activity
19992023
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 3.5k across the 59 of their papers we have counts for

collaborators

60 papers

astro-ph.GA2023★ 3 cited

Updated Inventory of Carbon Monoxide in The Taurus Molecular Cloud

Yan Duan, Di Li, Laurent Pagani +4

The most extensive survey of carbon monoxide (CO) gas in the Taurus molecular cloud relied on CO and CO emission only, distinguishing the region w…

astro-ph.GA2022★ 5 cited

Discovery of a New Molecular Bubble-Outflow Structure in the Taurus B18 Cloud

Yan Duan, Di Li, Paul F. Goldsmith +5

Star formation can produce bubbles and outflows, as a result of stellar feedback. Outflows and bubbles inject momentum and energy into the surrounding interstellar medium, and so a…

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.GA2021★ 7 cited

Multi-wavelength observations and modelling of a quiescent cloud LDN1512

M. Saajasto, M. Juvela, C. Lefevre +2

Light scattering at near-infrared wavelengths has been used to study the optical properties of the interstellar dust grains, but these studies are limited by the assumptions on the…

astro-ph.GA2021★ 17 cited

Evolution of dust porosity through coagulation and shattering in the interstellar medium

Hiroyuki Hirashita, Vladimir B. Il'in, Laurent Pagani +1

The properties of interstellar grains, such as grain size distribution and grain porosity, are affected by interstellar processing, in particular, coagulation and shattering, which…

astro-ph.IM2020★ 4 cited

Radio telescope total power mode: improving observation efficiency

Laurent Pagani, David Frayer, Bruno Pagani +1

Aims. Radio observing efficiency can be improved by calibrating and reducing the observations in total power mode rather than in frequency, beam, or position-switching modes. Metho…