PPT-The Stellar Populations of Galaxies

HW 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. Galaxies. T.Naab. , P. Johansson, R. . Cen. , K. . Nagamine. , R. . Joung. . and J.P.O.. PPPL:, 19 Dec . 2012. ApJ.L.,. 658,710 . (2007) ApJ.,697, . 38 . (2009). ApJ.L.,699,L178 (. 2009. ). ApJ.,725,2312 . . 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 . the full SED (. from. UV to . far-IR. ) of galaxies to put . constraints. on. dust. . attenuation. and star formation . determinations. , . from. z=0 to z=2. The CIGALE code and . its. application to Herschel . dust. . attenuation. and star formation histories . at. . high. . redshift. Véronique . Buat. Laboratoire d’Astrophysique de Marseille. Elbaz’s. lectures . (. david.elbaz3.free.fr/coursJ1.html), . 12 Oct 2012. Banyuls. MODELING COUNTS AND CIBA WITH MAIN SEQUENCE AND STARBURST GALAXIES. Matthieu. Béthermin. CEA . Saclay. In collaboration with Mark Sargent, . Emanuele. . Daddi. , . Georgios. . Giuseppina. . Battaglia. Instituto. de . Astrofisica. de Canarias, Tenerife. Credit. : ESO/. H.H.Heyer. Credit. : ESO/L. . Calçada. Karachentsev. et al. 2014. Individual . Red . Giant Branch . stars. 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. Scott Croom. Julia Bryant. Joss Bland-Hawthorn. Disturbed Things Come in . small. packages. Jessica V. Bloom. Kinematics can uncover processes shaping galaxy evolution. Bloom et al., 2016 (submitted). Dainis . Dravins. – Lund . Observatory. , Sweden. www.astro.lu.se. /~. dainis. KVA. Towards the science case for E-ELT . HIRES. , Cambridge UK, September 2012. STELLAR SURFACES. … where starlight and stellar spectra originate. . Ste. llar. . P. opulations . at intermediate redshift . S. urvey. w. ith . WEAVE. Bianca Poggianti – Angela . Iovino. (co-. Leads. ). o. n . behalf. of the . StePS. team . A. Mercurio, M. . HECTOR project scientist. Australian Astronomical Observatory. University of Sydney CAASTRO. With Joss Bland-Hawthorn, Jon Lawrence, Scott Croom and the Hector team. HECTOR . . - a . massive new . IFS instrument for . Multi-. Scale . Environmental . Influences on Galaxy Gas Content. Environmental processes can influence galaxy gas content. “Small” (dark matter halo) scale. Gas replenishment. c. osmological accretion. 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).