Hintze Centre for Astrophysical Surveys

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iPTF16fnl: a faint and fast tidal disruption event in an E+A galaxy

(2017)

Authors:

N Blagorodnova, S Gezari, T Hung, SR Kulkarni, SB Cenko, DR Pasham, L Yan, I Arcavi, S Ben-Ami, BD Bue, T Cantwell, Y Cao, AJ Castro-Tirado, R Fender, C Fremling, A Gal-Yam, AYQ Ho, A Horesh, G Hosseinzadeh, MM Kasliwal, AKH Kong, RR Laher, G Leloudas, R Lunnan, FJ Masci, K Mooley, JD Neill, P Nugent, M Powell, AF Valeev, PM Vreeswijk, R Walters, P Wozniak
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Constraints on the Progenitor of SN 2016gkg from Its Shock-cooling Light Curve

The Astrophysical Journal Letters American Astronomical Society 837:1 (2017) l2

Authors:

Iair Arcavi, Griffin Hosseinzadeh, Peter J Brown, Stephen J Smartt, Stefano Valenti, Leonardo Tartaglia, Anthony L Piro, José L Sanchez, Brent Nicholls, Berto LAG Monard, D Andrew Howell, Curtis McCully, David J Sand, John Tonry, Larry Denneau, Brian Stalder, Ari Heinze, Armin Rest, Ken W Smith, David Bishop
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The XXL survey: first results and future

Astronomische Nachrichten Wiley 338:2-3 (2017) 334-341

Authors:

M Pierre, C Adami, M Birkinshaw, Julien Devriendt, Matthew J Jarvis

Abstract:

The XXL survey currently covers two 25 deg2 patches with XMM observations of ~ 10ks. We summarise the scientific results associated with the first release of the XXL data set, that occurred mid 2016. We review several arguments for increasing the survey depth to 40 ks during the next decade of XMM operations. X-ray (z < 2) cluster, (z < 4) AGN and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi-λ observations, will lead to solid standalone cosmological constraints and provide a wealth of information on the formation and evolution of AGN, clusters and the X-ray background. In particular, it will offer a unique opportunity to pinpoint the z > 1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions.

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The most massive galaxies in clusters are already fully grown at z similar to 0.5

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 465:2 (2017) 2101-2119

Authors:

LJ Oldham, RCW Houghton, RL Davies
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Type Ibn Supernovae Show Photometric Homogeneity and Spectral Diversity at Maximum Light

The Astrophysical Journal American Astronomical Society 836:2 (2017) 158

Authors:

Griffin Hosseinzadeh, Iair Arcavi, Stefano Valenti, Curtis McCully, D Andrew Howell, Joel Johansson, Jesper Sollerman, Andrea Pastorello, Stefano Benetti, Yi Cao, S Bradley Cenko, Kelsey I Clubb, Alessandra Corsi, Gina Duggan, Nancy Elias-Rosa, Alexei V Filippenko, Ori D Fox, Christoffer Fremling, Assaf Horesh, Emir Karamehmetoglu, Mansi Kasliwal, GH Marion, Eran Ofek, David Sand, Francesco Taddia, WeiKang Zheng, Morgan Fraser, Avishay Gal-Yam, Cosimo Inserra, Russ Laher, Frank Masci, Umaa Rebbapragada, Stephen Smartt, Ken W Smith, Mark Sullivan, Jason Surace, Przemek Woźniak
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