Optical and IR Telescope Instrumentation and Detectors

By M. Iye, A. Moorwood. 2000

378 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/cf2baed54887bba8e0dbad5577437bbb61d3b052

How researchers see this paper

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

1. R. Genzel
2. P. Hopkins
3. M. Pettini
4. A. Shapley
5. J. Xavier Prochaska
6. C. Steidel
7. A. Helmi
8. A. Coil

Citations in the corpus

• The VLT-UVES survey for molecular hydrogen in high-redshift damped Lyman α systems: physical conditions in the neutral gas (2005, unknown): “Spectra were reduced using the UVES pipeline, and addition of individual exposures was performed using a sliding window and weighting the signal by the errors in each pixel.”
• The 2dF QSO Redshift Survey – XII. The spectroscopic catalogue and luminosity function (2004, unknown): “Further details can be found in Watson et al. (2000).”
• Probing the Interstellar Medium near Star-forming Regions with Gamma-Ray Burst Afterglow Spectroscopy: Gas, Metals, and Dust (2007, background): “We discuss the implications of these results in § 4 and conclude with a list of future directions.”
• The DEIMOS spectrograph for the Keck II Telescope: integration and testing (2003, background): “(5) The camera multiplets should be characterized fully before assembling them into the nal camera and before the camera is put into the spectrograph.”
• Oxygen, Sodium, Magnesium and Aluminium as tracers of the Galactic Bulge Formation (2006, methodology): “In this paper, we analyse the stars observed with the red arm of the UVES spectrograph at a resolution R∼ 47000 (Dekker et al. 2000) in the range 4800-6800 Å.”
• VLT/UVES Abundances in Four Nearby Dwarf Spheroidal Galaxies. II. Implications for Understanding Galaxy Evolution (2002, methodology): “Our observations were obtained in visitor mode, with UT2/UVES (Dekker et al. 2000) on two separate visitor runs on Paranal, one in 2000 August, and one in 2001 January.”
• Molecular hydrogen in high-redshift Damped Lyman-alpha systems: The VLT/UVES database (2008, methodology): “All the quasars in our sample were observed with the Ultraviolet and Visual Echelle Spectrograph (UVES, Dekker et al. 2000) mounted on the ESO VLT-UT 2 (Kueyen) 8.2 m telescope on Cerro Paranal, Chile.”
• First stars XII. Abundances in extremely metal-poor turnoff stars,and comparison with the giants (2009, methodology): “The spectra were reduced using the UVES context within MIDAS (Ballester et al. 2000); see Paper V for details.”
• The metallicity distribution of bulge clump giants in Baade’s window (2011, methodology): “The data reduction was carried out using the girBLDRS1 pipeline developed at the Geneva Observatory (Blecha et al. 2000) and includes cosmic-ray removal, bias subtraction, flatfield correction, individual spectral extraction, and accurate wavelength calibration based on simultaneous calibration expo”
• A Geometric Determination of the Distance to the Galactic Center (2003, methodology): “On April 8/9 2003 (2003.27) we observed the Galactic Center on Kueyen (UT2 of the VLT) with the new MPE integral field spectrometer SPIFFI (Thatte et al. 1998, Eisenhauer et al. 2000).”
• First stars VIII. Enrichment of the neutron-capture elements in the early Galaxy (2007, unknown): “The observations were performed during several observing runs in 1999 and 2000 at the VLT-Kueyen telescope with the high-resolution spectrograph UVES (Dekker et al. 2000).”
• Complexity on Small Scales: The Metallicity Distribution of the Carina Dwarf Spheroidal Galaxy (2005, methodology): “05 (Blecha et al. 2000).”