TY  - GEN
AU  - Schmitt,Jérémy
AU  - Fadili,Jalal
AU  - Starck,Jean-Luc
AU  - Digel,Seth
AU  - Schmitt,Jérémy
AU  - Starck,Jean-Luc
AU  - Fadili,Jalal
AU  - Digel,Seth
TI  - Chapter 9 Poisson Noise Removal in Spherical Multichannel Images: Application to Fermi Data
SN  - 36580
PY  - 2012///
PB  - InTechOpen
KW  - Science: general issues
KW  - bicssc
KW  - spherical
KW  - poisson noise removal
KW  - Algorithm
KW  - Curvelet
KW  - Fermi Gamma-ray Space Telescope
KW  - Gamma ray
KW  - HEALPix
KW  - Shot noise
KW  - Standard deviation
KW  - Wavelet
N1  - Open Access
N2  - The Fermi Gamma-ray Space Telescope, which was launched by NASA in June 2008, is a powerful space observatory which studies the high-energy gamma-ray sky Atwood (2009).    Fermi's main instrument, the Large Area Telescope (LAT), detects photons in an energy range    between 20 MeV to greater than 300 GeV. The LAT is much more sensitive than its predecessor,    the EGRET telescope on the Compton Gamma Ray Observatory, and is expected to find    several thousand gamma-ray point sources, which is an order of magnitude more than its    predecessor EGRET Hartman et al. (1999)
UR  - https://library.oapen.org/bitstream/20.500.12657/32329/1/612622.pdf
UR  - https://library.oapen.org/bitstream/20.500.12657/32329/1/612622.pdf
UR  - https://library.oapen.org/bitstream/20.500.12657/32329/1/612622.pdf
UR  - https://directory.doabooks.org/handle/20.500.12854/29251
ER  -