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arXiv · 1508.03100

Two Type Ia Supernovae at Redshift ~2 : Improved Classification and Redshift Determination with Medium-band Infrared Imaging

Steven A. Rodney·Adam G. Riess·Daniel M. Scolnic·David O. Jones·Shoubaneh Hemmati·Alberto Molino·Curtis McCully·Bahram Mobasher·Louis-Gregory Strolger·Or Graur·Brian Hayden·Stefano Casertano
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Abstract

We present two supernovae (SNe) discovered with the Hubble Space Telescope (HST) in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), an HST multi-cycle treasury program. We classify both objects as Type Ia SNe and find redshifts of z = 1.80+-0.02 and 2.26 +0.02 -0.10, the latter of which is the highest redshift Type Ia SN yet seen. Using light curve fitting we determine luminosity distances and find that both objects are consistent with a standard Lambda-CDM cosmological model. These SNe were observed using the HST Wide Field Camera 3 infrared detector (WFC3-IR), with imaging in both wide- and medium-band filters. We demonstrate that the classification and redshift estimates are significantly improved by the inclusion of single-epoch medium-band observations. This medium-band imaging approximates a very low resolution spectrum (lambda/delta lambda ~ 100) which can isolate broad spectral absorption features that differentiate Type Ia SNe from their most common core collapse cousins. This medium-band method is also insensitive to dust extinction and (unlike grism spectroscopy) it is not affected by contamination from the SN host galaxy or other nearby sources. As such, it can provide a more efficient - though less precise - alternative to IR spectroscopy for high-z SNe.

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Steven A. Rodney, Adam G. Riess, Daniel M. Scolnic, David O. Jones, Shoubaneh Hemmati, Alberto Molino, Curtis McCully, Bahram Mobasher, Louis-Gregory Strolger, Or Graur, Brian Hayden, Stefano Casertano. 2015-08-13. Two Type Ia Supernovae at Redshift ~2 : Improved Classification and Redshift Determination with Medium-band Infrared Imaging. https://doi.org/10.3847/0004-6256/151/2/47

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