| Issue Date | Title | Author(s) | Citation |
| 1999 | Energy dependence of x-ray pulse profile of the crab pulsar | Mukerjee, K; Agrawal, P C; Paul, Biswajit; Rao, A R; Vahia, M N; Yadav, J S; Seetha, S; Kasturirangan, K | Bulletin of the Astronomical Society of India, 1999, Vol. 27, p181 |
| Feb-1998 | Observations of Cygnus X-1 during the two spectral states with the Indian X-ray Astronomy Experiment (IXAE) | Rao, A R; Agrawal, P C; Paul, Biswajit; Vahia, M N; Yadav, J S; Marar, T M K; Seetha, S; Kasturirangan, K | Astronomy and Astrophysics, 1998, Vol.330, p181-188 |
| Jan-1998 | Quasi-regular X-Ray bursts from GRS 1915+105 observed with the IXAE: possible evidence for matter disappearing into the event horizon of the black hole | Paul, Biswajit; Agrawal, P C; Rao, A R; Vahia, M N; Yadav, J S; Seetha, S; Kasturirangan, K | Astrophysical Journal, 1998, 492, pL63 |
| 1998 | Rapid X-Ray variability of CYG X-1 | Agrawal, P C; Paul, Biswajit; Rao, A R; Vahia, M N; Yadav, J S; Marar, T M K; Seetha, S; Kasturirangan, K | IAU Symposium, 1998, Vol. 188, AR No.382 |
| Apr-1997 | Rapid X-ray variability of the superluminal source GRS1915+105 | Paul, Biswajit; Agrawal, P C; Rao, A R; Vahia, M N; Yadav, J S; Marar, T M K; Seetha, S; Kasturirangan, K | Astronomy and Astrophysics, 1997, Vol.320, pL37-L40 |
| 1999 | X-ray bursts from GRS 1915+105 observed with IXAE | Yadav, J S; Agrawal, P C; Paul, Biswajit; Rao, A R; Vahia, M N; Seetha, S; Kasturirangan, K | Bulletin of the Astronomical Society of India, 1999, Vol. 27, p177 |
| 1998 | X-Ray timing studies of GRS 1915+105 | Paul, Biswajit; Agrawal, P C; Rao, A R; Vahia, M N; Yadav, J S; Marar, T M K; Seetha, S; Kasturirangan, K | IAU Symposium, 1998, Vol.188, p394 |
| Feb-1998 | X-ray variability of GRS 1915+105 during the low-hard state observed with the Indian X-ray astronomy experiment (IXAE) | Paul, Biswajit; Agrawal, P C; Rao, A R; Vahia, M N; Yadav, J S; Marar, T M K; Seetha, S; Kasturirangan, K | Astronomy and Astrophysics Supplement Series, 1998, Vol. 128, p145-151 |
