Difference: CosmoTelecon20180822 (1 vs. 2)

References

• We should get references as soon as possible, 6 images would be fine.
• Only redo them when the field has set for the year.
• Make sure all i-band fields have been observed before the end of the season.

Spectroscopic followup

• Currently we are limited by SEDm selection, and the sample gets biased around z ~ 0.08
• We have a daily stream of summaries send to slack. Maybe someone in Stockholm should look into what SNe we missed and why
• Using this we can define a proper filter for target selection
• We may want to run a deeper observing campaign, using also LCO and ePESSTO, maybe going 19.5 mag
• We need to find a place to store the spectra (DESY will be the best choice)
• There are many more Ia's found by SEDm but in different programs. We need to move those into Cosmology group but can't always access them on the marshal, thus we need to save them ourselves.
• For now try scanning the AMPEL test channel and ultimately should be added automatically. (Will set up Doodle for that)

Agenda

• Reference images
• Spectroscopic followup (SNIFS, ePESSTO etc)
• Plans for/progress on first papers

Minutes

Connection:

https://zoom.us/j/272828651

Or iPhone one-tap (US Toll): +16468769923,,272828651# or +16699006833,,272828651#

Or Telephone: Dial: +1 646 876 9923 (US Toll) or +1 669 900 6833 (US Toll) Meeting ID: 272 828 651 International numbers available: https://zoom.us/zoomconference?m=yUACqd9q0rOg7icOHZs3wWcqWHdt5lib

-- UlrichFeindt - 21 Aug 2018