SARAS CD/EoR Radiometer: Design and performance of the Digital Correlation Spectrometer
B. S. Girish, K. S. Srivani, Ravi Subrahmanyan, N. Udaya Shankar,, Saurabh Singh, T. Jishnu Nambissan, Mayuri Sathyanarayana Rao, R. Somashekar, and A. Raghunathan

TL;DR
The paper presents the design and performance evaluation of a digital correlation spectrometer for the SARAS radiometer, aimed at detecting the faint 21-cm signals from cosmic dawn and reionization epochs.
Contribution
It introduces a high spectral resolution, high dynamic range digital spectrometer based on a Virtex 6 FPGA, optimized for remote deployment and RFI resilience.
Findings
Achieved about 61 kHz spectral resolution.
Demonstrated low susceptibility to radio frequency interference.
Validated capability to detect signals from cosmic dawn and reionization.
Abstract
In the currently accepted model for cosmic baryon evolution, Cosmic Dawn and the Epoch of Reionization are significant times when first light from the first luminous objects emerged, transformed and subsequently ionized the primordial gas. The 21 cm hyperfine transition of neutral hydrogen, redshifted from these cosmic times to a frequency range of 40 to 200 MHz, has been recognized as an important probe of the physics of CD/EoR. The global 21-cm signal is predicted to be a spectral distortion of a few 10's to a few 100's of mK, which is expected to be present in the cosmic radio background as a trace additive component. SARAS, Shaped Antenna measurement of the background RAdio Spectrum, is a spectral radiometer purpose designed to detect the weak 21-cm signal from CD/EoR. An important subsystem of the radiometer, the digital correlation spectrometer, is developed around a high speed…
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