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    • Fulltext

       

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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/042/0073

    • Keywords

       

      Stars: gamma-ray burst: general; X-rays: bursts; methods: data analysis.

    • Abstract

       

      The Cadmium–Zinc–Telluride Imager on AstroSat has proven to be a very effective All-Sky monitor in the hard X-ray regime, detecting over three hundred GRBs and putting highly competitive upper limits on X-ray emissions from gravitational wave sources and fast radio bursts. We present the algorithmsused for searching for such transient sources in CZTI data, and for calculating upper limits in case of nondetections. We introduce CIFT: the CZTI Interface for Fast Transients, a framework used to streamline these processes. We present details of 87 new GRBs detected by this framework that were previously not detected in CZTI.

    • Author Affiliations

       

      Y. SHARMA1 2 A. MARATHE2 3 V. BHALERAO2 V. SHENOY2 G. WARATKAR2 D. NADELLA3 P. PAGE2 P. HEBBAR2 4 A. VIBHUTE5 D. BHATTACHARYA5 A. R. RAO6 S. VADAWALE7

      1. Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA.
      2. Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India.
      3. National Institute of Technology Karnataka, Surathkal, Mangalore 575 025, India.
      4. University of Alberta, Edmonton, AB T6G 2E1, Canada.
      5. Inter-University Centre for Astronomy and Astrophysics, P.O. Bag 4, Ganeshkhind, Pune 411 007, India.
      6. Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400 005, India.
      7. Physical Research Laboratory, Ahmedabad 380 009, India.

    • Dates

       
      Published
      6 July 2021
      Manuscript received
      3 November 2020
      Accepted
      17 January 2021
      Final version published online
      6 July 2021

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

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