The fractional rms pulsed amplitude is 7.4%, and the soft (1-3 kev) pulse profile contains a significant second harmonic.
We also recovered the x-raypulsations in archival 2012 xmm-newton observations, allowing us to measure a long-term pulsar spin-down rate of hz/s and to infer a pulsar surface dipole magnetic field strength of g. we show that the mass transfer in the binary is likely non-conservative, and wediscuss various scenarios for mass loss from the system.
Process variations and device aging impose profound challenges for circuit
designers. Without a precise understanding of the impact of variations on the
delay of circuit paths, guardbands, which keep
Recently, researchers have found time cells in the hippocampus that appear to
contain information about the timing of past events. Some researchers have
argued that time cells are taking a Laplace tra
This paper presents Sinsy, a deep neural network (DNN)-based singing voice
synthesis (SVS) system. In recent years, DNNs have been utilized in statistical
parametric SVS systems, and DNN-based SVS sys
We present a new analysis of the profile data from the 47 millisecond pulsars
comprising the 12.5-year data set of the North American Nanohertz Observatory
for Gravitational Waves (NANOGrav), which is
We consider a general class of individual-level, stochastic, susceptible-infected-susceptible models on a hypergraph, and focus on a mean field approximation proposed in [arruda et al.
Noisy Intermediate-Scale Quantum (NISQ) technology proposes requirements that
cannot be fully satisfied by existing Quantum Programming Languages (QPLs) or
frameworks. First, noisy qubits require repe
We present the first 2.5 years of data from the MeerKAT Pulsar Timing Array
(MPTA), part of MeerTime, a MeerKAT Large Survey Project. The MPTA aims to
precisely measure pulse arrival times from an ens
We develop a bayesian semi-parametric model for the estimating the impact of dynamic treatment rules on survival among patients diagnosed with pediatric acute myeloid leukemia (aml).
The data consist of a subset of patients enrolledin the phase iii phase iii aaml1031 clinical trial in which patients move through a sequence of four treatment courses.
High-precision measurements of the pulsar dispersion measure (DM) are
possible using telescopes with low-frequency wideband receivers. We present an
initial study of the application of the wideband ti
We model the impact of non-uniform cloud cover on transit transmission
spectra. Patchy clouds exist in nearly every solar system atmosphere, brown
dwarfs, and transiting exoplanets. Our major findings
We challenge the longstanding assumption that the mean-field approximation
for variational inference in Bayesian neural networks is severely restrictive,
and show this is not the case in deep networks
We present a simple model that uses time series momentum in order to
construct strategies that systematically outperform their benchmark. The
simplicity of our model is elegant: We only require a benc
We study infinite horizon discounted Mean Field Control (MFC) problems with
common noise through the lens of Mean Field Markov Decision Processes (MFMDP).
We allow the agents to use actions that are r
A 1+1d abelian anomaly-free chiral fermion and chiral gauge theory with a generic theta instanton term violates the charge-conjugation-time-reversal (ct) and parity parity (parity) discrete symmetries.
An analogous"strong cp problem'"is identified in a toy model in 2-dimensional spacetime.
We compare transittimings of 262 hot jupiters from the transiting giant planet explorer (tess) with the archival ephemeris and find 31 of them having significant tess timing offsets of minutes, among which wasp-161b shows the most significant offset of minutes.
Our refined ephemeris gives the transit timing at a median precision of 1.11 minutes until 2025 and 1.86 minutes until 2030. for some particular targets, timing offsets are due to tidaldissipation.
Clinical prediction models estimate an individual's risk of a particular
health outcome, conditional on their values of multiple predictors. A developed
model is a consequence of the development datas
We prove that if we use the hamming distance to compute distances between graphs, then the frechet mean (or median) graph of anensemble of inhomogeneous random graphs is obtained by thresholding the expected adjacency matrix of the ensemble.
We show that the result also holds for the sample mean (or median) when the population expected adjacency matrixis replaced with the sample mean adjacency matrix.
We analyze the timing and extent of Northern European temperature falls
during the Little Ice Age, using standard temperature reconstructions. However,
we can find little evidence of temporal dependen