activity
20062025
most citedFirst supra-THz Heterodyne Array Receivers for Astronomy with the SOFIA Observatory

81 citations · 342 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.IM2025

AMKID -- a large KID-based camera at the APEX telescope

N. Reyes, A. Weiss, S. J. C. Yates +26

The thermal emission at sub-millimeter wavelengths carries unique information in many astronomical applications ranging from disks and planet formation around young stars, to galax…

astro-ph.GA2023★ 2 cited

Observing the LMC with APEX: Signatures of Large-scale Feedback in the Molecular Clouds of 30 Doradus

Konstantin Grishunin, Axel Weiss, Dario Colombo +9

Stellar feedback plays a crucial role in star formation and the life cycle of molecular clouds. The intense star formation region 30 Doradus, which is located in the Large Magellan…

astro-ph.GA2023★ 13 cited

SOFIA FEEDBACK Survey: The Pillars of Creation in [C II] and Molecular Lines

Ramsey L. Karim, Marc W. Pound, Alexander G. G. M. Tielens +11

We investigate the physical structure and conditions of photodissociation regions (PDRs) and molecular gas within the Pillars of Creation in the Eagle Nebula using SOFIA FEEDBACK o…

astro-ph.GA2022★ 10 cited

Living on the edge of the Central Molecular Zone: G1.3 is the more likely candidate for gas accretion into the CMZ

Laura A. Busch, Denise Riquelme, Rolf Güsten +3

The 1.3deg (G1.3) and 1.6deg (G1.6) cloud complexes in the Central Molecular Zone (CMZ) of our Galaxy have been proposed to possibly reside at the intersection region of the X1 and…

astro-ph.GA2022★ 6 cited

ATLASGAL-selected massive clumps in the inner Galaxy. X. Observations of atomic carbon at 492 GHz

Min-Young Lee, Friedrich Wyrowski, Karl Menten +2

(Abridged) In this paper, we investigate the physical conditions of [CI]-traced gas in high-mass star-forming regions by analyzing APEX [CI] 492 GHz single-pointing observations of…

astro-ph.GA2021★ 33 cited

Self-absorption in [CII], CO, and HI in RCW120. Building up a geometrical and physical model of the region

S. Kabanovic, N. Schneider, V. Ossenkopf-Okada +19

Revealing the 3D dynamics of HII regions and their associated molecular clouds is important for understanding the longstanding problem as to how stellar feedback affects the densit…