PPT-The Solar-Stellar Spectrograph (SSS) Project Review

JEFFREY HALL LOWELL OBSERVATORY FLAGSTAFF AZ Project Timeline 1988 1992 1996 2000 2004 2008 2012 Constructionearly observing Rebuild 1 Broad survey Solar analog survey Rebuild 2 AD boundary. Stuart . Ryder. Australian Gemini Office. . Australian Astronomical Observatory. Outline. Radio – Optical synergies. ATAC . “open skies” access . to. (UKST). AAT. Gemini. Magellan. Time exchange. Soroush Sotoudeh. . (University of Minnesota). Daniel . Weisz. , Andrew Dolphin, Evan Skillman. 06/29/2015 – . STScI. Workshop on IMF. Outline. Introduction. Observations and data. IMF analysis and results. 1. /28. Important for transits (see next slides).. . Transit depth = [ . R. planet. (. λ. ,t. ) / . R. star. (. λ,t. ) ]. 2. Not so important for eclipses because the eclipse is a simple difference, and the stellar variability typically is slower than the eclipse: . complexity of . starbirth. in unprecedented clarity . to yield evidence . for orphan stars . National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . Wendy . Tang and S. Yueh. CAP_RC has the smallest RMSD and close to zero bias with respect to the buoy SSS at 1 m depth.. REMSS SSS in general has a negative bias (-0.2 . psu. ) and larger RMSD in the western Pacific and Indian Ocean. Is this a surface stratification effect?. Transiting Exoplanets. Dainis Dravins. 1. , . Hans-Günter Ludwig. 2. ,. Erik Dahlén. 1. ,. Martin Gustavsson. 1. , . Hiva. Pazira. 1. . 1. . Lund Observatory, Sweden, . 2. . Landessternwarte. A first of its kind collaboration between:. Indiana Office of Community and Rural Affairs (OCRA). Indiana Housing and Community Development Authority (IHCDA). Indiana Department of Transportation (INDOT). . Matt Crouch.  . Project Manager. Kathleen . Weissenberger. State CDBG Director. Indiana Office of Community and Rural Affairs. 2014 Regional Conference. Indiana’s Stellar Communities. A first of its kind collaboration between:. life appearance conditions. Call of interest. Hyper-Emblematic. project. P2IO. Expression of interest . Stellar and Planetary Formation . Keywords:. Structure and dynamics, Radiation, Magnetic fields,. Larry J. Paxton. GUVI co-PI. SSUSI PI. Why spectrograph mode?. Spectrograph mode returns the entire spectrum. When SSUSI was designed the data rate was . set as spare words in the OLD data stream – about . Commissioning, Upgrades and Future. Wenda . Cao & NST Team. BBSO was built by Caltech in 1969.. Observatory . was transferred from Caltech to NJIT in July 1997. . The dome sits at the end of a 1000 ft. causeway on Big Bear Lake’s north shore at 6,750 foot elevation.. LES JARDINS has revolutionized lighting concept by integrating design and technology. Engineers and designers at LES JARDINS share the goal to make outdoor lighting beautiful, smart and clean. Jeffrey . Linsky. JILA and APAS. Solar Focus Group. April 12, 2019. Why are the Lyman-α and EUV fluxes important?. Lyman-α is the brightest line in the solar UV spectrum.. Lyman-α is as bright as the entire UV spectra of M dwarf stars.. Brian C. Smith, Ph.D. ,Princeton Instruments . Jason McClure, Ph.D. Princeton Instruments. Dan Heller, Ph.D. Memorial Sloan-Kettering Cancer Center. Ed Gooding, Ph.D. Princeton Instruments. An Aberration Free Spectrograph for .