TY  - CHAP
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
AB  - 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).
DO  - 10.5772/36580
ID  - OAPEN ID: 612622
ID  - OAPEN ID: OCN: 1030819426
KW  - spherical
KW  - poisson noise removal
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
L1  - https://library.oapen.org/bitstream/id/092ee899-6a11-47e8-9dfc-b37ea98056e9/612622.pdf
LA  - English
LK  - http://library.oapen.org/handle/20.500.12657/32329
PB  - InTechOpen
PY  - 2012
TI  - Chapter 9 Poisson Noise Removal in Spherical Multichannel Images: Application to Fermi Datanull
ER  - 
