output
20192022
most citedMIGHTEE-HI: The baryonic Tully-Fisher relation over the last billion years

50 citations

10 papers

astro-ph.GA202224 cited

MIGHTEE-HI: the HI Size-Mass relation over the last billion years

Sambatriniaina H. A. Rajohnson, Bradley S. Frank, Anastasia A. Ponomareva +15

We present the observed HI size-mass relation of galaxies from the MIGHTEE Survey Early Science data. The high sensitivity of MeerKAT allows us to detect galaxies spanning mo…

astro-ph.GA202224 cited

The Westerbork Coma Survey: A blind, deep, high-resolution HI survey of the Coma cluster

D. Cs. Molnar, P. Serra, T. van der Hulst +11

We present the blind Westerbork Coma Survey probing the HI content of the Coma galaxy cluster with the Westerbork Synthesis Radio Telescope. The survey covers the inner 1 Mp…

astro-ph.GA202150 cited

MIGHTEE-HI: The baryonic Tully-Fisher relation over the last billion years

Anastasia A. Ponomareva, Wanga Mulaudzi, Natasha Maddox +17

Using a sample of 67 galaxies from the MIGHTEE Survey Early Science data we study the HI-based baryonic Tully-Fisher relation (bTFr), covering a period of one billion years (…

astro-ph.GA202141 cited

A MeerKAT view of pre-processing in the Fornax A group

D. Kleiner, P. Serra, F. M. Maccagni +18

We present MeerKAT neutral hydrogen (HI) observations of the Fornax A group, that is likely falling into the Fornax cluster for the first time. Our HI image is sensitive to 1.4 x 1…

astro-ph.GA202010 cited

The Evolution of the Low-Frequency Radio AGN Population to in the ELAIS N1 Field

E. F. Ocran, A. R. Taylor, M. Vaccari +4

We study the cosmic evolution of radio sources out to using a GMRT 610 MHz survey covering 1.86 deg of the ELAIS N1 field with a minimum/median rms noise 7…

astro-ph.GA202028 cited

A Wide-area GMRT 610~MHz survey of ELAIS N1 field

C. H. Ishwara-Chandra, A. R. Taylor, D. A. Green +3

In this paper we present a wide-area 610 MHz survey of the ELAIS\,N1 field with the GMRT, covering an area of 12.8 deg at a resolution of 6 arcsec and with an rms noise of $\si…