These will be sent back to the ISSDC which has the primary re-sponsibility for data archival and dissemination. 7.11.19 A09 Update Proposers can request monitoring observations with a minimum interval of 3 days between two consecutive observations. Observations and Analysis 2.1. We combine the UVIT data with the data in the longer wavelengths to identify and characterize the detected stars. Note: This software has been certified for scientific use by the instrument team.

All cross-matches were done with a maximum separation of 3''. This will allow a more comprehensive view of the X-ray behavior of … 7.11.19 A09 Update Proposers can request monitoring observations with a minimum interval of 3 days between two consecutive observations.

New!! UVIT. Example Results: NGC 2336 . UVIT Data We observed M67 with the UVIT on ASTROSAT,thefirst Indian space observatory, launched on 2015 September 28.
15.10.19 Cycle A09 Announcement of Opportunity proposal submission opened.. A new version of UVIT pipeline is available UVIT level2 pipeline software (UL2P V6.3). 3.2 Photometric Calibration 3.2.1 Standard Calibrators Two standard stars were observed as part of the UVIT We have processed these data through the JUDE software (Murthy et al.2016;Murthy et al.2017) to create photon event lists and images of the sky.

However, please carfully read the documentation for proper use. The analysis of the X-ray data will be combined with analysis of the X-ray data from the other AstroSat observing sessions of Her X-1 (A02 and A03) for which UVIT was not operating. The Level 1 data are distributed as a single gzipped tar …

The telescope has three channels: FUV (130–180nm),NUV(200–300nm), and VIS (350–550nm), where the VIS channel is mainly used to … UVIT Sample data and Basic Analysis software. UVIT pipeline (when completed), and Level 2 data prod-ucts, suitable for scienti c analysis, will be created. 26.04.19 Cycle A08 Legacy proposal submission closed. Flux measurements from UV to IR bands were obtained as follows: FUV (1542 ± 200 Å) and NUV (2274 ± 530 Å) from GALEX; U (3630 ± 296 Å), B (4358 ± 502 Å), V (5366 ± 470 Å), R (6454 ± 776 Å), and I (8100 ± …
The near-simultaneous observations of M67 were carried out by the UVIT on 2017 April 23. Swarna K Ghosh On behalf of : UVIT team, SAC-ISRO team ASTROSAT AO-1 Workshop @ IUCAA, 13/14-Jul-2016 UVIT Data Analysis Pipeline Home » Data & Analysis » Results » UVIT.

New!! JUDE: An alternative UVIT pipeline Jayant Murthy a, P. T. Rahnab, Firoza Sutaria , Margarita Safonovac,∗, S. B. Gudennavarb, S. G. Bubblyb aIndian Institute of Astrophysics, Bengaluru bDepartment of Physics, Christ University, Bengaluru cM. Image: Recent updates.