LAMOST DR6 Low Resolution Spectra

A machine-readable interface to the LAMOST6 low resolution spectra based on SSAP and datalink.
ICRS position of target object
Size of the region of interest around POS
Wavelength (range) of interest (or symbolic bandpass names)
Midpoint of exposure (MJD)
MIME type of the file served
Angular diameter of aperture
Signal-to-noise ratio estimated for this dataset
Redshift of target object
Common name of object observed.
Object class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)
Date last published.
Type of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).
Spatial resolution of data
Type of wavelength calibration
A short handle naming the collection this spectrum belongs to.
Lower limit to spectral resolution power (λ/Δλ) as a single number.
Dataset identifier assigned by the publisher
Dataset identifier assigned by the creator
Shell pattern of target observed (case insensitive)
Shell pattern of target observed (case sensitive)
This is queryData for the default operation; some services support getData as well
Only return the TOP "best" records (on this service, this usually is equivalent to MAXREC, so no ranking is implied).
Return compressed results?
An identifier for a certain run. Opaque to the service
Sort by
Limit to items.
[Result link] [bookmark]

Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences.

Please also see the LAMOST Data Policy.