PPT-Effects of Stellar Variability:

1 28 Important for transits see next slides Transit depth R planet λ t R star λt 2 Not so important for eclipses because the eclipse is a simple difference and the stellar variability typically is slower than the eclipse . . atmospheres. a . very. . short. . introduction. Part I. Ewa Niemczura. Astronomical. . Institute. , . UWr. eniem@astro.uni.wroc.pl. Stellar. spectra. Stellar. spectra. One picture is worth 1000 words, but . Patricia . Sánchez-Blázquez. (UAM). Jairo. Mendez-Abreu (IAC). Sebastian F Sánchez (UNAM). Isabel Perez (UGR). Fabian Rosales-Ortega (UAM). And . the CALIFA collaboration. Resolved stellar . population. young stars . with . LSST. Gregory J. Herczeg. KIAA. Star Formation: . ISM/Molecular Clouds . Pre-main sequence stellar evolution. (low-mass case). HD141569, . Clampin. et al.. Classical T . Tauri. Stars. M. Reddy, A. . Livorine. , R. . Naini. , H. Sucharew, A. Vagal. University of Cincinnati Neuroscience Institute. Poster No: EP-65. Control No: 1041. Disclosures. Mahati Reddy : None. Ned Bair . US Army Corps of Engineers Cold Regions Research and Engineering Laboratory. Earth Research Institute, UC - Santa Barbara. AVPRO. 9-10AM 2/27/14. 1. Campbell. , C.: Spatial variability of slab stability and fracture properties in avalanche starting zones, M.Sc., University of . 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. Solubles. Breitling, B.J. and K.J. Herrick . POET LLC, Sioux Falls SD. ABSTRACT. METHODS. Distillers grains with . solubles. (. DDGS. ) is an ingredient that is commonly included in livestock ration formulations. Several reasons for the widespread use of DDGS include a favorable nutrient profile, competitive cost, and availability. However, as with all co-products, one reason for exclusion from ration formulation is a concern regarding variability. It was our objective to address this concern by characterizing the quality of DDGS across 27 ethanol . Ned Bair . US Army Corps of Engineers Cold Regions Research and Engineering Laboratory. Earth Research Institute, UC - Santa Barbara. AVPRO. 9-10AM 2/27/14. 1. Campbell. , C.: Spatial variability of slab stability and fracture properties in avalanche starting zones, M.Sc., University of . Key variable is . mass. of star. directly measured only for binary stars, but it determines position on main sequence. Cluster ages. Main-sequence luminosity increases . much. faster than mass. therefore massive stars use up their fuel much faster. from PROBA2/LYRA/SWAP. R. . Kariyappa. (guest investigator), . S. T. Kumar, M. Dominique, . D. . Berghmans. , L. Dame, C.L. . Pradeep. Objectives. Analyze the source of variability of. . Lyra. channels 3 and 4 . a tale of 1965. Leonid Gurvits Ken . Kellermann. JIVE and TU Delft NRAO. The Netherlands USA. w. ith contributions . by Mikhail . Larionov. and . . Alexander Midler. 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). Study Case: Al . Tadamon. Locality. Blue Nile State, Sudan . . Maha . Abdelgaffar. Gamal . Abdo. Pastoralism. Pastoralism in Sudan is a traditional way of life. It is a product of climatic and environmental factors that has become a form of natural resources use and management. It is increasingly affected by the change in temperature, shifts in rainy seasons and intense rains.. JEFFREY HALL. LOWELL OBSERVATORY, FLAGSTAFF, AZ. Project Timeline. 1988 1992 1996 2000 2004 2008 2012 . Construction/early observing. Rebuild 1. Broad survey. Solar analog survey. Rebuild 2. A/D boundary.