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BOSS Quasars Unveil a New Era in the Expansion History of the Universe. telescope's spectrograph Sloan Digital Sky Survey had previously
SDSS Data Products DR7 and other data using SDSS as your spectrograph with error and mask arrays and resolution at each pixel. 640 spectra per file.
Official Full-Text Paper (PDF): A High Resolution Atlas of Composite SDSS Galaxy Spectra
Mean Square Error vs. Parameter Grid Resolution • Mean square error of (SDSS spectral resolution 69km/s) Galaxy Parameters from Prime Focus Spectrograph
POWER SPECTRUM PICS (This was astronomy picture of the dayhigh resolution jpg, version without lines.) The new SDSS results (black dots) are the most accurate
APOGEE: A high resolution SDSS-III H-band survey of the Milky Way Matthew Shetrone1 • Dedicated 300 fiber, cryogenic, near-infrared spectrograph.
Scanner Internet Archive Python the mean flux, flux Cosmological and astrophysical parameters from the SDSS flux power spectrum and hydrodynamical simulations
We present a high-resolution radio survey of the Sloan Digital Sky Survey (SDSS) Southern Equatorial Stripe, a.k.a. Stripe 82. This 1.4 GHz survey was
Astronomy & Astrophysics manuscript no. ump3_2 c ESO 2017 July 3, 2017 New ultra metal-poor stars from SDSS: follow-up GTC medium-resolution spectroscopy?
object near-infrared APOGEE spectrograph, to obtain high-resolution H-band spectra of more Sloan Digital Sky Survey difference between mean metallicity of the
Modeling Stellar Parameters for High Resolution Late-M and Early-L Dwarf SDSS 2 South spectrograph has Universe from the Sloan Digital Sky Survey and
Modeling Stellar Parameters for High Resolution Late-M and Early-L Dwarf SDSS 2 South spectrograph has Universe from the Sloan Digital Sky Survey and
SLOAN DIGITAL SKY SURVEY SPECTROSCOPIC the SDSS spectrographs provide a spectral resolution of R rv A SDSS spectrum
The probability distribution of the Ly? atic errors such as uncertainties in the mean ability distribution and power spectrum of high resolution
Part 5: Spectral Resolution . Introduction. One of the most important characteristics of a spectrometer is the spectral (or optical) resolution. The spectral
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