PPT-Stellar Atmospheres behind

Transiting Exoplanets Dainis Dravins 1 HansGünter Ludwig 2 Erik Dahlén 1 Martin Gustavsson 1 Hiva Pazira 1 1 Lund Observatory Sweden 2 Landessternwarte. - 201 3 Welcome to Stellar Partner Program Our partner prog ram, aims at building a select group of Partners to work together as a team, to reach the next level of success in the field of data recov Mansi M. Kasliwal (Caltech). On behalf of the. PALOMAR TRANSIENT FACTORY. The Eventful Universe. March . 18, 2010. Why “Local” Universe?. 2. The Eventful Universe/ Kasliwal . Mar 18, 2010. Gravitational Waves: . Jupiters. Fred Adams, Univ. Michigan. Extreme Solar Systems II. Jackson, Wyoming, September 2011. Hot . Jupiters. can Evaporate. HD209458b (Vidal-. Madjar. et al. 2003, 2004; Desert et al. 2008; Sing et al. 2008; . LLC. April 2013. Indian Coastal . Barge Proposal. Disclaimer. While this presentation has been prepared in good . faith . Stellar Ocean Transport, . LLC (“SOT”) does . not take responsibility for any third party representation or warranty, explicitly or implied, as to the truth, accuracy or completeness of the information in this presentation or any other information relating to it whether written, oral or in a visual or an electronic form. The presentation may include references to and summaries of valuations and reports prepared by third parties that have not been independently verified by or on behalf of . H.-W. Rix IMPRS Galaxies Course March 11, 2011. Goal:. Determine . n. *. (M. *. ,. t. age. ,[Fe. /H],. R. ). . for a population of galaxies. How many stars of what mass and metallicity . formed when and where in galaxies?. 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: . metallicity. gradients . in disk galaxies from . integrated stellar populations. Patricia Sánchez-. Blázquez. . And the CALIFA collaboration. Evolution of the . metallicity. gradients in cosmological simulations. Revision . lecture. Lecture slides available in . powerpoint. and . pdf. from. www.star.le.ac.uk. /~. mbu. /. lectures.html. Everything taught in the course is examinable…... However, here is a crib sheet of what to focus on. Distances:. Parallax Detected!. . The Problem Faced by Astronomers. [cast your mind back to the 1700s and 1800s]. There are . hundreds of thousands . of stars visible through small telescopes. Only a tiny fraction of them will display measureable heliocentric parallax -- and you don’t know which they are!. 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). Sergei . popov. Sizes and masses. 1312.3323. Radius vs. mass. 1604.07558. Results of modeling.. Old (relaxed) planets.. Colors correspond to . different fractions . of light elements.. Light elements contribution. 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. . 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:.