349 citations · 1.3k across the 28 of their papers we have counts for
29 papers
Refining the origins of the gamma-ray binary 1FGL J1018.6-5856
B. Marcote, M. Ribó, J. M. Paredes +2
Gamma-ray binaries are systems composed of a massive star and a compact object that exhibit emission from radio to very high energy gamma rays. They are ideal laboratories to study…
A subarcsecond near-infrared view of massive galaxies at z > 1 with Gemini Multiconjugate Adaptive Optics
M. Lacy, K. Nyland, M. Mao +14
We present images taken using the Gemini South Adaptive Optics Imager (GSAOI) with the Gemini Multiconjugate Adaptive Optics System (GeMS) in three 2 arcmin fields in the Spitz…
The First VLBI Detection of a Spiral DRAGN Core
Minnie Y. Mao, Jay M. Blanchard, Frazer Owen +8
The existence of spiral DRAGNs challenges standard galaxy formation theories. We present the first observation of 0313192, the archetypal spiral DRAGN, at VLBI resolutions. Spir…
Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [CI]
B. H. C. Emonts, M. D. Lehnert, H. Dannerbauer +9
The circumgalactic medium (CGM) of the massive Spiderweb Galaxy, a conglomerate of merging proto-cluster galaxies at z=2.2, forms an enriched interface where feedback and recycling…
Molecular Gas in the Halo Fuels the Growth of a Massive Cluster Galaxy at High Redshift
B. H. C. Emonts, M. D. Lehnert, M. Villar-Martin +19
The largest galaxies in the Universe reside in galaxy clusters. Using sensitive observations of carbon-monoxide, we show that the Spiderweb Galaxy -a massive galaxy in a distant pr…
The Discovery of a Low-Luminosity SPIRAL DRAGN
D. D. Mulcahy, M. Y. Mao, I. Mitsuishi +7
Standard galaxy formation models predict that large-scale double-lobed radio sources, known as DRAGNs, will always be hosted by elliptical galaxies. In spite of this, in recent yea…