467,364 research outputs found
Radio astronomical polarimetry and phase-coherent matrix convolution
A new phase-coherent technique for the calibration of polarimetric data is
presented. Similar to the one-dimensional form of convolution, data are
multiplied by the response function in the frequency domain. Therefore, the
system response may be corrected with arbitrarily high spectral resolution,
effectively treating the problem of bandwidth depolarization. As well, the
original temporal resolution of the data is retained. The method is therefore
particularly useful in the study of radio pulsars, where high time resolution
and polarization purity are essential requirements of high-precision timing. As
a demonstration of the technique, it is applied to full-polarization baseband
recordings of the nearby millisecond pulsar, PSR J0437-4715.Comment: 8 pages, 4 figures, accepted for publication in Ap
A new ultra high energy gamma ray telescope at Ohya mine
The search for ultra high energy gamma rays coming from point sources is one of the main experimental aims. A fast air shower timing system was constructed at ICRR for the study of the angular resolution of the system and operated approximately half a year. The characteristics of the surface array of Ohya air shower telescope is described
Testing general relativity with accretion onto compact objects
The X-ray emission of neutron stars and black holes presents a rich
phenomenology that can lead us to a better understanding of their nature and to
address more general physics questions: Does general relativity apply in the
strong gravity regime? Is spacetime around black holes described by the Kerr
metric? This white paper considers how we can investigate these questions by
studying reverberation mapping and quasi-periodic oscillations in accreting
systems with a combination of high-spectral and high-timing resolution. In the
near future, we will be able to study compact objects in the X-rays in a new
way: advancements in transition-edge sensors (TES) technology will allow for
electron-volt-resolution spectroscopy combined with nanoseconds-precision
timing.Comment: White paper submitted for Astro2020 Decadal Survey. 8 pages, 2
figure
Performance of Particle Flow Calorimetry at CLIC
The particle flow approach to calorimetry can provide unprecedented jet
energy resolution at a future high energy collider, such as the International
Linear Collider (ILC). However, the use of particle flow calorimetry at the
proposed multi-TeV Compact Linear Collider (CLIC) poses a number of significant
new challenges. At higher jet energies, detector occupancies increase, and it
becomes increasingly difficult to resolve energy deposits from individual
particles. The experimental conditions at CLIC are also significantly more
challenging than those at previous electron-positron colliders, with increased
levels of beam-induced backgrounds combined with a bunch spacing of only 0.5
ns. This paper describes the modifications made to the PandoraPFA particle flow
algorithm to improve the jet energy reconstruction for jet energies above 250
GeV. It then introduces a combination of timing and p_T cuts that can be
applied to reconstructed particles in order to significantly reduce the
background. A systematic study is performed to understand the dependence of the
jet energy resolution on the jet energy and angle, and the physics performance
is assessed via a study of the energy and mass resolution of W and Z particles
in the presence of background at CLIC. Finally, the missing transverse momentum
resolution is presented, and the fake missing momentum is quantified. The
results presented in this paper demonstrate that high granularity particle flow
calorimetry leads to a robust and high resolution reconstruction of jet
energies and di-jet masses at CLIC.Comment: 14 pages, 11 figure
AXTAR: Mission Design Concept
The Advanced X-ray Timing Array (AXTAR) is a mission concept for X-ray timing
of compact objects that combines very large collecting area, broadband spectral
coverage, high time resolution, highly flexible scheduling, and an ability to
respond promptly to time-critical targets of opportunity. It is optimized for
submillisecond timing of bright Galactic X-ray sources in order to study
phenomena at the natural time scales of neutron star surfaces and black hole
event horizons, thus probing the physics of ultradense matter, strongly curved
spacetimes, and intense magnetic fields. AXTAR's main instrument, the Large
Area Timing Array (LATA) is a collimated instrument with 2-50 keV coverage and
over 3 square meters effective area. The LATA is made up of an array of
supermodules that house 2-mm thick silicon pixel detectors. AXTAR will provide
a significant improvement in effective area (a factor of 7 at 4 keV and a
factor of 36 at 30 keV) over the RXTE PCA. AXTAR will also carry a sensitive
Sky Monitor (SM) that acts as a trigger for pointed observations of X-ray
transients in addition to providing high duty cycle monitoring of the X-ray
sky. We review the science goals and technical concept for AXTAR and present
results from a preliminary mission design study.Comment: 19 pages, 10 figures, to be published in Space Telescopes and
Instrumentation 2010: Ultraviolet to Gamma Ray, Proceedings of SPIE Volume
773
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