The formal meeting starts at 9 am. All talks unless notes are marked by * which means 45=15+10+10+10 I quote from Homework 2 Leads should feel free to expand or contract the manifesto assgined to them. Each lead is responsible for a total of 45 minutes broken as follows: a 15 minute (uninterruped) presentation of the major science goals, 10 minutes of discussion, 10 minutes (uninterrupted) of suggested projects and then 10 minutes of open discussion. The chair of the session will be asked to strictly follow the schedule.
0900 Welcome & initial remarks: Kawai, Kulkarni, Suzuki (10)
0910
Landscape of Time Domain Surveys: Kulkarni (10+10)
0930 DESI & Spare Fibers: Peter Nugent (30+15) (discussion;
no presentation)
1015
Redshift completeness of current galaxy samples:
Fremling (*)
1100 Coffee break
1115
Peculiar velocity survey:
AKim (*)
1230 Lunch
1330
Distribution of local matter on BAO scale:
Suzuki (*)
1415
Towards an accurate rate of Core-collapse SNe:
Tanaka & De (*)
1500
Search of BH via Microlensing:
Dawson (*)
1545 Break
1600
Search for BH via other approaches (ellipsoidal mod, RV):
Mao (*)
1645
Discussion: Spectrometers tuned classification, Konidaris (30)
1715
TDA with TESS Michael Fausnaugh, MIT (talk given by SRK) [15]
1730 End (onsen time!)
1900 Dinner at Senhime
Onsen time!
1000
Tomo-e-Gozen:
Tanaka (10+5)
1015
Dark Energy Camera Surveys:
Dawson (10+5)
1030
Chinese Supernova Surveys:
Wang (10+5)
1045
Zwicky Coaddition Facility: Goldstein (10+5)
1100
Progenitors of SN - early observations:
Tominaga & Ho (*)
1145
Exploring extra-galactic explosions phase space:
Moriya & Maeda (*)
1230 lunch
1330
Discussion- SRG in the era of TDA & MMS
[Rau] (20)
1350
Discussion- Leave no TDE behind
(Blagorodnova) (20)
1410
Discussion- Tomo-e Gozen & Follow up [Jiang, Maeda] (20)
1430
Discussion- Near IR TDA [De] (20)
1450
Discussion- TDA+MMS and GW astronomy [Tanaka] (20)
1510 Break
1530 Discussion: Kawai, Konidaris, Nugent, Suzuki, Yasuda
Rush to Nikko station (Express train to Tokyo leaves at 5:23p)