212 citations · 396 across the 11 of their papers we have counts for
12 papers
Channel-Level Mask Guidance for Slimmable Image Compression
Chen Chen, Chenggang Wu, Yongbiao Chen +3
Learned image compression (LIC) has achieved promising rate-distortion performance, but most methods lack scalability for diverse platforms with varying computational and storage c…
Space waste: An update of the anthropogenic matter injection into Earth atmosphere
Leonard Schulz, Karl-Heinz Glassmeier, Moritz Herberhold +4
Large satellite constellations are one of the main reasons for an increasing amount of mass being brought into low Earth orbit in recent years. After end of life, the satellites, a…
A photochemical PHO network for hydrogen-dominated exoplanet atmospheres
Elspeth K. H. Lee, Shang-Min Tsai, Julianne I. Moses +3
Due to the detection of phosphine PH3 in the Solar System gas giants Jupiter and Saturn, PH3 has long been suggested to be detectable in exosolar substellar atmospheres too. Howeve…
Structure, variability, and origin of the low-latitude nightglow continuum between 300 and 1,800 nm: Evidence for HO emission in the near-infrared
Stefan Noll, John M. C. Plane, Wuhu Feng +5
The Earth's mesopause region between about 75 and 105 km is characterised by chemiluminescent emission from various lines of different molecules and atoms. This emission was and is…
Bottom-up dust nucleation theory in oxygen-rich evolved stars II. Magnesium and calcium aluminate clusters
David Gobrecht, S. Rasoul Hashemi, John M. C. Plane +3
Spinel (MgAlO) and krotite (CaAlO) are alternative candidates to alumina (AlO) as primary dust condensates in the atmospheres of oxygen-rich evolved…
ATOMIUM: Probing the inner wind of evolved O-rich stars with new, highly excited HO and OH lines
A. Baudry, K. T. Wong, S. Etoka +17
Water and the hydroxyl radical are major constituents of the envelope of O-rich late-type stars. Transitions involving energy levels that are highly excited have been observed in b…
The VLT/SPHERE view of the ATOMIUM cool evolved star sample. I. Overview: Sample characterization through polarization analysis
M. Montargès, E. Cannon, A. de Koter +32
Aims. Through the ATOMIUM project, based on an ALMA large program, we aim to present a consistent view of a sample of 17 nearby cool evolved stars (Aymptotic Giant Branch and red s…
Experimental study of the removal of excited state phosphorus atoms by HO and H: implications for the formation of PO in stellar winds
Kevin M. Douglas, David Gobrecht, John M. C. Plane
The reactions of the low-lying metastable states of atomic phosphorus, P(D) and P(P), with HO and H were studied by the pulsed laser photolysis at 248 nm of PCl…
ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars: Motivation, sample, calibration, and initial results
C. A. Gottlieb, L. Decin, A. M. S. Richards +33
This overview paper presents ATOMIUM, a Large Programme in Cycle 6 with the Atacama Large Millimeter-submillimeter Array (ALMA). The goal of ATOMIUM is to understand the dynamics a…
Bottom-up dust nucleation theory in oxygen-rich evolved stars I. Aluminium oxide clusters
David Gobrecht, John M. C. Plane, Stefan T. Bromley +3
Aluminum oxide (alumina, AlO) is a promising candidate as a primary dust condensate in the atmospheres of oxygen-rich evolved stars. Therefore, alumina \textit{seed} pa…
ATOMIUM: Halide molecules around the S-type AGB star W Aquilae
T. Danilovich, M. Van de Sande, J. M. C. Plane +36
S-type asymptotic giant branch (AGB) stars are thought to be intermediates in the evolution of oxygen- to carbon-rich AGB stars. The chemical compositions of their circumstellar en…
Dust formation in the oxygen-rich AGB star IK Tau
D. Gobrecht, I. Cherchneff, A. Sarangi +2
We model the synthesis of molecules and dust in the inner wind of the oxygen-rich Mira-type star IK Tau, by considering the effects of periodic shocks induced by the stellar pulsat…