959 citations · 1.5k across the 10 of their papers we have counts for
10 papers
PALACE v1.0: Paranal Airglow Line And Continuum Emission model
Stefan Noll, Carsten Schmidt, Patrick Hannawald +2
Below about 2.3 m, the nighttime emission of the Earth's atmosphere is dominated by non-thermal radiation from the mesosphere and thermosphere. As this airglow can even outshine…
Structure, variability, and origin of the low-latitude nightglow continuum between 300 and 1,800 nm: Evidence for HO emission in the near-infrared
Stefan Noll, John M. C. Plane, Wuhu Feng +5
The Earth's mesopause region between about 75 and 105 km is characterised by chemiluminescent emission from various lines of different molecules and atoms. This emission was and is…
Climatologies of Various OH Lines From About 90,000 X-shooter Spectra
Stefan Noll, Carsten Schmidt, Wolfgang Kausch +2
The nocturnal mesopause region of the Earth's atmosphere radiates chemiluminescent emission from various roto-vibrational bands of hydroxyl (OH), which is therefore a good tracer o…
The ESO's Extremely Large Telescope Working Groups
Paolo Padovani, Michele Cirasuolo, Remco van der Burg +82
Since 2005 ESO has been working with its community and industry to develop an extremely large optical/infrared telescope. ESO's Extremely Large Telescope, or ELT for short, is a re…
Effective Emission Heights of Various OH Lines From X-shooter and SABER Observations of a Passing Quasi-2-Day Wave
Stefan Noll, Carsten Schmidt, Wolfgang Kausch +2
Chemiluminescent radiation of the vibrationally and rotationally excited OH radical, which dominates the nighttime near-infrared emission of the Earth's atmosphere in wide waveleng…
Comparison of VLT/X-shooter OH and O2 rotational temperatures with consideration of TIMED/SABER emission and temperature profiles
S. Noll, W. Kausch, S. Kimeswenger +2
Rotational temperatures Trot derived from lines of the same OH band are an important method to study the mesopause region near 87 km. To measure realistic temperatures, the rotatio…
Flux calibration of medium-resolution spectra from 300 nm to 2500 nm: Model reference spectra and telluric correction
S. Moehler, A. Modigliani, W. Freudling +8
While the near-infrared wavelength regime is becoming more and more important for astrophysics there is a marked lack of spectrophotometric standard star data that would allow the…
An atmospheric radiation model for Cerro Paranal. I. The optical spectral range
S. Noll, W. Kausch, M. Barden +4
The Earth's atmosphere affects ground-based astronomical observations. Scattering, absorption, and radiation processes deteriorate the signal-to-noise ratio of the data received. F…
Spectral energy distributions of an AKARI-SDSS-GALEX sample of galaxies
V. Buat, E. Giovannoli, T. T. Takeuchi +5
The nearby universe remains the best laboratory to understand physical properties of galaxies and is a reference for any comparison with high redshift observations. The all sky (or…
Analysis of galaxy SEDs from far-UV to far-IR with CIGALE: Studying a SINGS test sample
S. Noll, D. Burgarella, E. Giovannoli +3
Photometric data of galaxies covering the rest-frame wavelength range from far-UV to far-IR make it possible to derive galaxy properties with a high reliability by fitting the atte…