Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8100
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dc.contributor.authorKumar, Harsh-
dc.contributor.authorBhalerao, Varun-
dc.contributor.authorAnupama, G. C-
dc.contributor.authorBarway, Sudhanshu-
dc.contributor.authorCoughlin, Michael W-
dc.contributor.authorDe, Kishalay-
dc.contributor.authorDeshmukh, Kunal-
dc.contributor.authorDutta, Anirban-
dc.contributor.authorGoldstein, Daniel A-
dc.contributor.authorJassani, Adeem-
dc.contributor.authorJoharle, Simran-
dc.contributor.authorKarambelker, Viraj-
dc.contributor.authorKhandagale, Maitreya-
dc.contributor.authorKumar, B-
dc.contributor.authorSaraogi, Divita-
dc.contributor.authorSharma, Yashvi-
dc.contributor.authorShenoy, Vedant-
dc.contributor.authorSinger, Leo-
dc.contributor.authorSingh, A-
dc.contributor.authorWaratkar, Gaurav-
dc.date.accessioned2022-12-22T04:16:14Z-
dc.date.available2022-12-22T04:16:14Z-
dc.date.issued2022-11-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 516, No. 3, pp. 4517–4528en_US
dc.identifier.issn1365-2966-
dc.identifier.urihttp://hdl.handle.net/2248/8100-
dc.descriptionRestricted Accessen_US
dc.description.abstractS190426c/GW190426 152155 was the first probable neutron star–black hole merger candidate detected by the LIGO-Virgo Collaboration. We undertook a tiled search for optical counterparts of this event using the 0.7-m GROWTH-India Telescope. Over a period of two weeks, we obtained multiple observations over a 22.1 deg2 area, with a 17.5 per cent probability of containing the source location. Initial efforts included obtaining photometry of sources reported by various groups, and a visual search for sources in all galaxies contained in the region. Subsequently, we have developed an image subtraction and candidate vetting pipeline with ∼ 94 per cent efficiency for transient detection. Processing the data with this pipeline, we find several transients, but none that are compatible with kilonova models. We present the details of our observations, the working of our pipeline, results from the search, and our interpretations of the non-detections that will work as a pathfinder during the O4 run of LVK.en_US
dc.language.isoenen_US
dc.publisherOxford University Press on behalf of Royal Astronomical Societyen_US
dc.relation.urihttps://doi.org/10.1093/mnras/stac2516-
dc.rights© Royal Astronomical Society-
dc.subjectMethods: data analysisen_US
dc.subjectTechniques: image processingen_US
dc.subjectBlack holeen_US
dc.subjectNeutron star mergersen_US
dc.titleGROWTH on S190426c II: GROWTH-India Telescope search for an optical counterpart with a custom image reduction and candidate vetting pipelineen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications



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