Assessment 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 ArticleThe SLUGGS survey: a new mask design to reconstruct the stellar populations...
Integral field unit spectrographs allow the 2D exploration of the kinematics and stellar populations of galaxies, although they are generally restricted to small fields-of-view. Using the large...
View ArticleThe Herschel-ATLAS Data Release 1 Paper I: Maps, Catalogues and Number Counts...
We present the first major data release of the largest single key-project in area carried out in open time with the Herschel Space Observatory. The Herschel Astrophysical Terahertz Large Area Survey...
View ArticleA Roadmap to Interstellar Flight [Replacement]
In the nearly 60 years of spaceflight we have accomplished wonderful feats of exploration that have shown the incredible spirit of the human drive to explore and understand our universe. Yet in those...
View ArticleSearch for low-mass WIMPs in a 0.6 kg day exposure of the DAMIC experiment at...
We present results of a dark matter search performed with a 0.6 kg day exposure of the DAMIC experiment at the SNOLAB underground laboratory. We measured the energy spectrum of ionization events in the...
View ArticleDesign and development of an ambient-temperature continuously-rotating...
We describe the development of an ambient-temperature continuously-rotating half-wave plate (HWP) for study of the Cosmic Microwave Background (CMB) polarization by the POLARBEAR-2 (PB2) experiment....
View ArticleBaTMAn: Bayesian Technique for Multi-image Analysis
This paper describes the Bayesian Technique for Multi-image Analysis (BaTMAn), a novel image segmentation technique based on Bayesian statistics, whose main purpose is to characterize an astronomical...
View ArticleA GMRT survey of regions towards the Taurus Molecular Cloud at 323 and 608 MHz
We present observations of three active sites of star formation in the Taurus Molecular Cloud complex taken at 323 and 608 MHz (90 and 50 cm, respectively) with the Giant Metrewave Radio Telescope...
View ArticleRegaining the FORS: making optical ground-based transmission spectroscopy of...
Transmission spectroscopy facilitates the detection of molecules and/or clouds in the atmospheres of exoplanets. Such studies rely heavily on space-based or large ground-based observatories, as one...
View ArticleAn interferometric view of binary stars
The study of binary stars is critical to apprehend many of the most interesting classes of stars. Moreover, quite often, the study of stars in binary systems is our only mean to constrain stellar...
View ArticleTraining telescope operators and support astronomers at Paranal
The operations model of the Paranal Observatory relies on the work of efficient staff to carry out all the daytime and nighttime tasks. This is highly dependent on adequate training. The Paranal...
View ArticleUncertainty Limits on Solutions of Inverse Problems over Multiple Orders of...
Astroparticle experiments such as IceCube or MAGIC require a deconvolution of their measured data with respect to the response function of the detector to provide the distributions of interest, e.g....
View ArticleCollimating Slicer for Optical Integral Field Spectroscopy
Integral Field Spectroscopy (IFS) is a technique that gives simultaneously the spectrum of each spatial sampling element in a given object field. It is a powerful tool which rearranges the data cube...
View ArticleThe ERIS Adaptive Optics System
ERIS is the new AO instrument for VLT-UT4 led by a Consortium of Max-Planck Institut fuer Extraterrestrische Physik, UK-ATC, ETH-Zurich, ESO and INAF. The ERIS AO system provides NGS mode to deliver...
View ArticleBICEP3 focal plane design and detector performance
BICEP3, the latest telescope in the BICEP/Keck program, started science observations in March 2016. It is a 550mm aperture refractive telescope observing the polarization of the cosmic microwave...
View ArticleDetectors and cooling technology for direct spectroscopic biosignature...
Direct spectroscopic biosignature characterization (hereafter "biosignature characterization") will be a major focus for future space observatories equipped with coronagraphs or starshades. Our aim in...
View ArticleThe Australian Space Eye: studying the history of galaxy formation with a...
The Australian Space Eye is a proposed astronomical telescope based on a 6U CubeSat platform. The Space Eye will exploit the low level of systematic errors achievable with a small space based telescope...
View ArticleDNest4: Diffusive Nested Sampling in C++ and Python [Replacement]
In probabilistic (Bayesian) inferences, we typically want to compute properties of the posterior distribution, describing knowledge of unknown quantities in the context of a particular dataset and the...
View ArticleA New Method for Finding Point Sources in High-energy Neutrino Data...
The IceCube collaboration has reported the first detection of high-energy astrophysical neutrinos including $\sim 50$ high-energy starting events, but no individual sources have been identified. It is...
View ArticleDynamic system classifier [Replacement]
Stochastic differential equations describe well many physical, biological and sociological systems, despite the simplification often made in their derivation. Here the usage of simple stochastic...
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