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

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 (. Ankit Sethia. 1. , Ganesh Dasika. 2. , . Mehrzad. Samadi. 1. ,. Scott Mahlke. 1. 1-University of Michigan. 2-ARM R&D Austin. 1. Introduction. 2. High Throughput – 1 . TeraFlop. . High Energy Efficiency. The University Of Michigan. 2011. 2. Vehicle: i. . 3. Vehicle: ii.. Nose. Main Chute . Separation. Bay. Main Chute Separation. 4. Vehicle: iii.. Main Chute Seperation. Aviation Bay. Aviation Bay Access Cut. 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. anomaly. An abnormal, irregular fact or occurrence. Snow in Florida may be considered an anomaly.. apogee. Highest or farthest point; climax. It is very hard to reach the apogee of Mount Everest.. Antonym- Perigee. Mark Morris. UCLA. ABSTRACT -- The . well-defined, massive disk of young stars orbiting within 0.5 pc of the Galactic black hole (GBH) is strongly tilted with respect to the Galactic plane. In the context of in situ formation mechanisms, this orientation is inherited from that of the gas disk that formed these stars on the order of 6 million years ago. The tilt can be understood by positing that clouds fall toward the GBH on near-zero angular momentum orbits and form dispersion rings as they self-intersect after . Interim Meeting. U of A Phase A2 Work Update. ORBITALS Science Team, University of Alberta. CSA HQ, St. Hubert, 2010/03/17. WP 2.1.1 Launch and Orbit. Work by Louis . Ozeke. New 8 hour period orbit with magnetic conjunctions to multiple ground segments. 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. 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:. Ankit Sethia. 1. , Ganesh Dasika. 2. , . Mehrzad. Samadi. 1. ,. Scott Mahlke. 1. 1-University of Michigan. 2-ARM R&D Austin. 1. Introduction. 2. High Throughput – 1 . TeraFlop. . High Energy Efficiency. 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. REDEFINED. no longer need to spend resources managing their residential network,. the immediate and noticeable impact on staff is the return of time and focus that can be dedicated. . to mission-critical goals; such as core infrastructure and enterprise technology projects.. 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. life appearance conditions. Call of interest. Hyper-Emblematic. project. P2IO. Expression of interest . Stellar and Planetary Formation . Keywords:. Structure and dynamics, Radiation, Magnetic fields,.