activity
20022026
most citedWeak Lensing Results from the 75 Square Degree CTIO Survey

197 citations · 883 across the 26 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

MIGHTEE: The Host-Galaxy Associated Catalogue of the Radio Sources in MIGHTEE Continuum Data Release 1

C. L. Hale, J. Hamlett, I. H. Whittam +34

Radio continuum surveys provide samples of active galactic nuclei (AGN) and star forming galaxies (SFGs) to high redshifts, free of biases due to dust obscuration. However, radio d…

astro-ph.GA2026

SuperMIGHTEE : Spectral Ages of Remnant Radio Galaxy Candidates in the XMM-LSS Field

Sushant Dutta, Veeresh Singh, C. H. Ishwara Chandra +8

Remnant radio galaxies, whose lobes are no longer replenished by jets from the active galactic nucleus (AGN), offer key constraints on AGN duty cycles and the timescales of radio j…

astro-ph.GA2026

A MIGHTEE robust measurement of the star formation rate-radio correlation

Charlotte L. Jackson, Matt J. Jarvis, Imogen H. Whittam +9

Determining the relationship between star-formation rate (SFR) and the radio luminosity () is critical if we are to trace the star-formation history of the Universe dust-a…

astro-ph.GA2026★ 1 cited

MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to

Joel Hamlett, Catherine L. Hale, Matt J. Jarvis +3

Radio-AGN are observed to be more strongly clustered than non-active galaxies, though it is unclear whether this is simply due to their preference for massive host galaxies, or if…

astro-ph.GA2026★ 1 cited

MIGHTEE: The evolving radio luminosity functions of star-forming galaxies to and the cosmic history of star formation

Nijin J. Thykkathu, Matt J. Jarvis, Imogen H. Whittam +9

A key question in extragalactic astronomy is how the star-formation rate density (SFRD) evolves over cosmic time. A powerful way of addressing this question is using radio-continuu…

astro-ph.CO2026

A JWST Paschen-alpha Calibration of the Radio Luminosity-Star Formation Rate Relation at z~1.3

Nick Seymour, Catherine Hale, Imogen Whittam +17

As radio emission from normal galaxies is a dust-free tracer of star formation, tracing the star formation history of the Universe is a key goal of the SKA and ngVLA. In order to i…