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 2020Show all

27 papers · 1 filter

astro-ph.IM20205 cited

Design and pre-flight performance of SPIDER 280 GHz receivers

E. C. Shaw, P. A. R. Ade, S. Akers +79

In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimize…

astro-ph.SR202056 cited

On the Use of Field RR Lyrae as Galactic Probes. II. A new S calibration to estimate their metallicity

J. Crestani, M. Fabrizio, V. F. Braga +33

We performed the largest and most homogeneous spectroscopic survey of field RR Lyraes (RRLs). We secured 6,300 high resolution (HR, R35,000) spectra for 143 RRLs (11…

physics.ins-det202033 cited

Characterization of SABRE crystal NaI-33 with direct underground counting

M. Antonello, I. J. Arnquist, E. Barberio +43

Ultra-pure NaI(Tl) crystals are the key element for a model-independent verification of the long standing DAMA result and a powerful means to search for the annual modulation signa…

astro-ph.SR202044 cited

PBjam: A Python package for automating asteroseismology of solar-like oscillators

M. B. Nielsen, G. R. Davies, W. H. Ball +14

Asteroseismology is an exceptional tool for studying stars by using the properties of observed modes of oscillation. So far the process of performing an asteroseismic analysis of a…

astro-ph.EP202065 cited

WASP-186 and WASP-187: two hot Jupiters discovered by SuperWASP and SOPHIE with additional observations by TESS

N. Schanche, G. Hébrard, A. Collier Cameron +15

We present the discovery of two new hot Jupiters identified from the WASP survey, WASP-186b and WASP-187b (TOI-1494.01 and TOI-1493.01). Their planetary nature was established from…

astro-ph.HE2020

Can jets make the radioactively powered emission from neutron star mergers bluer?

Lorenzo Nativi, Mattia Bulla, Stephan Rosswog +5

Neutron star mergers eject neutron-rich matter in which heavy elements are synthesised. The decay of these freshly synthesised elements powers electromagnetic transients ("macronov…