Spectrum
The reduction pipeline v2 produces two output fits files. The main output of the reduction pipeline is a spectrum and this is stored in a fits file (Sci_...sp_ech_main.fits). The fits
file has two extensions. In the first extension, only the image header is contained with informations for and from the reduction. In the second extension, the data are stored as a
binary table with an own header. The format of this table is:
Name |
Dimension |
Description |
WAVE |
(Pixel, Relative order) |
Wavelength array of each order |
SPEC_BLZ |
(Pixel, Relative order) |
Blaze normalised spectrum of each order |
BLAZE |
(Pixel, Relative order) |
Blaze function (flat field spectrum) of each order |
SIG |
(Pixel, Relative order) |
Signal to noise of each order |
SPEC_NORM |
(Pixel, Relative order) |
Normalised spectrum of each order |
WAVE_MERG |
(Pixel) |
Merged wavelength |
SPEC_MERG |
(Pixel) |
Merged blaze normalised spectrum |
F_SPEC_MERG |
(Pixel) |
Error of the merged blaze normalised spectrum |
SPEC_MERG_NORM |
(Pixel) |
Merged normalised spectrum |
F_SPEC_MERG_NORM |
(Pixel) |
Error of the merged normalised spectrum |
INST_RESP_FUNC |
(Pixel) |
Instrumental response function |
RESPONCE_CURVE_DAY_VAR |
(Pixel) |
Correction of the small scale variations in the spectrum |
for a spectrum with one exposure and for spectrum with multi exposures with a very low S/N in the single exposure.
For a spectrum based on multi exposures, the format is:
Name |
Dimension |
Description |
WAVE |
(Pixel, Relative order) |
Wavelength array of each order |
SPEC_BLZ |
(Pixel, Relative order) |
Blaze normalised spectrum of each order |
BLAZE |
(Pixel, Relative order) |
Blaze function (flat field spectrum) of each order |
SIG |
(Pixel, Relative order) |
Signal to noise of each order |
SPEC_NORM |
(Pixel, Relative order) |
Normalised spectrum of each order |
SINGLE_OBS_SPEC |
(Spectrum,Pixel, Relative order) |
Array with the single spectrum of each order |
WAVE_MERG |
(Pixel) |
Merged wavelength |
SPEC_MERG |
(Pixel) |
Merged blaze normalised spectrum |
F_SPEC_MERG |
(Pixel) |
Error of the merged blaze normalised spectrum |
SPEC_MERG_NORM |
(Pixel) |
Merged normalised spectrum |
F_SPEC_MERG_NORM |
(Pixel) |
Error of the merged normalised spectrum |
INST_RESP_FUNC |
(Pixel) |
Instrumental response function |
RESPONCE_CURVE_DAY_VAR |
(Pixel) |
Correction of the small scale variations in the spectrum |
The secondary output is a small fits file. The notation is Sci_...sp_ech_small.fits. This file include only the blaze normalised spectrum.
This file is readable in IRAF or in FV without problems.
If one use the IDL read procedure readheros.pro than is the output a table with the columns wavelength and flux.
The format of the pipline v1 output one can find
here.