A flux-calibrated, high-resolution atlas of optical sky emission from UVES

By R. Hanuschik. 2003

157 citations recorded by the source corpus.

Subfields: Atomic and Molecular Physics, and Optics, Mechanical Engineering, Statistics and Probability

View Paper: https://www.semanticscholar.org/paper/967d469a3de65f373d4867af1fbad438f6a70c32

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atomic and Molecular Physics, and Optics

1. D. Weinberg
2. France.
3. M. Ishak
4. John M. O’Meara
5. J. Xavier Prochaska
6. C. Allende Prieto
7. Daniel J. Eisenstein
8. Carlos S. Frenk

In Mechanical Engineering

1. N. Evans II
2. W. Kausch
3. Stefan Kimeswenger
4. J. Vinther
5. Stefan Noll
6. A. Jones
7. M. Barden
8. C. Szyszka

In Statistics and Probability

1. D. Geisler
2. John M. O’Meara
3. A. Ross
4. J. Xavier Prochaska
5. Carlos S. Frenk
6. N. Evans II
7. W. Kausch
8. Stefan Kimeswenger

Citations in the corpus

• J1154+2443: a low-redshift compact star-forming galaxy with a 46 per cent leakage of Lyman continuum photons (2017, background): “Furthermore, the Hα having an observed wavelength of 8986.8Å and full width at half maximum of 6Å, it could be affected by residuals of the relatively strong night sky emission lines with wavelengths 8982.3Å, 8985.7Å and 8988.3Å (Hanuschik 2003).”
• Evidence of Environmental Dependencies of Type Ia Supernovae from the Nearby Supernova Factory indicated by Local H$\alpha$ (2013, background): “The night sky spectrum is a combination of the atmospheric molecular emission, zodiacal light, scattered star light, along with the moon contribution if any (Hanuschik 2003).”
• Nearby Supernova Factory Observations of SN 2005gj: Another Type Ia Supernova in a Massive Circumstellar Envelope (2006, methodology): “The wavelength calibration arcs were obtained at the beginning of the night; since LRIS suffers from flexure, the wavelength zero points were adjusted for each spectrum using the night-sky lines referenced to the high-resolution night-sky spectrum of Hanuschik (2003).”
• The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument (2022, methodology): “This external sky spectrum is derived from a set of high-resolution spectra from Hanuschik (2003), convolved to the resolution of the DESI spectrographs.”
• The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation (2022, methodology): “In our case, we use the dark sky spectrum derived from UVES (Hanuschik 2003) and the nominal air mass for the attenuation.”
• ACCURATE STELLAR KINEMATICS AT FAINT MAGNITUDES: APPLICATION TO THE BOÖTES I DWARF SPHEROIDAL GALAXY (2011, methodology): “…the continuum from the sky or from the stellar spectra, then we fitted the residual spectrum in pixel space by a sum of n×LSFs (Line Spread Functions) at the locations given by the catalogue of sky lines from Hanuschik (2003) after applying the polynomial correction to the wavelengths. λ = λ̃”
• An atmospheric radiation model for Cerro Paranal - I. The optical spectral range (2012, methodology): “There is an unpublished UVES 800U spectrum related to the study of Hanuschik (2003) that covers the gap.”
• The Giant Gemini GMOS survey of zem > 4.4 quasars – I. Measuring the mean free path across cosmic time (2014, methodology): “A sky spectrum was also extracted and compared to an archived solution based on the Paranal sky measurements (Hanuschik 2003) to estimate a rigid shift of the wavelength solution due to instrument flexure.”