Instrument Design and Performance for Optical/Infrared Ground-based Telescopes,
By M. Iye, A. Moorwood. 2003
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View Paper: https://www.semanticscholar.org/paper/25273f47358a4c2e6f02777ee5afba1d4c21bfda
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Citations in the corpus
- Kinemetry of SINS High-Redshift Star-Forming Galaxies: Distinguishing Rotating Disks from Major Mergers (2008, methodology): “The SINGS galaxies were observed in H emission with the FANTOMM Fabry-Perot scanning interferometer (Hernandez et al. 2003).”
- PTF12os and iPTF13bvn. Two stripped-envelope supernovae from low-mass progenitors in NGC 5806 (2016, methodology): “…phase, one using the NOT and the Andalucia Faint Object Spectrograph (ALFOSC) at 250 d past discovery, one with the Deep Extragalactic Imaging Multi-Object Spectrograph (DEIMOS; Faber et al. 2003) All spectra were reduced using standard pipelines and procedures for each telescope and instrument.”
- Ultraviolet to Mid-Infrared Observations of Star-forming Galaxies at z ~ 2: Stellar Masses and Stellar Populations (2005, methodology): “Near-IR Imaging We observed the HS1700+64 field during two observing runs, 2003 May and 2003 October, using the Palomar 5.1m Hale telescope and the Wide Field Infrared Camera (WIRC; Wilson et al. 2003).”
- THE SINFONI BLACK HOLE SURVEY: THE BLACK HOLE FUNDAMENTAL PLANE REVISITED AND THE PATHS OF (CO)EVOLUTION OF SUPERMASSIVE BLACK HOLES AND BULGES (2016, methodology): “In summary, our SINFONI black hole sample consists of 30 galaxies that we observed with the Spectrograph for INtegral Field Observations in the Near Infrared (Eisenhauer et al. 2003; Bonnet et al. 2003, SINFONI,) at the UT4 of the Very Large Telescope under nearly diffraction limited conditions.”
- The Star Formation Rate Density and Dust Attenuation Evolution over 12 Gyr with the VVDS Surveys (2011, background): “…(VVDS) is a spectroscopic investigation of distant sources, carried out with the highmultiplex, wide-field (224 arcmin2) VIsible Multi-Object Spectrograph (VIMOS, Le Fèvre et al. 2003) mounted at the Nasmyth focus of MELIPAL, the third of the four 8.2m ESOVLT Unit Telescopes in Paranal, Chile.”