The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
An atmospheric radiation model for Cerro Paranal: I. The optical spectral range⋆
Open accessAbstract
Aims. The Earth’s atmosphere affects ground-based astronomical observations. Scattering, absorption, and radiation processes deteriorate the signal-to-noise ratio of the data received. For scheduling astronomical observations it is, therefore, important to accurately estimate the wavelength-dependent effect of the Earth’s atmosphere on the observed flux.
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Citations
Cites
The dancing sky: 6 years of night-sky observations at Cerro Paranal
Patat, F. (2008) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20079279 · Cited by 97
Cited by
Smette, A., Sana, H., Noll, S., Horst, H., Kausch, W., Kimeswenger, S., Barden, M., Szyszka, C., Jones, A. M., Gallenne, A., et al. (2015) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201423932 · Cited by 758
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Metadata
- Authors
- Noll, S., Kausch, W., Barden, M., Jones, A. M., Szyszka, C., Kimeswenger, S., & Vinther, J.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2012-07
- Volume
- 543
- Pages
- A92
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4289875276
- Cited by
- 310
- References
- 1
- FWCI
- 11.29
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Noll, S., Kausch, W., Barden, M., Jones, A. M., Szyszka, C., Kimeswenger, S., & Vinther, J. (2012). An atmospheric radiation model for Cerro Paranal: I. The optical spectral range⋆. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201219040
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