ABOUT LAMBDA

Simulations Product Table

Simulations
Product Release Date Frequency [GHz] Stokes Description
High Resolution Microwave
Full Sky Simulations
2019 27,30,39,44,70,93,100,143
145,217,225,280,353
I Realistic, full-sky, HEALPix Nside=4096 (~1 arcmin) resolution simulations of the microwave sky.Modeled components include CMB, SZ, compact sources and diffuse Galactic emission. This is an update to the Sehgal/etal 2009 release and includes Simons Observatory forecasts. Simons Observatory Collaboration (2019)
High Resolution Microwave Full Sky Simulations 2009 30,90,148,219,277,350 I Realistic, full-sky, half-arcminute resolution simulations of the microwave sky. Modeled components include lensed and unlensed CMB, SZ, compact sources and dust emission. Sehgal et al. (2010)
TIGRESS Dust Emission Maps 2019 353 IQU Full-sky, HEALPix Nside=128 synthetic dust thermal emission maps computed for multiple time-steps and multiple observers within the solar neighborhood. Models are generated by numerical simulations that employ a multiphase, turbulent, magnetized interstellar medium (MHD code and TIGRESS ISM framework). Kim et al. (2019)

A service of the HEASARC and of the Astrophysics Science Division at NASA/GSFC
Goddard Space Flight Center, National Aeronautics and Space Administration
HEASARC Director: Dr. Alan P. Smale
LAMBDA Director: Dr. Eric R. Switzer
NASA Official: Dr. Eric R. Switzer
Web Curator: Mr. Michael R. Greason