Cardiff University | Prifysgol Caerdydd ORCA
Online Research @ Cardiff 
WelshClear Cookie - decide language by browser settings

The MeerKAT Fornax Survey

Serra, P., De Blok, W.J.G., Bryan, G.L., Colafrancesco, S., Dettmar, R.-J., Frank, B.S., Govoni, F., Józsa, G.I.G., Kraan-Korteweg, R.C., Loubser, S.I., Maccagni, F.M, Murgia, M., Oosterloo, T.A., Peletier, R.F., Pizzo, R., Ramatsoku, M., Richter, L., Smith, Matthew ORCID:, Trager, S.C., Van Gorkom, J.H. and Verheijen, M.A.W. 2016. The MeerKAT Fornax Survey. Presented at: MeerKAT Science: On the Pathway to the SKA, Stellenbosch, South Africa, 25-27 May 2016. MeerKAT Science: On the Pathway to the SKA. , vol.277 10.22323/1.277.0008

[thumbnail of 1709.01289.pdf]
PDF - Published Version
Available under License Creative Commons Attribution Non-commercial No Derivatives.

Download (1MB) | Preview


We present the science case and observations plan of the MeerKAT Fornax Survey, an HI and radio continuum survey of the Fornax galaxy cluster to be carried out with the SKA precursor MeerKAT. Fornax is the second most massive cluster within 20 Mpc and the largest nearby cluster in the southern hemisphere. Its low X-ray luminosity makes it representative of the environment where most galaxies live and where substantial galaxy evolution takes place. Fornax's ongoing growth makes it an excellent laboratory for studying the assembly of clusters, the physics of gas accretion and stripping in galaxies falling in the cluster, and the connection between these processes and the neutral medium in the cosmic web. We will observe a region of 12 deg2 reaching a projected distance of 1.5 Mpc from the cluster centre. This will cover a wide range of environment density out to the outskirts of the cluster, where gas-rich in-falling groups are found. We will: study the HI morphology of resolved galaxies down to a column density of a few times 1e+19 cm−2 at a resolution of 1 kpc; measure the slope of the HI mass function down to M(HI) 5e+5 M(sun); and attempt to detect HI in the cosmic web reaching a column density of 1e+18 cm−2 at a resolution of 10 kpc.

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: In Press
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Date of First Compliant Deposit: 6 December 2017
Last Modified: 03 Nov 2022 10:14

Actions (repository staff only)

Edit Item Edit Item


Downloads per month over past year

View more statistics