activity
20092026
most citedA super-Earth and two sub-Neptunes transiting the nearby and quiet M dwarf TOI-270

121 citations · 1k across the 38 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

28 papers · 1 filter

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.SR2021★ 119 cited

Constraining the Evolution of Cataclysmic Variables via the Masses and Accretion Rates of their Underlying White Dwarfs

A. F. Pala, B. T. Gänsicke, D. Belloni +28

We report on the masses (), effective temperatures () and secular mean accretion rates () of 43 cataclysmic variable (CV) wh…

astro-ph.SR2021

The 2019 outburst of the 2005 classical nova V1047 Cen: a record breaking dwarf nova outburst or a new phenomenon?

E. Aydi, K. V. Sokolovsky, J. S. Bright +28

We present a detailed study of the 2019 outburst of the cataclysmic variable V1047~Cen, which hosted a classical nova eruption in 2005. The peculiar outburst occurred 14 years afte…

astro-ph.SR2020

IM Normae: The Death Spiral of a Cataclysmic Variable?

Joseph Patterson, Jonathan Kemp, Berto Monard +18

We present a study of the orbital light curves of the recurrent nova IM Normae since its 2002 outburst. The broad "eclipses" recur with a 2.46 hour period, which increases on a tim…

astro-ph.SR2020★ 26 cited

The Spin-Period History of Intermediate Polars

Joseph Patterson, Enrique de Miguel, Jonathan Kemp +25

We report the detailed history of spin-period changes in five intermediate polars (DQ Herculis, AO Piscium, FO Aquarii, V1223 Sagittarii, and BG Canis Minoris) during the 30-60 yea…

astro-ph.SR2019★ 3 cited

Infrared spectroscopy of the recent outburst in V1047 Cen (Nova Centauri 2005)

T. R. Geballe, D. P. K. Banerjee, A. Evans +14

Fourteen years after its eruption as a classical nova (CN), V1047 Cen (Nova Cen 2005) began an unusual re-brightening in 2019 April. The amplitude of the brightening suggests that…

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★ 23 cited

Fast-Cadence TESS Photometry and Doppler Tomography of the Asynchronous Polar CD Ind: A Revised Accretion Geometry from Newly Proposed Spin and Orbital Periods

Colin Littlefield, Peter Garnavich, Koji Mukai +5

The TESS spacecraft observed the asynchronous polar CD Ind at a two-minute cadence almost continuously for 28 days in 2018, covering parts of 5 consecutive cycles of the system's 7…

astro-ph.SR2019★ 11 cited

NSV 1440: First WZ Sge-type Object in AM CVn stars and candidates

Keisuke Isogai, Taichi Kato, Berto Monard +5

In 2015 and 2017, the AM CVn candidate NSV 1440 showed superoutbursts having the characteristic features of WZ Sge-type dwarf novae (DNe). By analogy with hydrogen-rich cataclysmic…

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.SR2018★ 25 cited

Evidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73-033933.0

A. F. Pala, B. T. Gänsicke, T. R. Marsh +21

We present high-time-resolution photometry and phase-resolved spectroscopy of the short-period () cataclysmic variable SDSS J123813.73-033933.…

astro-ph.SR2018★ 33 cited

Multiwavelength observations of V407 Lupi (ASASSN-16kt) --- a very fast nova erupting in an intermediate polar

E. Aydi, M. Orio, A. P. Beardmore +19

We present a detailed study of the 2016 eruption of nova V407 Lupi (ASASSN-16kt), including optical, near-infrared, X-ray, and ultraviolet data from SALT, SMARTS, SOAR, Chandra, Sw…

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…

astro-ph.SR2018★ 26 cited

High-Time-Resolution Photometry of AR Scorpii: Confirmation of the White Dwarf's Spin-Down

Robert A. Stiller, Colin Littlefield, Peter Garnavich +3

The unique binary AR Scorpii consists of an asynchronously rotating, magnetized white dwarf (WD) that interacts with its red-dwarf companion to produce a large-amplitude, highly co…

astro-ph.SR2018★ 11 cited

Orbital Period Increase in ES Ceti

Enrique de Miguel, Joseph Patterson, Jonathan Kemp +5

We report a long-term study of the eclipse times in the 10-minute helium binary ES Ceti. The binary period increases rapidly, with P/P-dot = 6.2x10^6 yr. This is consistent with th…

astro-ph.SR2017★ 8 cited

Orbital Period Changes in WZ Sagittae

Joseph Patterson, Geoffrey Stone, Jonathan Kemp +19

We report a long-term (1961-2017) study of the eclipse times in the dwarf nova WZ Sagittae, in an effort to learn its rate of orbital-period change. Some wiggles with a time scale…

astro-ph.SR2017★ 23 cited

A Bright Short Period M-M Eclipsing Binary from the KELT Survey: Magnetic Activity and the Mass-Radius Relationship for M-dwarfs

Jack B. Lubin, Joseph E. Rodriguez, George Zhou +26

We report the discovery of KELT J041621-620046, a moderately bright (J10.2) M dwarf eclipsing binary system at a distance of 393 pc. KELT J041621-620046 was first identi…

astro-ph.SR2017★ 99 cited

Effective Temperatures of Cataclysmic Variable White Dwarfs as a Probe of their Evolution

A. F. Pala, B. T. Gänsicke, D. Townsley +29

We present HST spectroscopy for 45 cataclysmic variables (CVs), observed with HST/COS and HST/STIS. For 36 CVs, the white dwarf is recognisable through its broad Ly absorption p…

astro-ph.SR2017★ 20 cited

Resynchronization of the Asynchronous Polar CD Ind

G. Myers, J. Patterson, E. de Miguel +6

CD Ind is one of only four confirmed asynchronous polars (APs). APs are strongly magnetic cataclysmic variables of the AM Herculis subclass with the characteristic that their white…

astro-ph.SR2016★ 21 cited

Return of the King: Time-Series Photometry of FO Aquarii's Initial Recovery from its Unprecedented 2016 Low State

Colin Littlefield, Peter Garnavich, Mark R. Kennedy +28

In 2016 May, the intermediate polar FO~Aqr was detected in a low state for the first time in its observational history. We report time-resolved photometry of the system during its…

astro-ph.SR2016★ 10 cited

GW Librae: Still Hot Eight Years Post-Outburst

Paula Szkody, Anjum S. Mukadam, Boris T. Gaensicke +8

We report continued Hubble Space Telescope (HST) ultraviolet spectra and ground-based optical photometry and spectroscopy of GW Librae eight years after its largest known dwarf nov…

astro-ph.SR2016★ 21 cited

GW Librae: A unique laboratory for pulsations in an accreting white dwarf

O. Toloza, B. T. Gaensicke, J. J. Hermes +22

Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic variables. These stars offer insight into the excitation of pulsation modes in atmos…

astro-ph.SR2016★ 23 cited

T Pyxidis: Death by a Thousand Novae

Joseph Patterson, Arto Oksanen, Jonathan Kemp +14

We report a 20-year campaign to track the 1.8 hour photometric wave in the recurrent nova T Pyxidis, using the global telescope network of the Center for Backyard Astrophysics. Dur…

astro-ph.SR2013★ 4 cited

The Death Spiral of T Pyxidis

Joseph Patterson, Arto Oksanen, Berto Monard +12

We report a long campaign to track the 1.8 hr photometric wave in the recurrent nova T Pyxidis, using the global telescope network of the Center for Backyard Astrophysics. During 1…