A. Goobar

TL;DR: In this paper , the authors evaluate the performance of the Integral Field Unit in the OSIRIS spectrograph on the 10 . 4 m Gran Telescopio CANARIAS (GTC) by performing absolute spectro-photometry over the entire 3600 − 10000 Å spectral range and evaluate the observational prospects and performance of MAAT on the GTC to do the following: a) study the impact of the equation of state on the kilonova light curve, and determine to what extent bounds on neutron star radii or compactness deriving from KN peak magnitudes can be identified and b) measure the Hubble constant, with precision improved by up to 40%, when both gravitational wave data and photometric-light curves are used.

TL;DR: In this article , the authors measured photometry for each of the four images of SN Zwicky, which are resolved in three WFC3/UVIS filters (F475W, F625W, and F814W) but unresolved with WFC 3/IR F160W, to find consistency between lens-model-predicted time delays (≲1 day), and delays estimated with the single epoch of Hubble Space Telescope colors (≼3.5 days).

TL;DR: The SuperNova/Acceleration Probe (SNAP) as discussed by the authors was the first NIR system to detect Type Ia supernovae between z = 1 and 1.7.

TL;DR: In this article, the first results from a systematic search for high redshift Type Ia supernovae were reported, and the light curves were all broadened (time dilated) as expected from the expanding universe hypothesis.