UV Astronomy ASTROSAT/UVIT

UV Astronomy ASTROSAT/UVIT

UV Astronomy 2014-2020 Jayant Murthy Indian Institute of Astrophysics [email protected] [email protected] http://www.iiap.res.in June 8, 2010 UV Astronomy 1 Goals Lessons learned from TAUVEX. Student built satellites. UV Astronomy in the next decade. June 8, 2010 UV Astronomy 2 TAUVEX Set of three UV imagers with 20 cm mirrors. First proposed in late 1970s. Planned for Spectrum X Gamma Indefinitely postponed. Proposed for ISRO launch in 2001. June 8, 2010 UV Astronomy 3 TAUVEX Timeline Then ISRO Chairman came to Israel. Science Minister went to India. Signed on Dec. 25, 2003. Intended for 2005 launch. Progressive delays. Original proponents retired/left. Mounted onto spacecraft in Nov. 2009. Taken off spacecraft in Dec. 2009. June 8, 2010 UV Astronomy 4 Current Status Promised another launch by ISRO. Delays in communications between ISA and ISRO. Delays in ISRO launches. Status highly uncertain. June 8, 2010 UV Astronomy 5 ISRO Launch Opportunities Two types of launches actively encouraged. Commercial launches. Student launches. Small satellite slots effectively booked for the next 3 years. Free launches and support for science likely to be minimal. June 8, 2010 UV Astronomy 6 Student options First was AnuSat. Ham radio beacon. Studsat. Group of engineering colleges. To be launched with the next PSLV. Pratham: IIT (Bombay) – upper atmosphere work. Jugnu: IIT (Kanpur) – remote sensing. June 8, 2010 UV Astronomy 7 GALEX GALEX status FUV power supply has failed. Carrying on with NUV. Completed most of all-sky survey. AIS fields with 100 – 300 second exposure. Excludes Galactic plane and other bright regions. Magellanic Clouds. Orion. June 8, 2010 UV Astronomy 8 Diffuse sky with GALEX June 8, 2010 UV Astronomy 9 COS/STIS High resolution spectroscopy (1200 – 3200 Å). R from 2,000 – 40,000. June 8, 2010 UV Astronomy 10 SPEAR/FIMS UCB/Korea collaboration. Two imaging spectrographs. Spectral images of sky. EUV detector did not work properly. June 8, 2010 UV Astronomy 11 WSO/UV Echelle spectrograph R = 20,000 Long Slit Spectrograph. R = 600 - 1000. June 8, 2010 UV Astronomy 12 ASTROSAT/UVIT FUV, NUV, optical detectors. Spatial resolution 1.5”. Prospective launch date in 2012. Data are essentially propietary. June 8, 2010 UV Astronomy 13 Possibilities for Small Satellites No survey of the Galactic plane. Too bright for both GALEX and UVIT. June 8, 2010 UV Astronomy 14.

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