M. R. Goad
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View article: A 43 day transiting Neptune and two 25 day Saturns from TESS, NGTS and ASTEP
A 43 day transiting Neptune and two 25 day Saturns from TESS, NGTS and ASTEP Open
Beyond orbital periods of 10 days, there is a dearth of known transiting gas giants. On longer orbits, planets are less affected by their host star, and become ideal probes of planet formation, migration and evolution. We report the discov…
View article: TOI-333b: A Neptune Desert planet around a F7V star
TOI-333b: A Neptune Desert planet around a F7V star Open
Observations have shown that planets similar to Neptune are rarely found orbiting Sun-like stars with periods up to ~4 days, defining the so-called Neptune desert region. Therefore, the detection of each individual planet in this region ho…
View article: Continuum Reverberation Mapping of 18 AGN Over Four Years
Continuum Reverberation Mapping of 18 AGN Over Four Years Open
Continuum reverberation mapping probes the size scale of the optical continuum-emitting region in active galactic nuclei (AGN). The source of this emission has long been thought to originate from the accretion disk, but recent studies sugg…
View article: The variability of active galaxies – I. Broad-band noise X-ray power spectra from <i>XMM–Newton</i> and <i>Swift</i>
The variability of active galaxies – I. Broad-band noise X-ray power spectra from <i>XMM–Newton</i> and <i>Swift</i> Open
Accreting supermassive black holes at the centres of galaxies are the engine of active galactic nuclei (AGNs). X-ray light curves of unabsorbed AGNs show dramatic random variability on time-scales ranging from seconds to years. The power s…
View article: Detection and characterisation of a 106-day transiting Jupiter: TOI-2449 b/NGTS-36 b
Detection and characterisation of a 106-day transiting Jupiter: TOI-2449 b/NGTS-36 b Open
Context . Only a handful of transiting giant exoplanets with orbital periods longer than 100 days are known. These warm exoplanets are valuable objects, as their radius and mass can be measured and lead to an in-depth characterisation of t…
View article: UV/optical active galactic nuclei reverberation mapping: using a SmallSat to trade time resolution for spatial resolution to study accretion disks around supermassive black holes at the centers of galaxies
UV/optical active galactic nuclei reverberation mapping: using a SmallSat to trade time resolution for spatial resolution to study accretion disks around supermassive black holes at the centers of galaxies Open
View article: Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 b
Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 b Open
Only a handful of transiting giant exoplanets with orbital periods longer than 100 days are known. These warm exoplanets are valuable objects as their radius and mass can be measured leading to an in-depth characterisation of the planet's …
View article: Departures from standard disc predictions in intensive ground-based monitoring of three AGNs
Departures from standard disc predictions in intensive ground-based monitoring of three AGNs Open
We present ground-based multiband light curves of the AGN Mrk 509, NGC 4151, and NGC 4593 obtained contemporaneously with Swift monitoring. We measure cross-correlation lags relative to Swift UVW2 (1928 Å) and test the standard prediction …
View article: Echo mapping of the black hole accretion flow in NGC 7469
Echo mapping of the black hole accretion flow in NGC 7469 Open
Reverberation mapping (RM) can measure black hole accretion disc sizes and radial structure through observable light travel time lags that should increase with wavelength as $\tau \propto \lambda ^{4/3}$ due to the disc’s $T\propto r^{-3/4…
View article: Investigating the Variable Continuum Lags in PG 2130+099
Investigating the Variable Continuum Lags in PG 2130+099 Open
Broadband photometric reverberation mapping (RM) provides a measure of the size of the continuum-emitting region in active galactic nuclei (AGN). Previous monitoring campaigns of PG 2130+099 disagree as to whether the continuum-emitting re…
View article: <i>NGTS</i>-EB-7, an eccentric, long-period, low-mass eclipsing binary
<i>NGTS</i>-EB-7, an eccentric, long-period, low-mass eclipsing binary Open
Despite being the most common types of stars in the Galaxy, the physical properties of late M dwarfs are often poorly constrained. A trend of radius inflation compared to evolutionary models has been observed for earlier type M dwarfs in e…
View article: NGTS-31b and NGTS-32b: two inflated hot Jupiters orbiting subgiant stars
NGTS-31b and NGTS-32b: two inflated hot Jupiters orbiting subgiant stars Open
We present the discoveries of NGTS-31b(= TOI-2721), and NGTS-32b, two hot Jupiters from the Next Generation Transit Survey (NGTS) transiting slightly evolved stars. The orbital periods, radii, and masses are 4.16 and 3.31 d, 1.61 and 1.42 …
View article: NGTS-33b: a young super-Jupiter hosted by a fast-rotating massive hot star
NGTS-33b: a young super-Jupiter hosted by a fast-rotating massive hot star Open
In the last few decades, planet search surveys have been focusing on solar-type stars, and only recently the high-mass regimes. This is mostly due to challenges arising from the lack of instrumental precision, and more importantly, the inh…
View article: NGTS-33b: A Young Super-Jupiter Hosted by a Fast Rotating Massive Hot Star
NGTS-33b: A Young Super-Jupiter Hosted by a Fast Rotating Massive Hot Star Open
In the last few decades planet search surveys have been focusing on solar type stars, and only recently the high-mass regimes. This is mostly due to challenges arising from the lack of instrumental precision, and more importantly, the inhe…
View article: AGN STORM 2. X. The Origin of the Interband Continuum Delays in Mrk 817*
AGN STORM 2. X. The Origin of the Interband Continuum Delays in Mrk 817* Open
The local ( z = 0.0315) active galactic nucleus (AGN) Mrk 817 was monitored over more than 500 days with space-borne and ground-based instruments as part of a large international campaign, AGN STORM 2. Here, we present a comprehensive anal…
View article: AGN STORM 2: X. The origin of the interband continuum delays in Mrk 817
AGN STORM 2: X. The origin of the interband continuum delays in Mrk 817 Open
The local (z=0.0315) AGN Mrk 817, was monitored over more than 500 days with space-borne and ground-based instruments as part of a large international campaign AGN STORM 2. Here, we present a comprehensive analysis of the broad-band contin…
View article: AGN STORM 2. VII. A Frequency-resolved Map of the Accretion Disk in Mrk 817: Simultaneous X-Ray Reverberation and UVOIR Disk Reprocessing Time Lags
AGN STORM 2. VII. A Frequency-resolved Map of the Accretion Disk in Mrk 817: Simultaneous X-Ray Reverberation and UVOIR Disk Reprocessing Time Lags Open
X-ray reverberation mapping is a powerful technique for probing the innermost accretion disk, whereas continuum reverberation mapping in the UV, optical, and infrared (UVOIR) reveals reprocessing by the rest of the accretion disk and broad…
View article: AGN STORM 2. IX. Studying the Dynamics of the Ionized Obscurer in Mrk 817 with High-resolution X-Ray Spectroscopy
AGN STORM 2. IX. Studying the Dynamics of the Ionized Obscurer in Mrk 817 with High-resolution X-Ray Spectroscopy Open
We present the results of the XMM-Newton and NuSTAR observations taken as part of the ongoing, intensive multiwavelength monitoring program of the Seyfert 1 galaxy Mrk 817 by the AGN Space Telescope and Optical Reverberation Mapping 2 (AGN…
View article: Intensive Broadband Reverberation Mapping of Fairall 9 with 1.8 yr of Daily Swift Monitoring
Intensive Broadband Reverberation Mapping of Fairall 9 with 1.8 yr of Daily Swift Monitoring Open
We present 1.8 yr of near-daily Swift monitoring of the bright, strongly variable Type 1 active galactic nucleus (AGN) Fairall 9. Totaling 575 successful visits, this is the largest such campaign reported to date. Variations within the UV/…
View article: AGN STORM 2. VII. A Frequency-resolved Map of the Accretion Disk in Mrk 817: Simultaneous X-ray Reverberation and UVOIR Disk Reprocessing Time Lags
AGN STORM 2. VII. A Frequency-resolved Map of the Accretion Disk in Mrk 817: Simultaneous X-ray Reverberation and UVOIR Disk Reprocessing Time Lags Open
X-ray reverberation mapping is a powerful technique for probing the innermost accretion disk, whereas continuum reverberation mapping in the UV, optical, and infrared (UVOIR) reveals reprocessing by the rest of the accretion disk and broad…
View article: AGN STORM 2. VIII. Investigating the Narrow Absorption Lines in Mrk 817 Using HST-COS Observations*
AGN STORM 2. VIII. Investigating the Narrow Absorption Lines in Mrk 817 Using HST-COS Observations* Open
We observed the Seyfert 1 galaxy Mrk 817 during an intensive multiwavelength reverberation mapping campaign for 16 months. Here, we examine the behavior of narrow UV absorption lines seen in the Hubble Space Telescope/Cosmic Origins Spectr…
View article: TOI-2490b – the most eccentric brown dwarf transiting in the brown dwarf desert
TOI-2490b – the most eccentric brown dwarf transiting in the brown dwarf desert Open
We report the discovery of the most eccentric transiting brown dwarf in the brown dwarf desert, TOI-2490b. The brown dwarf desert is the lack of brown dwarfs around main-sequence stars within $\sim 3$ au and is thought to be caused by diff…
View article: TOI-2490b- The most eccentric brown dwarf transiting in the brown dwarf desert
TOI-2490b- The most eccentric brown dwarf transiting in the brown dwarf desert Open
We report the discovery of the most eccentric transiting brown dwarf in the brown dwarf desert, TOI02490b. The brown dwarf desert is the lack of brown dwarfs around main sequence stars within $\sim3$~AU and is thought to be caused by diffe…
View article: Intensive broadband reverberation mapping of Fairall 9 with 1.8 years of daily Swift monitoring
Intensive broadband reverberation mapping of Fairall 9 with 1.8 years of daily Swift monitoring Open
We present 1.8 years of near-daily Swift monitoring of the bright, strongly variable Type 1 AGN Fairall 9. Totaling 575 successful visits, this is the largest such campaign reported to date. Variations within the UV/optical are well-correl…
View article: TOI-2447 b / NGTS-29 b: a 69-day Saturn around a Solar analogue
TOI-2447 b / NGTS-29 b: a 69-day Saturn around a Solar analogue Open
Discovering transiting exoplanets with relatively long orbital periods (>10 d) is crucial to facilitate the study of cool exoplanet atmospheres (Teq < 700 K) and to understand exoplanet formation and inward migration further out than…
View article: AGN STORM 2: VIII. Investigating the Narrow Absorption Lines in Mrk 817 Using HST-COS Observations
AGN STORM 2: VIII. Investigating the Narrow Absorption Lines in Mrk 817 Using HST-COS Observations Open
We observed the Seyfert 1 galaxy Mrk817 during an intensive multi-wavelength reverberation mapping campaign for 16 months. Here, we examine the behavior of narrow UV absorption lines seen in HST/COS spectra, both during the campaign and in…
View article: Photo-dynamical characterisation of the TOI-178 resonant chain
Photo-dynamical characterisation of the TOI-178 resonant chain Open
Context . The TOI-178 system consists of a nearby, late-K-dwarf with six transiting planets in the super-Earth to mini-Neptune regime, with radii ranging from to 2.9 R ⊕ and orbital periods between 1.9 and 20.7 days. All the planets, but t…
View article: AGN STORM 2: IX. Studying the Dynamics of the Ionized Obscurer in Mrk 817 with High-resolution X-ray Spectroscopy
AGN STORM 2: IX. Studying the Dynamics of the Ionized Obscurer in Mrk 817 with High-resolution X-ray Spectroscopy Open
We present the results of the XMM-Newton and NuSTAR observations taken as part of the ongoing, intensive multi-wavelength monitoring program of the Seyfert 1 galaxy Mrk 817 by the AGN Space Telescope and Optical Reverberation Mapping 2 (AG…
View article: TOI-2447 b / NGTS-29 b: a 69-day Saturn around a Solar analogue
TOI-2447 b / NGTS-29 b: a 69-day Saturn around a Solar analogue Open
Discovering transiting exoplanets with relatively long orbital periods ($>$10 days) is crucial to facilitate the study of cool exoplanet atmospheres ($T_{\rm eq} < 700 K$) and to understand exoplanet formation and inward migration further …
View article: Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data
Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data Open
We present the results from the first two years of the Planet Hunters Next Generation Transit Survey (NGTS) citizen science project, which searches for transiting planet candidates in data from the NGTS by enlisting the help of members of …