activity
19972003
most citedAutomated Stellar Spectral Classification and Parameterization for the Masses

5 citations · 5 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph2003

New Resources to Explore the Old Galaxy: Mining the SDSS

C. Allende Prieto, T. C. Beers, Y. Li +3

The Sloan Digital Sky Survey (SDSS) is collecting photometry and intermediate resolution spectra for ~ 10**5 stars in the thick-disk and stellar halo of the Milky Way. This massive…

astro-ph20025 cited

Automated Stellar Spectral Classification and Parameterization for the Masses

Ted von Hippel, Carlos Allende Prieto, Chris Sneden

Stellar spectroscopic classification has been successfully automated by a number of groups. Automated classification and parameterization work best when applied to a homogeneous da…

astro-ph2001

The Spectrum of the Th-Ar Hollow-Cathode Lamp Used with the 2dcoude Spectrograph

Carlos Allende Prieto

We have produced an atlas of the Th-Ar hollow-cathode lamp used with the 2dcoude spectrograph at McDonald Observatory. The atlas covers from 3611.9 to 10596.4 A at a resolving powe…

astro-ph2000

Hipparcos, IUE, and the Stellar Content of the Solar Neighbourhood

Carlos Allende Prieto

The spectroscopic parallaxes in the Hipparcos catalogue can be used to translate absolute stellar fluxes observed at Earth to the fluxes emerging at the stellar surface for nearby…

astro-ph1999

(Teff,log g,[Fe/H]) Classification of Low-Resolution Stellar Spectra using Artificial Neural Networks

Shawn Snider, Yuan Qu, Carlos Allende Prieto +4

New generation large-aperture telescopes, multi-object spectrographs, and large format detectors are making it possible to acquire very large samples of stellar spectra rapidly. In…

astro-ph1997

An Inversion Technique to Derive Model Photospheres in Late-Type Stars from High-Resolution Spectroscopy: The Sun

C. Allende Prieto, B. Ruiz Cobo, R. J. Garcia Lopez

An inversion technique has been developed to recover LTE one-dimensional model photospheres for late-type stars from very high-resolution high signal-to-noise stellar line profiles…