LESIA Observatoire de Paris-PSL CNRS Sorbonne Université Université de Paris

Miosotys data scheme 2011

mardi 5 juin 2012, par Morlot Hugo

MIOSOTYS data scheme

All the data are stored choronically with sub-dictionaries :

|— calib (inc. fibre-star assignment file for MEFOS, named as YYYYMM_ObsId.ASS.)
|— raw (all the original SPE images)
|— reduced (stores reduced images and lcs in FITS format)
|— ObsId_images
|— ObsId_(tag)_lcs (tag is a unique label for different photometric process, for example "gf06")

Each ObsId is uniquely corresponded to its ObsDate. The same ObsId in the different ObsDate DO NOT necessarily have the same target configuration. For example, 20110322_2_TNO02_01 could be different from 20110323_2_TNO02_01, where "_2_" affix designates that the data is hardware binned by factor of 2. For each observation, its unique identification is to combine both ObsDate and ObsId.

ObsDate ObsId(s)

20110321 TNO01_01 TNO02_01
20110322 TNO02_01 TNO04_01
20110323 TNO02_01 TNO05_01
20110324 TNO02_01 TNO05_01
20111214 TNO05_01
20111215 TNO01_01
20111216 TNO05_01 TNO08_01
20111217 TNO05_01 TNO08_01
20111218 TNO05_01 TNO08_01
20111219 TNO05_01 TNO08_01