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Daksha: on alert for high energy transients

dc.contributor.authorBhalerao, Varun
dc.contributor.authorVadawale, Santosh
dc.contributor.authorTendulkar, Shriharsh
dc.contributor.authorBhattacharya, Dipankar
dc.contributor.authorRana, Vikram
dc.contributor.authorAdalja, Hitesh Kumar L
dc.contributor.authorBelatikar, Hrishikesh
dc.contributor.authorBhaganagare, Mahesh
dc.contributor.authorDewangan, Gulab
dc.contributor.authorGhodgaonkar, Abhijeet
dc.contributor.authorGoyal, Shiv Kumar
dc.contributor.authorGunasekaran, Suresh
dc.contributor.authorGuruprasad, P J
dc.contributor.authorKoyande, Jayprakash G
dc.contributor.authorKulkarni, Salil
dc.contributor.authorKutty, APK
dc.contributor.authorLadiya, Tinkal
dc.contributor.authorMahapatra, Suddhasatta
dc.contributor.authorMarla, Deepak
dc.contributor.authorMate, Sujay
dc.contributor.authorMithun, N P S
dc.contributor.authorMote, Rakesh
dc.contributor.authorNarang, Sanjoli
dc.contributor.authorNema, Ayush
dc.contributor.authorNimbalkar, Sudhanshu
dc.contributor.authorPai, Archana
dc.contributor.authorPalit, Sourav
dc.contributor.authorPatel, Arpit
dc.contributor.authorPatel, Jinaykumar
dc.contributor.authorPradeep, Priya
dc.contributor.authorRamachandran, Prabhu
dc.contributor.authorSaiguhan, B S Bharath
dc.contributor.authorSaraogi, Divita
dc.contributor.authorSawant, Disha
dc.contributor.authorShanmugam, M
dc.contributor.authorSharma, Piyush
dc.contributor.authorShetye, Amit
dc.contributor.authorSingh, Nishant
dc.contributor.authorSingh, Shreeya
dc.contributor.authorSinghal, Akshat
dc.contributor.authorSreekumar, S
dc.contributor.authorSridhar, Srividhya
dc.contributor.authorSrinivasan, Rahul
dc.contributor.authorTallur, Siddharth
dc.contributor.authorTiwari, Neeraj K
dc.contributor.authorVadladi, Amrutha Lakshmi
dc.contributor.authorVaishnava, C S
dc.contributor.authorVishwakarma, Sandeep
dc.contributor.authorWaratkar, Gaurav
dc.date.accessioned2026-06-17T06:31:54Z
dc.date.available2026-06-17T06:31:54Z
dc.date.issued2024-06-11
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en_US
dc.description.abstractWe present Daksha, a proposed high energy transients mission for the study of electromagnetic counterparts of gravitational wave sources, and gamma ray bursts. Daksha will comprise of two satellites in low earth equatorial orbits, on opposite sides of the Earth. Each satellite will carry three types of detectors to cover the entire sky in an energy range from 1 keV to > MeV. Any transients detected on-board will be announced publicly within minutes of discovery. All photon data will be downloaded in ground station passes to obtain source positions, spectra, and light curves. In addition, Daksha will address a wide range of science cases including monitoring X-ray pulsars, studies of magnetars, solar flares, searches for fast radio burst counterparts, routine monitoring of bright persistent high energy sources, terrestrial gamma-ray flashes, and probing primordial black hole abundances through lensing. In this paper, we discuss the technical capabilities of Daksha, while the detailed science case is discussed in a separate paper.en_US
dc.identifier.citationExperimental Astronomy, 2024, Vol. 57 (24), AR No. 24en_US
dc.identifier.issn1572-9508
dc.identifier.urihttp://hdl.handle.net/2289/8760
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.relation.urihttps://doi.org/10.48550/arXiv.2211.12055en_US
dc.relation.urihttps://doi.org/10.1007/s10686-024-09926-yen_US
dc.rights© The Author(s)en_US
dc.subjectAstrophysicsen_US
dc.subjectEducation in Physicsen_US
dc.subjectHigh-Energy Astrophysicsen_US
dc.subjectSpace Physicsen_US
dc.subjectSpace Studiesen_US
dc.subjectTransient astrophysical phenomenaen_US
dc.subjectRadio Astronomy Surveys and Analytical Techniquesen_US
dc.titleDaksha: on alert for high energy transientsen_US
dc.typeArticleen_US

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