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K2 observations of SN 2018oh reveal a two-component rising light curve for a Type Ia Supernova
Konkoly Observatory, ePESSTO, University of Arizona, K2 Mission Team, KEGS, Kepler Spacecraft Team, Pan-STARRS, DECam, ASAS-SN, PTSS/TNTS, Las Cumbres Observatory, ATLAS, C. Frohmaier
- University of California at Santa Cruz
- Space Telescope Science Institute
- Johns Hopkins University
- University of California at Berkeley
- Lawrence Berkeley National Laboratory
- Carnegie Institution of Washington
- Harvard University
- Rutgers - The State University of New Jersey, New Brunswick
- The University of Chicago
- NASA Ames Research Center
- Bay Area Environmental Research Institute
- NASA Goddard Space Flight Center
- University of Maryland, Baltimore
- University of Notre Dame
- Australian National University
- ARC Centre of Excellence for All-sky Astrophysics
- University of Maryland, College Park
- Gemini Observatory
- National Optical Astronomy Observatory
- SETI Institute
- Universidade Federal de Campina Grande
- Ball Corporation
- University of Colorado Boulder
- University of Hawai'i at Mānoa
- Queen's University Belfast
- Tsinghua University
- Lancaster University
- University of Southampton
Research output: Contribution to journal › Article › peer-review
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