THE GEMINI SPECTRAL LIBRARY OF NEAR-IR LATE-TYPE STELLAR TEMPLATES AND ITS APPLICATION FOR VELOCITY DISPERSION MEASUREMENTS
Autor: | Thaisa Storchi-Bergmann, Claudia Winge, Rogemar A. Riffel |
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Rok vydání: | 2009 |
Předmět: |
Stellar kinematics
Cosmology and Nongalactic Astrophysics (astro-ph.CO) Instrumentation FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics spectroscopic [Techniques] Astronomia infravermelha Astrophysics::Solar and Stellar Astrophysics miscellaneous [Astronomical data bases] Spectral resolution data analysis [Methods] Instrumentation and Methods for Astrophysics (astro-ph.IM) Astrophysics::Galaxy Astrophysics Physics Supermassive black hole Resolution (electron density) Velocity dispersion Astronomy and Astrophysics Espectros estelares Galaxy Galáxias ativas Buracos negros Stars Space and Planetary Science late-type [Stars] Astrophysics::Earth and Planetary Astrophysics Astrophysics - Instrumentation and Methods for Astrophysics Astrophysics - Cosmology and Nongalactic Astrophysics |
Zdroj: | Repositório Institucional da UFRGS Universidade Federal do Rio Grande do Sul (UFRGS) instacron:UFRGS |
ISSN: | 1538-4365 0067-0049 |
Popis: | We present a spectroscopic library of late spectral type stellar templates in the near-IR range 2.15-2.42microns, at R=5300-5900 resolution, oriented to support stellar kinematics studies in external galaxies, such as the direct determination of the masses of supermassive black-holes in nearby active (or non-active) galaxies. The combination of high spectral resolution and state-of-the-art instrumentation available in 8-m class telescopes has made the analysis of circumnuclear stellar kinematics using the near-IR CO band heads one of the most used techniques for such studies, and this library aims to provide the supporting datasets required by the higher spectral resolution and larger spectral coverage currently achieved with modern near-IR spectrographs. Examples of the application for kinematical analysis are given for data obtained with two Gemini instruments, but the templates can be easily adjusted for use with other near-IR spectrographs at similar or lower resolution. The example datasets are also used to revisit the "template mismatch" effect and the dependence of the velocity dispersion values obtained from the fitting process with the characteristics of the stellar templates. The library is available in electronic form from the Gemini web pages (link above). Comment: To appear in the ApJ Supplement Series, December 2009. AASTex, 25 pages, 17 figures. The library spectra are available in standard FITS format from the Gemini Observatory webpage at http://www.gemini.edu/sciops/instruments/nearir-resources/?q=node/10167 |
Databáze: | OpenAIRE |
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