Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Articles Article Faculty Publications -Articles Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Exploring the Central Region of NGC 1365 in the Ultraviolet Domain Description An account of the resource Active galactic nuclei (AGN) feedback and its impact on their host galaxies are critical to our understanding of galaxy evolution. Here, we present a combined analysis of new high resolution ultraviolet (UV) data from the Ultraviolet Imaging Telescope (UVIT) on AstroSat and archival optical spectroscopic data from the Very Large Telescope/MUSE, for the Seyfert galaxy, NGC 1365. Concentrating on the central 5 kpc region, the UVIT images in the far- and near-UV show bright star-forming knots in the circumnuclear ring as well as a faint central source. After correcting for extinction, we found the star formation rate (SFR) surface density of the circumnuclear 2 kpc ring to be similar to other starbursts, despite the presence of an AGN outflow, as seen in [O iii] 5007 On the other hand, we found fainter UV and thus lower SFR in the direction southeast of the AGN relative to northwest in agreement with observations at other wavelengths from JWST and Atacama Large Millimeter/submillimeter Array. The AGN outflow velocity is found to be lesser than the escape velocity, suggesting that the outflowing gas will rain back into the galaxy. The deep UV data have also revealed diffuse UV emission in the direction of the AGN outflow. By combining [O iii] and UV data, we found the diffuse emission to be of AGN origin. 2024. The Author(s). Published by the American Astronomical Society. Creator An entity primarily responsible for making the resource Kurian K.S.; Stalin C.S.; Wylezalek D.; Lyubenova M.; Adhikari T.P.; Devaraj A.; Sagar R.; Kissler-Patig M.; Mondal S. Source A related resource from which the described resource is derived Astrophysical Journal, Vol-974, No. 1 Publisher An entity responsible for making the resource available Institute of Physics Date A point or period of time associated with an event in the lifecycle of the resource 2024-01-01 Identifier An unambiguous reference to the resource within a given context <a href="https://doi.org/10.3847/1538-4357/ad6b93" target="_blank" rel="noreferrer noopener">https://doi.org/10.3847/1538-4357/ad6b93</a> <br /><br /><a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85206517174&amp;doi=10.3847%2F1538-4357%2Fad6b93&amp;partnerID=40&amp;md5=787d129f66f602939a280541b563bc4f" target="_blank" rel="noreferrer noopener">https://www.scopus.com/inward/record.uri?eid=2-s2.0-85206517174&amp;doi=10.3847%2f1538-4357%2fad6b93&amp;partnerID=40&amp;md5=787d129f66f602939a280541b563bc4f</a> Rights Information about rights held in and over the resource All Open Access; Gold Open Access Relation A related resource ISSN: 0004637X Format The file format, physical medium, or dimensions of the resource Online Language A language of the resource English Type The nature or genre of the resource Article Coverage The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant Kurian K.S., Indian Institute of Astrophysics, Koramangala, Block II, Bangalore, 560034, India, Pondicherry University, Puducherry, Kalapet, 605014, India; Stalin C.S., Indian Institute of Astrophysics, Koramangala, Block II, Bangalore, 560034, India; Wylezalek D., Astronomisches Rechen-Institut, Zentrum fur Astronomie der Universitat Heidelberg, Monchhofstr. 12-14, Heidelberg, 69120, Germany; Lyubenova M., European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching bei Mchen, 85748, Germany; Adhikari T.P., CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Anhui, Hefei, 230026, China, School of Astronomy and Space Science, University of Science and Technology of China, Anhui, Hefei, 230026, China; Devaraj A., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Sagar R., Indian Institute of Astrophysics, Koramangala, Block II, Bangalore, 560034, India; Kissler-Patig M., ESAESACEuropean Space Agency, Camino Bajo del Castillo s/n, Villafranca del Castillo, Madrid, 28692, Spain; Mondal S., Indian Institute of Astrophysics, Koramangala, Block II, Bangalore, 560034, India