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New paper: Transit visibility zones of the solar system planets ?>

New paper: Transit visibility zones of the solar system planets

New paper by my PhD student Rob Wells: The detection of thousands of extrasolar planets by the transit method naturally raises the question of whether potential extrasolar observers could detect the transits of the Solar System planets. We present a comprehensive analysis of the regions in the sky from where transit events of the Solar System planets can be detected. We specify how many different Solar System planets can be observed from any given point in the sky, and find…

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Arcus, a new high-resolution X-ray spectrometer in space ?>

Arcus, a new high-resolution X-ray spectrometer in space

Very good news: the Arcus mission – a high-resolution X-ray spectrograph onboard a small space telescope – has received funding from NASA for a concept study! I am part of the proposal team as an international collaborator, our PI is Randall Smith from the Harvard-Smithsonian Center for Astrophysics. We just received 2 million US$ funding through NASA’s MIDEX mission call for phase A, and we will be working frantically on Arcus for the next year to demonstrate it can actually…

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New paper: Next Generation Transit Survey (1) ?>

New paper: Next Generation Transit Survey (1)

I’m happy to be part of the Next Generation Transit Survey (NGTS) collaboration, a ground-based array of telescopes in Chile searching for exoplanets transiting their host stars. We have just published a paper on detecting false positives with NGTS, namely background transits of dim stars across brighter stars, through centroid vetting. The paper is accepted for publication by Monthly Notices of the Royal Astronomical Society. “Centroid vetting of transiting planet candidates from the Next Generation Transit Survey”, accepted by MNRAS…

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New paper: Magnetic activity of old cool stars ?>

New paper: Magnetic activity of old cool stars

Happy to report that my PhD student Rachel Booth has successfully published her first paper! It’s a very interesting analysis of the magnetic activity of old cool stars, with a surprising find about the decline of activity at old stellar ages. Our paper has also been featured on the Astrobites blog: https://astrobites.org/2017/07/03/adventures-in-watchmaking-for-cool-stars/. Here’s the abstract of the paper: Stars with convective envelopes display magnetic activity, which decreases over time due to the magnetic braking of the star. This age-dependence of…

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Conference “Atmospheres of disks and planets” at castle Ringberg ?>

Conference “Atmospheres of disks and planets” at castle Ringberg

I just spent a really exciting week at castle Ringberg in south Germany, where the Max-Planck Institute for Astronomy held a conference on exoplanet formation and atmospheric composition. Lots of interesting discussions and new results. I was invited to give a talk on the topic of “Stellar activity and planet characterisation” – one of my favourite topics to talk about. My personal highlight of the conference was Yamila Miguel’s presentation about the latest results from the Juno mission: we finally…

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Today’s seminar: R Coronae Borealis stars ?>

Today’s seminar: R Coronae Borealis stars

Today Geoff Clayton from Louisiana State University gave a talk about R Coronae Borealis stars at our astrophysics seminar. These kinds of stars show erratic drops of several magnitudes in brightness over hundreds of years (R Coronae Borealis itself was discovered to be variable in 1795), and it’s still a somewhat open question what these things actually *are*. It’s not at all my field of study, but it was a really interesting talk and exactly the kind of talk I…

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New paper: Testing if Fomalhaut b is a neutron star ?>

New paper: Testing if Fomalhaut b is a neutron star

Happy to report that our paper has also been picked for presentation on the Astrobites blog: https://astrobites.org/2017/03/24/a-neutron-star-in-the-eye-of-sauron/. Here’s the abstract of the paper: Fomalhaut b is a directly imaged object in the debris disk of the star Fomalhaut. It has been hypothesized to be a planet, however there are issues with the observed colours of the object that do not fit planetary models. An alternative hypothesis is that the object is a neutron star in the near fore- or background…

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New paper on magnetic cycle simulation of Proxima Centauri ?>

New paper on magnetic cycle simulation of Proxima Centauri

The recent discovery of an Earth-like exoplanet around Proxima Centauri has shined a spot light on slowly rotating fully convective M-stars. When such stars rotate rapidly (period <20 days), they are known to generate very high levels of activity that is powered by a magnetic field much stronger than the solar magnetic field. Recent theoretical efforts are beginning to understand the dynamo process that generates such strong magnetic fields. However, the observational and theoretical landscape remains relatively uncharted for fully…

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New papers on the ARCUS mission ?>

New papers on the ARCUS mission

Arcus is a NASA/MIDEX mission under development in response to the anticipated 2016 call for proposals. It is a freeflying, soft X-ray grating spectrometer with the highest-ever spectral resolution in the 8-51 Å (0.24 – 1.55 keV) energy range. The Arcus bandpass includes the most sensitive tracers of diffuse million-degree gas: spectral lines from O VII and O VIII, H- and He-like lines of C, N, Ne and Mg, and unique density- and temperature-sensitive lines from Si and Fe ions….

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New paper on the disappearing disk of TYC 8241 2652 1 ?>

New paper on the disappearing disk of TYC 8241 2652 1

TYC 8241 2652 1 is a young star that showed a strong mid-infrared (mid-IR, 8-25 mu) excess in all observations before 2008 consistent with a dusty disk. Between 2008 and 2010 the mid-IR luminosity of this system dropped dramatically by at least a factor of 30 suggesting a loss of dust mass of an order of magnitude or more. We aim to constrain possible models including removal of disk material by stellar activity processes, the presence of a binary companion,…

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