TY - CHAP
T1 - DEMON: a proposal for a satellite-borne experiment to study dark matter and dark energy
AU - Berciano Alba, Alicia
AU - Borges de Silva, Pedro
AU - Eichelberger, Hans
AU - Giovacchini, Francesca
AU - Godolt, Mareike
AU - Hasinger, Günther
AU - Lerchster, Michael
AU - Lusset, Vincent
AU - Mattana, Fabio
AU - Mellier, Yannick
AU - Michalowski, Michal
AU - Monteserin-Sanchez, Carlos
AU - Noviello, Fabio
AU - Persson, Carina
AU - Santovincenzo, Andrea
AU - Schneider, Peter
AU - Zhang, Ming
AU - Östman, Linda
PY - 2006/7/1
Y1 - 2006/7/1
N2 - We outline a novel satellite mission concept, DEMON, aimed at advancing
our comprehension of both dark matter and dark energy, taking full
advantage of two complementary methods: weak lensing and the statistics
of galaxy clusters. We intend to carry out a 5000 deg2
combined IR, optical and X-ray survey with galaxies up to a redshift of
z~2 in order to determine the shear correlation function. We will also
find ~100000 galaxy clusters, making it the largest survey of this type
to date. The DEMON spacecraft will comprise one IR/optical and eight
X-ray telescopes, coupled to multiple cameras operating at different
frequency bands. To a great extent, the technology employed has already
been partially tested on ongoing missions, therefore ensuring improved
reliability.
AB - We outline a novel satellite mission concept, DEMON, aimed at advancing
our comprehension of both dark matter and dark energy, taking full
advantage of two complementary methods: weak lensing and the statistics
of galaxy clusters. We intend to carry out a 5000 deg2
combined IR, optical and X-ray survey with galaxies up to a redshift of
z~2 in order to determine the shear correlation function. We will also
find ~100000 galaxy clusters, making it the largest survey of this type
to date. The DEMON spacecraft will comprise one IR/optical and eight
X-ray telescopes, coupled to multiple cameras operating at different
frequency bands. To a great extent, the technology employed has already
been partially tested on ongoing missions, therefore ensuring improved
reliability.
U2 - 10.1117/12.670660
DO - 10.1117/12.670660
M3 - Chapter
VL - 6266
SP - 91
BT - Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray
ER -