Now showing items 1-8 of 8

    • The mass profile of the Milky Way to the virial radius from the Illustris simulation 

      Taylor, Corbin; Boylan-Kolchin, Michael; Torrey, Paul; Vogelsberger, Mark; Hernquist, Lars Eric (Oxford University Press (OUP), 2016)
      We use particle data from the Illustris simulation, combined with individual kinematic constraints on the mass of the Milky Way (MW) at specific distances from the Galactic Centre, to infer the radial distribution of the ...
    • Measuring Distances and Reddenings for a Billion Stars: Toward a 3d Dust Map From Pan-Starrs 1 

      Green, Gregory Maurice; Schlafly, Edward F.; Finkbeiner, Douglas; Jurić, Mario; Rix, Hans-Walter; Burgett, Will; Chambers, Kenneth C.; Draper, Peter W.; Flewelling, Heather; Kudritzki, Rolf Peter; Magnier, Eugene; Martin, Nicolas; Metcalfe, Nigel; Tonry, John; Wainscoat, Richard; Waters, Christopher (IOP Publishing, 2014)
      We present a method to infer reddenings and distances to stars based only on their broad-band photometry, and show how this method can be used to produce a three-dimensional (3D) dust map of the Galaxy. Our method samples ...
    • The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution 

      Juric, Mario; Ivezic, Zeljko; Brooks, Alyson; Lupton, Robert H.; Schlegel, David; Finkbeiner, Douglas; Padmanabhan, Nikhil; Bond, Nicholas; Sesar, Branimir; Rockosi, Constance M.; Knapp, Gillian R.; Gunn, James E.; Sumi, Takahiro; Schneider, Donald P.; Barentine, J. C.; Brewington, Howard J.; Brinkmann, J.; Fukugita, Masataka; Harvanek, Michael; Kleinman, S. J.; Krzesinski, Jurek; Long, Dan; Neilsen, Eric H. Jr.; Nitta, Atsuko; Snedden, Stephanie A.; York, Donald G. (IOP Publishing, 2008)
      Using the photometric parallax method we estimate the distances to ~48 million stars detected by the Sloan Digital Sky Survey (SDSS) and map their three-dimensional number density distribution in the Galaxy. The currently ...
    • The Milky Way Tomography with SDSS. II. Stellar Metallicity 

      Ivezic, Zeljko; Sesar, Branimir; Juric, Mario; Bond, Nicholas; Dalcanton, Julianne; Rockosi, Constance M.; Yanny, Brian; Newberg, Heidi J.; Beers, Timothy C.; Allende Prieto, Carlos; Wilhelm, Ron; Lee, Young Sun; Sivarani, Thirupathi; Norris, John E.; Bailer‐Jones, Coryn A. L.; Re Fiorentin, Paola; Schlegel, David; Uomoto, Alan; Lupton, Robert H.; Knapp, Gillian R.; Gunn, James E.; Covey, Kevin R.; Smith, J. Allyn; Miknaitis, Gajus; Doi, Mamoru; Tanaka, Masayuki; Fukugita, Masataka; Kent, Steve; Finkbeiner, Douglas; Munn, Jeffrey A.; Pier, Jeffrey R.; Quinn, Tom; Hawley, Suzanne; Anderson, Scott; Kiuchi, Furea; Chen, Alex; Bushong, James; Sohi, Harkirat; Haggard, Daryl; Kimball, Amy; Barentine, John; Brewington, Howard; Harvanek, Mike; Kleinman, Scott; Krzesinski, Jurek; Long, Dan; Nitta, Atsuko; Snedden, Stephanie; Lee, Brian; Harris, Hugh; Brinkmann, Jonathan; Schneider, Donald P.; York, Donald G. (IOP Publishing, 2008)
      Using effective temperature and metallicity derived from SDSS spectra for ~60,000 F- and G-type main-sequence stars (0.2 < g − r < 0.6), we develop polynomial models for estimating these parameters from the SDSS u − g and ...
    • The Milky Way Tomography with SDSS. III. Stellar Kinematics 

      Bond, Nicholas A.; Ivezic, Zeljko; Sesar, Branimir; Juric, Mario; Munn, Jeffrey A.; Kowalski, Adam; Loebman, Sarah; Roskar, Rok; Beers, Timothy C.; Dalcanton, Julianne; Rockosi, Constance M.; Yanny, Brian; Newberg, Heidi J.; Allende Prieto, Carlos; Wilhelm, Ron; Lee, Young Sun; Sivarani, Thirupathi; Majewski, Steven R.; Norris, John E.; Bailer-Jones, Coryn A. L.; Fiorentin, Paola Re; Schlegel, David; Uomoto, Alan; Lupton, Robert H.; Knapp, Gillian R.; Gunn, James E.; Covey, Kevin R.; Smith, J. Allyn; Miknaitis, Gajus; Doi, Mamoru; Tanaka, Masayuki; Fukugita, Masataka; Kent, Steve; Finkbeiner, Douglas; Quinn, Tom R.; Hawley, Suzanne; Anderson, Scott; Kiuchi, Furea; Chen, Alex; Bushong, James; Sohi, Harkirat; Haggard, Daryl; Kimball, Amy; McGurk, Rosalie; Barentine, John; Brewington, Howard; Harvanek, Mike; Kleinman, Scott; Krzesinski, Jurek; Long, Dan; Nitta, Atsuko; Snedden, Stephanie; Lee, Brian; Pier, Jeffrey R.; Harris, Hugh; Brinkmann, Jonathan; Schneider, Donald P. (IOP Publishing, 2010)
      We study Milky Way kinematics using a sample of 18.8 million main-sequence stars with r < 20 and proper-motion measurements derived from Sloan Digital Sky Survey (SDSS) and POSS astrometry, including ~170,000 stars with ...
    • A Millimeter-wave Galactic Plane Survey with the BICEP Polarimeter 

      Bierman, E. M.; Matsumura, T.; Dowell, C. D.; Keating, B. G.; Ade, P.; Barkats, D.; Barron, D.; Battle, J. O.; Bock, J. J.; Chiang, H. C.; Culverhouse, T. L.; Duband, L.; Hivon, E. F.; Holzapfel, W. L.; Hristov, V. V.; Kaufman, J. P.; Kovac, John M; Kuo, C. L.; Lange, A. E.; Leitch, E. M.; Mason, P. V.; Miller, N. J.; Nguyen, H. T.; Pryke, C.; Richter, S.; Rocha, G. M.; Sheehy, C.; Takahashi, Y. D.; Yoon, K. W. (IOP Publishing, 2011)
      In order to study inflationary cosmology and the Milky Way Galaxy's composition and magnetic field structure, Stokes I, Q, and U maps of the Galactic plane covering the Galactic longitude range 260? < ? < 340? in three ...
    • A Pan-STARRS1 View of the Bifurcated Sagittarius Stream 

      Slater, C. T.; Bell, E. F.; Schlafly, E. F.; Juric, M.; Martin, N. F.; Rix, H.-W.; Bernard, E. J.; Burgett, W. S.; Chambers, K. C.; Finkbeiner, Douglas; Goldman, B.; Kaiser, N.; Magnier, E. A.; Morganson, E. P.; Price, P. A.; Tonry, J. L. (IOP Publishing, 2012)
      We use data from the Pan-STARRS1 survey to present a panoramic view of the Sagittarius tidal stream in the southern Galactic hemisphere. As a result of the extensive sky coverage of Pan-STARRS1, the southern stream is ...
    • The QUaD Galactic Plane Survey 1: Maps And Analysis of Diffuse Emission 

      Culverhouse, T.; Ade, P.; Bock, J.; Bowden, M.; Brown, M.; Cahill, G.; Castro, P.; Church, S.; Friedman, R.; Ganga, K.; Gear, W.; Gupta, S.; Hinderks, J.; Kovac, John M; Lange, A.; Leitch, E.; Melhuish, S.; Memari, Y.; Murphy, J.; Orlando, A.; Schwarz, R.; O'Sullivan, C.; Piccirillo, L.; Pryke, C; Rajguru, N.; Rusholme, B.; Taylor, A.; Thompson, K.; Turner, A.; Wu, E.; Zemcov, M. (IOP Publishing, 2010)
      We present a survey of ∼ 800 square degrees of the galactic plane observed with the QUaD telescope. The primary product of the survey are maps of Stokes I, Q and U parameters at 100 and 150 GHz, with spatial resolution 5 ...