IIA Institutional Repository

Characterization of an optical transfer function–based phasing technique for India’s large segmented mirror telescope

Show simple item record

dc.contributor.author Radhika, Dharmadhikari
dc.contributor.author Parihar, P. S
dc.date.accessioned 2026-04-22T04:08:44Z
dc.date.available 2026-04-22T04:08:44Z
dc.date.issued 2026-02
dc.identifier.citation The Astronomical Journal, Vol. 171, No. 2, 101 en_US
dc.identifier.issn 1538-3881
dc.identifier.uri http://hdl.handle.net/2248/8905
dc.description Open Access en_US
dc.description Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI
dc.description.abstract The upcoming 10 m class large Indian telescope is proposed to be built using segmented mirror technology. To achieve diffraction-limited image quality with a segmented mirror telescope, it is important to phase mirror segments with very high precision. We have explored an optical transfer function (OTF)–based technique for segment phasing. The major advantage of this approach is that it enables highly accurate phase measurements over a large capture range without requiring dedicated complex optics or mechanisms. Through extensive simulations and laboratory experiments, we have tested the feasibility of using this technique for the proposed large telescope. From extensive simulations, we found that by using optical filters of different bandwidths, the modulation transfer function allows a measurement of piston errors as large as 50–100 μm and can reduce this down to 25–30 nm. Another advantage of using the OTF is that it inherently allows simultaneous measurement of phase errors in a large number of mirror segments without the use of any specialized optical elements. In this paper we present our results from simulations and laboratory experiments in relation to the proposed 10 m class segmented mirror telescope. en_US
dc.language.iso en en_US
dc.publisher American Astronomical Society en_US
dc.relation.uri https://doi.org/10.3847/1538-3881/ae2d1c
dc.rights © 2026. The Author(s).
dc.subject Optical telescopes en_US
dc.subject Astronomical instrumentation en_US
dc.subject Astronomical optics en_US
dc.title Characterization of an optical transfer function–based phasing technique for India’s large segmented mirror telescope en_US
dc.type Article en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account