Search Results - "Buckley, D A H"
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ASASSN-18tb: a most unusual Type Ia supernova observed by TESS and SALT
Published in Monthly notices of the Royal Astronomical Society (01-08-2019)“…ABSTRACT We present photometric and spectroscopic observations of the unusual Type Ia supernova ASASSN-18tb, including a series of Southern African Large…”
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Early Spectral Evolution of Classical Novae: Consistent Evidence for Multiple Distinct Outflows
Published in The Astrophysical journal (01-12-2020)“…The physical mechanism driving mass ejection during a nova eruption is still poorly understood. Possibilities include ejection in a single ballistic event, a…”
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A Reverse Shock in GRB 181201A
Published in The Astrophysical journal (20-10-2019)“…We present comprehensive multiwavelength radio to X-ray observations of GRB 181201A spanning from 150 s to 163 days after the burst, comprising the first joint…”
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Lowly Polarized Light from a Highly Magnetized Jet of GRB 190114C
Published in The Astrophysical journal (01-04-2020)“…We report multicolor optical imaging and polarimetry observations of the afterglow of the first TeV-detected gamma-ray burst (GRB), GRB 190114C, using the…”
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The early afterglow of GRB 190829A
Published in Monthly notices of the Royal Astronomical Society (29-03-2022)“…ABSTRACT GRB 190829A at z = 0.0785 is the fourth closest long GRB ever detected by the Neil Gehrels Swift observatory, and the third confirmed case with a very…”
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Multi-wavelength observations of the binary system PSR B1259−63/LS 2883 around the 2014 periastron passage
Published in Monthly notices of the Royal Astronomical Society (01-12-2015)“…We report on the results of the extensive multi-wavelength campaign from optical to GeV γ-rays of the 2014 periastron passage of PSR B1259−63, which is a…”
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Enhanced optical activity 12 d before X-ray activity, and a 4 d X-ray delay during outburst rise, in a low-mass X-ray binary
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT X-ray transients, such as accreting neutron stars, periodically undergo outbursts, thought to be caused by a thermal-viscous instability in the…”
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The evolution of rapid optical/X-ray timing correlations in the initial hard state of MAXI J1820+070
Published in Monthly notices of the Royal Astronomical Society (17-06-2021)“…ABSTRACT We report on a multiepoch campaign of rapid optical/X-ray timing observations of the superbright 2018 outburst of MAXI J1820+070, a black hole…”
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Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii
Published in Nature astronomy (23-01-2017)“…The variable star AR Scorpii (AR Sco) was recently discovered to pulse in brightness every 1.97 min from ultraviolet wavelengths into the radio regime. The…”
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New binaries among UV-selected, hot subdwarf stars and population properties
Published in Monthly notices of the Royal Astronomical Society (11-07-2015)“…We have measured the orbital parameters of seven close binaries, including six new objects, in a radial velocity survey of 38 objects comprising a hot subdwarf…”
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Targeted search for young radio pulsars in the SMC: discovery of two new pulsars
Published in Monthly notices of the Royal Astronomical Society (11-08-2019)“…ABSTRACT We report the first rotation powered pulsars discovered in the Small Magellanic Cloud (SMC) in more than a decade. PSR J0043–73 and PSR J0052–72 were…”
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Spectropolarimetry and photometry of the early afterglow of the gamma-ray burst GRB 191221B
Published in Monthly notices of the Royal Astronomical Society (11-08-2021)“…ABSTRACT We report on results of spectropolarimetry of the afterglow of the long gamma-ray burst GRB 191221B, obtained with SALT/RSS and VLT/FORS2, as well as…”
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Identification of high-mass X-ray binaries selected from XMM–Newton observations of the LMC
Published in Monthly notices of the Royal Astronomical Society (01-04-2018)“…Abstract The Large Magellanic Cloud (LMC) currently hosts around 23 high-mass X-ray binaries (HMXBs) of which most are Be/X-ray binaries. The LMC XMM–Newton…”
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LSST Survey Strategy in the Galactic Plane and Magellanic Clouds
Published in The Astrophysical journal. Supplement series (01-07-2023)“…Abstract Galactic science encompasses a wide range of subjects in the study of the Milky Way and Magellanic Clouds, from young stellar objects to X-ray…”
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A major optical and X-ray outburst from the Magellanic Bridge source RX J0209.6–7427
Published in Monthly notices of the Royal Astronomical Society (01-05-2020)“…ABSTRACT RX J0209.6–7427 is an X-ray source in the Magellanic Bridge that was first detected in 1993, but not seen again till 2019. It has been identified as a…”
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A Close Binary Lens Revealed by the Microlensing Event Gaia20bof
Published in The Astronomical journal (01-07-2024)“…During the last 25 yr, hundreds of binary stars and planets have been discovered toward the Galactic bulge by microlensing surveys. Thanks to a new generation…”
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Identification of 1RXS J165424.6-433758 as a Polar Cataclysmic Variable
Published in The Astrophysical journal (01-11-2023)“…Abstract We present the results of our X-ray, ultraviolet, and optical follow-up campaigns of 1RXS J165424.6-433758, an X-ray source detected with the Swift…”
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The Swift Deep Galactic Plane Survey (DGPS) Phase I Catalog
Published in The Astrophysical journal. Supplement series (01-12-2023)“…Abstract The Swift Deep Galactic Plane Survey (DGPS) is a Swift Key Project consisting of 380 tiled pointings covering ∼40 deg 2 of the Galactic plane between…”
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Multiwavelength observations of nova SMCN 2016-10a – one of the brightest novae ever observed
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract We report on multiwavelength observations of nova Small Magellanic Cloud Nova 2016-10a. The present observational set is one of the most comprehensive…”
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Multi-site Observations of Pulsation in the Accreting White Dwarf SDSS J161033.64–010223.3 (V386 Ser)
Published in The Astrophysical journal (10-05-2010)“…Non-radial pulsations in the primary white dwarfs of cataclysmic variables can now potentially allow us to explore the stellar interior of these accretors…”
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