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

Miosotys data scheme 2010

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)

20100228 TNO01_01 XRB01_01
20100301 TNO01_01 XRB01_01
20100521 CVO01_01
20100523 CVO01_01 WDO01_01
20100524 CVO01_01 WDO02_01
20100525 TNO01_01
20101020 TNO02_01 WDO01_01
20101021 TNO02_01 WDO01_01
20101022 WDO02_01
20101023 CVO01_01
20101024 TNO03_01
20101202 CVO02_01 TNO01_01
20101203 CVO02_01 TNO01_01
20101204 CVO02_01 TNO02_01