Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey
The millimeter transient sky is largely unexplored, with measurements limited to follow-up of objects detected at other wavelengths. High-angular-resolution telescopes, designed for measurement of the cosmic microwave background (CMB), offer the possibility to discover new, unknown transient sources...
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American Astronomical Society
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Online Access: | https://authors.library.caltech.edu/71234/ https://authors.library.caltech.edu/71234/1/Whitehorn_2016_ApJ_830_143.pdf https://authors.library.caltech.edu/71234/2/1604.03507v2.pdf https://resolver.caltech.edu/CaltechAUTHORS:20161018-145206739 |
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ftcaltechauth:oai:authors.library.caltech.edu:71234 2023-05-15T18:22:36+02:00 Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey Whitehorn, N. Crites, A. T. Padin, S. 2016-10-20 application/pdf https://authors.library.caltech.edu/71234/ https://authors.library.caltech.edu/71234/1/Whitehorn_2016_ApJ_830_143.pdf https://authors.library.caltech.edu/71234/2/1604.03507v2.pdf https://resolver.caltech.edu/CaltechAUTHORS:20161018-145206739 en eng American Astronomical Society https://authors.library.caltech.edu/71234/1/Whitehorn_2016_ApJ_830_143.pdf https://authors.library.caltech.edu/71234/2/1604.03507v2.pdf Whitehorn, N. and Crites, A. T. and Padin, S. (2016) Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey. Astrophysical Journal, 830 (2). Art. No. 143. ISSN 0004-637X. doi:10.3847/0004-637X/830/2/143. https://resolver.caltech.edu/CaltechAUTHORS:20161018-145206739 <https://resolver.caltech.edu/CaltechAUTHORS:20161018-145206739> other Article PeerReviewed 2016 ftcaltechauth https://doi.org/10.3847/0004-637X/830/2/143 2021-11-18T18:39:22Z The millimeter transient sky is largely unexplored, with measurements limited to follow-up of objects detected at other wavelengths. High-angular-resolution telescopes, designed for measurement of the cosmic microwave background (CMB), offer the possibility to discover new, unknown transient sources in this band—particularly the afterglows of unobserved gamma-ray bursts (GRBs). Here, we use the 10 m millimeter-wave South Pole Telescope, designed for the primary purpose of observing the CMB at arcminute and larger angular scales, to conduct a search for such objects. During the 2012–2013 season, the telescope was used to continuously observe a 100 deg^2 patch of sky centered at R.A. 23h30m and decl. −55° using the polarization-sensitive SPTpol camera in two bands centered at 95 and 150 GHz. These 6000 hr of observations provided continuous monitoring for day- to month-scale millimeter-wave transient sources at the 10 mJy level. One candidate object was observed with properties broadly consistent with a GRB afterglow, but at a statistical significance too low (p = 0.01) to confirm detection. Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) South Pole The Astrophysical Journal 830 2 143 |
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Caltech Authors (California Institute of Technology) |
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English |
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The millimeter transient sky is largely unexplored, with measurements limited to follow-up of objects detected at other wavelengths. High-angular-resolution telescopes, designed for measurement of the cosmic microwave background (CMB), offer the possibility to discover new, unknown transient sources in this band—particularly the afterglows of unobserved gamma-ray bursts (GRBs). Here, we use the 10 m millimeter-wave South Pole Telescope, designed for the primary purpose of observing the CMB at arcminute and larger angular scales, to conduct a search for such objects. During the 2012–2013 season, the telescope was used to continuously observe a 100 deg^2 patch of sky centered at R.A. 23h30m and decl. −55° using the polarization-sensitive SPTpol camera in two bands centered at 95 and 150 GHz. These 6000 hr of observations provided continuous monitoring for day- to month-scale millimeter-wave transient sources at the 10 mJy level. One candidate object was observed with properties broadly consistent with a GRB afterglow, but at a statistical significance too low (p = 0.01) to confirm detection. |
format |
Article in Journal/Newspaper |
author |
Whitehorn, N. Crites, A. T. Padin, S. |
spellingShingle |
Whitehorn, N. Crites, A. T. Padin, S. Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey |
author_facet |
Whitehorn, N. Crites, A. T. Padin, S. |
author_sort |
Whitehorn, N. |
title |
Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey |
title_short |
Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey |
title_full |
Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey |
title_fullStr |
Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey |
title_full_unstemmed |
Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey |
title_sort |
millimeter transient point sources in the sptpol 100 square degree survey |
publisher |
American Astronomical Society |
publishDate |
2016 |
url |
https://authors.library.caltech.edu/71234/ https://authors.library.caltech.edu/71234/1/Whitehorn_2016_ApJ_830_143.pdf https://authors.library.caltech.edu/71234/2/1604.03507v2.pdf https://resolver.caltech.edu/CaltechAUTHORS:20161018-145206739 |
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South Pole |
geographic_facet |
South Pole |
genre |
South pole |
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South pole |
op_relation |
https://authors.library.caltech.edu/71234/1/Whitehorn_2016_ApJ_830_143.pdf https://authors.library.caltech.edu/71234/2/1604.03507v2.pdf Whitehorn, N. and Crites, A. T. and Padin, S. (2016) Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey. Astrophysical Journal, 830 (2). Art. No. 143. ISSN 0004-637X. doi:10.3847/0004-637X/830/2/143. https://resolver.caltech.edu/CaltechAUTHORS:20161018-145206739 <https://resolver.caltech.edu/CaltechAUTHORS:20161018-145206739> |
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op_doi |
https://doi.org/10.3847/0004-637X/830/2/143 |
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The Astrophysical Journal |
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830 |
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2 |
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143 |
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1766202008953421824 |