Sökning: onr:"swepub:oai:DiVA.org:uu-228017" > Observation of the ...
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000 | 13236naa a2203709 4500 | |
001 | oai:DiVA.org:uu-228017 | |
003 | SwePub | |
008 | 140702s2014 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-105915 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-2280172 URI |
024 | 7 | a https://doi.org/10.1103/PhysRevD.89.1020042 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1059152 URI |
040 | a (SwePub)uud (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Aartsen, M. G.4 aut |
245 | 1 0 | a Observation of the cosmic-ray shadow of the Moon with IceCube |
264 | 1 | c 2014 |
338 | a print2 rdacarrier | |
500 | a AuthorCount:282; | |
520 | a We report on the observation of a significant deficit of cosmic rays from the direction of the Moon with the IceCube detector. The study of this "Moon shadow" is used to characterize the angular resolution and absolute pointing capabilities of the detector. The detection is based on data taken in two periods before the completion of the detector: between April 2008 and May 2009, when IceCube operated in a partial configuration with 40 detector strings deployed in the South Pole ice, and between May 2009 and May 2010 when the detector operated with 59 strings. Using two independent analysis methods, the Moon shadow has been observed to high significance (> 6 sigma) in both detector configurations. The observed location of the shadow center is within 0.2 degrees of its expected position when geomagnetic deflection effects are taken into account. This measurement validates the directional reconstruction capabilities of IceCube. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
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710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t Physical Review Dg 89:10, s. 102004-q 89:10<102004-x 1550-7998x 1550-2368 |
856 | 4 | u https://arxiv.org/abs/1305.6811y arXiv:1305.6811 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-228017 |
856 | 4 8 | u https://doi.org/10.1103/PhysRevD.89.102004 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-105915 |
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