activity
20002021
most citedWater in star-forming regions with Herschel (WISH): II. Evolution of 557 GHz 110-101 emission in low-mass protostars

273 citations · 6k across the 110 of their papers we have counts for

collaborators

110 papers

astro-ph.GA2021★ 174 cited

Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy

E. F. van Dishoeck, L. E. Kristensen, the WISH team

(abridged) Data and results from the WISH key program are summarized, designed to provide a legacy data set to address its physics and chemistry. WISH targeted ~80 sources along th…

astro-ph.EP2021★ 17 cited

The far reaches of the beta Pictoris debris disk

Markus Janson, Alexis Brandeker, Göran Olofsson +1

The nearby young star beta Pictoris hosts a rich and complex planetary system, with at least two giant planets and a nearly edge-on debris disk that contains several dynamical subp…

astro-ph.EP2021★ 203 cited

Large Interferometer For Exoplanets (LIFE): I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer mission

S. P. Quanz, M. Ottiger, E. Fontanet +68

One of the long-term goals of exoplanet science is the atmospheric characterization of dozens of small exoplanets in order to understand their diversity and search for habitable wo…

physics.pop-ph2020

First Life in the Universe

René Liseau

Here, we ask a simple question, i.e. "at what cosmic time, at the earliest, did life first appear in the universe?" Given what we know about the universe today, there may be some p…

astro-ph.SR2020★ 45 cited

Exocomets: A spectroscopic survey

I. Rebollido, C. Eiroa, B. Montesinos +18

While exoplanets are now routinely detected, the detection of small bodies in extrasolar systems remains challenging. Since the discovery of sporadic events interpreted as exocomet…

astro-ph.EP2019★ 6 cited

Upper limits on the water vapour content of the Pictoris debris disk

M. Cavallius, G. Cataldi, A. Brandeker +3

The debris disk surrounding ~Pictoris has been observed with ALMA to contain a belt of CO gas with a distinct peak at 85 au. This CO clump is thought to be the result of a…