z - KICP Workshops - University of Chicago
z - KICP Workshops - University of Chicago
z - KICP Workshops - University of Chicago
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AFTA and Euclid have complementary strengths for dark energy studies<br />
AFTA:<br />
Deep Infrared Survey (2000 sq. deg)<br />
Lensing:<br />
• High Resoluaon (70 -‐250 gal/arcmin 2 )<br />
• 5 lensing power spectrum<br />
Supernovae:<br />
• High quality IFU spectra <strong>of</strong> 2700 SN<br />
Redshio survey<br />
• High number density <strong>of</strong> galaxies<br />
• Redshio range extends to z = 3<br />
Euclid:<br />
Wide op3cal Survey (15000 sq. deg)<br />
Lensing:<br />
• Lower Resoluaon (30 gal/arcmin 2 )<br />
• 1 lensing power spectrum<br />
No supernovae program<br />
Redshio survey:<br />
• Low number density <strong>of</strong> galaxies<br />
• Significant number <strong>of</strong> low redshio galaxies<br />
Deep AFTA SURVEY (250) Wide AFTA SURVEY (70) Euclid (30 gal arcmin -‐2 -‐<br />
)<br />
More Accurate Dark MaMer Maps<br />
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