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zadetkov: 3.396
41.
  • The 2021 outburst of the re... The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study
    Page, K L; Beardmore, A P; Osborne, J P ... Monthly Notices of the Royal Astronomical Society, 06/2022, Letnik: 514, Številka: 2
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    ABSTRACT On 2021 August 8, the recurrent nova RS Ophiuchi (RS Oph) erupted again, after an interval of 15.5 yr. Regular monitoring by the Neil Gehrels Swift Observatory began promptly, on August 9.9 ...
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42.
  • A real-time transient detec... A real-time transient detector and the living Swift -XRT point source catalogue
    Evans, P A; Page, K L; Beardmore, A P ... Monthly Notices of the Royal Astronomical Society, 01/2023, Letnik: 518, Številka: 1
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    ABSTRACT We present the Living Swift-XRT Point Source (LSXPS) catalogue and real-time transient detector. This system allows us for the first time to carry out low-latency searches for new transient ...
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43.
  • Swift follow-up of the grav... Swift follow-up of the gravitational wave source GW150914
    Evans, P. A; Kennea, J. A; Barthelmy, S. D ... Monthly notices of the Royal Astronomical Society. Letters, 07/2016, Letnik: 460, Številka: 1
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    The Advanced Laser Interferometer Gravitational-Wave Observatory (ALIGO) observatory recently reported the first direct detection of gravitational waves (GW) which triggered ALIGO on 2015 September ...
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44.
  • Near-infrared Studies of No... Near-infrared Studies of Nova V1674 Herculis: A Shocking Record Breaker
    Woodward, C. E.; Banerjee, D. P. K.; Geballe, T. R. ... Astrophysical journal. Letters, 11/2021, Letnik: 922, Številka: 1
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    Abstract We present near-infrared spectroscopy of Nova Herculis 2021 (V1674 Her), obtained over the first 70 days of its evolution. This fastest nova on record displays a rich emission line spectrum, ...
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45.
  • Multiwavelength observation... Multiwavelength observations of nova SMCN 2016-10a – one of the brightest novae ever observed
    Aydi, E; Page, K L; Kuin, N P M ... Monthly Notices of the Royal Astronomical Society, 02/2018, Letnik: 474, Številka: 2
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    Abstract We report on multiwavelength observations of nova Small Magellanic Cloud Nova 2016-10a. The present observational set is one of the most comprehensive for any nova in the Small Magellanic ...
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46.
  • Swift/UVOT follow-up of gra... Swift/UVOT follow-up of gravitational wave alerts in the O3 era
    Oates, S R; Marshall, F E; Breeveld, A A ... Monthly Notices of the Royal Astronomical Society, 10/2021, Letnik: 507, Številka: 1
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    ABSTRACT In this paper, we report on the observational performance of the Swift Ultra-violet/Optical Telescope (UVOT) in response to the gravitational wave (GW) alerts announced by the Advanced Laser ...
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47.
  • The remarkable outburst of ... The remarkable outburst of the highly evolved post-period-minimum dwarf nova SSS J122221.7−311525
    Neustroev, V. V; Marsh, T. R; Zharikov, S. V ... Monthly Notices of the Royal Astronomical Society, 06/2017, Letnik: 467, Številka: 1
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    Abstract We report extensive 3-yr multiwavelength observations of the WZ Sge-type dwarf nova SSS J122221.7−311525 during its unusual double superoutburst, the following decline and in quiescence. The ...
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48.
  • The panchromatic spectrosco... The panchromatic spectroscopic evolution of the classical CO nova V339 Delphini (Nova Del 2013) until X-ray turnoff
    Shore, S. N.; Mason, E.; Schwarz, G. J. ... Astronomy & astrophysics, 06/2016, Letnik: 590
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    Context. Classical novae are the product of thermonuclear runaway-initiated explosions occurring on accreting white dwarfs. Aims. V339 Del (Nova Delphinus 2013) was one of the brightest classical ...
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50.
  • Infrared spectroscopy of th... Infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco
    Evans, A; Banerjee, D P K; Woodward, C E ... Monthly Notices of the Royal Astronomical Society, 05/2023, Letnik: 522, Številka: 4
    Journal Article
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    ABSTRACT We present near-infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco, over the period from 5.4 to 45.6 d after outburst. This is the most intensive infrared study of this ...
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zadetkov: 3.396

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