papers

Publications (18)

astro-ph.SR2026

The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III

Y. Katsukawa, J. C. del Toro Iniesta, S. K. Solanki +54

The Sunrise balloon-borne solar observatory is equipped with a one-meter aperture optical telescope, offering a unique platform for uninterrupted seeing-free observations across ul…

astro-ph.IM2018

The upGREAT dual frequency heterodyne arrays for SOFIA

C. Risacher, R. Güsten, J. Stutzk +30

We present the performance of the upGREAT heterodyne array receivers on the SOFIA telescope after several years of operations. This instrument is a multi-pixel high resolution (R >…

hep-lat2011

Progress Report on Computing Excited-State Hadron Masses in Lattice QCD

C. Morningstar, A. Bell, J. Bulava +4

Our progress in computing the spectrum of excited baryons and mesons in lattice QCD is described. Sets of spatially-extended hadron operators with a variety of different momenta ar…

hep-lat2011

Excited-State Hadrons using the Stochastic LapH Method

C. Morningstar, A. Bell, J. Bulava +4

Progress in computing the spectrum of excited baryons and mesons in lattice QCD is described. Large sets of spatially-extended hadron operators are used. A new method of stochastic…

astro-ph.IM2025

The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument description

A. Feller, A. Gandorfer, B. Grauf +46

The third science flight of the balloon-borne solar observatory Sunrise carries three entirely new post-focus science instruments with spectropolarimetric capabilities, concurrentl…

nucl-ex2020

Absence of Low-Energy Shape Coexistence in Ge: The Nonobservation of a Proposed Excited 0 Level at 639 keV

F. H. Garcia, C. Andreoiu, G. C. Ball +28

The Ge structure was investigated in a high-statistics -decay experiment of Ga using the GRIFFIN spectrometer at TRIUMF-ISAC through , -, - and…

astro-ph.IM2010

The Wave-Front Correction System for the Sunrise Balloon-Borne Solar Observatory

T. Berkefeld, W. Schmidt, D. Soltau +21

This paper describes the wave-front correction system developed for the Sunrise balloon telescope, and provides information about its in-flight performance. For the correction of l…

physics.plasm-ph2020

Time-resolved fast turbulent dynamo in a laser plasma

A. F. A. Bott, P. Tzeferacos, L. Chen +25

Understanding magnetic-field generation and amplification in turbulent plasma is essential to account for observations of magnetic fields in the universe. A theoretical framework a…

astro-ph.IM2019

The Polarimetric and Helioseismic Imager on Solar Orbiter

S. K. Solanki, J. C. del Toro Iniesta, J. Woch +121

This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the Sun from o…

astro-ph.IM2016

The upGREAT 1.9 THz multi-pixel high resolution spectrometer for the SOFIA Observatory

C. Risacher, R. Guesten, J. Stutzki +19

We present a new multi-pixel high resolution (R >10^7) spectrometer for the Stratospheric Observatory for Far-Infrared Astronomy (SOFIA). The receiver uses 2 x 7-pixel subarrays in…

hep-lat2010

The excited hadron spectrum in lattice QCD using a new variance reduction method

Colin Morningstar, A. Bell, C. Y. Chen +6

Progress in calculating the spectrum of excited baryons and mesons in lattice QCD is described. Correlation matrices of sets of spatially-extended hadron operators have been studie…

hep-ph2009

The GENIE Neutrino Monte Carlo Generator

C. Andreopoulos, A. Bell, D. Bhattacharya +13

GENIE is a new neutrino event generator for the experimental neutrino physics community. The goal of the project is to develop a `canonical' neutrino interaction physics Monte Carl…

physics.plasm-ph2020

Transport of high-energy charged particles through spatially-intermittent turbulent magnetic fields

L. E. Chen, A. F. A. Bott, P. Tzeferacos +22

Identifying the sources of the highest energy cosmic rays requires understanding how they are deflected by the stochastic, spatially intermittent intergalactic magnetic field. Here…

hep-lat2010

The excited hadron spectrum in lattice QCD using a new method of estimating quark propagation

C. Morningstar, A. Bell, J. Bulava +7

Progress in determining the spectrum of excited baryons and mesons in lattice QCD is described. Large sets of carefully-designed hadron operators have been studied and their effect…

astro-ph.GA2014

The host galaxies of X-ray selected Active Galactic Nuclei to z=2.5: Structure, star-formation and their relationships from CANDELS and Herschel/PACS

D. J. Rosario, D. H. McIntosh, A. van der Wel +60

We study the relationship between the structure and star-formation rate (SFR) of X-ray selected low and moderate luminosity active galactic nuclei (AGNs) in the two Chandra Deep Fi…

physics.ins-det2009

Fast Beam Conditions Monitor BCM1F for the CMS Experiment

A. Bell, E. Castro, R. Hall-Wilton +8

The CMS Beam Conditions and Radiation Monitoring System, BRM, will support beam tuning, protect the CMS detector from adverse beam conditions, and measure the accumulated dose clos…

physics.ins-det2018

Production and Integration of the ATLAS Insertable B-Layer

B. Abbott, J. Albert, F. Alberti +373

During the shutdown of the CERN Large Hadron Collider in 2013-2014, an additional pixel layer was installed between the existing Pixel detector of the ATLAS experiment and a new, s…

astro-ph.GA2018

The State-of-Play of Anomalous Microwave Emission (AME) Research

Clive Dickinson, Y. Ali-Haïmoud, A. Barr +30

Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range -60 GHz. AME was first detected in 1996 and recogni…