GHZ2 at z=12.3 shows a stratified ISM with coexisting density zones and needs an additional hard ionising component beyond pure radiation-bounded stellar models to match its emission lines and variability.
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4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
representative citing papers
The HI-halo mass relation follows a double power-law with turnover near 10^11.2 solar masses; centrals dominate the HI budget below ~6e12 solar masses while satellites dominate above, and photometric members boost high-mass halo HI by 1.5-3x.
The paper outlines engineering and scientific applications of antenna-level buffering in SKA-LOW, drawing on experience from LOFAR, ATCA, Parkes, and OVRO-LWA.
citing papers explorer
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Investigating ionising sources and the complex interstellar medium of GHZ2 at $z=12.3$
GHZ2 at z=12.3 shows a stratified ISM with coexisting density zones and needs an additional hard ionising component beyond pure radiation-bounded stellar models to match its emission lines and variability.
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DINGO/GAMA /WAVES: HI-halo mass relation
The HI-halo mass relation follows a double power-law with turnover near 10^11.2 solar masses; centrals dominate the HI budget below ~6e12 solar masses while satellites dominate above, and photometric members boost high-mass halo HI by 1.5-3x.
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Applications of antenna-level buffering
The paper outlines engineering and scientific applications of antenna-level buffering in SKA-LOW, drawing on experience from LOFAR, ATCA, Parkes, and OVRO-LWA.
- Actions of highly eccentric orbits