Paolo Giommi

Dr. Paolo Giommi

orcid

Research Focus & Metrics

Academic Career Length

43Years (1984-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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20 August 2004 in The Astrophysical Journal
Verified
Journal Article
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NGN. Gehrels
N. Gehrels
GCG. Chincarini
G. Chincarini
PGPaolo Giommi
Paolo Giommi
KMK. O. Mason
K. O. Mason
JNJ. A. Nousek
J. A. Nousek
WZW. W. Zhang
W. W. Zhang

8 May 2009 in The Astrophysical Journal
Verified
Journal Article
Closed access
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WAW. B. Atwood
W. B. Atwood
AAA. A. Abdo
A. A. Abdo
MAM. Ackermann
M. Ackermann
WAW. Althouse
W. Althouse
BAB. Anderson
B. Anderson
MZM. Ziegler
M. Ziegler

1 October 2005 in Space Science Reviews
Verified
Journal Article
Closed access
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DBDavid N. Burrows
David N. Burrows
JHJ. E. Hill
J. E. Hill
JNJ. A. Nousek
J. A. Nousek
JKJ. A. Kennea
J. A. Kennea
AWA. Wells
A. Wells
GHG. D. Hartner
G. D. Hartner

30 May 2013 in The Astrophysical Journal
Verified
Journal Article
Open access
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FHFiona A. Harrison
Fiona A. Harrison
WCWilliam W. Craig
William W. Craig
FCFinn E. Christensen
Finn E. Christensen
CHCharles J. Hailey
Charles J. Hailey
WZWilliam W. Zhang
William W. Zhang
CUC. Megan Urry
C. Megan Urry

12 June 2015 in The Astrophysical Journal Supplement Series
Verified
Journal Article
Open access
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FAF. Acero
F. Acero
MAM. Ackermann
M. Ackermann
MAM. Ajello
M. Ajello
AAA. Albert
A. Albert
WAW. B. Atwood
W. B. Atwood
SZS. Zimmer
S. Zimmer
We present a catalog of high-energy gamma-ray sources detected by the Large Area Telescope (LAT), the primary science instrument on the Fermi Gamma-ray Space Telescope (Fermi), during the first 11 months of the science phase of the mission, which began on 2008 August 4. The First Fermi-LAT catalog (1FGL) contains 1451 sources detected and characterized in the 100 MeV to 100 GeV range. Source detection was based on the average flux over the 11-month period, and the threshold likelihood Test Statistic is 25, corresponding to a significance of just over 4 sigma. The 1FGL catalog includes source location regions, defined in terms of elliptical fits to the 95% confidence regions and power-law spectral fits as well as flux measurements in 5 energy bands for each source. In addition, monthly light curves are provided. Using a protocol defined before launch we have tested for several populations of gamma-ray sources among the sources in the catalog. For individual LAT-detected sources we provide firm identifications or plausible associations with sources in other astronomical catalogs. Identifications are based on correlated variability with counterparts at other wavelengths, or on spin or orbital periodicity. For the catalogs and association criteria that we have selected, 630 of the sources are unassociated. Care was taken to characterize the sensitivity of the results to the model of interstellar diffuse gamma-ray emission used to model the bright foreground, with the result that 161 sources at low Galactic latitudes and toward bright local interstellar clouds are flagged as having properties that are strongly dependent on the model or as potentially being due to incorrectly modeled structure in the Galactic diffuse emission.

4 September 2014 in Experimental Astronomy
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Journal Article
Closed access
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HRH. Rauer
H. Rauer
CCC. Catala
C. Catala
CAC. Aerts
C. Aerts
TAT. Appourchaux
T. Appourchaux
WBW. Benz
W. Benz
KZK. Zwintz
K. Zwintz