PPT-M Dwarfs as Targets for JWST

Courtney Dressing amp David Charbonneau HarvardSmithsonian Center for Astrophysics JWST Transit Planning Meeting March 12 2014 Funding provided by NSF GRFP awarded to CD amp NASA Kepler PSP awarded to DC. 101 Slide Set:. New Neighbors. Developed by. . the WISE Team. 0. Topic:. Nearby brown dwarfs . Concepts: . Solar neighborhood, brown dwarfs, binary systems. Missions: . WISE, Gemini, Spitzer. Coordinated by . White Dwarfs . in . SDSS . . Estimating the Mean Mass of Normal . DAs . and . DBs . Kepler. Scot . Kleinman. , Atsuko Nitta. B. árbara. Castanheira, . Detlev. Koester. Marcos Diaz . H. a. H. b. German Fairy tale by the Brothers Grimm in 1812. Inspired from old Slavic Mythology . Witches eat hearts of people and drink their blood . Vampires may have come from these myths . Original Story . Queen pricks her finger and admires the blood on the snow wishing for a child that resembled blood on the snow. R. epeatability. WFC3 – spatial . s. can mode analysis – . work in progress. Mark Swain, Pieter . Deroo. , . Kiri. . Wagstaff. IPAC . JWST workshop . 3/11/14. Jet Propulsion Laboratory, California Institute of Technology. of transiting planets. . Drake Deming. University of Maryland at College Park. K2 Science Conference, November 5, 2015. In the early days of transiting planets, we were interested in what JWST could . NIRCam. Grism Mode for Transit Observations. C. Beichman, Dimitra . Touli. ,. Gautam . Vasisht. , Roger Smith. Tom Greene. 4 March 2014. JWST grism simulator. 1. Caltech Detector Testbed. Caltech testbed (Roger Smith) projects simulated spectra and other images onto HgCdTe array to assess precision photometry for transits, weak lensing, etc. for Explorer concepts, JWST, WFIRST, EUCLID. Space . Telescope. John . Mather . JWST . Senior Project Scientist . AAAC Oct 13 2011. JWST . Science Updates. 4 (. original) . major themes: first light, galaxy assembly, star & planet formation, evolution of planetary systems. 2 Foreword The reductions in antibiotic use that have been achieved by the UK livestock sectors over the last ve years has been a great success story, and the creation of the previous sector tar 40 Balmer jump and slopes 4000 age Very young population x0000- emission lines UV slopes Old star populations in high-z objects eg Egami et al 2005 Eyles et al 2005 Richard et al 2011 Zeng e Nicholas Fantin. NGVS Meeting, . September 22. nd. , 2016. Outline. Motivation. Selecting White Dwarf Candidates. Photometric and Kinematic Properties. Halo White Dwarfs. Next Steps. Summary. Motivation. Catherine A. Clark. With Gerard T. van belle, Elliott . Horch. , and . Kaspar. Von Braun. Why M-Dwarfs?. Over 70% of stars in the galaxy are M-dwarfs. Henry et al. 2006. Winters et al. 2015. M-type stars are currently the best place to detect habitable exoplanets. How Galaxies form Stars – August 24 2016 . Robbert. Verbeke. 1. Bert . Vandenbroucke. Sven De . Rijcke. Ghent University. 1. Robbert.verbeke@ugent.be. @. Rbhfd. Λ. CDM. Standard model for cosmology. Max Millar-Blanchaer. Jet Propulsion Laboratory, California Institute of Technology. ExoSoCal. Sept. 2018. Models by . Stolker. et al. 2017. Copyright 2018 California Institute of Technology. Rajan. contained in this document is subject to export controls under the International Traffic in Arms Regulations (Title 22, CFR . Presented by Basil Jeffers. JWST Project Lead EEE Parts Engineer. JWST Worldwide Team/Partners. .