Campuses:
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| private:teleconsnotes20170712 [2017/07/12 16:53] – flauger | private:teleconsnotes20170712 [2017/07/19 13:02] (current) – hanany | ||
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| ====== Telecon Notes 20170712 ====== | ====== Telecon Notes 20170712 ====== | ||
| - | Attendance: \\ | + | Attendance: |
| Notes by: Raphael\\ | Notes by: Raphael\\ | ||
| + | === Actions === | ||
| + | * Finalize dates + time for Foregrounds workshop (Raphael) | ||
| + | * Communicate with Nobu, Mark/Bill re science workshop (Shaul) | ||
| + | === Workshops === | ||
| + | * Foregrounds | ||
| + | * Currently aiming for last week of October or first week of November | ||
| + | * Some rooms cost money. Shaul says to not worry about cost of rooms. | ||
| + | * Raphael says he would have time to finalize dates and rooms during the week of July 17, when he is back at San Diego | ||
| + | * Science + Complementarity | ||
| + | * Shaul talked with Mark. Some preference for May 2018 | ||
| + | * JB: Possibly coordinate with series of workshops for LiteBIRD? Previous workshops in 12/15 (Japan) and 1/17 (Montreal) Third workshop proposed around 1/18. Shaul suggested that they focus on technology or systematics, | ||
| + | * SH: Should workshops be endorsed by both teams? May not be good at this point? | ||
| + | * Shaul to communicate with Mark/Bill, and Nobu (LiteBIRD) | ||
| - | | + | === WG === |
| - | - Foregrounds | + | |
| - | - Currently aiming for last week of October or first week of November | + | * Slides posted |
| - | | + | |
| - | - Current target date is May 2018 | ||
| - | - JB: Possibly coordinate with series of workshops for LiteBIRD? Previous workshops in 12/15 (Japan) and 1/17 (Montreal) Third workshop proposed around 1/18 | ||
| - | - SH: Should workshops be endorsed by both teams? May not be good at this point? | ||
| - | | ||
| - | * Update from Fundamental Physics WG - Raphael | ||
| * Update from Extragalactic WG - Nick Battaglia | * Update from Extragalactic WG - Nick Battaglia | ||
| + | * Recently formed extragalactic science working group, currently 15 members (+pending) | ||
| + | * current approach: extragalactic science cases given CORE design | ||
| + | * Galaxy clusters: - finding clusters, cosmology, CIB and radio contamination, | ||
| + | * Galaxy formation at z > 2 - properties of star-formation (SF) during the peak of SF via the CIB | ||
| + | * Velocity fields - cosmology, contamination, | ||
| + | * Thermodynamic of galaxy formation - feedback, non-thermal pressure, ionized baryon content | ||
| + | * Reionization - Optical depth constraints, | ||
| + | * Gravitational lensing? Need to involve experts in lensing/ | ||
| + | * SH: what resolution is needed? at 150 GHz CMBP will not have 1' resolution. | ||
| + | * SH: What frequencies are important for cluster science? NB: up to 500-600 GHz | ||
| - | - Recently formed extragalactic science working group, currently 15 members (+pending) | + | === More on NASA slides (continuation from 2 weeks ago) === |
| - | - current approach: extragalactic science cases given CORE design | + | |
| - | - Galaxy clusters: - finding clusters, cosmology, CIB and radio contamination, | + | |
| - | - Galaxy formation at z > 2 - properties of star-formation (SF) during the peak of SF via the CIB | + | |
| - | - Velocity fields - cosmology, contamination, | + | |
| - | - Thermodynamic of galaxy formation - feedback, non-thermal pressure, ionized baryon content | + | |
| - | - Reionization - Optical depth constraints, | + | |
| - | - Gravitational lensing? Need to involve experts in lensing/ | + | |
| - | + | ||
| - | JM: Why are Planck beams not diffraction limited at high frequencies? | + | |
| - | BC: Not enough signal band width | + | |
| - | JM: Can we handle signal band width for diffraction limited beams at ~800 GHz? | + | |
| - | SH, NB: What is needed for cluster science? 500-600 GHz? | + | |
| - | + | ||
| - | * More on NASA slides (continuation from 2 weeks ago) - Shaul | + | |
| - | | + | |