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The $f(R)$ halo mass function in the cosmic web

(2017)

Authors:

Francesca von Braun-Bates, Hans A Winther, David Alonso, Julien Devriendt
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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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Radiation hardness studies of AMS HV-CMOS 350 nm prototype chip HVStripV1

Journal of Instrumentation IOP Publishing 12:02 (2017) P02010

Authors:

K Kanisauskas, A Affolder, K Arndt, R Bates, M Benoit, FD Bello, A Blue, D Bortoletto, M Buckland, C Buttar, P Caragiulo, D Das, J Dopke, A Dragone, F Ehrler, V Fadeyev, Z Galloway, H Grabas, IM Gregor, P Grenier, A Grillo, B Hiti, M Hoeferkamp, LBA Hommels, BT Huffman, Jaya John, C Kenney, J Kramberger, Z Liang, I Mandic, D Maneuski, F Martinez-Mckinney, S MacMahon, L Meng, M Mikuž, D Muenstermann, R Nickerson, I Peric, P Phillips, R Plackett, F Rubbo, J Segal, S Seidel, A Seiden, I Shipsey, W Song, M Staniztki, D Su, C Tamma, R Turchetta

Abstract:

CMOS active pixel sensors are being investigated for their potential use in the ATLAS inner tracker upgrade at the HL-LHC. The new inner tracker will have to handle a significant increase in luminosity while maintaining a sufficient signal-to-noise ratio and pulse shaping times. This paper focuses on the prototype chip "HVStripV1" (manufactured in the AMS HV-CMOS 350nm process) characterization before and after irradiation up to fluence levels expected for the strip region in the HL-LHC environment. The results indicate an increase of depletion region after irradiation for the same bias voltage by a factor of ≈2.4 and ≈2.8 for two active pixels on the test chip. There was also a notable increase in noise levels from 85 e− to 386 e− and from 75 e− to 277 e− for the corresponding pixels.
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The Progenitor and Early Evolution of the Type IIb SN 2016gkg

The Astrophysical Journal Letters American Astronomical Society 836:1 (2017) l12

Authors:

L Tartaglia, M Fraser, DJ Sand, S Valenti, SJ Smartt, C McCully, JP Anderson, I Arcavi, N Elias-Rosa, L Galbany, A Gal-Yam, JB Haislip, G Hosseinzadeh, DA Howell, C Inserra, SW Jha, E Kankare, P Lundqvist, K Maguire, S Mattila, D Reichart, KW Smith, M Smith, M Stritzinger, M Sullivan, F Taddia, L Tomasella
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