A project for developing an HPC facility with PetaFlop computing capacity for conducting a real-time commensal search for Fast Radio Bursts (FRBs) and pulsars
with the GMRT is funded under the National Supercomputing Mission (NSM). The Centre for Development of Advanced Computing (CDAC) and NCRA have
signed a Memorandum of Understanding (MoU) to jointly build the data centre to host 60 of CDAC's indigenously developed Rudra servers
hosting 90 A100 GPUs, 10s TB memory and 2 PB storage. This instrument aims to discover more than a few hundred fast transient sources with host
galaxy association as well as several hundreds of pulsars over the next few years of scientific operation.
The system will be equipped to accept GMRT digitiser outputs at a rate of 25 GB/s using 32 of 10Gb fibre links and process them on a 24*7 basis.
The correlator and beamformer will form 2000 beams covering 50% of the field-of-view using phased addition of visibilities of
all the antennas within a moderate length of baselines. The time-domain event detection system searching for millisecond bursts and periodic signals up to a dispersion measure
(DM) limit of 2000 pc cm-3 over a frequency range of 300-1460 MHz is being developed in collaboration with the Oxford e-Research Centre, University of Oxford. A team for developing the Deep Learning classifier for optimising
triggers for baseband voltage capturing and imaging is formed with IIT-Palakkad and Industry partners Nvidia under
the NVIDIA AI Technology Center (NVAITC) project. The design activities for building the data centre having the required power, cooling and EMI shielding are currently undergoing at the observatory. The successful execution of this project will enable transformational, high-impact science in time-domain astronomy with the GMRT along with being a trigger for cutting-edge technology development in the country.
The Executive Board of the National Supercomputing Mission (NSM-EB) Co-Chaired by Secretary MeitY and Secretary DST have approved the establishment of an HPC facility at the GMRT funded under NSM Phase-3.