activity
20042017
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 1.6k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.IM2017★ 18 cited

Data processing pipeline for Herschel HIFI

R. F. Shipman, S. F. Beaulieu, D. Teyssier +26

{Context}. The HIFI instrument on the Herschel Space Observatory performed over 9100 astronomical observations, almost 900 of which were calibration observations in the course of t…

astro-ph.SR2014★ 3 cited

The origin of organic emission in NGC 2071

T. A. van Kempen, C. McCoey, S. Tisi +2

Context: The physical origin behind organic emission in embedded low-mass star formation has been fiercely debated in the last two decades. A multitude of scenarios have been propo…

astro-ph.SR2014★ 42 cited

The hot core towards the intermediate mass protostar NGC7129 FIRS 2: Chemical similarities with Orion KL

A. Fuente, J. Cernicharo, P. Caselli +8

NGC 7129 FIRS 2 (hereafter FIRS 2) is an intermediate-mass (2 to 8 Msun) protostar located at a distance of 1250 pc. High spatial resolution observations are required to resolve th…

astro-ph.GA2013★ 48 cited

Deuterated water in the solar-type protostars NGC 1333 IRAS 4A and IRAS 4B

A. Coutens, C. Vastel, S. Cabrit +19

Aims. The aim of this paper is to study deuterated water in the solar-type protostars NGC1333 IRAS4A and IRAS4B, to compare their HDO abundance distribution with other star-forming…

astro-ph.GA2013★ 47 cited

Herschel-HIFI observations of high-J CO and isotopologues in star-forming regions: from low- to high-mass

I. San Jose-Garcia, J. C. Mottram, L. E. Kristensen +9

Context; Our understanding of the star formation process has traditionally been confined to certain mass or luminosity boundaries because most studies focus only on low-, intermedi…

astro-ph.SR2012★ 47 cited

OH far-infrared emission from low- and intermediate-mass protostars surveyed with Herschel-PACS

S. F. Wampfler, S. Bruderer, A. Karska +10

OH is a key species in the water chemistry of star-forming regions, because its presence is tightly related to the formation and destruction of water. This paper presents OH observ…