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Issue DateTitleAuthor(s)Citation
Nov-2012 Fast holographic deconvolution: a new technique for Precision radio interferometrySullivan, I.S.; Morales, M.F.; Hazelton, B.J.; Deshpande, A.A.; Prabhu, T.; Roshi, Anish D.; Udaya Shankar, N.; Srivani, K.S.; Subrahmanyan, Ravi; +40 Co-authorsThe Astrophysical Journal, 2012, 759, 17,
Mar-2005 Fluctuation properties and polar emission mapping of pulsar B0834+06 at decametre wavelengthsAsgekar, Ashish; Deshpande, A.A.Monthly Notices of the Royal Astronomical Society, 2005, Vol.357, Issue 4, p1105-1112.
20-Feb-2007 Further evidence for collimated particle beams from pulsars and precessionDeshpande, A.A.; Radhakrishnan, V.Astrophysical Journal, 2007, Vol.656, p1038-1043
Dec-2013 The giant lobes of Centaurus a observed at 118 MHz with the Murchison widefield arrayMcKinley, B.; Briggs, F.; Deshpande, A.A.; Prabhu, T.; Udaya Shankar, N.; Srivani, K.S.; Subrahmanyan, Ravi; +50 Co authorsMonthly Notices of the Royal Astronomical Society, 2013, Vol. 436, p1286-1301
20-Jul-2006 H I density distribution driven by supernovae: A simulation studyHodge, Jacqueline A.; Deshpande, A.A.Astrophysical Journal, 2006, Vol.646, p232-239
Jul-2007 HI Density Distribution Driven by Supernovae:A Simulation StudyHodge, Jacqueline A.; Deshpande, A.A.ASP Conference Series, Vol. 365, 2007, p158-161
Dec-2003 Hi density distribution driven by supernova ejecta: a simulation studyHodge, Jacqueline A.; Deshpande, A.A.Bulletin of the American Astronomical Society, 2003, Vol.35, p1381
1989 IAU-URSI symposium on radio astronomical seeingDeshpande, A.A.Current Science, 1989, Vol.58, p897-898
Oct-1998 Improving pulsar distances by modelling interstellar scatteringDeshpande, A.A.; Ramachandran, R.Monthly Notices of the Royal Astronomical Society, 1998, Vol.300, p577-582
2004 Initial results from the arecibo galactic plane methanol maser surveyPandian, J.D.; Goldsmith, P.F.; Deshpande, A.A.Bulletin of the American Astronomical Society, 2004, Vol.36, p1505
Jul-2006 Instantaneous radio spectra of giant pulses from the crab pulsar from decimeter to decameter wavelengthsPopov, M.V.; Kuzmin, A.D.; Ulyanov, O.M.; Deshpande, A.A.; Ershov, A.A.; Zakharenko, V.V.; Kondratev, V.I.; Kostyuk, S.V.; Losovski, B.Ya.; Soglasnov, V.A.Astronomy Reports, 2006, Vol.50, p562-568
Nov-2010 Interferometric imaging with the 32 element Murchison wide-field arrayOrd, S.M.; Mitchell, D.A.; Wayth, R.B.; Deshpande, A.A.; Gopalakrishna, M.R.; Kamini, P.A.; Madhavi, S.; Prabhu, T.; Roshi, Anish D.; Srivani, K.S.; Udaya Shankar, N.; and 50 co-authorsPublications of the Astronomical Society of the Pacific, 2010, Vol. 122, p1353
10-Sep-2014 Inter-relationship between the two emission cones of B1237+25Maan, Yogesh; Deshpande, A.A.Astrophysical Journal, 2014, Vol.792, p 130
1995 The interstellar medium surrounding the Vela supernova remnantSaravanan, T.P.; Deshpande, A.A.; Srinivasan, G.Journal of Astrophysics and Astronomy Supplement, 1995, Vol. 16, p275 -276.
Dec-2006 Intrinsic short-timescale variability in W3(OH) hydroxyl masersRamachandran, R.; Deshpande, A.A.; Goss, W.M.Astrophysical Journal, 2006, Vol.653, p1314-1324
Feb-1999 The large scale structure of the Galactic magnetic fieldIndrani, C.; Deshpande, A.A.New Astronomy, 1999, Vol.4, p33-40
1998 The large scale structure of the Galactic magnetic fieldIndrani, C.; Deshpande, A.A.New Astronomy, 1998, Vol.4, p33
Jan-2012 Light scattering from a magnetically tunable dense random medium with weak dissipation : ferrofluidShalini, M.; Sharma, D.; Deshpande, A.A.; Mathur, Deepak; Ramachandran, Hema; Kumar, N.European Physical Journal D, 2012, Vol.66, p30
2000 Linear polarization properties of pulsars at 35 & 327 MHzAsgekar, Ashish; Deshpande, A.A.ASP Conference Series, 2000, Vol.202, p245
20-Aug-2014 The low-frequency characteristics of PSR J0437–4715 observed with the Murchison wide-field arrayBhat, N. D .R.; Ord, S.M.; Tremblay, S.E.; Deshpande, A.A.; Prabhu, T.; Udaya Shankar, N.; Srivani, K.S.; Subrahmanyan, Ravi; +25 Co-authors-
Showing results 21 to 40 of 119
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