Analysis Framework for the Prompt Discovery of Compact Binary Mergers in...
We describe a stream-based analysis pipeline to detect gravitational waves from the merger of binary neutron stars, binary black holes, and neutron-star-black-hole binaries within ~ 1 minute of the...
View ArticleDetection and Removal of Artifacts in Astronomical Images [Replacement]
Astronomical images from optical photometric surveys are typically contaminated with transient artifacts such as cosmic rays, satellite trails and scattered light. We have developed and tested an...
View ArticleMaximizing the Probability of Detecting an Electromagnetic Counterpart of...
Compact binary coalescences are a promising source of gravitational waves for second-generation interferometric gravitational-wave detectors such as advanced LIGO and advanced Virgo. These are among...
View ArticleKinematics of an Ideal Fluid into a Spatially Flat Anisotropic Axisymmetric...
The Standard Cosmological Model assumes that the Universe is, on average, homogeneous and isotropic for large scales (z>1), but this principle has been questioned from the results about Cosmic...
View ArticleTemporal signatures of the Cherenkov light induced by extensive air showers...
We analyze temporal characteristics of signals from the wide field-of-view (WFOV) Cherenkov telescope (CT) detecting extensive air showers (EAS) of cosmic rays (CR) in coincidence with surface...
View ArticleAn Integrated Circuit for Radio Astronomy Correlators Supporting Large Arrays...
Radio telescopes that employ arrays of many antennas are in operation, and ever larger ones are being designed and proposed. Signals from the antennas are combined by cross-correlation. For $N$...
View ArticleA polyphase filter for many-core architectures [Replacement]
In this article we discuss our implementation of a polyphase filter for real-time data processing in radio astronomy. We describe in detail our implementation of the polyphase filter algorithm and its...
View ArticleAssessment of backgrounds of the ANAIS experiment for dark matter direct...
A large effort has been carried out to characterize the background of sodium iodide crystals within the ANAIS (Annual modulation with NaI Scintillators) project. In this paper, the background models...
View ArticleIntroduction to high-energy gamma-ray astronomy
The present issue is the first of of a two-volume review devoted to gamma-ray astronomy above 100 MeV which has witnessed considerable progress over the last 20 years. The motivations for research in...
View ArticleDeveloping Atmospheric Retrieval Methods for Direct Imaging Spectroscopy of...
Reflected light spectroscopy and photometry of cool, directly imaged extrasolar giant planets are expected to be performed in the next decade by space-based telescopes equipped with optical wavelength...
View ArticleHigh-cadence spectroscopy of M-dwarfs. I. Analysis of systematic effects in...
Understanding the sources of instrumental systematic noise is a must to improve the design of future spectrographs. In this study, we alternated observations of the well-suited pair of M-stars GJ...
View ArticleRadiative transfer with POLARIS: I. Analysis of magnetic fields through...
\textbf{Aims}: We present POLARIS (\textbf{POLA}rized \textbf{R}ad\textbf{I}ation \textbf{S}imulator), a newly developed three-dimensional Monte-Carlo radiative transfer code. POLARIS was designed to...
View ArticleAssessment of backgrounds of the ANAIS experiment for dark matter direct...
A large effort has been carried out to characterize the background of sodium iodide crystals within the ANAIS (Annual modulation with NaI Scintillators) project. In this paper, the background models...
View ArticleAssessment of backgrounds of the ANAIS experiment for dark matter direct...
A large effort has been carried out to characterize the background of sodium iodide crystals within the ANAIS (Annual modulation with NaI Scintillators) project. In this paper, the background models...
View ArticleExperience with wavefront sensor and deformable mirror interfaces for...
Recent advances in adaptive optics (AO) have led to the implementation of wide field-of-view AO systems. A number of wide-field AO systems are also planned for the forthcoming Extremely Large...
View ArticleExcitation and charge transfer in low-energy hydrogen atom collisions with...
A theoretical method for the estimation of cross sections and rates for excitation and charge transfer processes in low-energy hydrogen atom collisions with neutral atoms, based on an asymptotic...
View ArticleA supernova feedback implementation for the astrophysical simulation software...
Supernova (SN) explosions play an important role in the development of galactic structures. The energy and momentum imparted on the interstellar medium (ISM) in so called "supernova feedback" drives...
View ArticleA new angle for probing field-aligned irregularities with the Murchison...
Electron density irregularities in the ionosphere are known to be magnetically anisotropic, preferentially elongated along the lines of force. While many studies of their morphology have been...
View ArticleDirected Energy Missions for Planetary Defense [Replacement]
Directed energy for planetary defense is now a viable option and is superior in many ways to other proposed technologies, being able to defend the Earth against all known threats. This paper presents...
View ArticleTransiting Exoplanet Studies and Community Targets for JWST’s Early Release...
The James Webb Space Telescope will revolutionize transiting exoplanet atmospheric science due to its capability for continuous, long-duration observations and its larger collecting area, spectral...
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