A library of 0.5 to 2.5 m spectra of luminous cool stars

By Ariane Lançon, P. Wood. 2000

157 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/1d9ce57ac9a988b5e966351b562d4cac072eca33

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. C. Conroy
2. P. V. van Dokkum
3. M. Cushing
4. Joshua S. Speagle
5. Benjamin D. Johnson
6. J. Leja
7. Michael C. Liu
8. A. Burgasser

In Computational Mechanics

1. M. Cushing
2. G. Sloan
3. Benjamin D. Johnson
4. M. Meixner
5. J. Leja
6. C. Conroy
7. M. Groenewegen
8. P. Marigo

In Instrumentation

1. C. Conroy
2. P. V. van Dokkum
3. Joshua S. Speagle
4. Benjamin D. Johnson
5. M. Cushing
6. J. Leja
7. J. Rayner
8. W. Vacca

Citations in the corpus

• Dynamic model atmospheres of AGB stars - III. Effects of frequency-dependent radiative transfer (2003, background): “It is evident that the grey model is not able to reproduce the energy distribution of R Lep (bottom curve) correctly; the maximum of its energy distribution is far too blue.”
• The global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae, and the impact on the ISM evolution (2009, background): “Carbon-rich stars have HCN and C2H2 bands at 3.1 μm (Ridgway, Carbon & Hall 1978; Groenewegen, de Jong & Gaballe 1994; van Loon et al. 1999; Matsuura et al. 2002b, 2005) and CN in the J and H bands (Whitelock & Catchpole 1987; Lançon & Wood 2000).”
• THE INFRARED TELESCOPE FACILITY (IRTF) SPECTRAL LIBRARY: COOL STARS (2009, background): “The lines are known to come and go depending upon cycle and phase (e.g. Lançon & Wood 2000, in the NIR).”
• Evolutionary population synthesis: models, analysis of the ingredients and application to high‐z galaxies (2004, background): “Not only the absolutefl x in the near-IR region increases by nearly a factor 3, also peculiar absorption features appear (e.g. CN,C2 in C-stars andH2O and CO in O-stars, see e.g. Lançon & Wood 2000 for more details).”
• Asymptotic Giant Branch evolution at varying surface C/O ratio: effects of changes in molecular opacities (2002, background): “The spectra of cool giant stars – with spectral types MS-C – are dominated by totally different molecular absorption bands in the visual and infrared (e.g. Lançon & Wood 2000) depending on which, carbon or oxygen, is the most abundant element.”
• Stellar Population Inference with Prospector (2020, methodology): “Those libraries are supplemented with the TP-AGB library from Lançon & Wood (2000), the post-AGB library from Rauch (2003), and the WMBASIC hot star library from Eldridge et al. (2017).”