Detectors for exoplanets thrive in slight disorder

To study distant planets, SRON researchers are developing detectors that register the colour of each incoming photon. They are searching for a suitable material with a high degree of ‘disorder’ and therefore high electrical resistance in order to absorb as much light as possible. They have now discovered that too much disorder is also not ideal because it results in signal loss. Publication in Nature Communications.

What you see is a strong enlargement of a gold-coloured holder with an incoming and outgoing connection, which holds a somewhat brownish-looking wafer material, with a lighter-coloured chip in the centre.

Assembly of Demonstration Model for X-IFU camera is complete

SRON is responsible for building the camera for the X-IFU imaging spectrometer onboard the NewAthena X-ray space telescope. A latest Demonstration Model has now been successfully assembled in SRON’s cleanroom and is mounted into a cryogenic test setup which cools the detector stage to a temperature of 50 milliKelvin.

A gold-coloured mechanical structure with lots of mounting details and connector slots is carefully prepared for lifting it out of its black transport box.
A man, Jochem Baselmans, is standing next to a hanging experimental setup with lots of gold and silver couloured structures. It's the inside of a cryostat, used to cool experiments to very low temperatures. The man is holding a chip in it's mount, that he is about to test inside the cryostat soon.

XRISM sees surprisingly slow and dense wind from neutron star

A team of XRISM researchers, including SRON astronomers, has seen a surprisingly slow and thick wind blowing from the disc around a neutron star. Instead of the 200 million km/h that winds from supermassive black holes typically reach, the neutron star GX13+1 blows out a wind of only one million km/h. SRON provided the filter wheel including calibration sources to XRISM’s Resolve instrument.

We see a visual representation of a neutron star, pulling matter from it's companion star. The neutron star looks bright and white and appears fast spinning. Bright strokes coming from the bright dense smaller star in the middle seem to represent winds.

Gravitational Waves Celebrate 10-year Anniversary

Ten years ago, on 14 September 2015, the ground-based gravitational wave detector LIGO started its first observing run. About 1.4 billion years earlier, two black holes had collided in a far-away galaxy, producing a powerful gravitational wave. Already then, it was determined that the wave would reach the Earth on precisely 14 September 2015. Yet for it to become the first gravitational wave measured by humanity, a lot had to happen.

Two black circles are close together in a space. The image of the cloud- and mist-like structures near the two black circles becomes increasingly distorted the closer it is to the circles.

PLATO arrives in Noordwijk for final step towards launch

Are there planets similar to Earth? Do they orbit stars like our sun? Which type of parent stars and planets often go together? Which planets have an atmosphere that we can further investigate? From late 2026 onwards, the PLATO space telescope will search for answers.

We see a large hall with four people in laboratory clothing. Centrally in the image, we see the gold-coloured mirrors of 26 cameras from a satellite standing on a mobile platform. We see this through a layer of foil covering the entire satellite.
De nieuwsgierige SRON-mascotte Sam Space kijkt naar een planeet en een telescoop in de ruimte