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http://hdl.handle.net/2248/8100
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DC Field | Value | Language |
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dc.contributor.author | Kumar, Harsh | - |
dc.contributor.author | Bhalerao, Varun | - |
dc.contributor.author | Anupama, G. C | - |
dc.contributor.author | Barway, Sudhanshu | - |
dc.contributor.author | Coughlin, Michael W | - |
dc.contributor.author | De, Kishalay | - |
dc.contributor.author | Deshmukh, Kunal | - |
dc.contributor.author | Dutta, Anirban | - |
dc.contributor.author | Goldstein, Daniel A | - |
dc.contributor.author | Jassani, Adeem | - |
dc.contributor.author | Joharle, Simran | - |
dc.contributor.author | Karambelker, Viraj | - |
dc.contributor.author | Khandagale, Maitreya | - |
dc.contributor.author | Kumar, B | - |
dc.contributor.author | Saraogi, Divita | - |
dc.contributor.author | Sharma, Yashvi | - |
dc.contributor.author | Shenoy, Vedant | - |
dc.contributor.author | Singer, Leo | - |
dc.contributor.author | Singh, A | - |
dc.contributor.author | Waratkar, Gaurav | - |
dc.date.accessioned | 2022-12-22T04:16:14Z | - |
dc.date.available | 2022-12-22T04:16:14Z | - |
dc.date.issued | 2022-11 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, Vol. 516, No. 3, pp. 4517–4528 | en_US |
dc.identifier.issn | 1365-2966 | - |
dc.identifier.uri | http://hdl.handle.net/2248/8100 | - |
dc.description | Restricted Access | en_US |
dc.description.abstract | S190426c/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.iso | en | en_US |
dc.publisher | Oxford University Press on behalf of Royal Astronomical Society | en_US |
dc.relation.uri | https://doi.org/10.1093/mnras/stac2516 | - |
dc.rights | © Royal Astronomical Society | - |
dc.subject | Methods: data analysis | en_US |
dc.subject | Techniques: image processing | en_US |
dc.subject | Black hole | en_US |
dc.subject | Neutron star mergers | en_US |
dc.title | GROWTH on S190426c II: GROWTH-India Telescope search for an optical counterpart with a custom image reduction and candidate vetting pipeline | en_US |
dc.type | Article | en_US |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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GROWTH on S190426c II GROWTH-India Telescope search for an optical counterpart with a custom image reduction and candidate vetting pipeline.pdf Restricted Access | 4.47 MB | Adobe PDF | View/Open Request a copy |
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