PPT-Adding the s-Process to APOGEE Stellar Populations:

Author : giovanna-bartolotta | Published Date : 2017-03-18

Evolving the Line List Pushing to the Mdwarfs Verne V Smith NOAO Katia Cunha Matthew Shetrone Sten Hasselquist Diogo Souto Szabolcs Meszaros Jon Holtzman

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Adding the s-Process to APOGEE Stellar Populations:: Transcript

Evolving the Line List Pushing to the Mdwarfs Verne V Smith NOAO Katia Cunha Matthew Shetrone Sten Hasselquist Diogo Souto Szabolcs Meszaros Jon Holtzman APOGEEASPCAP Team . Michael Hayden (NMSU), Jo . Bovy. (IAS), Steve . Majewski. (. UVa. ), Jennifer Johnson (OSU), Gail . Zasowski. (JHU), Leo . Girardi. (. Padova. ), Carlos Allende-. Prieto. (IAC), Ana Garcia-Perez (. 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. Camera Installation Guide Version 1. 9 Apogee Imaging Systems Camera Installation Guide Page 2 of 25 Disclaimer Apogee Imaging Systems , Inc. assumes no liability for the use of the information con Michael Hayden (NMSU), Jo . Bovy. (IAS), Steve . Majewski. (. UVa. ), Jennifer Johnson (OSU), Gail . Zasowski. (JHU), Leo . Girardi. (. Padova. ), Carlos Allende-. Prieto. (IAC), Ana Garcia-Perez (. RADEMARKSOPYRIGHT EULA:Apogee Impose Tutorial Agfa and the Agfa rhombus are trademarks of Agfa-Gevaert N.V. or its affiliates.:APOGEE is a trademark of Agfa Graphics N.V.Those names and product names 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?. Jon Holtzman (NMSU). APOGEE team. We . want. . NEED. people to use APOGEE data, tools and documentation. Draft APOGEE DR10 documentation:. https://sdss3.org/internal/branches/v5/dr10/irspec. /. Data interfaces:. Marc Pinsonneault. Ohio State University. Collaborators:. The APOKASC . team. Melissa Ness. Marie Martig. The Need for Precision Stellar Astrophysics. Stars are important across a wide range of astrophysics. Akio K. INOUE (Osaka Sangyo University). Kousai. , . K. (Tohoku U), Iwata. , . I. (NAOJ), Matsuda. , Y. . (Caltech), . Nakamura, E. . (Tohoku U), . Horie. , M. . (Tohoku U), . Hayashino. , . T. (Tohoku U), . metallicity. gradients . in disk galaxies from . integrated stellar populations. Patricia Sánchez-. Blázquez. . And the CALIFA collaboration. Evolution of the . metallicity. gradients in cosmological simulations. G. . Fabbiano. Harvard-Smithsonian Center for Astrophysics. What are these X-ray sources?. See . Fabbiano. 1989, 2006 ARAA. L. X. >10. 37. erg s. -1. Accreting NS and BH in . binary system (XRB). . . . Sumit K. . Sarbadhicary. PITT-PACC, University of Pittsburgh. Team. - . Carles. . Badenes. (Pitt), Laura . Chomiuk. , Daniel Huizenga, Jessica Maldonado (MSU), . Damiano. . Caprioli. (U. Chicago). @. SDSSurveys. Karen . Masters . Spokesperson for the Sloan Digital Sky . Survey-IV. Haverford College/University . of Portsmouth. @. KarenLMasters. Eighteen Years of . Sloan Digital . Sky Surveys. 14 . 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.

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