Probing the intergalactic medium during the Epoch of Reionization using 21 cm signal power spectraASTRONOMY & ASTROPHYSICSIF5.82024-07-171OA
Towards 21-cm intensity mapping at z=2.28 with uGMRT using the tapered gridded estimator - IV. Wide-band analysisMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82024-03-121OA
Extracting the Global 21-cm signal from Cosmic Dawn and Epoch of Reionization in the presence of Foreground and IonosphereMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82024-01-092OA
Towards 21-cm intensity mapping at z=2.28 with uGMRT using the tapered gridded estimator - III. Foreground removalMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82023-08-212PRE
Towards 21-cm intensity mapping at z=2.28 with uGMRT using the tapered gridded estimator - II. Cross-polarization power spectrumMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82023-01-194OA
Towards 21-cm intensity mapping at z=2.28 with uGMRT using the tapered gridded estimator I: Foreground avoidanceMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82022-08-265OA
Improving constraints on the reionization parameters using 21-cm bispectrumJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICSIF5.92022-04-2217OA
Extracting the 21-cm Power Spectrum and the reionization parameters from mock datasets using Artificial Neural NetworksMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82022-03-1711OA
Using artificial neural networks to extract the 21-cm global signal from the EDGES dataMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82021-01-229OA
First Multi-redshift Limits on Post-Epoch of Reionization 21 cm Signal from z=1.96-3.58 Using uGMRTASTROPHYSICAL JOURNAL LETTERSIF11.72021-01-1415OA
Trigger Factor in Association with the ClpP1P2 Heterocomplex of Leptospira Promotes Protease/Peptidase ActivityACS OMEGAIF4.32021-01-072OAAI
Extracting the 21 cm Global signal using artificial neural networksMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82019-11-1512OAAI
Detailed study of ELAIS N1 field with the uGMRT - II. Source properties and spectral variation of foreground power spectrum from 300-500 MHz observationsMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82019-10-0429OAAI
Detailed study of the ELAIS N1 field with the uGMRT - I. Characterizing the 325 MHz foreground for redshifted 21 cm observationsMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82019-06-1019OAAI
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