Weber & Brahms at the National Concert Hall

Posted in Music with tags , , , , , , , , on April 25, 2026 by telescoper

It had been a month since my last visit to the National Concert Hall in Dublin, as I have had many distractions recently, so I was pleased to find the time yesterday evening to go again. The walk through Dublin was very pleasant in the fine weather, with lots of people outside the bars and pubs having a drink and enjoying the sunshine.

National Symphony Orchestra Ireland was conducted for the occasion by Peter Whelan for a concert of two pieces by Johannes Brahms either side of the Clarinet Concerto No. 1 by Carl Maria von Weber. When I first started writing this blog years ago, I mentioned that I didn’t really get why people think Brahms is so good. It’s not that I actively dislike Brahms, it’s just that I don’t find that he moves me as much as many other composers and so many people rave about him that I think I must be missing something. Anyway, I have persevered and now enjoy at least some of his music.

The Variations on a Theme by Joseph Haydn was written in 1873, when Brahms was three years before wrote his First Symphony. Interestingly it’s not clear whether the theme concerned was actually due to Haydn at all, but whoever supplied the raw material, this is one of the first compositions by anyone that featured a set of variations for a full orchestra. I had never heard this work before found it generally enjoyable, pedestrian in places, but with some excellent sections. There are 8 variations, bookended by the Introduction of the Theme and a Finale 7th variation is very lyrical and romantic, others are more upbeat and light-hearted.

After that introduction the Orchstra was joined on stage by Portuguese clarinetist Carlos Ferreira for the Clarinet Concerto No. 1 by Carl Maria von Weber. This is one of only two works by this composed that I’ve ever heard – the other being the Opera Oberon (which, incidentally has its original libretto in English) – and I have a couple of recordings on CD. It’s a very popular element of the clarinet repertoire and I’ve heard the last movement – a sprightly and tuneful Rondo – played on its own quite a few times on the radio. This piece was written in 1811 and you could say it provides an early Romantic contrast with the late Romantic style of Brahms. You can hear the influence of Mozart in it, and it has a slow-fast-slow three movement structure very reminiscent of the classical period.

I really enjoyed the playing of Carlos Ferreira. I especially liked the tone he produced and his ability to project even when apparently playing rather softly. The audience liked it too, and he got a standing ovation at the end (and did an encore).

After the wine break interval came the main course in the form of the Symphony No. 4 in E Minor by Johannes Brahms. This is of course a very familiar work, but that there’s always something new to find in it. and the 4th Symphony is a very fine work, which is now up among my favourite symphonies. There’s a great deal of interest in every moment from the simple phrase that introduces the first movement to the last movement, which is in three sections and which owes a lot to Bach and is almost a symphony in itself. It was performed beautifully last night by NSOI under the direction of Peter Whelan.

It was still quite warm in Dublin when I walked to Pearse Station to get the train back to Maynooth. The train filled up at Drumcondra with Shelbourne supporters on their way home from a match at Tolka Park, so it was much busier than usual but there wasn’t any trouble at all.

Weekly Update from the Open Journal of Astrophysics – 25/04/2026

Posted in OJAp Papers, Open Access, The Universe and Stuff with tags , , , , , , , , , , , , , , , , , , , , , , , , , , , , , on April 25, 2026 by telescoper

So here we are again, on a Saturday morning, with another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further five papers, bringing the number in Volume 9 (2026) to 87 and the total so far published by OJAp up to 535.

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 “Bayesian Cosmic Void Finding with Graph Flows” by Leander Thiele (U. Tokyo, Japan). This was published on Monday 20th April in the folder Cosmology and Nongalactic Astrophysics. The paper presents a method using a deep graph neural network to identify cosmic voids in sparse galaxy surveys, improving upon traditional deterministic algorithms by considering the problem’s probabilistic nature. The overlay is 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: "Bayesian Cosmic Void Finding with Graph Flows" by Leander Thiele (U. Tokyo, Japan)

doi.org/10.33232/001c.160855

April 20, 2026, 7:31 am 1 boosts 2 favorites

The second paper for this week, published on Wednesday 22nd April in the folder Astrophysics of Galaxies, is “Sifting for a Stream: The Morphology of the 300S Stellar Stream” by Benjamin Cohen (U. Chicago, USA) and 20 others distributed around the world. This study analyzes the morphology of the $300S$ stellar stream, revealing three density peaks, a possible gap, and a kink, suggesting significant influence from the Large Magellanic Cloud on its structure.

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: "Sifting for a Stream: The Morphology of the 300S Stellar Stream" by Benjamin Cohen (U. Chicago, USA) and 20 others distributed around the world.

doi.org/10.33232/001c.161089

April 22, 2026, 6:44 am 1 boosts 1 favorites

Next one up, the third paper of the week, is “IRMaGiC: Extending Luminous Red Galaxy Selection into the Infrared with Joint Rubin Observatory’s Large Survey of Space Time and Roman’s High Latitude Imaging Survey” by Zhiyuan Guo & Chris. W. Walter (Duke U., USA) and Eli S. Rykoff (Stanford U., USA) on behalf of the LSST Dark Energy Science Collaboration. This was published on Wednesday April 22nd in the folder Cosmology and Nongalactic Astrophysics. The paper introduces IRMaGiC, an algorithm that improves the selection and redshift estimation of Luminous Red Galaxies (LRGs) by incorporating infrared data, enhancing future cosmological surveys.

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: "IRMaGiC: Extending Luminous Red Galaxy Selection into the Infrared with Joint Rubin Observatory’s Large Survey of Space Time and Roman’s High Latitude Imaging Survey" by Zhiyuan Guo & Chris. W. Walter (Duke U., USA) and Eli S. Rykoff (Stanford U., USA) on behalf of the LSST Dark Energy Science Collaboration

doi.org/10.33232/001c.161093

April 22, 2026, 7:00 am 2 boosts 2 favorites

The fourth paper this week, published on Thursday April 23rd, is “The Diagnostic Temperature Discrepancy as Evidence for Non-Maxwellian Coronal Electrons” by Victor Edmonds (Final Stop Consulting, USA). This paper, in the folder Solar and Stellar Astrophysics, presents two methods of measuring electron temperature in the quiet solar corona yielding different results, suggesting non-Maxwellian electron velocity distributions may be responsible for the discrepancy.

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: "The Diagnostic Temperature Discrepancy as Evidence for Non-Maxwellian Coronal Electrons" by Victor Edmonds (Final Stop Consulting, USA)

doi.org/10.33232/001c.161223

April 23, 2026, 7:12 am 1 boosts 1 favorites

The fifth and final paper for this week was published on Friday 24th April in the folder Astrophysics of Galaxies. The title is “Galaxy evolution in the post-merger regime. IV – The long-term effect of mergers on galactic stellar mass growth and distribution” by Sara L. Ellison (U. Victoria, Canada) and Leonardo Ferreira (Universidade Federal do Rio Grande, Brazil). This study uses a large sample of post-merger galaxies to demonstrate that galaxy mergers trigger significant and extended stellar mass growth in their central regions, independent of stellar population modelling.

The overlay 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: "Galaxy evolution in the post-merger regime. IV – The long-term effect of mergers on galactic stellar mass growth and distribution" by Sara L. Ellison (U. Victoria, Canada) and Leonardo Ferreira (Universidade Federal do Rio Grande, Brazil)

doi.org/10.33232/001c.161257

April 24, 2026, 6:41 am 3 boosts 4 favorites

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: "Galaxy evolution in the post-merger regime. IV – The long-term effect of mergers on galactic stellar mass growth and distribution" by Sara L. Ellison (U. Victoria, Canada) and Leonardo Ferreira (Universidade Federal do Rio Grande, Brazil)

doi.org/10.33232/001c.161257

April 24, 2026, 6:41 am 3 boosts 4 favorites

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

P.S. Thanks to the efforts of a member of our Editorial Board, the Open Journal of Astrophysics now has a Wikipedia page.

The Red Disk – Joan Miró

Posted in Art with tags , , , on April 24, 2026 by telescoper

The Red Disk by Joan Miró (1960, Oil on Canvas, 45.7 × 54.9 cm, New Orleans Museum of Art).

From here:

Set against a dark blue, almost black surface, a white splotch of paint has been hurled out impulsively, and loses itself in innumerable spots and spatters, a cosmic gesture thrust against the empty void of nothingness – almost a metaphor of the artist’s creative activity. Some spots of colour flare up among this galaxy of creativity, of which the largest and most irregular is the red one which gave the painting its title. Minute symbols are scattered around the edges of the entire constellation – stars of hair and little hooks which give this action painting a new poetic dimension and connect it unmistakably with Miro’s world of symbols.

The Sharp End of Term

Posted in Biographical, Education, Maynooth with tags , , , on April 23, 2026 by telescoper

So here I am, sitting in the (empty) Physics Computer Lab. The formal Computational Physics lab sessions are over, but I’m on duty to provide help the students with their project work, which will take up the remaining two-and-a-bit weeks of term. It’s a lovely day outside which explains why there are very few people in the lab, and none of them have asked for help so I’ve been busy getting on with some work. Past experience with these sessions suggests that they’ll all come just before the project deadline, which is May 8th.

Up until last week I had a Computational Physics lecture at 9am on Thursdays, but the last one of those happened last Thursday. It was nice to have a more leisurely start this morning. I did think I might get a haircut on the way to work but when I passed my usual barber’s I saw it was full of people waiting their turn so I walked on. It seems that the good weather gave quite a few people the same urge to have shorter hair.

Yesterday was the last Class Test for my other class, Particle Physics, and I’ve taken the opportunity to correct all the scripts for that. I even had time to type up the solutions all neatly and tidily in Latex (including doing Feynman diagrams, which is fun).The end of that job means no more grading for that module until the main examination, which is about a month away. I do however, have lectures and tutorials still to do, including two at 9am on Tuesdays.

The finest weather is usually reserved for the exam period, of course, to maximize the annoyance of students. In my memory all my undergraduate examinations took place in very fine weather, with the exception of my Physics practical the night before which there was an enormous thunderstorm. Come to think of it, that could well have been a portent that warned me off experiments and made me become a theorist.

Maynooth University Library Cat Update

Posted in Maynooth with tags , , , on April 22, 2026 by telescoper

This week at Maynooth University numerous parties of schoolkids have been, and are being, shown around the campus. Naturally an important stop on this tour is the abode of Séamus the Library Cat. The weather has been nice this week so far, as it was today, so said feline has generally been out and about and making himself available to be admired. On my way to lunch I managed to bypass a large coach party of schoolgirls and reach the cat’s spot ahead of them. I found Séamus giving himself a good wash and brush-up in anticipation of the arrival of the visitors.

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 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: