Echellette spectrograph and imager
http://www.tauceti.caltech.edu/jspineda/jspinedaCV.pdf WebJun 7, 2006 · Abstract: We report on the design, development and commissioning of an Integral Field Unit (IFU) that has been built for the Echellette Spectrograph and Imager …
Echellette spectrograph and imager
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WebAug 11, 2024 · ABSTRACT We use medium-resolution Keck/Echellette Spectrograph and Imager spectroscopy of bright quasars to study cool gas traced by CaII 3934;3969 and NaI 5891;5897 absorption in the interstel- lar/circumgalactic media of 21 foreground star-forming galaxies at redshifts 0:03 <0:20 with stellar masses 7:4 logM =M 10:6. WebAug 6, 2014 · The Multi-Object Broadband Imaging Echellette (MOBIE) is the seeing-limited, visible-wavelength imaging multiobject spectrograph (MOS) planned for first-light use on the Thirty Meter Telescope (TMT).
WebSep 20, 2010 · We report Keck/Echellette Spectrograph and Imager and Very Large Telescope/Ultraviolet-Visual Echelle Spectrograph observations of three super-damped … WebApr 15, 2002 · The Echellette Spectrograph and Imager (ESI) is a multipurpose instrument which has been delivered by the Instrument Development Laboratory of Lick …
WebJul 1, 2010 · The Multi-Object Broadband Imaging Echellette (MOBIE) is the seeing-limited, optical spectrograph planned for the first generation of Thirty Meter Telescope (TMT) instruments1. WebJun 7, 2006 · The IFU passes a spectral range of 0.39-1.1 um with a throughput of between 45 % and 60 % depending on wavelength and field position. The IFU head resides in an …
WebJul 21, 2008 · Spectra obtained with the Echellette Spectrograph and Imager at the Keck Observatory are used to determine the central stellar velocity dispersions and to examine the emission-line properties. Overall, the stellar velocity dispersions are low (40-90 km/s), and we find 12 objects having sigma < 60 km/s, a range where very few Seyfert 2 …
Webtelescopes; spectrograph optics and wide-field correctors for the converted 6.5-m MMT and the 6.5-m Magellan telescopes; as well as the optical design concepts and camera designs for ESI, the medium-resolution echellette and for DEIMOS, the low-resolution multi-object spectrograph and imager, which are primary instruments on Keck 2. readcloud textbookWebApr 17, 2002 · We obtained an optical image of PSO J347+48 in the "Ellis-R" filter of the Echellette Spectrograph and Imager on the Keck II telescope (Keck-II/ESI; Sheinis et … how to store phonak hearing aidsWebI learned how to robustly reduce data of galaxies and quasars, taken with the Magellan Echellette (MagE) spectrograph at the Las Campanas Observatory in Chile by my mentor, Dr. Kathy Cooksey. readco holdingsWebAn image slicer-based Integral Field Unit (IFU) has been developed for the Echellette Spectrograph and Imager (ESI) Sheinis et al. (2002). The IFU is an optical system that remaps a 2-dimensional field of view (FOV) onto the 20 arc-second spectrograph slit while readco industries edmontonWebEchelle grating. An echelle grating (from French échelle, meaning "ladder") is a type of diffraction grating characterised by a relatively low groove density, but a groove shape … readcloud onlineWebApr 7, 2024 · To get a closer look, they conducted follow-up observations using Keck Observatory’s Low Resolution Imaging Spectrometer (LRIS) and Near Infrared Echellette Spectrograph (NIRES). how to store phone number in javaWebJan 6, 2024 · Based on data obtained from Keck Observatory’s Deep Imaging and Multi-Object Spectrograph and Near Infrared Echellette Spectrograph, the researchers determined SN 2024tlf’s progenitor red supergiant star — located in the NGC 5731 galaxy about 120 million light-years away from Earth — was 10 times more massive than the … how to store phone contacts on gmail