The vmspphot recipe

vmspphot

Synopsis

Apply to IFU or MOS 1D-extracted spectra a flux correction.

Description

This recipe can be used to apply a spectro-photometric flux calibration to any number of 1D-extracted spectral frames generated by the recipes vmmosobsstare, vmmosobsjitter, and vmifuscience.

Input files

DO category:                Type:       Explanation:            Required:
MOS_SCIENCE_REDUCED
or IFU_SCIENCE_REDUCED      Product     Extracted MOS or IFU spectra Y
EXTINCT_TABLE               Calib       Atmospheric extinction       Y
MOS_SPECPHOT_TABLE
or IFU_SPECPHOT_TABLE       Calib       Response curve               .

Output files

DO category:                Data type:  Explanation:
MOS_SCIENCE_FLUX_REDUCED
or IFU_SCIENCE_FLUX_REDUCED FITS image  Flux calibrated objects spectra

For more details, please refer to the VIMOS Pipeline User’s Guide.

Constructor

cpl.Recipe("vmspphot")

Create an object for the recipe vmspphot.

import cpl
vmspphot = cpl.Recipe("vmspphot")

Parameters

vmspphot.param.ApplyResponse

Apply instrument response. (bool; default: True) [default=True].

The following code snippet shows the default settings for the available parameters.

import cpl
vmspphot = cpl.Recipe("vmspphot")

vmspphot.param.ApplyResponse = True

You may also set or overwrite some or all parameters by the recipe parameter param, as shown in the following example:

import cpl
vmspphot = cpl.Recipe("vmspphot")
[...]
res = vmspphot( ..., param = {"ApplyResponse":True})

See also

cpl.Recipe for more information about the recipe object.

Bug reports

Please report any problems to ESO VIMOS Pipeline Team. Alternatively, you may send a report to the ESO User Support Department.