83 citations · 255 across the 8 of their papers we have counts for
8 papers
Constraining the geometry of the reflection nebula NGC 2023 with [O I]: Emission & Absorption
Bhaswati Mookerjea, Goeran Sandell, Rolf Guesten +3
We have mapped the NGC 2023 reflection nebula in the 63 and 145 micron transitions of [O I] and the 158 micron [C II] spectral lines using the heterodyne receiver upGREAT on SOFIA.…
Ionized gas in the Scutum spiral arm as traced in [N II] and [C II]
W. D. Langer, T. Velusamy, P. F. Goldsmith +5
Determining the properties of the warm ionized medium (WIM) at the leading edge of spiral arms is important for understanding its dynamics and cloud formation. The inner edge of th…
Terahertz hot electron bolometer waveguide mixers for GREAT
P. Pütz, C. E. Honingh, K. Jacobs +3
Supplementing the publications based on the first-light observations with the German Receiver for Astronomy at Terahertz frequencies (GREAT) on SOFIA, we present background informa…
The structure of hot gas in Cepheus B
B. Mookerjea, V. Ossenkopf, O. Ricken +6
By observing radiation-affected gas in the Cepheus B molecular cloud we probe whether the sequential star formation in this source is triggered by the radiation from newly formed s…
Balanced superconductor-insulator-superconductor mixer on a 9~m silicon membrane
M. P. Westig, K. Jacobs, J. Stutzki +3
We present a 380-520 GHz balanced superconductor-insulator-superconductor (SIS) mixer on a single silicon substrate. All radio-frequency (RF) circuit components are fabricated on a…
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…