activity
20182025
most citedExoClock Project III: 450 new exoplanet ephemerides from ground and space observations

77 citations · 254 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2025

Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour

Jaroslav Merc, Łukasz Wyrzykowski, Paul G. Beck +46

T CrB is a symbiotic recurrent nova that last erupted in 1946. Given its recurrence timescale of approximately 80 years, the next outburst is eagerly anticipated by the astronomica…

astro-ph.SR2024★ 1 cited

Caught in the Act: Observations of the Double-mode RR Lyrae V338 Boo During the Disappearance of a Pulsation Mode

Kenneth Carrell, Ronald Wilhelm, Andrew Tom +13

New results on the behavior of the double-mode RR Lyrae V338 Boo are presented. The Transiting Exoplanet Survey Satellite (TESS) observed this star again in 2022, and an observing…

astro-ph.SR2024

Optical and soft X-ray light-curve analysis during the 2022 eruption of U Scorpii: structural changes in the accretion disk

Katsuki Muraoka, Naoto Kojiguchi, Junpei Ito +52

We present our optical photometric observations of the 2022 eruption of the recurrent nova U Scorpii (U Sco) using 49,152 data points over 70 d following the optical peak. We have…

astro-ph.SR2023★ 1 cited

Lens mass estimate in the Galactic disk extreme parallax microlensing event Gaia19dke

M. Maskoliūnas, Ł. Wyrzykowski, K. Howil +74

We present the results of our analysis of Gaia19dke, an extraordinary microlensing event in the Cygnus constellation that was first spotted by the {\gaia} satellite. This event fea…

astro-ph.SR2023★ 6 cited

2021 superoutburst of WZ Sge-type dwarf nova V627 Pegasi lacks an early superhump phase

Yusuke Tampo, Taichi Kato, Naoto Kojiguchi +27

Superoutbursts in WZ Sge-type dwarf novae (DNe) are characterized by both early superhumps and ordinary superhumps originating from the 2:1 and 3:1 resonances, respectively. Howeve…

astro-ph.EP2022★ 77 cited

ExoClock Project III: 450 new exoplanet ephemerides from ground and space observations

A. Kokori, A. Tsiaras, B. Edwards +214

The ExoClock project has been created with the aim of increasing the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides o…

astro-ph.SR2022

The Periodic Signals of Nova V1674 Herculis (2021)

Joseph Patterson, Marguerite Epstein-Martin, Josie Enenstein +24

We present time-series photometry during eruption of the extremely fast nova V1674 Herculis (Nova Her 2021). The 2021 light curve showed periodic signals at 0.152921(3) d and 501.4…

astro-ph.SR2022★ 2 cited

Analysis of the IW And star ASAS J071404+7004.3

Taichi Kato, Kiyoshi Kasai, Elena P. Pavlenko +14

We made a time-resolved photometric campaign of the bright cataclysmic variable ASAS J071404+7004.3 in 2020. Inight et al. (2022, arXiv/2109.14514) recently published time-resolved…

astro-ph.SR2022

Investigating the low-flux states in six Intermediate Polars

Ava E. Covington, Aarran W. Shaw, Koji Mukai +30

We present optical photometry of six intermediate polars that exhibit transitions to a low-flux state. For four of these systems, DW Cnc, V515 And, V1223 Sgr and RX J2133.7+5107, w…

astro-ph.EP2021★ 56 cited

ExoClock project II: A large-scale integrated study with 180 updated exoplanet ephemerides

A. Kokori, A. Tsiaras, B. Edwards +102

The ExoClock project is an inclusive, integrated, and interactive platform that was developed to monitor the ephemerides of the Ariel targets to increase the mission efficiency. Th…

astro-ph.HE2021

Optical Variability Correlated with X-ray Spectral Transition in the Black-Hole Transient ASASSN-18ey = MAXI J1820+070

Keito Niijima, Mariko Kimura, Yasuyuki Wakamatsu +49

How a black hole accretes matter and how this process is regulated are fundamental but unsolved questions in astrophysics. In transient black-hole binaries, a lot of mass stored in…

astro-ph.SR2021★ 10 cited

Spectroscopic and Photometric Observations of Dwarf Nova Superoutbursts by the 3.8 m Telescope Seimei and the Variable Star Network

Yusuke Tampo, Keisuke Isogai, Naoto Kojiguchi +59

We present spectroscopic and photometric observations of 17 dwarf-nova superoutbursts obtained by KOOLS-IFU mounted on the 3.8 m telescope Seimei at Okayama Observatory of Kyoto Un…

astro-ph.SR2020★ 8 cited

Multi-wavelength photometry during the 2018 superoutburst of the WZ Sge-type dwarf nova EG Cancri

Mariko Kimura, Keisuke Isogai, Taichi Kato +45

We report on the multi-wavelength photometry of the 2018 superoutburst in EG Cnc. We have detected stage A superhumps and long-lasting late-stage superhumps via the optical photome…

astro-ph.SR2020

Carbon Star CGCS 673 identified as a Semi-regular variable star

Stephen M Brincat, Charles Galdies, Kevin Hills

This study shows that the carbon star CGCS 673 is a semi-regular (SR) variable star with a period of 135 d and an amplitude of 0.18 magnitudes in the V-band. The light curve obtain…

astro-ph.SR2020★ 16 cited

First Detection of Two Superoutbursts during Rebrightening Phase of a WZ Sge-type Dwarf Nova: TCP J21040470+4631129

Yusuke Tampo, Kojiguchi Naoto, Keisuke Isogai +51

We report photometric and spectroscopic observations and analysis of the 2019 superoutburst of TCP J21040470+4631129. This object showed a 9-mag superoutburst with early superhumps…

astro-ph.SR2019★ 28 cited

The Rise and Fall of the King: The Correlation between FO Aquarii's Low States and the White Dwarf's Spindown

Colin Littlefield, Peter Garnavich, Mark R. Kennedy +45

The intermediate polar FO Aquarii (FO Aqr) experienced its first-reported low-accretion states in 2016, 2017, and 2018, and using newly available photographic plates, we identify p…

astro-ph.SR2019★ 11 cited

The PDS 110 observing campaign - photometric and spectroscopic observations reveal eclipses are aperiodic

Hugh P. Osborn, Matthew Kenworthy, Joseph E. Rodriguez +71

PDS 110 is a young disk-hosting star in the Orion OB1A association. Two dimming events of similar depth and duration were seen in 2008 (WASP) and 2011 (KELT), consistent with an ob…

astro-ph.SR2019★ 11 cited

Discovery of Standstills in the SU UMa-Type Dwarf Nova NY Serpentis

Taichi Kato, Elena P. Pavlenko, Nikolaj V. Pit +40

We found that the SU UMa-type dwarf nova NY Ser in the period gap [orbital period 0.097558(6) d] showed standstills twice in 2018. This is the first clear demonstration of a stands…

astro-ph.SR2018★ 9 cited

On the Nature of Long-Period Dwarf Novae with Rare and Low-Amplitude Outbursts

Mariko Kimura, Taichi Kato, Hiroyuki Maehara +35

There are several peculiar long-period dwarf-nova like objects, which show rare, low-amplitude outbursts with highly ionized emission lines. 1SWASP J162117441254, BD Pav, and V3…

astro-ph.SR2018★ 18 cited

ASASSN-16dt and ASASSN-16hg: Promising Candidates for a Period Bouncer

Mariko Kimura, Keisuke Isogai, Taichi Kato +13

We present optical photometry of superoutbursts in 2016 of two WZ Sge-type dwarf novae (DNe), ASASSN-16dt and ASASSN-16hg. Their light curves showed a dip in brightness between the…