Euclid Space Warps – help the hunt for galaxy-galaxy lenses!

Posted in Euclid, The Universe and Stuff with tags , , , on April 21, 2026 by telescoper
A collage of fourteen by eight squares containing examples of gravitational lenses. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by M. Walmsley, M. Huertas-Company, J.-C. Cuillandre.

I’m sharing the text of a press release from Euclid here to encourage readers to join in this new Zooniverse project.

–o–

In brief

With the launch of Space Warps, a new citizen science project on the Zooniverse platform, you can now join in the search to find rare and elusive strong gravitational lenses in never-before-seen images captured by the European Space Agency’s Euclid space telescope. The project aims at shining a light on dark matter in galaxies and providing clues about mysterious dark energy.

In-depth

Warps in spacetime do not only show up in science fiction movies like Interstellar. In real life, we can see the warping effect that gravity has on spacetime in the form of gravitational lensing.

The enormous gravity of a massive object – such as a galaxy or cluster of galaxies – distorts the shape of spacetime and can bend the light rays coming from a distant galaxy behind. By warping spacetime, the foreground galaxy acts like a magnifying glass.

Light from the background object that would be obscured doesn’t travel in a straight line anymore. Instead, it curves around the intervening mass, often producing multiple images, stretched arcs, or even a complete ring known as ‘Einstein ring’, like the one recently discovered by Euclid.

Strong gravitational lenses offer a striking demonstration of Einstein’s theory of general relativity, showing that matter in the Universe can act as a natural telescope, bringing distant objects into sight.

ESA’s Euclid telescope is revolutionising the studies of strong gravitational lensing by providing very sensitive imaging over large swaths of the sky in unprecedented detail. This is exactly what is needed to identify rare gravitational lenses.

In March 2025, 500 galaxy-galaxy strong lenses were found nestled in just the first 0.04% of Euclid data, most of them previously unknown. This pioneering catalogue was created thanks to the combined effort from citizen scientists, artificial intelligence (AI) and researchers.

Early glimpse of new Euclid images

As Euclid continues its survey, sending around 100 GB of data back to Earth every day, ESA and the Euclid Consortium once again need help from citizen scientists to identify strong gravitational lenses in a large data set.

For this, the Space Warps team has launched a citizen science project based on new Euclid images, which will be part of the future Euclid Data Release 1. While this data is not public yet, by participating in this new citizen science project you can get an early glimpse of these new images of galaxies captured by the telescope.

For this project, you will be inspecting new high quality imaging data from Euclid in which many previously unknown strong lenses are hiding. About three hundred thousand images pre-selected by AI algorithms will be shown, which are fine-tuned with the results from the initial citizen-science Euclid strong lens search. These are the highest ranked candidates from a whopping 72 million galaxies from DR1 that were classified by the AI algorithms. Scientists expect that this exquisite high-quality data will reveal more than 10 000 new lenses.

What can we learn from strong lenses

The Euclid mission explores how the Universe has expanded and how its structure has changed through cosmic history using mainly two methods: weak lensing and baryonic acoustic oscillations. From this, scientists can learn more about the role of gravity and the nature of dark matter and dark energy.

Strong gravitational lenses can also provide insights into these central questions. For example, strong lensing features can ‘weigh’ individual galaxies and clusters of galaxies. This reveals the total matter (whether dark or light) and traces the distribution of dark matter. By studying strong lenses across cosmic time, scientists can trace the expansion of the Universe and its apparent acceleration. This will provide additional insight into the role of dark energy.

“We’ve already seen the success of combining AI with visual inspection by citizen volunteers and scientists on Space Warps, efficiently finding hundreds of high‑probability lens candidates in an initial small Euclid search in 2024”, explains Aprajita Verma, Space Warps’ co-founder and project lead at the University of Oxford, UK.
“In this brand new DR1 data, 30 times larger than the initial search and together with our improved AI algorithms, we are expecting to find more than 10 000 high quality lens candidates. This is more than four times the number of lenses than we have been able to find since the first gravitational lens was discovered nearly 50 years ago.”

This step-change is possible thanks to Euclid. The mission can map large areas of the sky with unique sharpness, an ideal combination for finding rare objects like strong gravitational lenses.

“We can’t wait to see what we will find within this unprecedented dataset. Join us on Space Warps to take part in this exciting search!” concludes Aprajita.

About Euclid
Euclid was launched in July 2023 and started its routine science observations on 14 February 2024. The goal of the mission is to reveal the hidden influence of dark matter and dark energy on the visible Universe. Over a period of six years, Euclid will observe the shapes, distances and motions of billions of galaxies out to 10 billion light-years.

Euclid is a European mission, built and operated by ESA, with contributions from NASA. The Euclid Consortium – consisting of more than 2000 scientist from 300 institutes in 15 European countries, the USA, Canada, and Japan – is responsible for providing the scientific instruments and scientific data analysis. ESA selected Thales Alenia Space as prime contractor for the construction of the satellite and its service module, with Airbus Defence and Space chosen to develop the payload module, including the telescope. NASA provided the detectors of the Near-Infrared Spectrometer and Photometer, NISP. Euclid is a medium-class mission in ESA’s Cosmic Vision Programme.

Estella Solomons

Posted in Art, History with tags , , , , on April 20, 2026 by telescoper

Following yesterday’s post about the 1926 Irish Census I fell down a metaphorical rabbit hole following a request from a former colleague (who happens to be Jewish) to help find a relative of his who lived in Dublin at the time of the census. I found the person, which was nice, but was then sent this article  about an unrelated lady called Estella Solomons who was on the rebel side in the Easter Rising and helped the cause by hiding weapons in her garden.  It turns out that there was a significant Jewish presence in Dublin back then. In the North Side, around Portobello, there was an area dubbed ‘Little Jerusalem’.

Estella Solomons, self-portrait

I hadn’t heard of Estella Solomons before yesterday but she was a significant artist whose work was featured in an exhibition at the National Gallery in Dublin in 2022 (which I did not see). There is also a Wikipedia page about her. I found the above self-portrait online. I find it very striking.

Estella Solomons was born in 1882 and died in 1968 at the age of 86. She was 34 at the time of the Easter Rising and would have been 44 at the time of the 1926 census. I did find her in the online census but her age is recorded as 40. She married the poet Seumas O’Sullivan in 1926 but she is listed as “single” on the census form, so presumably they married later in the year.

There are two other women at her 1926 address, both servants, so she was obviously quite well off, but no sign of her husband.

More surprisingly Estella’s sex is given in the 1926 census as Male. She is in the 1911 census too, but recorded there as Female. I did consider the possibility that she might have been living as a man, but that does not fit with other details of her life. I think it is just a mistake.  Such records are not entirely free from errors.

I think this an example of the sort of confusion historians have to contend with when looking at historical documents!

The 1926 Census of Ireland

Posted in Biographical, History with tags , , , , , , on April 19, 2026 by telescoper

An interesting little booklet arrived in the post yesterday. It gives an overview of the 1926 census, which has just been made available online. This was the first census to be taken after the end of the War of Independence , the Irish Civil War, and the creation of the Irish Free State.

The census was taken on April 18th 1926 (i.e. 100 years ago yesterday) and the total population recorded was just 2,971, 992, a drop of 168,000 compared to the 1911 census (for the same 26 counties; this being after partition, the six counties of Northern Ireland are not included). The current population of the Republic is around 5.3 million.

This is indeed a full release of the census: not only names and numbers but also complete digital scans of all the returns can be downloaded. It’s fascinating to see the actually hand-written forms.

Out of curiosity I searched for the surname “Coles” in the 1926 census using the online platform and found only 25 entries, most of them in Wexford but also a small cluster in County Cork (in Cobh, actually). I know that “Coles” is not a common name in Ireland – it’s associated with England and Wales – but I hadn’t expected so few. There are a couple of entries in Dublin: one refers to a 32-year old woman called “Alfa Coles”. The latter record is completed in Irish – most of the others are in English. It seems people had much nicer handwriting in those days!

Some years ago I found that there is a Coles Coat of Arms and subsequently found that in Burkes General Armory (which details all the Coats of Arms registered in the UK and Ireland) the first entry under the surname Coles is indeed in Ireland, where it was confirmed in 1647. That date is during the Irish Confederate Wars, a couple of years before Oliver Cromwell arrived in Ireland with his army. One might surmise that this particular branch of the Coles lineage was somehow caught up in these hostilities, probably on the English side.

Anyway, as well as being a goldmine for historians, those of you out there with Irish lineage will no doubt find it interesting to search the 1926 census to find the records pertaining to your ancestors.

The next census of Ireland takes place on 9th May 2027.

P.S. If you do search the archive and find a record in Irish please remember that in Irish “man” is fear and “woman” is “bean” so “F” actually means “male” in Irish and “B” stands for “female” (unlike “M” and “F” in the English version).

Weekly Update from the Open Journal of Astrophysics – 18/04/2026

Posted in OJAp Papers, Open Access, The Universe and Stuff with tags , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , on April 18, 2026 by telescoper

It is Saturday morning, and therefore time for yet another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further six papers, bringing the number in Volume 9 (2026) to 82 and the total so far published by OJAp up to 530.

I will continue to include the posts made on our Mastodon account (on Fediscience) to encourage you to visit it. Mastodon is a really excellent service, and a more than adequate replacement for X/Twitter (which nobody should be using); these announcements also show the DOI for each paper.

The first paper to report this week is “Beyond Spherical geometry: Unraveling complex features of objects orbiting around stars from its transit light curve using deep learning” by Ushasi Bhowmick & Shivam Kumaran (Indian Space Research Institute, Ahmedabad, India). This study uses deep neural networks to predict the shape of objects orbiting stars based on their transit light curves, demonstrating the potential to extract geometric information from these systems. It was published on Monday 13th April in the folder Earth and Planetary Astrophysics and the overlay can be seen here:

You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

Open Journal of Astrophysics

New Publication at the Open Journal of Astrophysics: "Beyond Spherical geometry: Unraveling complex features of objects orbiting around stars from its transit light curve using deep learning" by Ushasi Bhowmick & Shivam Kumaran (ISRO, Ahmedabad, India)

doi.org/10.33232/001c.160561

April 13, 2026, 6:31 am 1 boosts 1 favorites

The second paper for this week, also published on Monday 13th April Apil in the folder but in the folder Astrophysics of Galaxies, is “statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys” by Elizaveta Sazonova (U. Waterloo, Canada) and an international cast of 18 others. This paper presents an investigation of potential biases in quantitative morphology metrics used in galaxy evolution studies, proposing two new measurements to resolve biases, and provides a related Python package (statmorph-lsst), which can be found here on github.

The overlay for this one is here:

The official version of the paper can be found on arXiv here and the Fediverse announcement here:

Open Journal of Astrophysics

New Publication at the Open Journal of Astrophysics: "statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys" by Elizaveta Sazonova (U. Waterloo, Canada) and an international cast of 18 others.

doi.org/10.33232/001c.160562

April 13, 2026, 6:51 am 3 boosts 1 favorites

Next one up, the third paper of the week, one of four published on Friday 17th April, is “Disentangling the galactic and intergalactic components in 313 observed Lyman-alpha line profiles between redshift 0 and 5” by Siddhartha Gurung-López (Universitat de València, Spain) and 7 others based in Spain and Germany. Published in the folder Astrophysics of Galaxies, this paper uses the zELDA package to analyze Lyman-alpha photons from star-forming galaxies, revealing IGM effects dominate Lyman-alpha observability at high redshifts, while galactic outflows become more important at lower z.

The overlay for this one is here:

The final, accepted version can be found on arXiv here and the Mastodon announcement is here:

Open Journal of Astrophysics

New Publication at the Open Journal of Astrophysics: "Disentangling the galactic and intergalactic components in 313 observed Lyman-alpha line profiles between redshift 0 and 5" by Siddhartha Gurung-López (Universitat de València, Spain) and 7 others based in Spain and Germany.

doi.org/10.33232/001c.160706

April 17, 2026, 7:19 am 1 boosts 0 favorites

The fourth paper this week, also published on Friday 17th April is “Using Symbolic Regression to Emulate the Radial Fourier Transform of the Sérsic Profile for Fast, Accurate and Differentiable Galaxy Profile Fitting” by Tim B. Miller (Northwestern University, USA) and Imad Pasha (Yale University, USA). This one is published in the folder Instrumentation and Methods for Astrophysics: it develops an emulator for galaxy profile fitting in Fourier space, improving speed by 2.5 times with minimal accuracy loss, aiding in managing increasing data flow.

The overlay is here:

The finally accepted version of this paper can be found here and the Mastodon announcement follows:

Open Journal of Astrophysics

New Publication at the Open Journal of Astrophysics: "Using Symbolic Regression to Emulate the Radial Fourier Transform of the Sérsic Profile for Fast, Accurate and Differentiable Galaxy Profile Fitting" by Tim B. Miller (Northwestern University, USA) and Imad Pasha (Yale University, USA)

doi.org/10.33232/001c.160755

April 17, 2026, 7:25 am 1 boosts 1 favorites

The fifth paper for this week is “The THESAN project: Lyman-alpha emitters as probes of ionized bubble sizes” by Meredith Neyer (MIT, USA) and 6 others based in the USA, Colombia, Canada, Japan and UK. The study uses THESAN simulations to explore how Lyman-alpha emitters (LAEs) trace ionized bubble sizes during the Epoch of Reionization, providing a framework for interpreting LAE surveys. This was published on Friday 17th April in the folder Astrophysics of Galaxies.

The overlay for this one is here:

You can find the authorized version of this paper on arXiv here and the Fediverse announcement is here:

Open Journal of Astrophysics

New Publication at the Open Journal of Astrophysics: "The THESAN project: Lyman-alpha emitters as probes of ionized bubble sizes" by Meredith Neyer (MIT, USA) and 6 others based in the USA, Colombia, Canada, Japan and UK.

doi.org/10.33232/001c.160756

April 17, 2026, 7:34 am 1 boosts 0 favorites

The sixth and final paper for this week is “Closed-Form Statistical Relations Between Projected Separation, Semimajor Axis, Companion Mass, and Host Acceleration” by Timothy D Brandt (Space Telescope Science Institute, USA). This was published on Friday 17th April in the folder Solar and Stellar Astrophysics. In this paper the author derives statistical relationships between radial velocity, a companion’s mass, and projected separation, useful for calculations requiring derivatives. The results are verified with empirical comparisons to existing literature.

The overlay for this one is here:

You can find the officially-accepted version on arXiv here and the Mastodon announcement here:

Open Journal of Astrophysics

New Publication at the Open Journal of Astrophysics: "Closed-Form Statistical Relations Between Projected Separation, Semimajor Axis, Companion Mass, and Host Acceleration" by Timothy D Brandt (Space Telescope Science Institute, USA)

doi.org/10.33232/001c.160757

April 17, 2026, 7:46 am 1 boosts 1 favorites

And that concludes this week’s update. I’ll do another one at the end of next week.

P.S. Just a reminder, for those of you into LinkedIn, that we now have a page there.

Biblical Me

Posted in Biographical, Politics with tags , , on April 17, 2026 by telescoper

It seems that after Donald Trump shared an image of himself as Jesus on social media,  ridiculous pictures of oneself in biblical settings have become all the rage. In that vein here is a picture of me downloading a paper from arXiv to read on my tablet:

The Perseus Cluster

Posted in Euclid, Maynooth, The Universe and Stuff with tags , , , , on April 16, 2026 by telescoper

In a vain attempt to convince my readership that I know anything about observational astronomy, I thought I’d share this image of the central regions of the Perseus Cluster (also known as Abell 426) made by my final-year project students:

Picture Credit: Ben Doyle

The image was taken last November using the 1.20m reflecting telescope at the Observatoire de Haute-Provence where the final-year astrophysics students from Maynooth spent a week last November on a field trip taking various observations. The exposure was 240 seconds and the field of view is about 15 arcminutes on a side. Most of the objects in the image are galaxies, rather than stars.

I asked my students to look at this cluster (which is about 10 degrees across), partly because it appears near the Zenith in November so would be a good target, partly because it is nearby so the galaxies in it are therefore quite bright, and partly because it was observed by Euclid and featured among the Early Release Observations. The Euclid telescope is also 1.20m in diameter, but because it has a very fancy camera and is in space, Euclid reveals far more galaxies but I was nevertheless impressed at how well this turned out!

The Original Peaky Blinders Jazz Band

Posted in History, Jazz, Television with tags , , , , on April 15, 2026 by telescoper

I’ve been greatly enjoying the boxed set of six seasons of Peaky Blinders that I received as a gift recently. I may do a sort of review when I get to the end, but until then I thought I’d throw in a few tangential things. This post is an example. Here’s another one. This clip is from Episode 2 of Series 1, when the Shelby family are celebrating the reopening of the Garrison pub after it was destroyed by a firebomb earlier on. Listen to the background music at the start.

The music being played is Livery Stable Blues by the Original Dixieland Jazz Band, a record I blogged about here. Released in 1917, it is no exaggeration to say that this was the first every commercial jazz record; I blogged about the 100th anniversary of its release.

The band was originally called the “Original Dixieland Jass Band“. A few months later they changed the “Jass” to “Jazz” – it is claimed because people kept defacing their posters by removing the letter “J” – and the new name stuck. The Original Dixieland Jazz Band is usually referred by Jazz buffs as the ODJB.

Led by cornettist Nick LaRocca and clarinettist Larry Shields, the ODJB was a group of white musicians from in and around New Orleans who had picked up their musical ideas from listening to musicians there, including playing for the pioneering mixed-race band led by Papa Laine, before moving to Chicago which is where they were spotted by representatives of the Victor label. Although the sound quality isn’t great, it gives a good insight to what ealy jazz drummers were like – thumping bass and tom-toms but little use of the cymbals – and shows Larry Shields was a dab hand at glissandi

Series 1 of Peaky Blinders is set in 1919 (mainly in Birmingham but also with scenes in London). Not a lot of people know that the ODJB actually visited England in 1919. They performed in review at the Hammersmith Palais and then did a command performance in front of King George V, who (apparently) particularly enjoyed their version of Tiger Rag. There is no evidence that they visited Birmingham, but we get a glimpse before the above clip of a band decked out to look like them, playing live in the Garrison pub. I very much enjoy little details like that!

John Venn’s Bowling Machine

Posted in Cricket, mathematics with tags , , on April 14, 2026 by telescoper

Most readers of this blog will be aware of the existence of Venn Diagrams, but not a lot of people know that their creator, John Venn, invented a mechanical bowling machine for use by cricketers in batting practice. Recently some folks at Cambridge University built a replica of this machine, presumably with the aid of some sort of diagram, and here’s a fascinating video about it.

Modern bowling machines fire the ball at you like a cannon, but this machine has the virtue of the batter being able to see the arm coming over which must help a little. This creation is also able to impart quite a bit of spin, in either direction but it looks like it should be quite easy to pick. The examples shown in the video also demonstratte that batting is only partly about hand-eye coordination – a key element is how to move your feet!

Back for the Last Four Weeks…

Posted in Biographical, Education, Maynooth with tags , , , on April 13, 2026 by telescoper

So the Easter break is over and I was back to campus today armed with a very long to-do list. I’m pleased to say I’ve ticked all the items off except the last, which was to prepare my lecture for 9am tomorrow. I’ll do that after supper.

I was very tired this morning after doing a bit of gallivanting for a couple of days. Am I too old to be carrying on like that? Yes. Do I intend to stop? No. Although I had a lot to do I didn’t have any lectures or tutorials so I was able to knuckle down and get on with things, interrupted only by an obligatory telecon.

We have four weeks left until the end of lectures for Semester 2. To be precise it’s four weeks minus one Bank Holiday (on Monday 4th May) which makes it 3.8 (working) weeks, but I don’t have lectures on Mondays so this isn’t very relevant to me. My Particle Physics module will continue in the same vein until the end of teaching but Computational Physics changes after this week, with lectures and formal lab sessions ending allowing the students time to do their mini-projects (which they have already started). They will still have access to the labs and be able to consult the demonstrators for help on their projects, though they can work at home (or somewhere else) instead if they prefer.

Other signs of the approaching end of term is that the May Examination timetable has been published, the required papers are being printed, schedules of student presentations are being circulated, and arrangements being made to mark projects.

When teaching is over for the academic year , and before exam marking starts, assuming a whole day of decent weather arrives, I plan to walk from Maynooth into Dublin along the Royal Canal. That’s a distance of 27 km. I do intend to walk the length of the National Famine Way later this year, but I was convinced to do one stage first to see if my knees can take it. The final leg of the Famine Way is from Maynooth to Dublin, which is convenient because if I’m forced to give up I can easily get the bus or train home, as I can if I reach the end.

Now for a quick supper, write my lecture for tomorrow morning, and have an early night!

A Hungarian Rhapsody

Posted in Music, Politics with tags , , , , on April 12, 2026 by telescoper

Back home to the news that Viktor Orbán has been ousted in today’s election in Hungary I thought I’d share something celebratory. Here is a classic recording of the Hungarian Rhapsody No. 2 in C-sharp minor by Franz Liszt played by György Cziffra. The second is by far the most famous of the 19 Hungarian Rhapsodies Liszt wrote, although it is based on Romanian rather than Hungarian tunes. Many recordings are available – I have three on CD – and this is my favourite. Cziffra was a very talented jazz musician too (here is his take on Duke Ellington’s Sophisticated Lady); Liszt himself was no mean improviser.

I’m not sure of the recording date, but it was made in Hungary (when Hungary was still behind the Iron Curtain) so it would have to be before 1956, as Cziffra escaped to Vienna then and eventually took up French citizenship.