Difference: CosmoTelecon20191113 ( vs. 1)

Revision 12019-11-20 - SuhailDhawan

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META TOPICPARENT name="CosmoTelecons"

Agenda

1. Discussion on the timeline of the analysis

2. Update on the calibration

-- Suhail Dhawan - 2019-11-20

Minutes

Google doc on the analysis pipeline:

https://docs.google.com/document/d/15bOoLY1IuPSw6OxpR5VUc_80lseKcYJs2anpUJLv18I/edit?usp=sharing

  • Bright transient survey year 1 is a good starting point. 335 SNe with i-band; 77 with > 15 pre-explosion images
  • Coadds with background rms calculated: Notebook on snova02
  • Difference imaging with hotpants
  • Run SALT2 on the lightcurves with outlier rejection (or not?) Rahul has the machinery.
  • Not using BBC, derive survey parameters from SimSurvey
Simeon gave an update on the calibration. The difference between the median mag and Pan-Starrs is correlated with the lunar phase.

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