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Issue DateTitleAuthor(s)Citation
20-Jan-2008 Can we detect the anisotropic shape of quasar H II regions during reionization through the small-scale redshifted 21 cm power spectrum?Sethi, S.K.; Haiman, ZoltanThe Astrophysical Journal, 2008, Vol.673, p1-13
28-Jul-2010 Carbon ionization states and the cosmic far-UV background with He II absorptionVasiliev, Evgenii O.; Sethi, S.K.; Nath, Biman B.Astrophysical Journal, 2010, Vol. 719, p1343
2005 CMBR anisotropies: from WMAP to planckSethi, S.K.Bulletin of the Astronomical Society of India, 2005, Vol.33, p349
10-Jul-2015 Confirmation of wide-field signatures in redshifted 21 cm power spectraThyagarajan, Nithyanandan; Jacobs, Daniel C; Bowman, D Judd; Deshpande, A.A.; Sethi, S.K.; Srivani, K.S.; Subrahmanyan, Ravi; Paul, Sourabh; Prabhu, T.; Udaya shankar, N.; +30 Co-authorsAstrophysical Journal Letters, 2015, Vol. 807, pL-28
Jul-2001 Constraints on ΩB, Ωm, and h from MAXIMA and BOOMERANGPadmanabhan, T.; Sethi, S.K.The Astrophysical Journal, 2001, Vol.555, p125
Aug-1998 Contribution of galaxies to the background hydrogen-ionizing fluxDevriendt, J.E.G.; Sethi, S.K.; Guiderdoni, B.; Nath, Biman B.Monthly Notices of the Royal Astronomical Society, 1998, Vol.298, p708-718
2000 Cosmic microwave background polarization data and galactic foregrounds: estimation of cosmological parametersPrunet, S.; Sethi, S.K.; Bouchet, F.R.Monthly Notices of the Royal Astronomical Society, 2000, Vol.314, p348
Dec-1999 Cosmic microwave background radiation anisotropies and data analysisSethi, S.K.Pramana, 1999, Vol.53, p951
1998 Decaying Neutrinos and Large-Scale Structure FormationBharadwaj, Somnath; Sethi, S.K.Astrophysical Journal Supplement Series, 1998, Vol.114, p37
Aug-2011 Detecting neutral hydrogen in emission at redshift z ≃ 1Kandai, Nishikanta; Sethi, S.K.; Matteo, T.D.; Croft, Rupert A.C.; Springel, V.; Jana, Anirban; Gardner, Jeffrey P.Monthly Notices of the Royal Astronomical Society, 2011, Vol.415, p2580
Apr-2009 Estimation of cosmological prameters from neutral hydrogen observations of the post-reionization epochBharadwaj, Somnath; Sethi, S.K.; Saini, T.D.Physical Review D, 2009, Vol.79, p083538
1992 Extended inflation from Kaluza-Klein theoriesMajumdar, A.S.; Sethi, S.K.Physical Review D, 1992, Vol.46, p5315
1992 Extended inflation with nonminimally coupled inflaton fieldPanchapakesan, N.; Sethi, S.K.International Journal of Modern Physics A, 1992, Vol.7, p6665
Mar-1998 Galactic dust polarized emission at high latitudes and CMB polarizationSethi, S.K.; Prunet, S.; Bouchet, F.R.Astronomy and Astrophysics, 1998, Vol.339, p187
Oct-2005 Generation of magnetic field in the pre-recombination eraGopal, Rajesh; Sethi, S.K.Monthly Notices of the Royal Astronomical Society, 2005, Vol.363, Issue 2, p521-528.
10-May-2014 H I absorption from the epoch of reionization and primordial magnetic fieldsVasiliev, Evgenii O.; Sethi, S.K.Astrophysical Journal, 2014, Vol.786, p142
2001 HI fluctuations at large redshifts: I–visibility correlationBharadwaj, Somnath; Sethi, S.K.Journal of Astrophysics and Astronomy, 2001, Vol. 22, p293-307
10-Apr-2005 High redshift intergalactic medium: Probes and physical modelsSethi, S.K.Current Science, 2005, Vol. 88, p1117-1124.
Nov-2005 HI signal from re-ionization epochSethi, S.K.Monthly Notices of the Royal Astronomical Society, 2005, Vol.363, Issue 3, p818-830.
2006 HI signal from the epoch of reionization: A pilot observation with the GMRTRoshi, Anish D.; Sethi, S.K.; Pen, U.L.; Subrahmanyan, Ravi26th meeting of the IAU, Joint Discussion 12, 21 August 2006, Prague
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