VEGA: Visible spEctroGraph and polArimeter for the CHARA array: principle and performance

By D. Mourard, J. Clausse, A. Marcotto, K. Perraut, I. Tallon-Bosc, P. Bério, A. Blazit, D. Bonneau, S. Bosio, Y. Bresson and 23 more. 2009

135 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/622c62f2f9e24f314fe4378cb1c947f0915aaadf

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In Astronomy and Astrophysics

1. B. Mason
2. W. Hartkopf
3. N. Turner
4. T. T. ten Brummelaar
5. H. Mcalister
6. L. Sturmann
7. J. Sturmann
8. C. Farrington

In Computational Mechanics

1. W. Hartkopf
2. B. Mason
3. N. Turner
4. P. J. Goldfinger
5. C. Farrington
6. H. Mcalister
7. L. Sturmann
8. J. Sturmann

In Instrumentation

1. W. Hartkopf
2. B. Mason
3. P. J. Goldfinger
4. C. Farrington
5. N. Turner
6. H. Mcalister
7. L. Sturmann
8. J. Sturmann

Citations in the corpus

• An investigation of the close environment of β Cephei with the VEGA/CHARA interferometer (2010, methodology): “The VEGA instrument works in the visible domain and provides a maximum angular resolution of 0.3 mas (Mourard et al. 2009).”
• SEPARATED FRINGE PACKET OBSERVATIONS WITH THE CHARA ARRAY. II. ω ANDROMEDA, HD 178911, AND ξ CEPHEI (2014, methodology): “Full details of the VEGA instrument can be found in Mourard et al. (2009).”
• Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer (2017, unknown): “…2.048±0.009 2.097±0.009 Ligi et al. (2016) 2.12±0.02 Ligi et al. (2012) 2.041±0.043 Baines et al. (2010) 172167 3.280±0.016 2.930±0.007 Monnier et al. (2012) 3.08±0.03a Mourard et al. (2009) 3.202±0.005a Absil et al. (2006) 3.329±0.006 Aufdenberg et al. (2006) 3.225±0.032 Mozurkewich et al.…”