Instrument Sensitivity Optimization
Instrument Sensitivity Optimization is a methodological framework in observational astronomy that systematically enhances the detection capability of infrared telescopes by minimizing instrumental noise and maximizing signal-to-noise ratio through precise calibration, cryogenic stabilization, and spectral filtering techniques.
103
Publications
5.9K
Citations
919
Authors
277
Institutions
Publications per year
2017–2026
17
Parents
103
X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope
J. Vernet, H. Dekker, S. D’Odorico et al. · Astronomy and Astrophysics · 2011 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +15
Monte Carlo design studies for the Cherenkov Telescope Array
K. Bernlöhr, A. Barnacka, Y. Becherini et al. · Astroparticle Physics · 2012 · 235 citations · Full text
1–5 of 103
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277
Jet Propulsion Laboratory
Pasadena, United States
8 h-index
49 publications
2.8K citations
California Institute of Technology
Pasadena, United States
8 h-index
34 publications
1.1K citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
26 publications
4.4K citations
Goddard Space Flight Center
Greenbelt, United States
6 h-index
14 publications
499 citations
University of California, Berkeley
Berkeley, United States
6 h-index
17 publications
1.1K citations
Stanford University
Stanford, United States
5 h-index
28 publications
1.1K citations
European Southern Observatory
Garching bei München, Germany
5 h-index
48 publications
24.3K citations

University of Toronto
Toronto, Canada
4 h-index
6 publications
578 citations
1–8 of 277
17 publications · 580 citations
14
h-index
5 publications · 195 citations
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ApJ · 5 publications · 405 citations
5
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4 publications · 1.4K citations
4
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PASP · 3 publications · 59 citations
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1–5