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Current redshift: | Adjust redshift: |
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Model Template: | URL: rescale model: | |||||||||||||||||||||||||||||||
Z_CONF_PERSON: | Toggle plot elements: |
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CLASS_PERSON: | NONE STAR GALAXY QSO QSO_BAL BLAZAR | EXTRAS: | ||||||||||||||||||||||||||||||
ISSUE: | Smoothing: | |||||||||||||||||||||||||||||||
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http://erosita-bhm.mpe.mpg.de/speccy/speccy.html?specfile={URL}(substitute URL of a valid speccy file)
Speccy expects plain ASCII text files as input.
Header entries are prefixed by a hash+space and contain "key = value" pairs. e.g. '# PLATE = 1234'
The main body of the speccy file should contain five comma-separated columns
(with all fluxes in units 10-17 erg cm-2 s-1 Å-1):
Observed Vacuum Wavelength (Å), Flux, FluxError, SkyFlux, ModelFlux
Template files must contain (at least) two comma-separated columns:
Rest-frame Vacuum Wavelength (Å), ModelFlux (Fλ)
Note. Only the first two columns of template files are noticed, and so a regular Speccy spectrum file can be used as a template
CLASS_PERSON | Z_CONF_PERSON | |||
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0 | 1 | 2 | 3 | |
NONE | No vote | Bad Spectrum | No Signal | Continuum only |
STAR | Star_? | Star | ||
QSO | QSO_? | QSO_Z? | QSO | |
GALAXY | Galaxy_Z? | Galaxy | ||
QSO_BAL | QSO_BAL_Z? | QSO_BAL | ||
BLAZAR | BLAZAR_Z? | BLAZAR |
Line Name | Rest wavelength (Å, vacuum) |
Abs./Em.? | Reference |
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