activity
20062016
most citedFirst observations with CONDOR, a 1.5 THz heterodyne receiver

40 citations · 182 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2016★ 11 cited

Analysis of antenna position measurements and weather station network data during the ALMA Long Baseline Campaign of 2015

Todd R. Hunter, Robert Lucas, Dominique Broguiere +5

In a radio interferometer, the determination of geometrical antenna positions relies on accurate calibration of the dry and wet delay of the atmosphere above each antenna. For the…

astro-ph.GA2010★ 14 cited

Photon Dominated Regions in NGC 3603

M. Röllig, C. Kramer, C. Rajbahak +32

Aims: We aim at deriving the excitation conditions of the interstellar gas as well as the local FUV intensities in the molecular cloud surrounding NGC 3603 to get a coherent pictur…

astro-ph.GA2009★ 16 cited

The molecular environment of the massive star forming region NGC 2024: Multi CO transition analysis

M. Emprechtinger, M. C. Wiedner, R. Simon +10

NGC 2024, a sites of massive star formation, have complex internal structures caused by cal heating by young stars, outflows, and stellar winds. These complex cloud structures lead…

astro-ph2008★ 36 cited

Submillimeter Line Emission from LMC N159W: a Dense, Clumpy PDR in a Low Metallicity Environment

J. L. Pineda, N. Mizuno, J. Stutzki +30

Star formation at earlier cosmological times takes place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation…

astro-ph2007★ 31 cited

12CO 4-3 and [CI] 1-0 at the centers of NGC 4945 and Circinus

M. Hitschfeld, M. Aravena, C. Kramer +30

Studying molecular gas in the central regions of the star burst galaxies NGC4945 and Circinus enables us to characterize the physical conditions and compare them to previous local…

astro-ph2007★ 34 cited

Clumpy photon-dominated regions in Carina. I. [CI] and mid-J CO lines in two 4'x4' fields

C. Kramer, M. Cubick, M. Roellig +31

The Carina region is an excellent astrophysical laboratory for studying the feedback mechanisms of newly born, very massive stars within their natal giant molecular clouds (GMCs) a…