collaborators

11 papers

astro-ph.GA2026

Investigating radio source population spatial characteristics of diffuse Galactic synchrotron emission in the GAMA-23 field with uGMRT Band-3

Rashmi Sagar, Abhirup Datta, Aishrila Mazumder

We present uGMRT Band-3 observations of the Galaxy and Mass Assembly (GAMA)-23 field. The observations consist of a total of 33 hours spread over 50 pointings, corresponding to $\s…

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.CO2026

Interferometric HI Intensity Mapping of the Late Time Universe with SKA-Mid

Aishrila Mazumder, Zhaoting Chen, Junaid Townsend +6

We discuss the progress towards using the SKA-Mid for interferometric neutral hydrogen (HI) intensity mapping surveys. By mapping the distribution of cosmic HI distribution through…

astro-ph.CO2026

Tracing Large-scale Structure with the MeerKLASS On-the-Fly Survey: Angular Clustering of Radio Sources at 816 MHz

Sourabh Paul, Suman Chatterjee, Keith Grainge +8

We present the first measurement of the angular two-point correlation function \(w(θ)\) of radio sources from the MeerKAT Large Area Synoptic Survey (MeerKLASS) UHF on-the-fly (OT…

astro-ph.CO2026

Mitigating residual foregrounds and systematic errors in SKA1-Low AA* EoR observations via Bayesian Gaussian Process Regression

Samit Kumar Pal, Abhirup Datta, Aishrila Mazumder +1

The redshifted 21\,cm line is an emerging tool in observational cosmology that can serve as a direct probe of the intergalactic medium throughout the cosmic timeline. However, the…

astro-ph.GA2026

Measurements of the HI intensity mapping power spectrum at low redshifts with MIGHTEE data: comparison with detected HI galaxies

Junaid Townsend, Mario G. Santos, Suman Chatterjee +6

Line intensity mapping provides a statistical approach to tracing the large-scale distribution of matter in the Universe. We apply the HI intensity mapping technique to interferome…