.
Mauskopf, P.
Moncelsi, L.
Netterfield, C. B.
Novak, G.
Pascale, E.
Olmi, L.
Patanchon, G.
Rex, M.
Savini, G.
Scott, D.
Semisch, C.
Thomas, N.
Truch, M. D. P.
Tucker, C.
Tucker, G. S.
Viero, M. P.
Ward-Thompson, D.
Wiebe, D. V.
author_sort Marsden, G.
title The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol
title_short The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol
title_full The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol
title_fullStr The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol
title_full_unstemmed The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol
title_sort balloon-borne large-aperture submillimeter telescope for polarization: blast-pol
publisher HAL CCSD
publishDate 2008
url https://hal.in2p3.fr/in2p3-00330537
https://doi.org/10.1117/12.788413
op_coverage Marseille, France
long_lat ENVELOPE(-68.705,-68.705,-71.251,-71.251)
geographic Arctic
Milky Way
geographic_facet Arctic
Milky Way
genre Antarc*
Antarctica
Arctic
genre_facet Antarc*
Antarctica
Arctic
op_source Proceedings of SPIE: Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
https://hal.in2p3.fr/in2p3-00330537
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, Jun 2008, Marseille, France. ⟨10.1117/12.788413⟩
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in2p3-00330537
https://hal.in2p3.fr/in2p3-00330537
ARXIV: 0805.4420
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doi:10.1117/12.788413
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container_title SPIE Proceedings, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
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spelling ftunivnantes:oai:HAL:in2p3-00330537v1 2023-05-15T13:32:12+02:00 The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol Marsden, G. Ade, P.A.R. Benton, S. Bock, J. J. Chapin, E. L. Chung, J. Devlin, M. J. Dicker, S. Fissel, L. Griffin, M. Gundersen, J. O. Halpern, M. Hargrave, P. C. Hughes, D. H. Klein, J. Korotkov, A. Mactavish, C. J. Martin, P. G. Martin, T. G. Matthews, T. G. Mauskopf, P. Moncelsi, L. Netterfield, C. B. Novak, G. Pascale, E. Olmi, L. Patanchon, G. Rex, M. Savini, G. Scott, D. Semisch, C. Thomas, N. Truch, M. D. P. Tucker, C. Tucker, G. S. Viero, M. P. Ward-Thompson, D. Wiebe, D. V. APC - Cosmologie AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS) William D. Duncan Wayne S. Holland Stafford Withington Jonas Zmuidzinas Marseille, France 2008-06-26 https://hal.in2p3.fr/in2p3-00330537 https://doi.org/10.1117/12.788413 en eng HAL CCSD Spie Optical Engineering Press info:eu-repo/semantics/altIdentifier/arxiv/0805.4420 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.788413 in2p3-00330537 https://hal.in2p3.fr/in2p3-00330537 ARXIV: 0805.4420 BIBCODE: 2008SPIE.7020E.1M doi:10.1117/12.788413 Proceedings of SPIE: Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV https://hal.in2p3.fr/in2p3-00330537 Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, Jun 2008, Marseille, France. ⟨10.1117/12.788413⟩ [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/conferenceObject Conference papers 2008 ftunivnantes https://doi.org/10.1117/12.788413 2023-03-08T02:50:40Z International audience The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) is a sub-orbital experiment designed to study the process of star formation in local galaxies (including the Milky Way) and in galaxies at cosmological distances. Using a 2m Cassegrain telescope, BLAST images the sky onto a focal plane, which consists of 270 bolometric detectors split between three arrays, observing simultaneously in 30% wide bands, centered at 250, 350, and 500 ?m. The diffraction-limited optical system provides a resolution of 30" at 250 ?m. The pointing system enables raster-like scans with a positional accuracy of ~30", reconstructed to better than 5" rms in postflight analysis. BLAST had two successful flights, from the Arctic in 2005, and from Antarctica in 2006, which provided the first high-resolution and large-area (~0.8-200 deg2) submillimeter surveys at these wavelengths. As a pathfinder for the SPIRE instrument on Herschel, BLAST shares with the ESA satellite similar focal plane technology and scientific motivation. A third flight in 2009 will see the instrument modified to be polarization-sensitive (BLAST-pol). With its unprecedented mapping speed and resolution, BLAST-pol will provide insights into Galactic star-forming nurseries, and give the necessary link between the larger, coarse resolution surveys and the narrow, resolved observations of star-forming structures from space and ground based instruments being commissioned in the next 5 years. Conference Object Antarc* Antarctica Arctic Université de Nantes: HAL-UNIV-NANTES Arctic Milky Way ENVELOPE(-68.705,-68.705,-71.251,-71.251) SPIE Proceedings, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV 7020 702002