At the Chicago meeting it was agreed that it would be useful to provide common inputs for all science forecasting, to include extra-galactic foreground, galactic foreground and noise maps at a range of frequencies. It was further agreed that, in order to support the widest range of uses, these would be provided as all-sky HEALPix maps at Nside-8192.
Possible sky-model inputs are:
- Extra-galactice: Alvarez/Battaglia/Bond, PSM
- Galactic: pySM, PSM
Please add to these lists as appropriate.
Inputs will be hosted at NERSC, where everyone is welcome to sign-up for an account under the "Data Analysis for Post-Planck CMB Experiments" allocation (PI Borrill). The files will then be located in the shared CMB-S4 file space (/project/projectdirs/cmbs4). In order to manage this space, all files stored there should be owned by the cmbs4 project account but accessible to the cmbs4 group. To do this:
- log in to the cmbs4 project account following the instructions [here]
- sync the files to an appropriate subdirectory in the project space
- ensure that the permissions are set appropriately (g+rX,o-rwx)
Remember to include a README and to post the details on this wiki page.
For any NERSC issues, including access to the filegroup and/or project account, please contact Julian Borrill.
- 1 Data Challenge 1
Data Challenge 1
Intended as a simple test to develop our practice, compare spectral- and map-based forecasting, contrast different map-based codes and methods, and coordinate r and non-r science forecasting.
|Beam FWHM (arcmin)||76.6||57.5||27.0||24.2||15.9||14.8||10.7||8.5|
- Tophat bandpasses described in this posting, added to above table --Cbischoff (talk) 15:51, 8 November 2016 (UTC)
- Beam widths copied from Victor's posting here --Cbischoff (talk) 19:20, 14 December 2016 (UTC)
Scalar, tensor & non-Gaussian CMB: Borrill
- Planck cosmology + interesting values of r, f_NL
Extragalactic foregrounds: Alvarez / Battaglia / Bond / Stein
Galactic foregrounds: pySM / Ben
- Nside 512 maps with delta-function bandpasses delivered at 20, 25, 30, 35, 40, 45, 50, 60, 70, 80, 85, 90, 95, 100, 120, 140, 145, 150, 155, 165, 195, 215, 220, 235, 245, 270, 280, 340, 350, 400, 545, 860 GHz (CMB-S4 + S3, WMAP, Planck & LiteBIRD frequencies)
Noise: homogeneous isotropic matched to N_ell: Victor / Clem / Colin / John K
Masks: Clem / John K
- Using BICEP/Keck apodization mask (fsky ~ 1%) shown in fourth figure here
- Dec 7: Beta version of Phase 1 maps
- Dec 14: Telecon
- Dec 17: Noise power (N_ell) prescriptions to Clem from Victor and Colin
- Dec 21: A few realizations of Phase 1 maps delivered by Clem
- Dec 21: Telecon (note phase shift)
- Jan 4: Telecon
- Jan 18: Telecon
- Feb 1: Telecon
- Feb 15: Telecon
- Feb 27, 28, Mar 1: S4 general meeting at SLAC
- Mar 2, 3: S4 CDT meeting at SLAC