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Issue DateTitleAuthor(s)Citation
20-Sep-2014Study of redshifted H I from the epoch of reionization with drift scanPaul, Sourabh; Sethi, S.K.; Subrahmanyan, Ravi; Udaya Shankar, N.; Dwarakanath, K.S.; Deshpande, A.A.; Srivani, K.S.; +25 Co-authorsAstrophysical Journal, 2014, Vol.793, p 28
10-Oct-2016Low-frequency observations of linearly polarized structures in the interstellar medium near the south galactic poleLenc, E.; Deshpande, A.A.; Dwarakanath, K.S.; Paul, Sourabh; Prabu, T.; Udaya Shankar, N.; Sethi, S.K.; Srivani, K.S.; Subrahmanyan, Ravi; +50 Co-authorsAstrophysical Journal, 2016, Vol. 830, p 38
20-Dec-2016Delay spectrum with phase-tracking arrays: extracting the Hi power spectrum from the epoch of reionizationPaul, Sourabh; Sethi, S.K.; Dwarakanath, K.S.; Udaya Shankar, N.; Subrahmanyan, Ravi; Prabu, T.; Srivani, K.S.; +40 Co-authorsAstrophysical Journal, 2016, Vol. 833, p 213
10-Jul-2015Confirmation of wide-field signatures in redshifted 21 cm power spectraThyagarajan, Nithyanandan; Jacobs, Daniel C; Bowman, Judd D.; Deshpande, A.A.; Sethi, S.K.; Srivani, K.S.; Subrahmanyan, Ravi; Paul, Sourabh; Prabu, T.; Udaya Shankar, N.; +30 Co-authorsAstrophysical Journal Letters, 2015, Vol. 807, pL-28
1-May-2015Foregrounds in wide-field redshifted 21 cm power spectraThyagarajan, Nithyanandan; Paul, Sourabh; Prabu, T.; Udaya Shankar, N.; Sethi, S.K.; Srivani, K.S.; Subrahmanyan, Ravi; +25 Co-authorsAstrophysical Journal, 2015, Vol. 804, p 14
Mar-2016The Importance of wide-field foreground removal for 21 cm Cosmology: A Demonstration with early MWA epoch of reionization observationsPober, J.C.; Hazelton, B.J.; Deshpande, A.A.; Prabu, T.; Sethi, S.K.; Udaya Shankar, N.; Paul, Sourabh; Subrahmanyan, Ravi; Srivani, K.S.; +60 Co-authorsThe Astrophysical Journal, 2016, Vol.819, p 8
20-Aug-2018Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWALI, W; Paul, Sourabh; Sethi, S.K.; Udaya Shankar, N.; Subrahmanyan, Ravi; + 51 Co-authorsAstrophysical Journal, 2018, Vol. 863, p170