activity
19992025
most citedThe fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees

322 citations · 3.4k across the 103 of their papers we have counts for

collaborators
Showing 2017Show all

8 papers · 1 filter

astro-ph.SR201718 cited

A Spectroscopic and Photometric Investigation of the Mercury-Manganese Star KIC 6128830

Stefan Hümmerich, Ewa Niemczura, Przemysław Walczak +4

The advent of space-based photometry provides the opportunity for the first precise characterizations of variability in Mercury-Manganese (HgMn/CP3) stars, which might advance our…

physics.ins-det2017

Performance of a First Microhexcavity Plasma Panel Detector with Muons

Alexis Mulski, Yan Benhamou, Erez Etzion +6

The microhexcavity plasma panel detector is a type of gaseous particle detector consisting of a close-packed array of millimeter-size hexagonal cells. The cells are biased to opera…

astro-ph.SR201797 cited

Forming spectroscopic massive proto-binaries by disk fragmentation

D. M. -A. Meyer, R. Kuiper, W. Kley +2

The surroundings of massive protostars constitute an accretion disc which has numerically been shown to be subject to fragmentation and responsible for luminous accretion-driven ou…

astro-ph.GA201732 cited

Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios

T. Kettlety, J. Hesling, S. Phillipps +11

Recent work has suggested that mid-IR wavelengths are optimal for estimating the mass-to-light ratios of stellar populations and hence the stellar masses of galaxies. We compare st…

physics.ins-det2017

Microhexcavity Plasma Panel Detectors

Alexis Mulski, Daniel S. Levin, Yan Benhamou +8

Plasma panel detectors are a variant of micropattern detectors that are sensitive to ionizing radiation. They are motivated by the design and operation of plasma display panels. Th…

astro-ph.EP201734 cited

Asteroseismic masses of retired planet-hosting A-stars using SONG

D. Stello, D. Huber, F. Grundahl +9

To better understand how planets form, it is important to study planet occurrence rates as a function of stellar mass. However, estimating masses of field stars is often difficult.…