CHARM2: An updated Catalog of High Angular Resolution Measurements

By A. Richichi, I. Percheron, M. Khristoforova. 2005

310 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/b82af8d88a0010b10311f0126c9fb46c2df0d3cd

How researchers see this paper

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In Astronomy and Astrophysics

1. C. Soubiran
2. D. Gies
3. U. Heiter
4. F. Th'evenin
5. Paulina Jofré
6. P. J. Goldfinger
7. A. Weiss
8. A. Korn

In Atomic and Molecular Physics, and Optics

1. D. Gies
2. A. Korn
3. F. Th'evenin
4. O. Lühe
5. S. Ridgway

In Instrumentation

1. C. Soubiran
2. U. Heiter
3. Paulina Jofré
4. P. J. Goldfinger
5. A. Weiss
6. A. Korn
7. C. Farrington
8. Y. Touhami

Citations in the corpus

• Gaia FGK benchmark stars: Effective temperatures and surface gravities (2015, methodology): “Direct measurements The catalogues of Pasinetti Fracassini et al. (2001) and Richichi et al. (2005) and the literature were searched for angular diameter determinations, and the data were extracted from the original references.”
• SURVEYING THE BRIGHT STARS BY OPTICAL INTERFEROMETRY. I. A SEARCH FOR MULTIPLICITY AMONG STARS OF SPECTRAL TYPES F-K (2016, methodology): “For γ Vir, the orbital elements of Scardia et al. (2007), primary and secondary star angular diameters of 1.59 mas (Richichi et al. 2005), and a Δm=0.1 resulting from the GRIDFIT search (Section 5.2), were used as inputs to the binary model.”
• SearchCal: a Virtual Observatory tool for searching calibrators in optical long-baseline interferometry II. The faint-object case (2006, methodology): “In some particular cases this parameter is either a measured value taken from catalog CHARM (Richichi et al., 2005) or an estimated value taken from the lists of stars of reference published by Bordé et al. (2002) or Mérand et al. (2005).”
• Basic physical parameters of a selected sample of evolved stars (2006, methodology): “The observed apparent diametersθ are taken from the CHARM2 catalogue (Richichi et al. 2005), which in most cases consist of indirect estimates of stellar diameters using fits to spectrophotometric data, and are available for about one third of our sample.”
• STELLAR DIAMETERS AND TEMPERATURES. I. MAIN-SEQUENCE A, F, AND G STARS (2011, methodology): “As an update, the CHARM2 Catalogue (Richichi et al. 2005) provides a compilation of stellar diameters by means of direct measurements by high angular resolution methods, as well as indirect estimates.”