Main Page V1
This is the start page for the CMB-S4 wiki
- 1 Slides for CMB-S4 Telecon October 13, 2017
- 2 CMB-S4 Interim Collaboration Coordination Committee (ICCC)
- 3 CMB-S4 Concept Definition Task Force
- 4 Collaboration Voting
- 5 Mailing Lists
- 6 GitHub Repositories
- 7 CMB-S4 Science Book
- 8 CMB-S4 Instrument Technical Papers
- 9 Workshops
- 10 CMB-S4 Presentations
- 11 Simulation Products and Forecasting:
- 12 Logbooks and Notes
Slides for CMB-S4 Telecon October 13, 2017
CMB-S4 Interim Collaboration Coordination Committee (ICCC)
From now until approximately March, 2018, the Interim Collaboration Coordination Committee (ICCC) for CMB-S4 will coordinate the activities of the Working Groups formed to work on collaboration bylaws and technical and science efforts. The ICCC will work to facilitate cross-group communications, help coordinate schedules and milestones for the Working Groups, and prepare preliminary documents for ratification by the full S4 collaboration. The goal date for ratification is March, 2018. The ICCC will meet periodically with representatives from the DOE and NSF to keep them updated on progress and to receive their input and advice. The ICCC has 15 members (see link to list below); the co-chairs are John Carlstrom and Suzanne Staggs. If you have input or questions about the ICCC work, you may email the entire ICCC using s4-iccc_at_box.uchicago.edu, or individual members (included in the list linked below). The ICCC will disband once the governance bylaws are ratified and its successor has been established.
CMB-S4 Concept Definition Task Force
In December 2016 the NSF-NASA-DOE Astronomy and Astrophysics Advisory Committee (AAAC) established an Cosmic Microwave Background Stage 4 Concept Definition Task Force (CMB-S4 CDT) as a subcommittee to develop a concept for implementing a ground-based CMB-S4 experiment. (Link to NSF CDT site.)
List of S4 Registered Voters as of 1 Sept 2017: File:S4-Voter-Registration-final-20170901-for-display-v1.pdf
As agreed upon at the Aug 2017 Workshop, the Interim Collaboration Coordination Committee (ICCC) for the S4 will coordinate the activities of the Working Groups formed to work on collaboration bylaws and technical and science efforts. The ICCC will have 15 members. S4 registered voters will choose 7 members, and the remaining members will be appointed by the S4 Workshops Science Organizing Committee to ensure diversity on the ICCC, including career experience, institutional sizes, projects, locations of institutions, etc. The ICCC will elect its own chair, and other positions as needed (like deputy chair and secretary). The ICCC will disband once the governance bylaws are ratified.
Table of S4 ICCC Self Nominations: File:S4-ICCC-Self-Nominations-final-20170901-for-display.pdf
To sign up for the main CMB-S4 email list, go to this page: CMB-S4 main mailing list sign-up page.
CMB-S4 Science Book
The purpose of Science Book is to set the scientific goals for CMB-S4 and specify the measurements needed to achieve them, which will then be translated into the instrument requirements. This will set the stage for defining the instrument.
- The First Edition of CMB-S4 Science Book is posted on the arXiv and also available here: File:CMB-S4 ScienceBook 1stEdition arxiv version.pdf
The history of posted Science Book drafts can be found here: CMB-S4 Science Book Comments.
The Concept Definition Task Force has been tasked with writing down science requirements, with three suggested levels (sky's the limit, minimum worth doing, something in between). John C. has, in turn, asked the Science Book chapter leads to create a summary table of requirements from the book. A workbook / dialog for putting that table together is here: Putting Together the CMB-S4 Science Book Requirements Table.
CMB-S4 Instrument Technical Papers
Goal of CMB-S4 instrument technical papers are to summarize the current state of the technology and identify R\&D efforts necessary to advance it for possible use in CMB-S4. CMB-S4 will require a scale-up in number of elements, frequency coverage, and bandwidth relative to current instruments. Because it is searching for lower magnitude signals, it will also require stronger control of systematic uncertainties.
- UMICH-2015: Cosmology with CMB-S4 workshop at the University of Michigan September 21-22, 2015
- LBNL-2016: Cosmology with CMB-S4 workshop at LBNL, Berkeley CA March 7-9, 2016
- UChicago-2016: Cosmology with CMB-S4 workshop at the University of Chicago, September 19-20, 2016.
- SLAC-2017: Cosmology with CMB-S4 workshop at the SLAC National Accelerator Laboratory, Feb. 27-28, 2017 (March 1 additional meetings)
- Harvard-2017: Cosmology with CMB-S4 workshop at Harvard University, Aug. 24-25, 2017.
Post your CMB-S4 talks on the page linked here.
Simulation Products and Forecasting:
- r forecast telecon notes
- r forecast results summary spreadsheet
- Data Challenges
- Wish List and Existing Capability for Simulated Maps
- Simulation and Forecasting Logbook