Relevant bibliographies by topics / Burst Localisation

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Book chapters
  4. Conference papers

Academic literature on the topic 'Burst Localisation'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "Burst Localisation"

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Walker, C. R. H., R. P. Breton, P. A. Harrison, et al. "LOFT-e: Localisation Of Fast Transients with e-MERLIN." Proceedings of the International Astronomical Union 13, S337 (2017): 422–23. http://dx.doi.org/10.1017/s1743921317010377.

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AbstractThe majority of fast radio bursts (FRBs) are poorly localised, hindering their potential scientific yield as galactic, intergalactic, and cosmological probes. LOFT-e, a digital backend for the U.K.’s e-MERLIN seven-telescope interferometer will provide commensal search and real-time detection of FRBs, taking full advantage of its field of view (FoV), sensitivity, and observation time. Upon burst detection, LOFT-e will store raw data offline, enabling the sub-arcsecond localisation provided by e-MERLIN and expanding the pool of localised FRBs. The high-time resolution backend will addit
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Sreeramamurthy, Vanapalli, Saptarsi Dutta, Sankarsan Padhy, and Aniruddha Bose. "Determining Point of Burst of Artillery Shells using Acoustic Source Localisation." Defence Science Journal 64, no. 6 (2014): 517–23. http://dx.doi.org/10.14429/dsj.64.8112.

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Oostrum, L. C., Y. Maan, J. van Leeuwen, et al. "Repeating fast radio bursts with WSRT/Apertif." Astronomy & Astrophysics 635 (March 2020): A61. http://dx.doi.org/10.1051/0004-6361/201937422.

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Context. Repeating fast radio bursts (FRBs) present excellent opportunities to identify FRB progenitors and host environments as well as to decipher the underlying emission mechanism. Detailed studies of repeating FRBs might also hold clues as to the origin of FRBs as a population. Aims. We aim to detect bursts from the first two repeating FRBs, FRB 121102 (R1) and FRB 180814.J0422+73 (R2), and to characterise their repeat statistics. We also want to significantly improve the sky localisation of R2 and identify its host galaxy. Methods. We used the Westerbork Synthesis Radio Telescope to condu
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Nicastro, Luciano, Cristiano Guidorzi, Eliana Palazzi, Luca Zampieri, Massimo Turatto, and Angela Gardini. "Multiwavelength Observations of Fast Radio Bursts." Universe 7, no. 3 (2021): 76. http://dx.doi.org/10.3390/universe7030076.

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The origin and phenomenology of the Fast Radio Burst (FRB) remains unknown despite more than a decade of efforts. Though several models have been proposed to explain the observed data, none is able to explain alone the variety of events so far recorded. The leading models consider magnetars as potential FRB sources. The recent detection of FRBs from the galactic magnetar SGR J1935+2154 seems to support them. Still, emission duration and energetic budget challenge all these models. Like for other classes of objects initially detected in a single band, it appeared clear that any solution to the
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Melandri, A., A. Rossi, S. Benetti, et al. "Unveiling the enigma of ATLAS17aeu." Astronomy & Astrophysics 621 (January 2019): A81. http://dx.doi.org/10.1051/0004-6361/201833814.

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Aims. The unusual transient ATLAS17aeu was serendipitously detected within the sky localisation of the gravitational wave trigger GW 170104. The importance of a possible association with gravitational waves coming from a binary black hole merger led to an extensive follow-up campaign, with the aim of assessing a possible connection with GW 170104. Methods. With several telescopes, we carried out both photometric and spectroscopic observations of ATLAS17aeu, for several epochs, between ∼3 and ∼230 days after the first detection. Results. We studied in detail the temporal and spectroscopic prope
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Wadelin, Frances R., Keith A. Spriggs, Franco H. Falcone, and David M. Heery. "Transcriptional and Translational Regulation of the Cancer-Testis Antigen PRAME Mediated by Pathogen-Associated Molecular Patterns." Blood 116, no. 21 (2010): 2475. http://dx.doi.org/10.1182/blood.v116.21.2475.2475.

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Abstract Abstract 2475 PRAME (preferentially expressed antigen in melanoma) is a germinal tissue-specific gene that is expressed at high levels in a number of haematological malignancies. In AML, PRAME is a positive prognostic indicator, being associated with a favourable response to chemotherapy and increased overall survival, even in the presence of unfavourable karyotypes. In contrast, over-expression of PRAME mRNA is associated with poor prognosis in CML, NHL, HD, CLL and myeloma, being associated with progressive disease and chemo-resistance. Despite proposals to implement PRAME as a tool
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Sim, Neil, Sven Gottschalk, Robert Pal, et al. "Wavelength-dependent optoacoustic imaging probes for NMDA receptor visualisation." Chemical Communications 51, no. 82 (2015): 15149–52. http://dx.doi.org/10.1039/c5cc06277b.

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The cellular localisation and binding specificity of two NMDAR-targeted near-IR imaging probes has been examined by microscopy, followed by exemplification of MSOT to monitor simulated glutamate bursts in cellulo and a preliminary study in mice observing the signal in the brain.
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Marnoch, Lachlan, Stuart D. Ryder, Keith W. Bannister, et al. "A search for supernova-like optical counterparts to ASKAP-localised fast radio bursts." Astronomy & Astrophysics 639 (July 2020): A119. http://dx.doi.org/10.1051/0004-6361/202038076.

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Fast radio bursts (FRBs) are millisecond-scale radio pulses, which originate in distant galaxies and are produced by unknown sources. The mystery remains partially because of the typical difficulty in localising FRBs to host galaxies. Accurate localisations delivered by the Commensal Real-time ASKAP Fast Transients (CRAFT) survey now provide an opportunity to study the host galaxies and potential transient counterparts of FRBs at a large range of wavelengths. In this work, we investigate whether the first three FRBs accurately localised by CRAFT have supernova-like transient counterparts. We o
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Walker, Charles R. H., Yin-Zhe Ma, and René P. Breton. "Constraining the redshifts of unlocalised fast radio bursts." Astronomy & Astrophysics 638 (June 2020): A37. http://dx.doi.org/10.1051/0004-6361/201833157.

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Context. The relationship between the dispersion measures (DMs) and redshifts of fast radio bursts (FRBs) is of scientific interest. Upcoming commensal surveys may detect and localise many FRBs to the sub-arcsecond angular resolutions required for accurate redshift determination. Meanwhile, it is important to exploit sources accumulated with more limited localisation to their maximum scientific potential. Aims. We present techniques for the DM-redshift analysis of large numbers of unlocalised FRBs, accounting for uncertainties due to their extragalactic DM components, redshift dependences, and
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Caleb, M., C. Flynn, M. Bailes, et al. "First interferometric detections of Fast Radio Bursts." Proceedings of the International Astronomical Union 13, S337 (2017): 322–23. http://dx.doi.org/10.1017/s1743921317008973.

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AbstractThe class of radio transients called Fast Radio Bursts (FRBs) encompasses enigmatic single pulses, each unique in its own way, hindering a consensus for their origin. The key to demystifying FRBs lies in discovering many of them in order to identity commonalities – and in real time, in order to find potential counterparts at other wavelengths. The recently upgraded UTMOST in Australia, is undergoing a backend transformation to rise as a fast transient detection machine. The first interferometric detections of FRBs with UTMOST, place their origin beyond the near-field region of the tele
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Dissertations / Theses on the topic "Burst Localisation"

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Okeya, Olanrewaju Isaac. "Detection and localisation of pipe bursts in a district metered area using an online hydraulic model." Thesis, University of Exeter, 2018. http://hdl.handle.net/10871/33823.

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This thesis presents a research work on the development of new methodology for near-real-time detection and localisation of pipe bursts in a Water Distribution System (WDS) at the District Meters Area (DMA) level. The methodology makes use of online hydraulic model coupled with a demand forecasting methodology and several statistical techniques to process the hydraulic meters data (i.e., flows and pressures) coming from the field at regular time intervals (i.e. every 15 minutes). Once the detection part of the methodology identifies a potential burst occurrence in a system it raises an alarm.
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Pelassa, Véronique. "Détection, localisation et étude des propriétés spectrales de sursauts gamma observés à haute énergie avec l'expérience Fermi." Thesis, Montpellier 2, 2010. http://www.theses.fr/2010MON20161/document.

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Les sursauts gamma sont des sources astrophysiques parmi les plus brillantes du ciel. Dans le modèle standard actuel, leur émission prompte (X et gamma) est due à des particules chargées accélérées au sein de jets relativistes émis à la formation de trous noirs de masses stellaire. L'émission rémanente observée de la radio aux X serait due à l'interaction de ces jets avec le milieu interstellaire. Le LAT, détecteur à création de paire du télescope spatial Fermi, permet depuis juin 2008 l'étude du ciel gamma de 20 MeV à plus de 300 GeV avec des performances inégalées. Le GBM, détecteur de sourc
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Book chapters on the topic "Burst Localisation"

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Romano, Michele. "Review of Techniques for Optimal Placement of Pressure and Flow Sensors for Leak/Burst Detection and Localisation in Water Distribution Systems." In The Handbook of Environmental Chemistry. Springer International Publishing, 2019. http://dx.doi.org/10.1007/698_2019_405.

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Conference papers on the topic "Burst Localisation"

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Jijomon C.M. and A. R. Jayan. "An offline signal processing technique for accurate localisation of stop release bursts in vowel-consonant-vowel utterances." In 2015 International Conference on Control Communication & Computing India (ICCC). IEEE, 2015. http://dx.doi.org/10.1109/iccc.2015.7432947.

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