Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Leiden Observatory3.6k papers
- Centre National de la Recherche ScientifiqueFR2.4k papers
- Max Planck Institute for AstronomyDE1.4k papers
- European Southern ObservatoryCL1.4k papers
- Max Planck Institute for Extraterrestrial PhysicsDE1.3k papers
- California Institute of TechnologyUS1.1k papers
- University of GroningenNL1.1k papers
- Center for Astrophysics Harvard & SmithsonianUS1k papers
- Royal ObservatoryGB942 papers
- University of AmsterdamNL941 papers
- University College LondonGB886 papers
- University of CambridgeGB870 papers
22 papers · 2 filters
The Mid-Infrared Instrument for the James Webb Space Telescope: IV. The Low Resolution Spectrometer
S. Kendrew, S. Scheithauer, P. Bouchet +13
The Low Resolution Spectrometer of the MIRI, which forms part of the imager module, will provide R~100 long-slit and slitless spectroscopy from 5 to 12 micron. The design is optimi…
The Hera Saturn Entry Probe Mission
O. Mousis, D. H. Atkinson, T. Spilker +41
The Hera Saturn entry probe mission is proposed as an M--class mission led by ESA with a contribution from NASA. It consists of one atmospheric probe to be sent into the atmosphere…
Next Generation Very Large Array Memo No. 5: Science Working Groups -- Project Overview
C. L. Carilli, M. McKinnon, J. Ott +17
We summarize the design, capabilities, and some of the priority science goals of a next generation Very Large Array (ngVLA). The ngVLA is an interferometric array with 10x larger e…
Sapporo2: A versatile direct -body library
Jeroen Bédorf, Evghenii Gaburov, Simon Portegies Zwart
Astrophysical direct -body methods have been one of the first production algorithms to be implemented using NVIDIA's CUDA architecture. Now, almost seven years later, the GPU is…
The prototype detection unit of the KM3NeT detector
KM3NeT Collaboration, S. Adrián-Martínez, M. Ageron +246
A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80km offshore the Italian coast. KM3NeT in its final configuration will conta…
The JCMT Gould Belt Survey: A Quantitative Comparison Between SCUBA-2 Data Reduction Methods
S. Mairs, D. Johnstone, H. Kirk +18
Performing ground-based submillimetre observations is a difficult task as the measurements are subject to absorption and emission from water vapour in the Earth's atmosphere and ti…
The ASKAP/EMU Source Finding Data Challenge
A. M. Hopkins, M. T. Whiting, N. Seymour +31
The Evolutionary Map of the Universe (EMU) is a proposed radio continuum survey of the Southern Hemisphere up to declination +30 deg., with the Australian Square Kilometre Array Pa…
The LOFAR Multifrequency Snapshot Sky Survey (MSSS) I. Survey description and first results
G. H. Heald, R. F. Pizzo, E. Orrú +147
We present the Multifrequency Snapshot Sky Survey (MSSS), the first northern-sky LOFAR imaging survey. In this introductory paper, we first describe in detail the motivation and de…
The Mid-Infrared Instrument for the James Webb Space Telescope, X. Operations and Data Reduction
Karl D. Gordon, C. H. Chen, Rachel E. Anderson +26
We describe the operations concept and data reduction plan for the Mid- Infrared Instrument (MIRI) for the James Webb Space Telescope (JWST). The overall JWST operations concept is…
The Mid-Infrared Instrument for JWST, II: Design and Build
G. S. Wright, David Wright, G. B. Goodson +70
The Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) provides measurements over the wavelength range 5 to 28.5 microns. MIRI has, within a single 'package',…
The Mid-Infrared Instrument for the James Webb Space Telescope I: Introduction
G. H. Rieke, G. S. Wright, T. Boeker +15
MIRI (the Mid-Infrared Instrument for the James Webb Space Telescope (JWST)) operates from 5 to 28.5 microns and combines over this range: 1.) unprecedented sensitivity levels; 2.)…
How Astronomers View Education and Public Outreach: An Exploratory Study
Lisa Dang, Pedro Russo
Over the past few years, there have been a few studies on the development of an interest in science and scientists' views on public outreach. Yet, to date, there has been no global…
Machine Learning based photometric redshifts for the KiDS ESO DR2 galaxies
Stefano Cavuoti, Massimo Brescia, Crescenzo Tortora +9
We estimated photometric redshifts (zphot) for more than 1.1 million galaxies of the ESO Public Kilo-Degree Survey (KiDS) Data Release 2. KiDS is an optical wide-field imaging surv…
Calibrating the absolute amplitude scale for air showers measured at LOFAR
A. Nelles, J. R. Hörandel, T. Karskens +74
Air showers induced by cosmic rays create nanosecond pulses detectable at radio frequencies. These pulses have been measured successfully in the past few years at the LOw Frequency…
The General Single-Dish Data Format: A Retrospective
Tim Jenness, Elizabeth B. Stobie, Ronald J. Maddalena +5
The General Single-Dish Data format (GSDD) was developed in the mid-1980s as a data model to support centimeter, millimeter and submillimeter instrumentation at NRAO, JCMT, the Uni…
Laboratory Photo-chemistry of PAHs: Ionization versus Fragmentation
Junfeng Zhen, Pablo Castellanos, Daniel M. Paardekooper +5
Interstellar polycyclic aromatic hydrocarbons (PAHs) are expected to be strongly processed by vacuum ultraviolet photons. Here, we report experimental studies on the ionization and…
An Overview of the 2014 ALMA Long Baseline Campaign
ALMA Partnership, E. B. Fomalont, C. Vlahakis +246
A major goal of the Atacama Large Millimeter/submillimeter Array (ALMA) is to make accurate images with resolutions of tens of milliarcseconds, which at submillimeter (submm) wavel…
The ALMA Band 9 receiver - Design, construction, characterization, and first light
A. M. Baryshev, R. Hesper, F. P. Mena +24
We describe the design, construction, and characterization of the Band 9 heterodyne receivers (600-720 GHz) for the Atacama Large Millimeter / submillimeter Array (ALMA). The ALMA…
SETI reloaded, Next Generation Radio Telescopes, Transients and Cognitive Computing
Michael A. Garrett
The Search for Extra-terrestrial Intelligence (SETI) using radio telescopes is an area of research that is now more than 50 years old. Thus far, both targeted and wide-area surveys…
Preliminary design of the full-Stokes UV and visible spectropolarimeter for UVMag/Arago
Martin Pertenais, Coralie Neiner, Laurent Pares +3
The UVMag consortium proposed the space mission project Arago to ESA at its M4 call. It is dedicated to the study of the dynamic 3D environment of stars and planets. This space mis…
The SFXC software correlator for Very Long Baseline Interferometry: Algorithms and Implementation
A. Keimpema, M. M. Kettenis, S. V. Pogrebenko +13
In this paper a description is given of the SFXC software correlator, developed and maintained at the Joint Institute for VLBI in Europe (JIVE). The software is designed to run on…
Fiber scrambling for high-resolution spectrographs. II. A double fiber scrambler for Keck Observatory
Julien F. P. Spronck, Debra A. Fischer, Zachary Kaplan +4
We have designed a fiber scrambler as a prototype for the Keck HIRES spectrograph, using double scrambling to stabilize illumination of the spectrometer and a pupil slicer to incre…