Structure of the outputs¶
There are two different ways to get access to the data extracted from the images: from the Data
object or
from the files that are written to the disk, with the store_data()
function.
In memory¶
In order to access the data in memory, one can refer to the Data
documentation and Data
,
thus being able to find all that is necessary.
In Disk¶
There are two possible ways of storing data on disk: we either store data as a text file, whose structure does not allow for proper organization of the data, or a fits file. We shall now look into the structure of each one of them.
Text file¶
Fits file¶
-
create_fits
(master_folder, data_fits, **kwargs)¶ - Export the results to a fits file, containing the light curves and a correspondence of star to Cv and
- respective radius factor.
Parameters: - master_folder – Path in which the data shall be stored
- data_fits –
Data
object. - kwargs –
Notes
- Data stored in the header unit of the file :
Keyword data
method type of mask used detect tracking method initial initial detection method grid size of the background grid CDPP_TYPE CDPP algorithm in use
- In the data unit of the file, we have each star, with the corresponding
- time, rotation angle, flux values and uncertainties