PPT-Halo Metallicity in NGC 891

An XrayUV Perspective Edmund Hodges Kluck Joel Bregman University of Michigan How do baryons cycle in and out of galaxies and how does this impact galaxy evolution What happened to the missing baryons. stars. T. . Sivarani. . Indian Institute of Astrophysics, Bangalore. Chemical abundances of . metal poor stars. Probing the first stars – Stellar archeology. Looking for the fossil records of early star formation and Galaxy evolution . 5. th. Feb 2015. Introducing HALO. Contents. Halo – Rapid Deployment Demonstration Kit. Easy to Transport : . HALO RDD Kit is easy to transport – comes packed in a . pelicase. for easy transport. H.FOURATI, W.FEKI, E.DAOUD, H.ABID*, S.HADDAR*, M.A.KAMOUN, Z.MNIF AYADI Radiology service, . Suggested Reading. . Hot halo (via X-ray lines). http://. adsabs.harvard.edu. /abs/2012ApJ...756L...8G. https://arxiv.org/pdf/1211.3137.pdf. Disk-halo (via optical & UV lines). http://adsabs.harvard.edu/abs/2012ARA%26A..50..491P. Lessons from the. Illustris Simulation . Shy . Genel. Hubble Fellow. Columbia University. Genel 2016, . ApJ. in press. (. arXiv:1602.02773. ). How Environment Affects Galaxy Metallicity:. Lessons from the. Ralf Herbrich. Applied Games Group. Microsoft Research Cambridge. Microsoft Research. 1991. 1997. 1998. 2001. 2005. 2008. Overview. Why Machine Learning and Games?. Machine Learning in Video Games. Drivatars. Dana . Balser. (NRAO) . Loren Anderson (WVU), Tom . Bania. (BU), & Trey Wenger (. UVa. ). Photo: Harry Morton. Key Capabilities of the GBT. Receivers cover 0.1 to 100 GHz . Excellent point-source sensitivity. Lisa Kewley. Australian National University. Thank you to the LOC and SOC. Jeff Rich. I-Ting Ho. Rebecca Davies. Anne . Medling. Credit . goes to. Elise Hampton. David Nicholls. Results in this talk are from:. David Spergel. What has changed?. Context:. Standard cosmological model. No galaxy is an island… (John Dunne vs. Immanuel Kant). Tools:. Statistical galactic astronomy. 100s of stars -> 100,000s -> 1e9 (GAIA +LSST). Hao. Zhang. University of Maryland/University of Liverpool/Cockcroft Institute. Outline. Introduction. Motivation to Study Beam Halo. Method. Adaptive Method Using Digital Micro-mirror Device. Experiment . Introduction. L.Gatignon, 16-12-2016. The HALO program. 2. The program is very old and this is clearly visible from the code (well written, but in old Fortran, coping with severe limitations of memory) and from the input and output formats. However, Maxwell’s laws have not changed and the program has been tested and validated over more than 40 years. This outweighs most if not all of the inconveniences (in my personal view),. Lerman Non-Invasive Halo ( NIH ). . Designed to address and overcome to complications associated with the use of the Traditional Invasive Halo. . Lerman NIH. Padded carbon composite. Lerman Non-Invasive Halo ( NIH ). . Designed to address and overcome to complications associated with the use of the Traditional Invasive Halo. . Lerman NIH. Padded carbon composite. at High Redshift Universe. KenTaro. Motohara . (. IoA. , . Univsersity. of Tokyo). Gas Phase . Metallicity. Gas Phase . Metallicity. (Oxygen Abundance) is crucial to understand galaxy formation/evolution, as it traces the previous star formation history. .