The next generation BLAST experiment
The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) was a suborbital experiment designed to map magnetic fields in order to study their role in star formation processes. BLASTPol made detailed polarization maps of a number of molecular clouds during its successful fli...
Published in: | Journal of Astronomical Instrumentation |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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World Scientific Publishing
2014
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Online Access: | https://orca.cardiff.ac.uk/id/eprint/157649/ https://doi.org/10.1142/S2251171714400017 https://orca.cardiff.ac.uk/id/eprint/157649/1/s2251171714400017.pdf |
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Cardiff University: ORCA (Online Research @ Cardiff) |
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The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) was a suborbital experiment designed to map magnetic fields in order to study their role in star formation processes. BLASTPol made detailed polarization maps of a number of molecular clouds during its successful flights from Antarctica in 2010 and 2012. We present the next-generation BLASTPol instrument (BLAST-TNG) that will build off the success of the previous experiment and continue its role as a unique instrument and a test bed for new technologies. With a 16-fold increase in mapping speed, BLAST-TNG will make larger and deeper maps. Major improvements include a 2.5-m carbon fiber mirror that is 40% wider than the BLASTPol mirror and ~3000 polarization sensitive detectors. BLAST-TNG will observe in three bands at 250, 350, and 500 μm. The telescope will serve as a pathfinder project for microwave kinetic inductance detector (MKID) technology, as applied to feedhorn-coupled submillimeter detector arrays. The liquid helium cooled cryostat will have a 28-day hold time and will utilize a closed-cycle 3He refrigerator to cool the detector arrays to 270 mK. This will enable a detailed mapping of more targets with higher polarization resolution than any other submillimeter experiment to date. BLAST-TNG will also be the first balloon-borne telescope to offer shared risk observing time to the community. This paper outlines the motivation for the project and the instrumental design. |
format |
Article in Journal/Newspaper |
author |
Galitzki, Nicholas Ade, Peter A. R. Angilè, Francesco E. Ashton, Peter Beall, James A. Becker, Dan Bradford, Kristi J. Che, George Cho, Hsiao-Mei Devlin, Mark J. Dober, Bradley J. Fissel, Laura M. Fukui, Yasuo Gao, Jiansong Groppi, Christopher E. Hillbrand, Seth Hilton, Gene C. Hubmayr, Johannes Irwin, Kent D. Klein, Jeffrey Van Lanen, Jeff Li, Dale Li, Zhi-Yun Lourie, Nathan P. Mani, Hamdi Martin, Peter G. Mauskopf, Philip Nakamura, Fumitaka Novak, Giles Pappas, David P. Pascale, Enzo Pisano, Giampaolo Santos, Fabio P. Savini, Giorgio Scott, Douglas Stanchfield, Sara Tucker, Carole Ullom, Joel N. Underhill, Matthew Vissers, Michael R. Ward-Thompson, Derek |
spellingShingle |
Galitzki, Nicholas Ade, Peter A. R. Angilè, Francesco E. Ashton, Peter Beall, James A. Becker, Dan Bradford, Kristi J. Che, George Cho, Hsiao-Mei Devlin, Mark J. Dober, Bradley J. Fissel, Laura M. Fukui, Yasuo Gao, Jiansong Groppi, Christopher E. Hillbrand, Seth Hilton, Gene C. Hubmayr, Johannes Irwin, Kent D. Klein, Jeffrey Van Lanen, Jeff Li, Dale Li, Zhi-Yun Lourie, Nathan P. Mani, Hamdi Martin, Peter G. Mauskopf, Philip Nakamura, Fumitaka Novak, Giles Pappas, David P. Pascale, Enzo Pisano, Giampaolo Santos, Fabio P. Savini, Giorgio Scott, Douglas Stanchfield, Sara Tucker, Carole Ullom, Joel N. Underhill, Matthew Vissers, Michael R. Ward-Thompson, Derek The next generation BLAST experiment |
author_facet |
Galitzki, Nicholas Ade, Peter A. R. Angilè, Francesco E. Ashton, Peter Beall, James A. Becker, Dan Bradford, Kristi J. Che, George Cho, Hsiao-Mei Devlin, Mark J. Dober, Bradley J. Fissel, Laura M. Fukui, Yasuo Gao, Jiansong Groppi, Christopher E. Hillbrand, Seth Hilton, Gene C. Hubmayr, Johannes Irwin, Kent D. Klein, Jeffrey Van Lanen, Jeff Li, Dale Li, Zhi-Yun Lourie, Nathan P. Mani, Hamdi Martin, Peter G. Mauskopf, Philip Nakamura, Fumitaka Novak, Giles Pappas, David P. Pascale, Enzo Pisano, Giampaolo Santos, Fabio P. Savini, Giorgio Scott, Douglas Stanchfield, Sara Tucker, Carole Ullom, Joel N. Underhill, Matthew Vissers, Michael R. Ward-Thompson, Derek |
author_sort |
Galitzki, Nicholas |
title |
The next generation BLAST experiment |
title_short |
The next generation BLAST experiment |
title_full |
The next generation BLAST experiment |
title_fullStr |
The next generation BLAST experiment |
title_full_unstemmed |
The next generation BLAST experiment |
title_sort |
next generation blast experiment |
publisher |
World Scientific Publishing |
publishDate |
2014 |
url |
https://orca.cardiff.ac.uk/id/eprint/157649/ https://doi.org/10.1142/S2251171714400017 https://orca.cardiff.ac.uk/id/eprint/157649/1/s2251171714400017.pdf |
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Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
https://orca.cardiff.ac.uk/id/eprint/157649/1/s2251171714400017.pdf Galitzki, Nicholas, Ade, Peter A. R. https://orca.cardiff.ac.uk/view/cardiffauthors/A0479492.html orcid:0000-0002-5127-0401 orcid:0000-0002-5127-0401, Angilè, Francesco E., Ashton, Peter, Beall, James A., Becker, Dan, Bradford, Kristi J., Che, George, Cho, Hsiao-Mei, Devlin, Mark J., Dober, Bradley J., Fissel, Laura M., Fukui, Yasuo, Gao, Jiansong, Groppi, Christopher E., Hillbrand, Seth, Hilton, Gene C., Hubmayr, Johannes, Irwin, Kent D., Klein, Jeffrey, Van Lanen, Jeff, Li, Dale, Li, Zhi-Yun, Lourie, Nathan P., Mani, Hamdi, Martin, Peter G., Mauskopf, Philip, Nakamura, Fumitaka, Novak, Giles, Pappas, David P., Pascale, Enzo, Pisano, Giampaolo https://orca.cardiff.ac.uk/view/cardiffauthors/A047942G.html orcid:0000-0003-4302-5681 orcid:0000-0003-4302-5681, Santos, Fabio P., Savini, Giorgio, Scott, Douglas, Stanchfield, Sara, Tucker, Carole https://orca.cardiff.ac.uk/view/cardiffauthors/A016987K.html orcid:0000-0002-1851-3918 orcid:0000-0002-1851-3918, Ullom, Joel N., Underhill, Matthew, Vissers, Michael R. and Ward-Thompson, Derek 2014. The next generation BLAST experiment. Journal of Astronomical Instrumentation 03 (02) , 1440001. 10.1142/S2251171714400017 https://doi.org/10.1142/S2251171714400017 file https://orca.cardiff.ac.uk/id/eprint/157649/1/s2251171714400017.pdf doi:10.1142/S2251171714400017 |
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https://doi.org/10.1142/S2251171714400017 |
container_title |
Journal of Astronomical Instrumentation |
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03 |
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ftunivcardiff:oai:https://orca.cardiff.ac.uk:157649 2023-06-11T04:05:25+02:00 The next generation BLAST experiment Galitzki, Nicholas Ade, Peter A. R. Angilè, Francesco E. Ashton, Peter Beall, James A. Becker, Dan Bradford, Kristi J. Che, George Cho, Hsiao-Mei Devlin, Mark J. Dober, Bradley J. Fissel, Laura M. Fukui, Yasuo Gao, Jiansong Groppi, Christopher E. Hillbrand, Seth Hilton, Gene C. Hubmayr, Johannes Irwin, Kent D. Klein, Jeffrey Van Lanen, Jeff Li, Dale Li, Zhi-Yun Lourie, Nathan P. Mani, Hamdi Martin, Peter G. Mauskopf, Philip Nakamura, Fumitaka Novak, Giles Pappas, David P. Pascale, Enzo Pisano, Giampaolo Santos, Fabio P. Savini, Giorgio Scott, Douglas Stanchfield, Sara Tucker, Carole Ullom, Joel N. Underhill, Matthew Vissers, Michael R. Ward-Thompson, Derek 2014-11-30 application/pdf https://orca.cardiff.ac.uk/id/eprint/157649/ https://doi.org/10.1142/S2251171714400017 https://orca.cardiff.ac.uk/id/eprint/157649/1/s2251171714400017.pdf en eng World Scientific Publishing https://orca.cardiff.ac.uk/id/eprint/157649/1/s2251171714400017.pdf Galitzki, Nicholas, Ade, Peter A. R. https://orca.cardiff.ac.uk/view/cardiffauthors/A0479492.html orcid:0000-0002-5127-0401 orcid:0000-0002-5127-0401, Angilè, Francesco E., Ashton, Peter, Beall, James A., Becker, Dan, Bradford, Kristi J., Che, George, Cho, Hsiao-Mei, Devlin, Mark J., Dober, Bradley J., Fissel, Laura M., Fukui, Yasuo, Gao, Jiansong, Groppi, Christopher E., Hillbrand, Seth, Hilton, Gene C., Hubmayr, Johannes, Irwin, Kent D., Klein, Jeffrey, Van Lanen, Jeff, Li, Dale, Li, Zhi-Yun, Lourie, Nathan P., Mani, Hamdi, Martin, Peter G., Mauskopf, Philip, Nakamura, Fumitaka, Novak, Giles, Pappas, David P., Pascale, Enzo, Pisano, Giampaolo https://orca.cardiff.ac.uk/view/cardiffauthors/A047942G.html orcid:0000-0003-4302-5681 orcid:0000-0003-4302-5681, Santos, Fabio P., Savini, Giorgio, Scott, Douglas, Stanchfield, Sara, Tucker, Carole https://orca.cardiff.ac.uk/view/cardiffauthors/A016987K.html orcid:0000-0002-1851-3918 orcid:0000-0002-1851-3918, Ullom, Joel N., Underhill, Matthew, Vissers, Michael R. and Ward-Thompson, Derek 2014. The next generation BLAST experiment. Journal of Astronomical Instrumentation 03 (02) , 1440001. 10.1142/S2251171714400017 https://doi.org/10.1142/S2251171714400017 file https://orca.cardiff.ac.uk/id/eprint/157649/1/s2251171714400017.pdf doi:10.1142/S2251171714400017 cc_by_4_0 Article PeerReviewed 2014 ftunivcardiff https://doi.org/10.1142/S2251171714400017 2023-05-04T22:39:23Z The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) was a suborbital experiment designed to map magnetic fields in order to study their role in star formation processes. BLASTPol made detailed polarization maps of a number of molecular clouds during its successful flights from Antarctica in 2010 and 2012. We present the next-generation BLASTPol instrument (BLAST-TNG) that will build off the success of the previous experiment and continue its role as a unique instrument and a test bed for new technologies. With a 16-fold increase in mapping speed, BLAST-TNG will make larger and deeper maps. Major improvements include a 2.5-m carbon fiber mirror that is 40% wider than the BLASTPol mirror and ~3000 polarization sensitive detectors. BLAST-TNG will observe in three bands at 250, 350, and 500 μm. The telescope will serve as a pathfinder project for microwave kinetic inductance detector (MKID) technology, as applied to feedhorn-coupled submillimeter detector arrays. The liquid helium cooled cryostat will have a 28-day hold time and will utilize a closed-cycle 3He refrigerator to cool the detector arrays to 270 mK. This will enable a detailed mapping of more targets with higher polarization resolution than any other submillimeter experiment to date. BLAST-TNG will also be the first balloon-borne telescope to offer shared risk observing time to the community. This paper outlines the motivation for the project and the instrumental design. Article in Journal/Newspaper Antarc* Antarctica Cardiff University: ORCA (Online Research @ Cardiff) Journal of Astronomical Instrumentation 03 02 |