Precision measurement of the most distant spectroscopically confirmed supernova ia with the Hubble Space Telescope

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Abstract

We report the discovery of a redshift 1.71 supernova in the GOODS-North field. The Hubble Space Telescope (HST) ACS spectrum has almost negligible contamination from the host or neighboring galaxies. Although the rest-frame-sampled range is too blue to include any Si II line, a principal component analysis allows us to confirm it as a Type Ia supernova with 92% confidence. A recent serendipitous archival HST WFC3 grism spectrum contributed a key element of the confirmation by giving a host-galaxy redshift of 1.713 ± 0.007. In addition to being the most distant SN Ia with spectroscopic confirmation, this is the most distant Ia with a precision color measurement. We present the ACS WFC and NICMOS 2 photometry and ACS and WFC3 spectroscopy. Our derived supernova distance is in agreement with the prediction of ΛCDM. © 2013. The American Astronomical Society. All rights reserved.

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Rubin, D., Knop, R. A., Rykoff, E., Aldering, G., Amanullah, R., Barbary, K., … Wang, A. L. (2013). Precision measurement of the most distant spectroscopically confirmed supernova ia with the Hubble Space Telescope. Astrophysical Journal, 763(1). https://doi.org/10.1088/0004-637X/763/1/35

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