P F Michelson
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Explore the profile of P F Michelson including associated specialties, affiliations and a list of published articles.
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Articles
34
Citations
90
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Recent Articles
11.
Preece R, Burgess J, von Kienlin A, Bhat P, Briggs M, Byrne D, et al.
Science
. 2013 Nov;
343(6166):51-4.
PMID: 24263132
Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 seconds is possibly the brightest well-isolated pulse observed to date. A...
12.
Ackermann M, Ajello M, Allafort A, Baldini L, Ballet J, Barbiellini G, et al.
Science
. 2013 Feb;
339(6121):807-11.
PMID: 23413352
Cosmic rays are particles (mostly protons) accelerated to relativistic speeds. Despite wide agreement that supernova remnants (SNRs) are the sources of galactic cosmic rays, unequivocal evidence for the acceleration of...
13.
Ackermann M, Ajello M, Allafort A, Schady P, Baldini L, Ballet J, et al.
Science
. 2012 Nov;
338(6111):1190-2.
PMID: 23118013
The light emitted by stars and accreting compact objects through the history of the universe is encoded in the intensity of the extragalactic background light (EBL). Knowledge of the EBL...
14.
Pletsch H, Guillemot L, Fehrmann H, Allen B, Kramer M, Aulbert C, et al.
Science
. 2012 Nov;
338(6112):1314-7.
PMID: 23112297
Millisecond pulsars, old neutron stars spun up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled"...
15.
Measurement of separate cosmic-ray electron and positron spectra with the fermi large area telescope
Ackermann M, Ajello M, Allafort A, Atwood W, Baldini L, Barbiellini G, et al.
Phys Rev Lett
. 2012 Feb;
108(1):011103.
PMID: 22304252
We measured separate cosmic-ray electron and positron spectra with the Fermi Large Area Telescope. Because the instrument does not have an onboard magnet, we distinguish the two species by exploiting...
16.
Fermi LAT Collaboration , Ackermann M, Ajello M, Ballet J, Barbiellini G, Bastieri D, et al.
Science
. 2012 Jan;
335(6065):189-93.
PMID: 22246769
Gamma-ray binaries are stellar systems containing a neutron star or black hole, with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution...
17.
Ackermann M, Ajello M, Albert A, Atwood W, Baldini L, Ballet J, et al.
Phys Rev Lett
. 2012 Jan;
107(24):241302.
PMID: 22242987
Satellite galaxies of the Milky Way are among the most promising targets for dark matter searches in gamma rays. We present a search for dark matter consisting of weakly interacting...
18.
Ackermann M, Ajello M, Allafort A, Baldini L, Ballet J, Barbiellini G, et al.
Science
. 2011 Nov;
334(6059):1103-7.
PMID: 22116880
The origin of Galactic cosmic rays is a century-long puzzle. Indirect evidence points to their acceleration by supernova shockwaves, but we know little of their escape from the shock and...
19.
Abdo A, Ackermann M, Ajello M, Allafort A, Baldini L, Ballet J, et al.
Science
. 2011 Jan;
331(6018):739-42.
PMID: 21212321
A young and energetic pulsar powers the well-known Crab Nebula. Here, we describe two separate gamma-ray (photon energy greater than 100 mega-electron volts) flares from this source detected by the...
20.
Abdo A, Ackermann M, Ajello M, Atwood W, Baldini L, Ballet J, et al.
Science
. 2010 Aug;
329(5993):817-21.
PMID: 20705855
Novae are thermonuclear explosions on a white dwarf surface fueled by mass accreted from a companion star. Current physical models posit that shocked expanding gas from the nova shell can...