Browsing by Author Dwarakanath, K.S.

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Issue DateTitleAuthor(s)Citation
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; Prabhu, T.; Srivani, K.S.; +40 Co-authorsAstrophysical Journal, 2016, Vol. 833, p 213
Mar-1995Detection of an H I disk in Hydra A?Dwarakanath, K.S.; Owen, F.N.; Van Gorkom, J.H.Astrophysical Journal Letters, 1995, Vol.442, p1-4
20-Jul-1998Detection of H I 21 centimeter absorption by the warm neutral mediumCarilli, C.L.; Dwarakanath, K.S.; Goss, W.M.Astrophysical Journal Letters, 1998, Vol.502, p.L79-L83
10-Mar-2002Detection of HI 21 centimeter line absorption in the warm neutral medium and in the outer arm of the galaxyDwarakanath, K.S.; Carilli, C.L.; Goss, W.M.Astrophysical Journal, 2002, Vol.567, p940-946
10-Jul-2009Diffuse radio emission in Abell 754Kale, Ruta; Dwarakanath, K.S.Astrophysical Journal, 2009, Vol. 699, p1883
Sep-2009Diffuse radio emission in the galaxy cluster Abell 754Kale, Ruta; Dwarakanath, K.S.ASP Conference Series, 2009, Vol.407, p237
Dec-2011Discovery of a giant radio halo in a massive merging cluster at z = 0.443Dwarakanath, K.S.; Malu, S.S.; Kale, RutaJournal of Astrophysics and Astronomy, 2011, Vol.32, p529.
Dec-2011Double relics in the outskirts of A3376: Accretion flows meet merger shocks?Kale, Ruta; Dwarakanath, K.S.; Bagchi, Joydeep; Paul, SurajitJournal of Astrophysics and Astronomy, 2011, Vol.32, p533
Sep-2005The Eridanus group of galaxies: key resultsOmar, A.; Dwarakanath, K.S.Bulletin of the Astronomical Society of India, 2005, Vol.33, p397
Dec-1994Evidence for free-free absorption from unshocked ejecta inside cas-AKassim, N.E.; Perley, R.A.; Dwarakanath, K.S.; Erickson, W.C.Bulletin of the American Astronomical Society, 1994, Vol. 26, p1394
Dec-1995Evidence for thermal absorption inside Cassiopeia AKassim, N.E.; Perley, R.A.; Dwarakanath, K.S.; Erickson, W.C.Astrophysical Journal Letters, 1995, Vol.455, pL59-L62
2002Extended extragalactic radio emissionOwen, F.N.; Ledlow, M.J.; Eilek, J.A.; Kassim, N.E.; Miller, N.A.; Dwarakanath, K.S.; Ivison, R.J.IAU Symposium, 2002, Vol.199, p171
20-Feb-2017Extragalactic peaked-spectrum radio sources at low frequenciesCallingham, J.R.; Ekers, R.D.; Gaensler, B.M.; Dwarakanath, K.S.; +20 Co-authorsThe Astrophysical Journal, 2017, Vol.836, p174
21-Nov-2014The First Murchison Widefield Array low-frequency radio observations of cluster scale non-thermal emission: the case of Abell 3667Hindson, L.; Johnston-Hollitt, M.; Dwarakanath, K.S.; Deshpande, A.A.; Prabhu, T.; Udaya Shankar, N.; Srivani, K.S.; Subrahmanyan, Ravi; +30 Co-authorsMonthly Notices of the Royal Astronomical Society, 2014, Vol. 445, p330-346
Jan-2017GaLactic and extragalactic all-sky Murchison widefield array (GLEAM) survey I: A low-frequency extragalactic catalogueHurley-Walker, N.; Dwarakanath, K.S.; Deshpande, A.A.; Prabu, T.; Udaya Shankar, N.; Srivani, K.S.; Subrahmanyan, Ravi; +40 Co-authorsMonthly Notices of the Royal Astronomical Society, 2017, Vol. 464, p1146-1167
Sep-2005Galactic halo HI clouds: recent GMRT resultsDwarakanath, K.S.Bulletin of the Astronomical Society of India, 2005, Vol.33, p347
Feb-2016The gas mass of star-forming galaxies at z≈1.3Kanekar, Nissim; Sethi, S.K.; Dwarakanath, K.S.Astrophysical Journal Letters, 2016, Vol. 818, pL28
22-Jun-2015GLEAM: The galactic and extragalactic all-sky MWA surveyWayth, R.B.; Lenc, E.; Deshpande, A.A.; Prabhu, T.; Udaya Shankar, N.; Srivani, K.S.; Subrahmanyan, Ravi; Dwarakanath, K.S.; +30 Co-authorsPublications of the Astronomical Society of Australia,2015,Vol.32, e025
Nov-2002GMRT and VLA observations of H I and OH from the Seyfert galaxy Mrk 1Omar, A.; Dwarakanath, K.S.; Rupen, M.; Anantharamaiah, K.R.Astronomy and Astrophysics, 2002, Vol.394, p405-414
2003GMRT detection of HI 21 cm associated absorption towards the z = 1.2 red quasar 3C 190Ishwara-Chandra, C.H.; Dwarakanath, K.S.; Anantharamaiah, K.R.Journal of Astrophysics and Astronomy, 2003, Vol. 24, p37-43.