The Arcetri Spectral Code binned line emission files format
Each emissivity line is structured using the following format:
(f11.1,41e13.4)
An example from the Ne=10^10 file (phot cm^3 s^-1) is given below:
1550.0 3.8815e-18 2.2909e-17 6.9024e-17 5.6234e-17 2.2751e-17 ...
with the following meaning:
1550.0
: Wavelength (Å) of the spectral bin;
3.8815e-18
: Emissivity in phot cm^3 s^-1 for
Log T = 4.0
;
2.2909e-17
: Emissivity in phot cm^3 s^-1 for
Log T = 4.1
;
6.9024e-17
: Emissivity in phot cm^3 s^-1 for
Log T = 4.2
;
5.6234e-17
: Emissivity in phot cm^3 s^-1 for
Log T = 4.3
;
2.2751e-17
: Emissivity in phot cm^3 s^-1 for
Log T = 4.4
;
...
: The series of emissivities is reported up to
Log T = 8.0
, with
Log T = 0.1
steps.
The format of the emissivity files in erg cm^3 s-1 is identical to this one.
Informations about the transitions in each spectral bin (wavelengths, identifications, type, etc...) can be found in the
Line list
(text)
Page created and maintained by E. Landi.
Mail comments regarding interface to
enricol@arcetri.astro.it
Mail comments regarding spectrum data to
mlandini@arcetri.astro.it, enricol@arcetri.astro.it