Asosiy kontentga oʻtish
AkademIndex

Xizmatlar

N. Metcalfe

11 ta ish

Durham University

AkademScholarda batafsil koʻrsatkichlar

  1. The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample

    D. Scolnic, D. O. Jones, A. Rest +37

    MaqolaOchiq kirish201843 iqtibos
    ABI

  2. The Pan-STARRS1 Database and Data Products

    H. Flewelling, E. A. Magnier, K. C. Chambers +36

    MaqolaOchiq kirish20205 iqtibos
    ABI

  3. SUPER-LUMINOUS TYPE Ic SUPERNOVAE: CATCHING A MAGNETAR BY THE TAIL

    C. Inserra, Stephen Smartt, Anders Jerkstrand +37

    MaqolaOchiq kirish20134 iqtibos
    ABI

  4. Hydrogen-poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey

    R. Lunnan, R. Chornock, E. Berger +31

    MaqolaOchiq kirish20184 iqtibos
    ABI

  5. RAPIDLY EVOLVING AND LUMINOUS TRANSIENTS FROM PAN-STARRS1

    M. R. Drout, R. Chornock, A. M. Soderberg +33

    MaqolaOchiq kirish20144 iqtibos
    ABI

  6. The Gemini–North Multi‐Object Spectrograph: Performance in Imaging, Long‐Slit, and Multi‐Object Spectroscopic Modes

    I. Hook, Inger Jørgensen, J. R. Allington‐Smith +4

    MaqolaOchiq kirish20043 iqtibos
    ABI

  7. Pan-STARRS Photometric and Astrometric Calibration

    E. A. Magnier, Edward F. Schlafly, Douglas P. Finkbeiner +20

    MaqolaOchiq kirish20203 iqtibos
    ABI

  8. CHARACTERIZATION OF THE PRAESEPE STAR CLUSTER BY PHOTOMETRY AND PROPER MOTIONS WITH 2MASS, PPMXL, AND Pan-STARRS

    P. F. Wang, W. P. Chen, C. C. Lin +31

    Maqola20143 iqtibos
    ABI

  9. Slowly fading super-luminous supernovae that are not pair-instability explosions

    M. Nicholl, Stephen Smartt, Anders Jerkstrand +57

    MaqolaOchiq kirish20132 iqtibos
    ABI

  10. Pan-STARRS Pixel Processing: Detrending, Warping, Stacking

    C. Waters, E. A. Magnier, P. A. Price +16

    MaqolaOchiq kirish20202 iqtibos
    ABI

  11. THE PAN-STARRS1 MEDIUM-DEEP SURVEY: THE ROLE OF GALAXY GROUP ENVIRONMENT IN THE STAR FORMATION RATE VERSUS STELLAR MASS RELATION AND QUIESCENT FRACTION OUT TO<i>z</i>∼ 0.8

    Lihwai Lin, Hung-Yu Jian, S. Foucaud +26

    Maqola20142 iqtibos
    ABI