Indirect Searches for Dark Matter with the Fermi Large Area Telescope1

Albert, Andrea

Open link

Publication date

December 2015

DOI

10.1016/j.phpro.2014.12.004

Publisher

The Authors. Published by Elsevier B.V.

Abstract

AbstractThere is overwhelming evidence that non-baryonic dark matter constitutes ∼ 27% of the energy density of the Universe. Weakly Interacting Massive Particles (WIMPs) are promising dark matter candidates that may produce γ rays via annihilation or decay detectable by the Fermi Large Area Telescope (LAT). A detection of WIMPs would also indicate the existence of physics beyond the Standard Model. We present recent results from the two cleanest indirect WIMP searches by the Fermi-LAT Collaboration: searches for γ-ray spectral lines and γ-ray emission associated with Milky Way dwarf spheroidal satellite galaxies

Extracted data

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Indirect Searches for Dark Matter with the Fermi Large Area Telescope1

Albert, Andrea

Open link

Publication date

December 2015

DOI

10.1016/j.phpro.2014.12.004

Publisher

The Authors. Published by Elsevier B.V.

Abstract

Extracted data

Ackermann, Markus
Albert, A.
Baldini, Luca
Ballet, Jean
Barbiellini, Guido
Bastieri, D.
Bechtol, K.
Bellazzini, R.
D. Blandford, R.
D. Bloom, E.
Bonamente, E.
W. Borgland, A.
Bottacini, E.
J. Brandt, T.
Bregeon, J.
Brigida, M.
Bruel, Pascal
Buehler, R.
H. Burnett, T.
A. Caliandro, G.
A. Cameron, R.
Caraveo, P. A.
M. Casandjian, J.
Cecchi, C.
Charles, E.
Chiang, J.
Ciprini, S.
Claus, R.
Cohen-Tanugi, J.
Conrad, J.
Cutini, S.
de Palma, F.
D. Dermer, C.
W. Digel, S.
Do Couto E Silva, E.
S. Drell, P.
Drlica-Wagner, A.
Essig, R.
Falletti, L.
Favuzzi, C.
J. Fegan, S.
B. Focke, W.
Fukazawa, Y.
Funk, S.
Fusco, P.
Gargano, F.
Germani, S.
Giglietto, N.
Giordano, F.
Giroletti, M.
Glanzman, T.
Godfrey, G.
A. Grenier, I.
Guiriec, S.
Gustafsson, M.
Hadasch, D.
Hayashida, M.
Hou, X.
E. Hughes, R.
P. Johnson, R.
S. Johnson, A.
Kamae, T.
Katagiri, H.
Kataoka, J.
Knödlseder, Jürgen
Kuss, M.
Lande, J.
Latronico, L.
Lee, S.-H.
M. Lionetto, A.
Llena Garde, M.
Longo, F.
Loparco, F.
N. Lovellette, M.
Lubrano, P.
N. Mazziotta, M.
E. Mcenery, J.
F. Michelson, P.
Mitthumsiri, W.
Mizuno, T.
A. Moiseev, A.
Monte, C.
E. Monzani, M.
Morselli, A.
V. Moskalenko, I.
Murgia, S.
Naumann-Godo, M.
P. Norris, J.
Nuss, E.
Ohsugi, T.
Okumura, A.
Orlando, E.
F. Ormes, J.
Ozaki, M.
Paneque, D.
Pelassa, V.
Pierbattista, M.
Piron, F.
Pivato, G.
Porter, T.A.
Rain'O, S.
Rando, R.
Razzano, M.
Reimer, A.
Reimer, O.
Ritz, S.
F.-W. Sadrozinski, H.
Sehgal, N.
Sgr'O, C.
J. Siskind, E.
Spinelli, P.
Strigari, L.
J. Suson, D.
Tajima, H.
Takahashi, H.
Tanaka, T.
G. Thayer, J.
B. Thayer, J.
Tibaldo, L.
Tinivella, M.
F. Torres, D.
Troja, E.
Uchiyama, Y.
L. Usher, T.
Vandenbroucke, J.
Vasileiou, V.
Vianello, G.
Vitale, V.
P. Waite, A.
Wang, P.
L. Winer, B.
S. Wood, K.
Yang, Z.
Zalewski, S.
Zimmer, S.

January 2012

Numerical simulations based on the Lambda-CDM model of cosmology predict a large number of as yet un...

Search for Dark Matter Satellites Using the FERMI-LAT

Ackermann, M.
/DESY
Albert, A.
U., /Ohio State
Baldini, L.
/INFN, Pisa
Ballet, J.
/DAPNIA, Saclay
Barbiellini, G.
/INFN, Trieste /Trieste U.
Bastieri, D.
/INFN, Padua /Padua U.
Bechtol, K.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bellazzini, R.
/INFN, Pisa
Blandford, R.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bloom, E.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /SLAC
Bonamente, E.
/INFN, Perugia /Perugia U.
Borgland, A.W.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bottacini, E.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Brandt, T.J.
/IRAP, Toulouse /Toulouse III U.
Bregeon, J.
/INFN, Pisa
Brigida, M.
/Bari U. /INFN, Bari
Bruel, P.
Polytechnique, /Ecole
Buehler, R.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Burnett, T.H.
/Washington U., Seattle
Caliandro, G.A.
/ICE, Bellaterra
Cameron, R.A.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /IASF, Milan /IASF, Milan /DAPNIA, Saclay /INFN, Perugia /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /ASDC, Frascati /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Stockholm U. /Stockholm U., OKC /ASDC, Frascati /Bari U. /INFN, Bari /Naval Research Lab, Wash., D.C. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Bari U. /INFN, Bari /Ecole Polytechnique /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Hiroshima U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Bari U. /INFN, Bari /INFN, Bari /INFN, Perugia /Perugia U. /Bari U. /INFN, Bari /Bari U. /INFN, Bari /Bologna Observ. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
authors.., /more

August 2012

Numerical simulations based on the {Lambda}CDM model of cosmology predict a large number of as yet u...

Indirect Searches for Dark Matter with the Fermi Large Area Telescope1

Albert, Andrea

December 2015

AbstractThere is overwhelming evidence that non-baryonic dark matter constitutes ∼ 27% of the energy...

Searching for New Physics with the Fermi Large Area Telescope

Johnson, Arne Christian

January 2019

Compelling astronomical evidence suggests that a majority of the matter in the Universe, known as da...

FERMI-LAT SENSITIVITY AND CONSTRAINTS ON DARK MATTER SIGNAL FROM THE MILKY WAY HOST HALO AND ITS SUBSTRUCTURE

Anderson, Brandon

January 2012

Despite overwhelming evidence of its existence, the exact nature of Dark Matter (DM) remains unknown...

Search for Dark Matter Satellites using the FERMI-LAT

Ackermann, Markus
Albert, A.
Baldini, Luca
Ballet, Jean
Barbiellini, Guido
Bastieri, D.
Bechtol, K.
Bellazzini, R.
D. Blandford, R.
D. Bloom, E.
Bonamente, E.
W. Borgland, A.
Bottacini, E.
J. Brandt, T.
Bregeon, J.
Brigida, M.
Bruel, Pascal
Buehler, R.
H. Burnett, T.
A. Caliandro, G.
A. Cameron, R.
Caraveo, P. A.
M. Casandjian, J.
Cecchi, C.
Charles, E.
Chiang, J.
Ciprini, S.
Claus, R.
Cohen-Tanugi, J.
Conrad, J.
Cutini, S.
de Palma, F.
D. Dermer, C.
W. Digel, S.
Do Couto E Silva, E.
S. Drell, P.
Drlica-Wagner, A.
Essig, R.
Falletti, L.
Favuzzi, C.
J. Fegan, S.
B. Focke, W.
Fukazawa, Y.
Funk, S.
Fusco, P.
Gargano, F.
Germani, S.
Giglietto, N.
Giordano, F.
Giroletti, M.
Glanzman, T.
Godfrey, G.
A. Grenier, I.
Guiriec, S.
Gustafsson, M.
Hadasch, D.
Hayashida, M.
Hou, X.
E. Hughes, R.
P. Johnson, R.
S. Johnson, A.
Kamae, T.
Katagiri, H.
Kataoka, J.
Knödlseder, Jürgen
Kuss, M.
Lande, J.
Latronico, L.
Lee, S.-H.
M. Lionetto, A.
Llena Garde, M.
Longo, F.
Loparco, F.
N. Lovellette, M.
Lubrano, P.
N. Mazziotta, M.
E. Mcenery, J.
F. Michelson, P.
Mitthumsiri, W.
Mizuno, T.
A. Moiseev, A.
Monte, C.
E. Monzani, M.
Morselli, A.
V. Moskalenko, I.
Murgia, S.
Naumann-Godo, M.
P. Norris, J.
Nuss, E.
Ohsugi, T.
Okumura, A.
Orlando, E.
F. Ormes, J.
Ozaki, M.
Paneque, D.
Pelassa, V.
Pierbattista, M.
Piron, F.
Pivato, G.
Porter, T.A.
Rain'O, S.
Rando, R.
Razzano, M.
Reimer, A.
Reimer, O.
Ritz, S.
F.-W. Sadrozinski, H.
Sehgal, N.
Sgr'O, C.
J. Siskind, E.
Spinelli, P.
Strigari, L.
J. Suson, D.
Tajima, H.
Takahashi, H.
Tanaka, T.
G. Thayer, J.
B. Thayer, J.
Tibaldo, L.
Tinivella, M.
F. Torres, D.
Troja, E.
Uchiyama, Y.
L. Usher, T.
Vandenbroucke, J.
Vasileiou, V.
Vianello, G.
Vitale, V.
P. Waite, A.
Wang, P.
L. Winer, B.
S. Wood, K.
Yang, Z.
Zalewski, S.
Zimmer, S.

January 2012

Numerical simulations based on the Lambda-CDM model of cosmology predict a large number of as yet un...

Search for Dark Matter Satellites Using the FERMI-LAT

Ackermann, M.
/DESY
Albert, A.
U., /Ohio State
Baldini, L.
/INFN, Pisa
Ballet, J.
/DAPNIA, Saclay
Barbiellini, G.
/INFN, Trieste /Trieste U.
Bastieri, D.
/INFN, Padua /Padua U.
Bechtol, K.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bellazzini, R.
/INFN, Pisa
Blandford, R.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bloom, E.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /SLAC
Bonamente, E.
/INFN, Perugia /Perugia U.
Borgland, A.W.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bottacini, E.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Brandt, T.J.
/IRAP, Toulouse /Toulouse III U.
Bregeon, J.
/INFN, Pisa
Brigida, M.
/Bari U. /INFN, Bari
Bruel, P.
Polytechnique, /Ecole
Buehler, R.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Burnett, T.H.
/Washington U., Seattle
Caliandro, G.A.
/ICE, Bellaterra
Cameron, R.A.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /IASF, Milan /IASF, Milan /DAPNIA, Saclay /INFN, Perugia /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /ASDC, Frascati /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Stockholm U. /Stockholm U., OKC /ASDC, Frascati /Bari U. /INFN, Bari /Naval Research Lab, Wash., D.C. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Bari U. /INFN, Bari /Ecole Polytechnique /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Hiroshima U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Bari U. /INFN, Bari /INFN, Bari /INFN, Perugia /Perugia U. /Bari U. /INFN, Bari /Bari U. /INFN, Bari /Bologna Observ. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
authors.., /more

August 2012

Numerical simulations based on the {Lambda}CDM model of cosmology predict a large number of as yet u...

Search for Dark Matter Satellites using the FERMI-LAT

Ackermann, Markus
Albert, A.
Baldini, Luca
Ballet, Jean
Barbiellini, Guido
Bastieri, D.
Bechtol, K.
Bellazzini, R.
D. Blandford, R.
D. Bloom, E.
Bonamente, E.
W. Borgland, A.
Bottacini, E.
J. Brandt, T.
Bregeon, J.
Brigida, M.
Bruel, Pascal
Buehler, R.
H. Burnett, T.
A. Caliandro, G.
A. Cameron, R.
Caraveo, P. A.
M. Casandjian, J.
Cecchi, C.
Charles, E.
Chiang, J.
Ciprini, S.
Claus, R.
Cohen-Tanugi, J.
Conrad, J.
Cutini, S.
de Palma, F.
D. Dermer, C.
W. Digel, S.
Do Couto E Silva, E.
S. Drell, P.
Drlica-Wagner, A.
Essig, R.
Falletti, L.
Favuzzi, C.
J. Fegan, S.
B. Focke, W.
Fukazawa, Y.
Funk, S.
Fusco, P.
Gargano, F.
Germani, S.
Giglietto, N.
Giordano, F.
Giroletti, M.
Glanzman, T.
Godfrey, G.
A. Grenier, I.
Guiriec, S.
Gustafsson, M.
Hadasch, D.
Hayashida, M.
Hou, X.
E. Hughes, R.
P. Johnson, R.
S. Johnson, A.
Kamae, T.
Katagiri, H.
Kataoka, J.
Knödlseder, Jürgen
Kuss, M.
Lande, J.
Latronico, L.
Lee, S.-H.
M. Lionetto, A.
Llena Garde, M.
Longo, F.
Loparco, F.
N. Lovellette, M.
Lubrano, P.
N. Mazziotta, M.
E. Mcenery, J.
F. Michelson, P.
Mitthumsiri, W.
Mizuno, T.
A. Moiseev, A.
Monte, C.
E. Monzani, M.
Morselli, A.
V. Moskalenko, I.
Murgia, S.
Naumann-Godo, M.
P. Norris, J.
Nuss, E.
Ohsugi, T.
Okumura, A.
Orlando, E.
F. Ormes, J.
Ozaki, M.
Paneque, D.
Pelassa, V.
Pierbattista, M.
Piron, F.
Pivato, G.
Porter, T.A.
Rain'O, S.
Rando, R.
Razzano, M.
Reimer, A.
Reimer, O.
Ritz, S.
F.-W. Sadrozinski, H.
Sehgal, N.
Sgr'O, C.
J. Siskind, E.
Spinelli, P.
Strigari, L.
J. Suson, D.
Tajima, H.
Takahashi, H.
Tanaka, T.
G. Thayer, J.
B. Thayer, J.
Tibaldo, L.
Tinivella, M.
F. Torres, D.
Troja, E.
Uchiyama, Y.
L. Usher, T.
Vandenbroucke, J.
Vasileiou, V.
Vianello, G.
Vitale, V.
P. Waite, A.
Wang, P.
L. Winer, B.
S. Wood, K.
Yang, Z.
Zalewski, S.
Zimmer, S.

January 2012

Numerical simulations based on the Lambda-CDM model of cosmology predict a large number of as yet un...

Search for Dark Matter Satellites Using the FERMI-LAT

Ackermann, M.
/DESY
Albert, A.
U., /Ohio State
Baldini, L.
/INFN, Pisa
Ballet, J.
/DAPNIA, Saclay
Barbiellini, G.
/INFN, Trieste /Trieste U.
Bastieri, D.
/INFN, Padua /Padua U.
Bechtol, K.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bellazzini, R.
/INFN, Pisa
Blandford, R.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bloom, E.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /SLAC
Bonamente, E.
/INFN, Perugia /Perugia U.
Borgland, A.W.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bottacini, E.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Brandt, T.J.
/IRAP, Toulouse /Toulouse III U.
Bregeon, J.
/INFN, Pisa
Brigida, M.
/Bari U. /INFN, Bari
Bruel, P.
Polytechnique, /Ecole
Buehler, R.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Burnett, T.H.
/Washington U., Seattle
Caliandro, G.A.
/ICE, Bellaterra
Cameron, R.A.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /IASF, Milan /IASF, Milan /DAPNIA, Saclay /INFN, Perugia /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /ASDC, Frascati /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Stockholm U. /Stockholm U., OKC /ASDC, Frascati /Bari U. /INFN, Bari /Naval Research Lab, Wash., D.C. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Bari U. /INFN, Bari /Ecole Polytechnique /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Hiroshima U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Bari U. /INFN, Bari /INFN, Bari /INFN, Perugia /Perugia U. /Bari U. /INFN, Bari /Bari U. /INFN, Bari /Bologna Observ. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
authors.., /more

August 2012

Numerical simulations based on the {Lambda}CDM model of cosmology predict a large number of as yet u...

Ackermann, Markus
Albert, A.
Baldini, Luca
Ballet, Jean
Barbiellini, Guido
Bastieri, D.
Bechtol, K.
Bellazzini, R.
D. Blandford, R.
D. Bloom, E.
Bonamente, E.
W. Borgland, A.
Bottacini, E.
J. Brandt, T.
Bregeon, J.
Brigida, M.
Bruel, Pascal
Buehler, R.
H. Burnett, T.
A. Caliandro, G.
A. Cameron, R.
Caraveo, P. A.
M. Casandjian, J.
Cecchi, C.
Charles, E.
Chiang, J.
Ciprini, S.
Claus, R.
Cohen-Tanugi, J.
Conrad, J.
Cutini, S.
de Palma, F.
D. Dermer, C.
W. Digel, S.
Do Couto E Silva, E.
S. Drell, P.
Drlica-Wagner, A.
Essig, R.
Falletti, L.
Favuzzi, C.
J. Fegan, S.
B. Focke, W.
Fukazawa, Y.
Funk, S.
Fusco, P.
Gargano, F.
Germani, S.
Giglietto, N.
Giordano, F.
Giroletti, M.
Glanzman, T.
Godfrey, G.
A. Grenier, I.
Guiriec, S.
Gustafsson, M.
Hadasch, D.
Hayashida, M.
Hou, X.
E. Hughes, R.
P. Johnson, R.
S. Johnson, A.
Kamae, T.
Katagiri, H.
Kataoka, J.
Knödlseder, Jürgen
Kuss, M.
Lande, J.
Latronico, L.
Lee, S.-H.
M. Lionetto, A.
Llena Garde, M.
Longo, F.
Loparco, F.
N. Lovellette, M.
Lubrano, P.
N. Mazziotta, M.
E. Mcenery, J.
F. Michelson, P.
Mitthumsiri, W.
Mizuno, T.
A. Moiseev, A.
Monte, C.
E. Monzani, M.
Morselli, A.
V. Moskalenko, I.
Murgia, S.
Naumann-Godo, M.
P. Norris, J.
Nuss, E.
Ohsugi, T.
Okumura, A.
Orlando, E.
F. Ormes, J.
Ozaki, M.
Paneque, D.
Pelassa, V.
Pierbattista, M.
Piron, F.
Pivato, G.
Porter, T.A.
Rain'O, S.
Rando, R.
Razzano, M.
Reimer, A.
Reimer, O.
Ritz, S.
F.-W. Sadrozinski, H.
Sehgal, N.
Sgr'O, C.
J. Siskind, E.
Spinelli, P.
Strigari, L.
J. Suson, D.
Tajima, H.
Takahashi, H.
Tanaka, T.
G. Thayer, J.
B. Thayer, J.
Tibaldo, L.
Tinivella, M.
F. Torres, D.
Troja, E.
Uchiyama, Y.
L. Usher, T.
Vandenbroucke, J.
Vasileiou, V.
Vianello, G.
Vitale, V.
P. Waite, A.
Wang, P.
L. Winer, B.
S. Wood, K.
Yang, Z.
Zalewski, S.
Zimmer, S.

January 2012

Numerical simulations based on the Lambda-CDM model of cosmology predict a large number of as yet un...

Search for Dark Matter Satellites Using the FERMI-LAT

Ackermann, M.
/DESY
Albert, A.
U., /Ohio State
Baldini, L.
/INFN, Pisa
Ballet, J.
/DAPNIA, Saclay
Barbiellini, G.
/INFN, Trieste /Trieste U.
Bastieri, D.
/INFN, Padua /Padua U.
Bechtol, K.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bellazzini, R.
/INFN, Pisa
Blandford, R.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bloom, E.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /SLAC
Bonamente, E.
/INFN, Perugia /Perugia U.
Borgland, A.W.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bottacini, E.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Brandt, T.J.
/IRAP, Toulouse /Toulouse III U.
Bregeon, J.
/INFN, Pisa
Brigida, M.
/Bari U. /INFN, Bari
Bruel, P.
Polytechnique, /Ecole
Buehler, R.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Burnett, T.H.
/Washington U., Seattle
Caliandro, G.A.
/ICE, Bellaterra
Cameron, R.A.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /IASF, Milan /IASF, Milan /DAPNIA, Saclay /INFN, Perugia /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /ASDC, Frascati /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Stockholm U. /Stockholm U., OKC /ASDC, Frascati /Bari U. /INFN, Bari /Naval Research Lab, Wash., D.C. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Bari U. /INFN, Bari /Ecole Polytechnique /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Hiroshima U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Bari U. /INFN, Bari /INFN, Bari /INFN, Perugia /Perugia U. /Bari U. /INFN, Bari /Bari U. /INFN, Bari /Bologna Observ. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
authors.., /more

August 2012

Numerical simulations based on the {Lambda}CDM model of cosmology predict a large number of as yet u...

Indirect Searches for Dark Matter with the Fermi Large Area Telescope1

Albert, Andrea

December 2015

AbstractThere is overwhelming evidence that non-baryonic dark matter constitutes ∼ 27% of the energy...

Searching for New Physics with the Fermi Large Area Telescope

Johnson, Arne Christian

January 2019

Compelling astronomical evidence suggests that a majority of the matter in the Universe, known as da...

FERMI-LAT SENSITIVITY AND CONSTRAINTS ON DARK MATTER SIGNAL FROM THE MILKY WAY HOST HALO AND ITS SUBSTRUCTURE

Anderson, Brandon

January 2012

Despite overwhelming evidence of its existence, the exact nature of Dark Matter (DM) remains unknown...

Search for Dark Matter Satellites using the FERMI-LAT

Ackermann, Markus
Albert, A.
Baldini, Luca
Ballet, Jean
Barbiellini, Guido
Bastieri, D.
Bechtol, K.
Bellazzini, R.
D. Blandford, R.
D. Bloom, E.
Bonamente, E.
W. Borgland, A.
Bottacini, E.
J. Brandt, T.
Bregeon, J.
Brigida, M.
Bruel, Pascal
Buehler, R.
H. Burnett, T.
A. Caliandro, G.
A. Cameron, R.
Caraveo, P. A.
M. Casandjian, J.
Cecchi, C.
Charles, E.
Chiang, J.
Ciprini, S.
Claus, R.
Cohen-Tanugi, J.
Conrad, J.
Cutini, S.
de Palma, F.
D. Dermer, C.
W. Digel, S.
Do Couto E Silva, E.
S. Drell, P.
Drlica-Wagner, A.
Essig, R.
Falletti, L.
Favuzzi, C.
J. Fegan, S.
B. Focke, W.
Fukazawa, Y.
Funk, S.
Fusco, P.
Gargano, F.
Germani, S.
Giglietto, N.
Giordano, F.
Giroletti, M.
Glanzman, T.
Godfrey, G.
A. Grenier, I.
Guiriec, S.
Gustafsson, M.
Hadasch, D.
Hayashida, M.
Hou, X.
E. Hughes, R.
P. Johnson, R.
S. Johnson, A.
Kamae, T.
Katagiri, H.
Kataoka, J.
Knödlseder, Jürgen
Kuss, M.
Lande, J.
Latronico, L.
Lee, S.-H.
M. Lionetto, A.
Llena Garde, M.
Longo, F.
Loparco, F.
N. Lovellette, M.
Lubrano, P.
N. Mazziotta, M.
E. Mcenery, J.
F. Michelson, P.
Mitthumsiri, W.
Mizuno, T.
A. Moiseev, A.
Monte, C.
E. Monzani, M.
Morselli, A.
V. Moskalenko, I.
Murgia, S.
Naumann-Godo, M.
P. Norris, J.
Nuss, E.
Ohsugi, T.
Okumura, A.
Orlando, E.
F. Ormes, J.
Ozaki, M.
Paneque, D.
Pelassa, V.
Pierbattista, M.
Piron, F.
Pivato, G.
Porter, T.A.
Rain'O, S.
Rando, R.
Razzano, M.
Reimer, A.
Reimer, O.
Ritz, S.
F.-W. Sadrozinski, H.
Sehgal, N.
Sgr'O, C.
J. Siskind, E.
Spinelli, P.
Strigari, L.
J. Suson, D.
Tajima, H.
Takahashi, H.
Tanaka, T.
G. Thayer, J.
B. Thayer, J.
Tibaldo, L.
Tinivella, M.
F. Torres, D.
Troja, E.
Uchiyama, Y.
L. Usher, T.
Vandenbroucke, J.
Vasileiou, V.
Vianello, G.
Vitale, V.
P. Waite, A.
Wang, P.
L. Winer, B.
S. Wood, K.
Yang, Z.
Zalewski, S.
Zimmer, S.

January 2012

Numerical simulations based on the Lambda-CDM model of cosmology predict a large number of as yet un...

Search for Dark Matter Satellites Using the FERMI-LAT

Ackermann, M.
/DESY
Albert, A.
U., /Ohio State
Baldini, L.
/INFN, Pisa
Ballet, J.
/DAPNIA, Saclay
Barbiellini, G.
/INFN, Trieste /Trieste U.
Bastieri, D.
/INFN, Padua /Padua U.
Bechtol, K.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bellazzini, R.
/INFN, Pisa
Blandford, R.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bloom, E.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /SLAC
Bonamente, E.
/INFN, Perugia /Perugia U.
Borgland, A.W.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bottacini, E.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Brandt, T.J.
/IRAP, Toulouse /Toulouse III U.
Bregeon, J.
/INFN, Pisa
Brigida, M.
/Bari U. /INFN, Bari
Bruel, P.
Polytechnique, /Ecole
Buehler, R.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Burnett, T.H.
/Washington U., Seattle
Caliandro, G.A.
/ICE, Bellaterra
Cameron, R.A.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /IASF, Milan /IASF, Milan /DAPNIA, Saclay /INFN, Perugia /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /ASDC, Frascati /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Stockholm U. /Stockholm U., OKC /ASDC, Frascati /Bari U. /INFN, Bari /Naval Research Lab, Wash., D.C. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Bari U. /INFN, Bari /Ecole Polytechnique /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Hiroshima U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Bari U. /INFN, Bari /INFN, Bari /INFN, Perugia /Perugia U. /Bari U. /INFN, Bari /Bari U. /INFN, Bari /Bologna Observ. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
authors.., /more

August 2012

Numerical simulations based on the {Lambda}CDM model of cosmology predict a large number of as yet u...

Search for Dark Matter Satellites using the FERMI-LAT

Ackermann, Markus
Albert, A.
Baldini, Luca
Ballet, Jean
Barbiellini, Guido
Bastieri, D.
Bechtol, K.
Bellazzini, R.
D. Blandford, R.
D. Bloom, E.
Bonamente, E.
W. Borgland, A.
Bottacini, E.
J. Brandt, T.
Bregeon, J.
Brigida, M.
Bruel, Pascal
Buehler, R.
H. Burnett, T.
A. Caliandro, G.
A. Cameron, R.
Caraveo, P. A.
M. Casandjian, J.
Cecchi, C.
Charles, E.
Chiang, J.
Ciprini, S.
Claus, R.
Cohen-Tanugi, J.
Conrad, J.
Cutini, S.
de Palma, F.
D. Dermer, C.
W. Digel, S.
Do Couto E Silva, E.
S. Drell, P.
Drlica-Wagner, A.
Essig, R.
Falletti, L.
Favuzzi, C.
J. Fegan, S.
B. Focke, W.
Fukazawa, Y.
Funk, S.
Fusco, P.
Gargano, F.
Germani, S.
Giglietto, N.
Giordano, F.
Giroletti, M.
Glanzman, T.
Godfrey, G.
A. Grenier, I.
Guiriec, S.
Gustafsson, M.
Hadasch, D.
Hayashida, M.
Hou, X.
E. Hughes, R.
P. Johnson, R.
S. Johnson, A.
Kamae, T.
Katagiri, H.
Kataoka, J.
Knödlseder, Jürgen
Kuss, M.
Lande, J.
Latronico, L.
Lee, S.-H.
M. Lionetto, A.
Llena Garde, M.
Longo, F.
Loparco, F.
N. Lovellette, M.
Lubrano, P.
N. Mazziotta, M.
E. Mcenery, J.
F. Michelson, P.
Mitthumsiri, W.
Mizuno, T.
A. Moiseev, A.
Monte, C.
E. Monzani, M.
Morselli, A.
V. Moskalenko, I.
Murgia, S.
Naumann-Godo, M.
P. Norris, J.
Nuss, E.
Ohsugi, T.
Okumura, A.
Orlando, E.
F. Ormes, J.
Ozaki, M.
Paneque, D.
Pelassa, V.
Pierbattista, M.
Piron, F.
Pivato, G.
Porter, T.A.
Rain'O, S.
Rando, R.
Razzano, M.
Reimer, A.
Reimer, O.
Ritz, S.
F.-W. Sadrozinski, H.
Sehgal, N.
Sgr'O, C.
J. Siskind, E.
Spinelli, P.
Strigari, L.
J. Suson, D.
Tajima, H.
Takahashi, H.
Tanaka, T.
G. Thayer, J.
B. Thayer, J.
Tibaldo, L.
Tinivella, M.
F. Torres, D.
Troja, E.
Uchiyama, Y.
L. Usher, T.
Vandenbroucke, J.
Vasileiou, V.
Vianello, G.
Vitale, V.
P. Waite, A.
Wang, P.
L. Winer, B.
S. Wood, K.
Yang, Z.
Zalewski, S.
Zimmer, S.

January 2012

Numerical simulations based on the Lambda-CDM model of cosmology predict a large number of as yet un...

Search for Dark Matter Satellites Using the FERMI-LAT

Ackermann, M.
/DESY
Albert, A.
U., /Ohio State
Baldini, L.
/INFN, Pisa
Ballet, J.
/DAPNIA, Saclay
Barbiellini, G.
/INFN, Trieste /Trieste U.
Bastieri, D.
/INFN, Padua /Padua U.
Bechtol, K.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bellazzini, R.
/INFN, Pisa
Blandford, R.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bloom, E.D.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /SLAC
Bonamente, E.
/INFN, Perugia /Perugia U.
Borgland, A.W.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Bottacini, E.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Brandt, T.J.
/IRAP, Toulouse /Toulouse III U.
Bregeon, J.
/INFN, Pisa
Brigida, M.
/Bari U. /INFN, Bari
Bruel, P.
Polytechnique, /Ecole
Buehler, R.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
Burnett, T.H.
/Washington U., Seattle
Caliandro, G.A.
/ICE, Bellaterra
Cameron, R.A.
/Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /IASF, Milan /IASF, Milan /DAPNIA, Saclay /INFN, Perugia /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /ASDC, Frascati /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Stockholm U. /Stockholm U., OKC /ASDC, Frascati /Bari U. /INFN, Bari /Naval Research Lab, Wash., D.C. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Montpellier U. /Bari U. /INFN, Bari /Ecole Polytechnique /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Hiroshima U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Bari U. /INFN, Bari /INFN, Bari /INFN, Perugia /Perugia U. /Bari U. /INFN, Bari /Bari U. /INFN, Bari /Bologna Observ. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.
authors.., /more

August 2012

Numerical simulations based on the {Lambda}CDM model of cosmology predict a large number of as yet u...

Indirect Searches for Dark Matter with the Fermi Large Area Telescope1

Abstract

Extracted data

Indirect Searches for Dark Matter with the Fermi Large Area Telescope1

Abstract

Extracted data

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