activity
20182021
most citedAn Ultra-Hot Neptune in the Neptune desert

85 citations · 402 across the 12 of their papers we have counts for

collaborators

21 papers

astro-ph.EP202118 cited

NGTS-14Ab: a Neptune-sized transiting planet in the desert

A. M. S. Smith, J. S. Acton, D. R. Anderson +35

Context: The sub-Jovian or Neptunian desert is a previously-identified region of parameter space where there is a relative dearth of intermediate-mass planets at short orbital peri…

astro-ph.EP202085 cited

An Ultra-Hot Neptune in the Neptune desert

James S. Jenkins, Matías R. Díaz, Nicolás T. Kurtovic +81

About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the…

astro-ph.SR202017 cited

Bow-shocks, nova shells, disc winds and tilted discs: The Nova-Like V341 Ara Has It All

N. Castro Segura, C. Knigge, J. A. Acosta-Pulido +21

V341 Ara was recently recognised as one of the closest (d ~ 150 pc) and brightest (V~ 10) nova-like cataclysmic variables. This unique system is surrounded by a bright emission neb…

astro-ph.SR202018 cited

NGTS clusters survey -- II. White-light flares from the youngest stars in Orion

James A. G. Jackman, Peter J. Wheatley, Jack S. Acton +18

We present the detection of high energy white-light flares from pre-main sequence stars associated with the Orion complex, observed as part of the Next Generation Transit Survey (N…

astro-ph.SR202043 cited

WD1032+011, an inflated brown dwarf in an old eclipsing binary with a white dwarf

S. L. Casewell, C. Belardi, S. G. Parsons +11

We present the discovery of only the third brown dwarf known to eclipse a non-accreting white dwarf. Gaia parallax information and multi-colour photometry confirm that the white dw…

astro-ph.EP202053 cited

Simultaneous TESS and NGTS Transit Observations of WASP-166b

Edward M. Bryant, Daniel Bayliss, James McCormac +21

We observed a transit of WASP-166 b using nine NGTS telescopes simultaneously with TESS observations of the same transit. We achieved a photometric precision of 152 ppm per 30 minu…