Interim Design Report

Abrams, R.; Agarwalla, Sanjib Kumar; Alekou, A.; Andreopoulos, C.; Ankenbrandt, C.; Antusch, Stefan; Apollonio, M.; Aslaninejad, M.; Back, J. J.; Ballett, P.; Barker, G. J.; Beard, K.; Benedetto, Elena; Bennett, J.R.J.; Berg, J. Scott; Bhattacharya, S.; Blackmore, V.; Blennow, Mattias; Blondel, A.; Bogacz, Alex; Bonesini, M.; Bontoiu, C.; Booth, C.N.; Bromberg, C.; Brooks, Stephen J.; Bross, A.; Caretta, O.; Cervera-Villanueva, A.; Choubey, Sandhya; Cline, D.; Cobb, J.H.; Coloma, Pilar; Coney, L.; Cummings, M. A.C.; Davenne, T.; Gouvêa, A. de; Densham, C.; Ding, Xuefeng; Donini, A.; Dornan, Peter; Dracos, M.; Dufour, Frédéric; Eccleston, R.S.; Edgecock, R.; Efthymiopoulos, I.; Ellis, M.; Fernández‐Martínez, E.; Fernow, R.; Flanagan, G.; Gallardo, J.; Gandhi, Raj; Garoby, R.; Gavela, Belén; Geer, S.; Gilardoni, S.; Gómez-Cadenas, J.J.; Goswami, Srubabati; Graves, Van; Gupta, R.; Hanson, G.; Harrison, P. F.; Hart, T.; Hernández, P.; Huber, Patrick; Indumathi, D.; Johnson, R. P.; Johnstone, C.; Karadzhov, Y.; Kelliher, David; Kirk, H.; Kopp, Joachim; Kudenko, Y.; Kuno, Y.; Kurup, A.; Kyberd, P.; Laing, A.; Li, T.; Lindner, M.; Long, Ken; Pavón, Judith; Loveridge, P.; Machida, S.; Majumdar, Debasish; Maltoni, Michele; Martín-Albo, J.; Martini, M.; Matev, R.; McDonald, K.T.; McFarland, A.; Meloni, Davide; Mezzetto, M.; Migliozzi, P.; Mishra, S. R.; Mokhov, N.; Mondal, N. K.; Morfín, J. G.; Mori, Y.; Morozov, Vasiliy; Neuffer, D.; Ota, Toshihiko; Palladino, V.; Parke, Stephen J.; Pascoli, Silvia; Pasternak, J.; Peltoniemi, J.; Petti, R.; Planche, Thomas; Popovic, M.; Pozimski, J.; Prior, G.; Prior, Christopher; Rees, G.H.; Rigolin, S.; Roberts, Thomas J.; Roblin, Y.; Rogers, C.; Samulyak, Roman; Schwetz-Mangold, Thomas; Simos, N.; Sinha, Nita; Škoro, G.; Snopok, P.; Soler, F. J. P.; Souchlas, N.; Strait, J.; Stratakis, Diktys; Striganov, S.; Tang, J.; Thomason, J. W. G.; Tortora, L.; Tsenov, R.; Winter, W.; Witte, Holger; Yasuda, Osamu; Yoshikawa, C.; Zisman, Michael S.

doi:10.2172/1051488

Cited by 8 publications

(1 citation statement)

References 273 publications

(430 reference statements)

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“…This is an afterimage observed in pixels which in previous exposures were subjected to high flux levels. See Long (2011) for more details on persistence. Our goal is to remove any persistence signal present in our data, in order to avoid contaminating later photometry.…”

Section: Ir Datamentioning

confidence: 99%

Powerful Activity in the Bright Ages. I. A Visible/Ir Survey of High Redshift 3c Radio Galaxies and Quasars

Hilbert

Chiaberge

Kotyla

et al. 2016

ApJS

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We present new rest frame UV and visible observations of 22 high-z (1 < z < 2.5) 3C radio galaxies and QSOs obtained with the Hubble Space Telescope's (HST) Wide Field Camera 3 (WFC3) instrument. Using a custom data reduction strategy in order to assure the removal of cosmic rays, persistence signal, and other data artifacts, we have produced high-quality science-ready images of the targets and their local environments. We observe targets with regions of UV emission suggestive of active star formation. In addition, several targets exhibit highly distorted host galaxy morphologies in the rest frame visible images. Photometric analyses reveals that brighter QSOs tend to be generally redder than their dimmer counterparts. Using emission line fluxes from the literature, we estimate that emission line contamination is relatively small in the rest frame UV images for the QSOs. Using archival VLA data, we have also created radio map overlays for each of our targets, allowing for analysis of the optical and radio axes alignment. Statistical properties of the observed sampleThe average completion rate for HST/WFC3 SNAPSHOT programs is currently (Cycle 20-21) ∼ 30% (Workman et al. 2014). This is most likely due to the STScI policy that lowers the scheduling priority of targets belonging to programs that reach the 35% completion rate limit. As a result, our program was efficiently scheduled in the first part of the HST Cycle 20. Unfortunately, as soon as we reached the 35% limit, the observations stopped, and no other targets were scheduled after

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Section: Ir Datamentioning

confidence: 99%

Powerful Activity in the Bright Ages. I. A Visible/Ir Survey of High Redshift 3c Radio Galaxies and Quasars

Hilbert

Chiaberge

Kotyla

et al. 2016

ApJS

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Muon colliders and neutrino factories

Kaplan¹,

collaborations²

2015

EPJ Web of Conferences

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Abstract. Muon colliders and neutrino factories are attractive options for future facilities aimed at achieving the highest lepton-antilepton collision energies and precision measurements of Higgs boson and neutrino mixing matrix parameters. The facility performance and cost depend on how well a beam of muons can be cooled. Recent progress in muon cooling design studies and prototype tests nourishes the hope that such facilities could be built starting in the coming decade. The status of the key technologies and their various demonstration experiments is summarized. Prospects "post-P5" are also discussed.

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A new type of accelerator for charged particle cancer therapy

Edgecock¹

2013

AIP Conference Proceedings

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Abstract. Non-scaling Fixed Field Alternating Gradient accelerators (ns-FFAGs) show great potential for the acceleration of protons and light ions for the treatment of certain cancers. They have unique features as they combine techniques from the existing types of accelerators, cyclotrons and synchrotrons, and hence look to have advantages over both for this application. However, these unique features meant that it was necessary to build one of these accelerators to show that it works and to undertake a detailed conceptual design of a medical machine. Both of these have now been done. This paper will describe the concepts of this type of accelerator, show results from the proof-of-principle machine (EMMA) and described the medical machine (PAMELA).

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Interim Design Report

Cited by 8 publications

References 273 publications

Powerful Activity in the Bright Ages. I. A Visible/Ir Survey of High Redshift 3c Radio Galaxies and Quasars

Powerful Activity in the Bright Ages. I. A Visible/Ir Survey of High Redshift 3c Radio Galaxies and Quasars

Muon colliders and neutrino factories

A new type of accelerator for charged particle cancer therapy

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