Scientists

1M2H Collaboration Papers

  • Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source, Coulter et al., published in Science
  • Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis, Drout et al., published in Science
  • Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger, Shappee et al., published in Science
  • The Unprecedented Properties ot the First Electromagnetic Counterpart to a Gravitational Wave Source, Siebert et al., published in The Astrophysical Journal
  • The Old Host-Galaxy Environment of SSS17A, The First Electromagnetic Counterpart to a Gravitational Wave Source, Pan et al., published in The Astrophysical Journal
  • Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event, Kasen et al., published in Nature
  • Electromagnetic Evidence that SSS17a is the Result of a Binary Neutron Star Merger, Kilpatrick et al., published in Science
  • A Neutron Star Binary Merger Model For GW170817/GRB170817A/SSS17A, Murguia-Berthier et al., published in The Astrophysical Journal Letters

Public Data

  • Initial Survey Imaging
  • Follow-up of SSS17a
  • Follow-up Template Imaging

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Contact

Ryan Foley

  • foley@ucsc.edu
  • 510-388-3364 (cell)

Enrico Ramirez-Ruiz

  • enrico@ucolick.org
  • 831-345-4117 (cell)

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