activity
20082024
most citedPlanck early results: first assessment of the High Frequency Instrument in-flight performance

190 citations · 650 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2024★ 2 cited

Communicating the gravitational-wave discoveries of the LIGO-Virgo-KAGRA Collaboration

Hannah Middleton, Christopher P L Berry, Nicolas Arnaud +34

The LIGO-Virgo-KAGRA (LVK) Collaboration has made breakthrough discoveries in gravitational-wave astronomy, a new field that provides a different means of observing our Universe. G…

astro-ph.IM2017★ 7 cited

Correcting the extended-source calibration for the Herschel-SPIRE Fourier-Transform Spectrometer

Ivan Valtchanov, R. Hopwood, G. Bendo +20

We describe an update to the Herschel-SPIRE Fourier-Transform Spectrometer (FTS) calibration for extended sources, which incorporates a correction for the frequency-dependent far-f…

astro-ph.EP2015★ 34 cited

The EChO science case

Giovanna Tinetti, Pierre Drossart, Paul Eccleston +347

The discovery of almost 2000 exoplanets has revealed an unexpectedly diverse planet population. Observations to date have shown that our Solar System is certainly not representativ…

astro-ph.IM2014★ 31 cited

SPIRE Point Source Photometry

Chris Pearson, Tanya Lim, Chris North +11

The different algorithms appropriate for point source photometry on data from the SPIRE instrument on-board the Herschel Space Observatory, within the Herschel Interactive Processi…

astro-ph.IM2013★ 136 cited

Flux calibration of the Herschel-SPIRE photometer

G. J. Bendo, M. J. Griffin, J. J. Bock +16

We describe the procedure used to flux calibrate the three-band submillimetre photometer in the Spectral and Photometric Imaging REceiver (SPIRE) instrument on the Herschel Space O…

astro-ph.IM2013★ 74 cited

Flux Calibration of Broadband Far Infrared and Submillimetre Photometric Instruments: Theory and Application to Herschel-SPIRE

M. J. Griffin, C. E. North, B. Schulz +15

Photometric instruments operating at far infrared to millimetre wavelengths often have broad spectral passbands (central wavelength/bandwidth ~ 3 or less), especially those operati…