Title

Date

Conclusion

continued from June 30th

I will talk about the model of stellar radiation field which we have created to predict the Interstellar radiation Field (ISRF) in the UV at any point in space within a few hundred parsecs of the Sun. I will also go through the steps that we have followed during the work.

Recently many jovian-mass planets have been detected around several nearby stars. One could expect the existence of more planets and planetisimals in these systems. Especially during the process of formation, the inter-planetary and star-planetary collisions could occur. Calculations show that at initial stages of these collisions the UV flushes are produced. The possibilities of detection will be discussed (this talk will be continued)

TAUVEX observations will be affected by the stray-light, mainly from the solar panels of GSAT. I will discuss modeling and analysis of this stray-light using the software `Radiance'.

I will present the results of various researchers on the Monte Carlo simulations of radiation transfer through dust. I will also discuss the work by seniors in our group, and my direction for the future work.

Sketches of derivations of deflection angle, effects of lensing, lensing phenomena, some applications of gravitational lensing.

I shall talk about the paper "The near-UV pulse profile and spectrum of the pulsar PSR B0656+14" by Yu. A. Shibhanov et al. (2005, Astron. Astrop., v440, p663). In the beginning, I shall give a good introduction to pulsars and their emission properties. Then, I move on to talk about the UV pulsar profiles.

The data from Tauvex/GSAT4 will be recieved at MCF/Hassan, from where the scientific part and the relevent parts of satellite telemetry will be archived on a server outside the ISRO network. An existing ISDN link would be used to transfer selected the data from that machine to IIA (whole dataset would arrive on DVDs). In this talk, I shall discuss the preliminary ideas on a quick-look and monitoring software.

I will present my study of properties of interstellar dust with emphasis on dust coagulation and thermal properties.

We will continue the introduction to the Data Pipeline Software. Various steps in running Data Pipeline will be explained and the running pipeline with the simulation data will be demonstrated.

This talk will introduce the audience to the Data Pipeline Software. In the beginning I will introduce and explain the data format for the pipeline. The various steps in running Data Pipeline will be discussed and, hopefully, the running pipeline with the simulation data will be demostrated.

This talk will introduce the audience to the Data Pipeline Software. We will discuss various steps in running Data Pipeline and demonstrate the running pipeline with the simulation data.

Active galaxies and their importance in the broader context will be introduced. Results from imaging them in the UV, including recent results from Galex will then be discussed.