Irtf spex
Webspex (8) beckman dk2a ratio recording spectroreflectometer (1) cassegrain spectrometer (1) ctio 1.0m 2dfrutti spectrograph (1) ctio 1.5-meter cassegrain spectrograph (1) fink spectrograph (1) large cassegrain spectrometer (1) larson ihw spectrograph (1) mark iii spectrograph (1) WebMar 4, 2024 · IRTF is the only NASA-owned ground-based astronomical telescope. The objective of the review is to examine the IRTF’s scientific productivity and to assess its …
Irtf spex
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WebApr 1, 2013 · IRTF SpeX observations that were selected for use. All selected frames were observed on 18 August 2009 with IRTF SpeX in short-wavelength, cross-dispersed mode (SXD). HD 1160 was the A0-type star used as a stellar standard for the removal of telluric absorptions features. WebMar 2, 2024 · We present a multi-epoch spectroscopic study of LkCa 4, a heavily spotted non-accreting T Tauri star. Using SpeX at NASA's Infrared Telescope Facility (IRTF), 12 spectra were collected over five consecutive nights, spanning 1.5 stellar rotations.
WebOct 17, 2016 · These observations of Jupiter represent quick-look images of the planet made using the scientific-grade guide camera (commonly called “Guide Dog”) on the moderate-resolution near-infrared facility spectrometer, SpeX, … WebOct 17, 2016 · These observations of Jupiter represent quick-look images of the planet made using the scientific-grade guide camera (commonly called “Guide Dog”) on the …
Webcollection: Fieber-Beyer IRTF Mainbelt Asteroid Spectra V2.0 The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained by Sherry Fieber-Beyer and archives reduced, calibrated spectra. WebJul 16, 2013 · IRTF/SpeX Spectroscopy and Imaging. WISE J1049−5319 was observed with IRTF/SpeX on 2013 March 15 (UT) in cloudy and windy conditions with poor and variable seeing (1 5–2 0 at J band). We deployed the 0 V = 6.87) at an airmass of 3.3 with the slit aligned to the same position angle. Internal flat field and Ar arc lamp exposures were …
Webspex (19) beckman dk2a ratio recording spectroreflectometer (3) cassegrain spectrometer (3) large cassegrain spectrometer (3) mark iii spectrograph (3) ctio 1.0m 2dfrutti spectrograph (2) ctio 1.5-meter cassegrain spectrograph
Webspex (19) beckman dk2a ratio recording spectroreflectometer (3) cassegrain spectrometer (3) large cassegrain spectrometer (3) mark iii spectrograph (3) ctio 1.0m 2dfrutti … my brother\u0027s best friend romance booksWebJun 18, 2014 · Abstract: The SpeX Prism Library (SPL) is a uniform compilation of low-resolution (R ~ 75-120), near-infrared (0.8-2.5 micron) spectra spanning a decade of … how to physically secure an sql serverWebdata set: FIEBER-BEYER IRTF MAINBELT ASTEROID SPECTRA V2.0 IRTF SpeX spectra of main belt asteroids from Fieber-Beyer (2010)as well as data obtained since time of V1.0 publication. SUPPORT ARCHIVES - EAR-A-I0046-3-FBIRTFSPEC-V2.0 - starting 2000-06-30T09:58:41Z; data set: FIEBER-BEYER IRTF MAINBELT ASTEROID SPECTRA V1.0 IRTF … how to physically describe a characterWebThe IRTF Extended Spectral Library is a collection of 0.7-2.5 um mostly stellar spectra observed at a resolving power of R ~ 2000 with the medium-resolution spectrograph, … how to physically rotate dell monitorhttp://irtfweb.ifa.hawaii.edu/~spex/ how to physically describe someonemy brother\u0027s bar coloradoWebThe 2001 IRTF SPeX data was used to identify Type II material based on observational geometry and evaluation of dust opacity. An represent spectra of this region was extracted using a 3x3 pixel box—shown in red in Figure 6. This represents ~0.9 arc seconds area of the disc and is consistent with our spatial resolution. my brother\u0027s barber birmingham al