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Plate MJD FiberID RUN2D RAplug Decplug Zpipe σZ Zwarning Class Subclass SNR EBOSS_TARGET1 Links
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Current redshift:         Adjust redshift: Scroll
window
Model Template: URL: rescale model:
Z_CONF_PERSON: Toggle plot elements:

CLASS_PERSON: NONE STAR GALAXY QSO QSO_BAL BLAZAR  EXTRAS:    
ISSUE: Smoothing:
COMMENTS:
GALEX DSS2 SDSS u SDSS gri PS1dr1 gri LSdr9 grz HSCdr2 grz 2MASS JHK VIKING Ks unWISE W1W2 VLASS 2-4GHz Zoom




Usage:

http://erosita-bhm.mpe.mpg.de/speccy/speccy.html?specfile={URL}
  (substitute URL of a valid speccy file)

Speccy File format:

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/Confidence matrix :

CLASS_PERSON Z_CONF_PERSON
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

Emission/absorption line list:

These are the lines that are plotted over the spectra.
Line Name Rest wavelength
(Å, vacuum)
Abs./Em.? Reference

Credits

This tool makes use of the legacysurvey.org viewer, and the hips2fits service provided by CDS.

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