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Search for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT

Supernovae (SNe) exploding in a dense circumstellar medium (CSM) are hypothesized to accelerate cosmic rays in collisionless shocks and emit GeV gamma rays and TeV neutrinos on a time scale of several months. We perform the first systematic search for gamma-ray emission in Fermi LAT data in the ener... Full description

Journal Title: arXiv.org Jun 26, 2015
Main Author: Ackermann, M
Other Authors: Arcavi, I , Baldini, L , Ballet, J , Barbiellini, G , Bastieri, D , Bellazzini, R , Bissaldi, E , Blandford, R , Bonino, R , Bottacini, E , Brandt, T , Bregeon, J , Bruel, P , Buehler, R , Buson, S , Caliandro, G , Cameron, R , Caragiulo, M , Caraveo
Format: Electronic Article Electronic Article
Language: English
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ID: DOI: 10.1088/0004-637X/807/2/169
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title: Search for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
format: Article
creator:
  • Ackermann, M
  • Arcavi, I
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Bastieri, D
  • Bellazzini, R
  • Bissaldi, E
  • Blandford, R
  • Bonino, R
  • Bottacini, E
  • Brandt, T
  • Bregeon, J
  • Bruel, P
  • Buehler, R
  • Buson, S
  • Caliandro, G
  • Cameron, R
  • Caragiulo, M
  • Caraveo
subjects:
  • Cosmic Rays
  • Gamma Rays
  • Luminosity
  • Flux
  • Windows (Intervals)
  • Confidence Intervals
  • Cosmic Rays
  • Gamma Rays
  • Searching
  • Supernovae
  • Neutrinos
ispartof: arXiv.org, Jun 26, 2015
description: Supernovae (SNe) exploding in a dense circumstellar medium (CSM) are hypothesized to accelerate cosmic rays in collisionless shocks and emit GeV gamma rays and TeV neutrinos on a time scale of several months. We perform the first systematic search for gamma-ray emission in Fermi LAT data in the energy range from 100 MeV to 300 GeV from the ensemble of 147 SNe Type IIn exploding in dense CSM. We search for a gamma-ray excess at each SNe location in a one year time window. In order to enhance a possible weak signal, we simultaneously study the closest and optically brightest sources of our sample in a joint-likelihood analysis in three different time windows (1 year, 6 months and 3 months). For the most promising source of the sample, SN 2010jl (PTF10aaxf), we repeat the analysis with an extended time window lasting 4.5 years. We do not find a significant excess in gamma rays for any individual source nor for the combined sources and provide model-independent flux upper limits for both cases....
language: eng
source:
identifier: DOI: 10.1088/0004-637X/807/2/169
fulltext: fulltext_linktorsrc
url: Link


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titleSearch for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
creatorAckermann, M ; Arcavi, I ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bellazzini, R ; Bissaldi, E ; Blandford, R ; Bonino, R ; Bottacini, E ; Brandt, T ; Bregeon, J ; Bruel, P ; Buehler, R ; Buson, S ; Caliandro, G ; Cameron, R ; Caragiulo, M ; Caraveo
contributorWood, M (pacrepositoryorg)
ispartofarXiv.org, Jun 26, 2015
identifierDOI: 10.1088/0004-637X/807/2/169
subjectCosmic Rays ; Gamma Rays ; Luminosity ; Flux ; Windows (Intervals) ; Confidence Intervals ; Cosmic Rays ; Gamma Rays ; Searching ; Supernovae ; Neutrinos
descriptionSupernovae (SNe) exploding in a dense circumstellar medium (CSM) are hypothesized to accelerate cosmic rays in collisionless shocks and emit GeV gamma rays and TeV neutrinos on a time scale of several months. We perform the first systematic search for gamma-ray emission in Fermi LAT data in the energy range from 100 MeV to 300 GeV from the ensemble of 147 SNe Type IIn exploding in dense CSM. We search for a gamma-ray excess at each SNe location in a one year time window. In order to enhance a possible weak signal, we simultaneously study the closest and optically brightest sources of our sample in a joint-likelihood analysis in three different time windows (1 year, 6 months and 3 months). For the most promising source of the sample, SN 2010jl (PTF10aaxf), we repeat the analysis with an extended time window lasting 4.5 years. We do not find a significant excess in gamma rays for any individual source nor for the combined sources and provide model-independent flux upper limits for both cases....
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52Hayashi, K
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55Horan, D
56Jogler, T
57Jóhannesson, G
58Kocevski, D
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61Lashner, J
62Latronico, L
63Longo, F
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100Thayer, J
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titleSearch for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
descriptionSupernovae (SNe) exploding in a dense circumstellar medium (CSM) are hypothesized to accelerate cosmic rays in collisionless shocks and emit GeV gamma rays and TeV neutrinos on a time scale of several months. We perform the first systematic search for gamma-ray emission in Fermi LAT data in the energy range from 100 MeV to 300 GeV from the ensemble of 147 SNe Type IIn exploding in dense CSM. We search for a gamma-ray excess at each SNe location in a one year time window. In order to enhance a possible weak signal, we simultaneously study the closest and optically brightest sources of our sample in a joint-likelihood analysis in three different time windows (1 year, 6 months and 3 months). For the most promising source of the sample, SN 2010jl (PTF10aaxf), we repeat the analysis with an extended time window lasting 4.5 years. We do not find a significant excess in gamma rays for any individual source nor for the combined sources and provide model-independent flux upper limits for both cases....
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titleSearch for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
authorAckermann, M ; Arcavi, I ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bellazzini, R ; Bissaldi, E ; Blandford, R ; Bonino, R ; Bottacini, E ; Brandt, T ; Bregeon, J ; Bruel, P ; Buehler, R ; Buson, S ; Caliandro, G ; Cameron, R ; Caragiulo, M ; Caraveo
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1Arcavi, I
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3Ballet, J
4Barbiellini, G
5Bastieri, D
6Bellazzini, R
7Bissaldi, E
8Blandford, R
9Bonino, R
10Bottacini, E
11Brandt, T
12Bregeon, J
13Bruel, P
14Buehler, R
15Buson, S
16Caliandro, G
17Cameron, R
18Caragiulo, M
19Caraveo, P
20Cavazzuti, E
21Cecchi, C
22Charles, E
23Chekhtman, A
24Chiang, J
25Chiaro, G
26Ciprini, S
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30D'Ammando, F
31de Angelis, A
32de Palma, F
33Desiante, R
34Drell, P
35Favuzzi, C
36Fegan, S
37Franckowiak, A
38Funk, S
39Fusco, P
40Gal-Yam, A
41Gargano, F
42Gasparrini, D
43Giglietto, N
44Giordano, F
45Giroletti, M
46Glanzman, T
47Godfrey, G
48Grenier, I
49Grove, J
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51Harding, A
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57Jóhannesson, G
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20Cavazzuti, E
21Cecchi, C
22Charles, E
23Chekhtman, A
24Chiang, J
25Chiaro, G
26Ciprini, S
27Claus, R
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29Cutini, S
30D'Ammando, F
31de Angelis, A
32de Palma, F
33Desiante, R
34Drell, P
35Favuzzi, C
36Fegan, S
37Franckowiak, A
38Funk, S
39Fusco, P
40Gal-Yam, A
41Gargano, F
42Gasparrini, D
43Giglietto, N
44Giordano, F
45Giroletti, M
46Glanzman, T
47Godfrey, G
48Grenier, I
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50Guiriec, S
51Harding, A
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53Hewitt, J
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61Lashner, J
62Latronico, L
63Longo, F
64Loparco, F
65Lovellette, M
66Lubrano, P
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68Mayer, M
69Mazziotta, M
70Mcenery, J
71Michelson, P
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98Suson, D
99Takahashi, H
100Thayer, J
101Tibaldo, L
102Torres, D
103Troja, E
104Vianello, G
105Werner, M
106Wood, K
107Wood, M
atitleSearch for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
jtitlearXiv.org
risdate20150626
formatjournal
genrearticle
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abstractSupernovae (SNe) exploding in a dense circumstellar medium (CSM) are hypothesized to accelerate cosmic rays in collisionless shocks and emit GeV gamma rays and TeV neutrinos on a time scale of several months. We perform the first systematic search for gamma-ray emission in Fermi LAT data in the energy range from 100 MeV to 300 GeV from the ensemble of 147 SNe Type IIn exploding in dense CSM. We search for a gamma-ray excess at each SNe location in a one year time window. In order to enhance a possible weak signal, we simultaneously study the closest and optically brightest sources of our sample in a joint-likelihood analysis in three different time windows (1 year, 6 months and 3 months). For the most promising source of the sample, SN 2010jl (PTF10aaxf), we repeat the analysis with an extended time window lasting 4.5 years. We do not find a significant excess in gamma rays for any individual source nor for the combined sources and provide model-independent flux upper limits for both cases....
copIthaca
pubCornell University Library, arXiv.org
doi10.1088/0004-637X/807/2/169
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pages1-15
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issue2
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date2015-06-26