IIA Institutional Repository

Development of 6U spectrograph payload for NUV studies

Show simple item record

dc.contributor.author Bharat Chandra, P
dc.date.accessioned 2021-06-28T12:46:12Z
dc.date.available 2021-06-28T12:46:12Z
dc.date.issued 2019-06
dc.identifier.citation M. Tech Thesis, University of Calcutta, Calcutta en_US
dc.identifier.uri http://hdl.handle.net/2248/7742
dc.description Thesis Supervisor Prof. Jayant Murthy en_US
dc.description.abstract One of the most exciting parts of the astrophysical spectrum is the near ultraviolet (NUV: 1800 – 3000Å), where there are a number of important atomic and molecular lines. The hot gas in the halo emits in NUV and also shocked regions of the interstellar medium (ISM) most notably supernova remnants (SNR). We will be building a spectrograph of 6U size to track emission lines over the entire spatial extent of a nebula which is the key to understanding its dynamics and evolution. The spectrograph has the unique combination of spectral and spatial resolution, sensitivity to investigate diffuse sources, and mission lifetime required to probe the physics of nebulae or the ISM. As the payload orbits the earth the resulting survey using the spectrograph will create a map of the sky covered within the field of view (FOV) of the payload constrained by the orbital inclination of the spacecraft. The payload will contain optics for the NUV spectrograph, an MCP based detector, FPGA based readout circuitry and other required electronics components en_US
dc.language.iso en en_US
dc.publisher Indian Institute of Astrophysics en_US
dc.rights © Indian Institute of Astrophysics
dc.title Development of 6U spectrograph payload for NUV studies en_US
dc.type Thesis en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account