It’s time for another Saturday update of activity at the Open Journal of Astrophysics. Since the last update we have published a further four papers, bringing the number in Volume 9 (2026) to 249 and the total so far published by OJAp up to 697.
I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also contain a clickable form of the DOI for each paper. Our Mastodon account has regular updates and other announcements from OJAp too, including posts from the OJAp blog.
The first paper this week was published on Tuesday 20th October in the folder Astrophysics of Galaxies. The title is “The Metallicity Distribution of the Ultra-Faint Dwarf Galaxy Segue 1” by Daisy Bissonette (U. Chicago, USA) and 8 others based in the USA, Australia and Canada. The article explains that new data on the metallicity of ultra-faint dwarf galaxy Segue 1 reveal a continuous, short-duration episode of star formation and chemical enrichment, confirming its classification as a galaxy.
The overlay for this one is here:
You can find the officially accepted version on arXiv here and the announcement on Fediverse here:
New Publication at the Open Journal of Astrophysics: "The Metallicity Distribution of the Ultra-Faint Dwarf Galaxy Segue 1" by Daisy Bissonette (U. Chicago, USA) and 8 others based in the USA, Australia and Canada.
The second paper for this week, also published on Tuesday 20th October in the folder Astrophysics of Galaxies, “Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages” by Elia Cenci & Melanie Habouzit (U. Geneva, Switzerland) and Dale D. Kocevski (Colby College, USA). This article uses simulations to explore UV emissions from galaxies hosting direct-collapse black holes (DCBHs), finding that these emissions evolve rapidly, reflecting changes in stellar mass and metal enrichment.
The overlay looks like this:
The official version of the paper can be found on arXiv here and the Fediverse announcement here:
New Publication at the Open Journal of Astrophysics: "Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages" by Elia Cenci & Melanie Habouzit (U. Geneva, Switzerland) and Dale D. Kocevski (Colby College, USA)
New Publication at the Open Journal of Astrophysics: "Dark Energy Survey Year 6 Results: improved mitigation of spatially varying observational systematics with masking for the MagLim++ lens sample" by M. Rodríguez-Monroy (Universidad Autónoma de Madrid, Spain) and 65 others from around the world.
New Publication at the Open Journal of Astrophysics: "Spectroscopic Binary Detection as Agent-Callable Tools: Detecting 40,000+ Main-Sequence Binary Candidates from SDSS DR19 APOGEE Spectra" by Serat Mahmud Saad and Yuan-Sen Ting (Ohio State University, USA).
That concludes this week’s update. I had anticipate that we’ll pass the 250 mark this week, but business has been slower than of late so we’ll have to wait until next week for that. It is noticeable that the arXiv submission process is slower now than it used to be, presumably because of the huge influx of AI slop that the moderators have to deal with.
The number of papers being submitted to the Open Journal of Astrophysics continues to rise, as demonstrated by the following graphic which shows the stats for new submissions for the last five years:
It’s very clear that the thicket is getting thicker and thicker as times goes on! The increasing number of articles is of course very welcome indeed, but it is increasing the load on our Editorial Board and that includes me! I think it’s time once again to look for more volunteers to join the team, in any area of astrophysics. As a reminder, here are the areas we cover, corresponding to the sections of astro-ph on the arXiv:
astro-ph.GA – Astrophysics of Galaxies. Phenomena pertaining to galaxies or the Milky Way. Star clusters, HII regions and planetary nebulae, the interstellar medium, atomic and molecular clouds, dust. Stellar populations. Galactic structure, formation, dynamics. Galactic nuclei, bulges, disks, halo. Active Galactic Nuclei, supermassive black holes, quasars. Gravitational lens systems. The Milky Way and its contents
astro-ph.CO – Cosmology and Nongalactic Astrophysics. Phenomenology of early universe, cosmic microwave background, cosmological parameters, primordial element abundances, extragalactic distance scale, large-scale structure of the universe. Groups, superclusters, voids, intergalactic medium. Particle astrophysics: dark energy, dark matter, baryogenesis, leptogenesis, inflationary models, reheating, monopoles, WIMPs, cosmic strings, primordial black holes, cosmological gravitational radiation
astro-ph.EP – Earth and Planetary Astrophysics. Interplanetary medium, planetary physics, planetary astrobiology, extrasolar planets, comets, asteroids, meteorites. Structure and formation of the solar system
astro-ph.HE – High Energy Astrophysical Phenomena. Cosmic ray production, acceleration, propagation, detection. Gamma ray astronomy and bursts, X-rays, charged particles, supernovae and other explosive phenomena, stellar remnants and accretion systems, jets, microquasars, neutron stars, pulsars, black holes
astro-ph.IM – Instrumentation and Methods for Astrophysics. Detector and telescope design, experiment proposals. Laboratory Astrophysics. Methods for data analysis, statistical methods. Software, database design
astro-ph.SR. – Solar and Stellar Astrophysics. White dwarfs, brown dwarfs, cataclysmic variables. Star formation and protostellar systems, stellar astrobiology, binary and multiple systems of stars, stellar evolution and structure, coronas. Central stars of planetary nebulae. Helioseismology, solar neutrinos, production and detection of gravitational radiation from stellar systems.
We are looking for experienced scientists in any of these areas, and it would be useful to have people who can cover a range of subjects (as some of our existing editors do). As I mentioned here, our most popular area is 1 (Astrophysics of Galaxies) but 2 (Cosmology and NonGalactic Astrophysics) is running it a close second. While I would welcome offers from people with expertise in either of those fields, Editors in any of the other areas listed above would be welcome additions. Since we don’t charge authors or readers we can not offer payment to Editors but it is nevertheless a way of providing a service to the community.
If you’re interested, please get in touch either through the Open Journal website here, or through a message Mastodon here, BlueSky here, or LinkedIn here.
Peter Coles Editor-in-Chief Open Journal of Astrophysics
It’s Saturday again, so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further eight papers, bringing the number in Volume 9 (2026) to 245 and the total so far published by OJAp up to 693. There was no arXiv update on Monday 12th October owing to a US holiday, and I was on strike on Wednesday 14th October, so there were no papers published on either 13th or 14th October.
I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also contain a clickable form of the DOI for each paper. Our Mastodon account has regular updates and other announcements from OJAp too, including posts from the OJAp blog.
New Publication at the Open Journal of Astrophysics: "Search for Gamma-ray emission from Abell 119 galaxy cluster using INTEGRAL/ISGRI, COMPTEL, and DAMPE data" by Siddhant Manna & Shantanu Desai (IIT Hyderabad Kandi, India)
New Publication at the Open Journal of Astrophysics: "Fast Astronomical Transients in Archival Photographic Plates: Using optical aberrations as a tool for discerning real images, from plate artifacts" by Ivo Busko (Independent Researcher)
New Publication at the Open Journal of Astrophysics "Differentiable Optics with dLux II: Optical Design Maximising Fisher Information" by Louis Desdoigts (Leiden Obs., NL), Benjamin Pope (Macquarie U., AU), Michael Gully-Santiago (U. Texas Austin, USA) & Peter Tuthill (U. Sydney, AU)
The fourth new article of the week, also published on Thursday 15th October, in the folder Astrophysics of Galaxies is “The Lumina Project: Intergalactic Clumping and Recombination Sinks” by Ali Sadain (U. Texas Dallas, USA) and 12 others based in the USA, S. Korea and Germany. The study uses simulations to examine the uneven recombination rates during the Epoch of Reionization, finding a universal clumping evolution and discrepancies in recombination rates due to photoheating.
The overlay is here:
The official version of the paper can be found on arXiv here and the Fediverse announcement here:
New Publication at the Open Journal of Astrophysics: "The Lumina Project: Intergalactic Clumping and Recombination Sinks" by Ali Sadain (U. Texas Dallas, USA) and 12 others based in the USA, S. Korea and Germany.
Paper Number Five for the week is “Blast.jl: Differentiable Non-Limber Power Spectra for Joint Clustering, Shear, and CMB lensing Analyses” by Sofia Chiarenza (U. Waterloo, Canada) and 6 others based in Canada, Italy, France and USA. This study, which is in the folder Cosmology and Nongalactic Astrophysics, presents an enhanced version of Blast.jl, a toolkit for computing non-Limber angular power spectra, incorporating various cosmological effects. Despite increased complexity, it maintains efficiency and supports gradient-based inference. It was also published on Thursday 15th October.
The overlay is here:
The officially-accepted version of the paper can be found on arXiv here and the Fediverse announcement here:
New Publication at the Open Journal of Astrophysics: "Blast.jl: Differentiable Non-Limber Power Spectra for Joint Clustering, Shear, and CMB lensing Analyses" by Sofia Chiarenza (U. Waterloo, Canada) and 6 others based in Canada, Italy, France and USA.
Sixth one up is “EMU detection of mysterious multiple component radio-continuum emission from nearby spiral Seyfert I type galaxy ‘Sand-timer’ (NGC 7213)” by Miroslav Filipović (Western Sydney U., Australia) and an international cast of 26 others. The observations presented in this paper reveal peculiar emissions and previously undetected features in the ‘Sand-timer’ galaxy NGC 7213, possibly due to black hole activity or a tidal disruption event.
The overlay is here:
The officially-accepted version of this paper is on arXiv here and the Mastodon announcement on the fediverse here:
New Publication at the Open Journal of Astrophysics: "Blast.jl: Differentiable Non-Limber Power Spectra for Joint Clustering, Shear, and CMB lensing Analyses" by Sofia Chiarenza (U. Waterloo, Canada) and 6 others based in Canada, Italy, France and USA.
The seventh paper of the week is “pynucastro 3: A community library for nuclear astrophysics” by Zhi Chen (Stony Brook U., USA) and 10 others, all based in the USA. This was published on Friday 16th October, i.e. yesterday, in the folder Instrumentation and Methods for Astrophysics. This article announces the latest release of pynucastro, a python library for nuclear astrophysics, includes new rate approximations, a stellar equation of state, StarLib support, and network exploration tools.
The overlay is here:
The officially accepted version is on arXiv here and the Mastodon announcement here:
New Publication at the Open Journal of Astrophysics: "pynucastro 3: A community library for nuclear astrophysics" by Zhi Chen (Stony Brook U., USA) and 10 others, all based in the USA.
The eighth, and last, of the new papers for this week is “A Deep Look at the Ultra-Faint Milky Way Satellite Virgo III with Rubin Observatory Data Preview 2” by Aashay Pai (U. Chicago, USA) and 12 others based in the USA. This study uses data from the Vera C. Rubin Observatory to analyze the ultra-faint Milky Way satellite, Virgo III, confirming Virgo III’s properties as an ultra-faint dwarf galaxy.
The overlay is here:
The final version of this paper is on the arXiv here and the Mastodon announcement here:
New Publication at the Open Journal of Astrophysics: "A Deep Look at the Ultra-Faint Milky Way Satellite Virgo III with Rubin Observatory Data Preview 2" by Aashay Pai (U. Chicago, USA) and 12 others based in the USA.
That concludes this week’s update. I anticipate that we’ll pass the 250 mark for 2026 next week, which means we’re well on target to publish over 300 papers and reach the 750 mark by the end of the year. I’ll do another update next weekend.
It’s Saturday again, so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further eight papers, bringing the number in Volume 9 (2026) to 237 and the total so far published by OJAp up to 685.
I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also contain a clickable form of the DOI for each paper. Our Mastodon account has regular updates and other announcements from OJAp too, including posts from the OJAp blog.
The first new paper this week was published on Monday 5th October in the folder Solar and Stellar Astrophysics. The title of the paper is “Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array” and it isby Tabetha Boyajian (Louisiana State University, USA) and 10 others based in the USA and Australia. This study uses interferometric measurements to determine precise characteristics of 27 nearby solar-type stars, including their radii, effective temperatures, and luminosities. The findings represent benchmarks for testing stellar evolutionary theory.
The overlay for this one is here:
You can find the officially accepted version on arXiv here and the announcement on Fediverse here:
New Publication at the Open Journal of Astrophysics: "Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array" by Tabetha Boyajian (Louisiana State University, USA) and 10 others based in the USA and Australia.
New Publication at the Open Journal of Astrophysics: "The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants" by Jessica Braudo and Noam Soker (Technion, Israel)
New Publication at the Open Journal of Astrophysics: "Balancing bias, baryons, and scale cuts in LSST 3x2pt analysis" by Ottavia Truttero (U. Edinburgh, UK) and 5 others on behalf of the The LSST Dark Energy Science Collaboration
New Publication at the Open Journal of Astrophysics: "High-Precision Differential Radial Velocities of C3PO Wide Binaries: A Test of Modified Newtonian Dynamics (MOND)" by Serat M. Saad and Yuan-Sen Ting (Ohio State University, USA)
New Publication at the Open Journal of Astrophysics: "Simulating the jittering-jets explosion mechanism: circum-jet rings account for observed core-collapse supernova remnant morphologies" by Muhammad Akashi & Noam Soker (Technion, Israel)
The sixth paper of the week is “Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnant N 132D” by Rami Z. E. Alsaberi (Western Sydney U. Australia) and 7 others. This was the first of three papers published on Friday 9th October, and it is in the folder High-Energy Astrophysical Phenomena. This one presents a radio continuum analysis of the Large Magellanic Cloud supernova remnant N 132D, revealing insights into its magnetic field structure, energetic properties, and particle acceleration.
The officially-accepted version of this paper is on arXiv here and the Mastodon announcement on the fediverse here:
New Publication at the Open Journal of Astrophysics: "Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnant N 132D" by Rami Z. E. Alsaberi (Western Sydney U. Australia) and 7 others
The seventh paper of the week is “New Signs Pointing Toward a Correlation Between Astrophysical Neutrinos and Radio Flares” by Yjan Gordon (U. Wisconsin-Madison), Peter S. Ferguson (U. Washington), Eric J. Hooper & Michael N. Martinez (U. Wisconsin-Madison); all in the USA. This was also published on Friday 7th October, but in the folder Astrophysics of Galaxies. It is very topical, in the light of the award of this year’s Nobel Prize for Physics to Francis Halzen for his work on IceCube. The paper explains how data from VLASS and IceCube Neutrino Observatory reveal a correlation between radio variability and astrophysical neutrino detection, suggesting radio flares contribute to about 13% of astrophysical neutrinos detected by IceCube.
The overlay is here:
The officially accepted version is on arXiv here and the Mastodon announcement here:
New Publication at the Open Journal of Astrophysics: "New Signs Pointing Toward a Correlation Between Astrophysical Neutrinos and Radio Flares" by Yjan Gordon (U. Wisconsin-Madison), Peter S. Ferguson (U. Washington), Eric J. Hooper & Michael N. Martinez (U. Wisconsin-Madison); all in the USA
New Publication at the Open Journal of Astrophysics: "Spectroscopic follow-up of compact object binary candidates from Gaia DR3: White dwarfs, neutron stars, black holes, and the parallax zeropoint" by Kareem El-Badry (Caltech, USA) and an international cast of 14 others.
That concludes this week’s update. We’re still on target to publish over 300 papers and reach the 750 mark by the end of the year. I’ll do another update next week.
There’s a short article on arXiv by astronomer Luigi Rolly Bedin with the title The Preprint Evolution: The Rise of Unreviewed Drafts on arXiv and its Implications for Astronomy and abstract:
The arXiv preprint server originally democratized astronomical research by digitizing the circulation of early manuscripts and removing the financial barriers of journal subscriptions. However, a system designed for the lower publication volumes of the 1990s has fractured under modern research output. Today, the sheer volume of unreviewed manuscripts—often tagged as “submitted”, “under review”, or “comments welcome” imposes a severe cognitiv “tax” on the community. Researchers are forced to track multiple, unvetted versions of the same work, creating a massive redundant workload. This practice also bypasses the blinded peer-review process by establishing premature precedence, and it takes a heavy toll on early-career researchers. The pressure to rapidly post unvetted results stifles independent research, pushing young scientists toward massive mainstream collaborations where individual creativity gets lost. In this Short Communication, I analyze a decade of astro-ph metadata to quantify this trend. To safeguard both researchers’ time and research freedom, I propose bifurcating submissions into two separate streams. Level-1 (peer-reviewed science) would host peer-reviewed science (accompanied by a journal acceptance or final DOI), while Level-2 (pre-review drafts) would be reserved for discussion drafts. This distinction would remove the unfair advantage of establishing false precedence through drafts and drastically cut the daily reading burden by allowing researchers to opt out of tracking unvetted versions.
arXiv:2609.35787
I’ve mentioned this paper on this blog because a couple of readers commented about it on a post earlier this week (here and here) I’ll leave it to readers to decide for themselves what they think about the suggestion of having a two-tier arXiv as described in the abstract. A rebuttal has been posted on arXiv here.
For myself I’ll just say that I think that, for such a short paper, it contains a very large number of unsubstantiated claims. I don’t doubt that the number of pre-review submissions has increased over the years, but are researchers really “forced to track multiple, unvetted versions of the same work, creating a massive redundant workload”? Is it really the case that the existence of unrefereed articles on arXiv “stifles independent research, pushing young scientists toward massive mainstream collaborations where individual creativity gets lost”? Where is the evidence for this claim? The claim of a `severe cognitive “tax” on the community’ seems a huge stretch to me too. If you really don’t want to read unrefereed articles on arXiv then you can just ignore those that don’t have a journal reference in their metadata.
I wrote a piece about preprints some time ago here. In it I tried to explain how preprints were initially used to circulate refereed work in advance of the final printed version being available, which often took many months after acceptance. Back in the old days these were usually produced by institutions with a distinctive design, logo, etc which gave them a professional look, which made it easier to distinguish `serious’ papers from crank material (which was also in circulation). This also suggested that some internal refereeing inside an institution had taken place before an “official” preprint was produced, lending it an air of trustworthiness. Smaller institutions couldn’t afford all this, so were somewhat excluded from the preprint business.
With the arrival of the arXiv the practice of circulating hard copies of preprints in astrophysics gradually died out, to be replaced by ever-increasing numbers of electronic articles. The arXiv does have some gatekeeping – in the sense there are some controls on who can deposit a preprint there – but it is far easier to circulate a preprint now than it was.
(I am, incidentally, very surprised that this article – with only reference (to itself) and no evidence to support its claims – passed the arXiv moderation process for astro-ph, but there you go…
Anyway, it is still the case that big institutions and collaborations insist on quite strict internal refereeing before publishing a preprint – and some even insist on waiting for a paper to be accepted by a journal before adding it to the arXiv – but there’s no denying that among the wheat there is quite a lot of chaff, some of which attracts media coverage that it does not deserve. It is also the case that some articles that have passed peer review are flawed in crucial ways not spotted by referees. No system that is operated by human beings will ever be flawless, and peer review is no different. Not everything in “Tier 1” is perfect.
The most important thing is for science to advance. Circulating a paper in advance of review can help to achieve that. I have very often found that comments from other researchers reading the arXiv version supply comments and suggestions far more useful than one gets from a journal reviewer. Sometimes they can spot a fundamental flaw missed by a referee. If you put your paper on arXiv ahead of official peer review you will subject it to an additional level of scrutiny, increasing the chance that the final version will turn out to be a useful contribution to the literature.
Nowadays, in astrophysics, the single most important point of access to scientific literature is through the arXiv, which is why the Open Journal of Astrophysics was set up as an overlay journal to provide a level of rigorous peer review for preprints, not only to provide a sort of quality mark but also to improve the paper through the editorial process. There’s your Tier 1 for you.
P.S. I didn’t think of this at the time but one of the reasons that the fraction of unreviewed preprints is increasing is simply that people are not very good at updating their arXiv entry when a paper is actually published. I noticed this with Euclid papers, for example, which are generally posted on arXiv as preprints and subsequently published in A&A. It was noticeable, however, that some authors do not update the arXiv metadata after acceptance.
It’s Saturday again, so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further 13 papers, including one correction to an article already published, bringing the number in Volume 9 (2026) to 229 and the total so far published by OJAp up to 677. This would have been a busy week even without the clutch of four MEGATRON papers announced on Wednesday!
I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also contain a clickable form of the DOI for each paper. Our Mastodon account has regular updates and other announcements from OJAp too, including posts from the OJAp blog.
The first new paper this week was published on Tuesday 28th September in the folder Solar and Stellar Astrophysics. The title is “Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics” and it is by G. Leidi (Heidelberger Institut für Theoretische Studie, Germany) and 14 others. PHLEGETHON is a magnetohydrodynamic code designed for multidimensional simulations in stellar astrophysics, capable of modeling a wide range of dynamical processes in stars. It is publicly accessible online.
The overlay for this one is here:
You can find the officially accepted version on arXiv here and the announcement on Fediverse here:
New Publication at the Open Journal of Astrophysics: "Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics" by G. Leidi (Heidelberger Institut für Theoretische Studie, Germany) and 14 others.
New Publication at the Open Journal of Astrophysics: "The impact of source and survey modelling on the connection between [O III] emitters and Ly-α forest transmission at z ~ 6" by Luke Conaboy (U. Nottingham, UK) and 5 others based in the UK, India and Germany.
Next we have four related papers produced by the MEGATRON Project, led by Harley Katz (U. Chicago) and Martin Rey (U. Bath, UK), Corentin Cadiou (IAP Paris, France). These were all published on Wednesday 30th September in the folder Astrophysics of Galaxies.
I mentioned this in a separate blog post here, so I won’t describe them in detail again here. Here are the four overlays:
The Mastodon announcement for these is in the form of a thread:
Today we have published four related papers produced by the MEGATRON Project, led by Harley Katz (U. Chicago) and Martin Rey (U. Bath, UK), Corentin Cadiou (IAP Paris, France)
These articles are announced in the following thread:
The four papers can be found on arXiv here, here, here and here.
The four MEGATRON papers were not the only ones published on Wednesday 30th September, however. We published “The Chirp-Mass Ladder: A New Rung Emerges” by Vaibhav Tiwari (U. Birmingham, UK) in the folder High-Energy Astrophysical Phenomena on that day too. This paper presents an analysis of 256 binary black-hole (BBH) events, suggesting a hierarchical merger scenario to explain the structured mass distribution, and encouraging further investigation into hierarchical mergers’ role in the BBH population. The overlay for this is here:
The accepted version of this one can be found on the arXiv here and the Mastodon announcement here:
New Publication at the Open Journal of Astrophysics: "Kinematics of the Weak Cool-Core Cluster A3571 Observed with XRISM: Low Cooling Rate Balanced by Low Heating Rate?" by Hannah McCall (U. Chicago, USA) and 12 others based around the world.
We now have four papers all published on Friday 2nd October (i.e. yesterday).
The first of this batch is “Analytical weak-lensing shear response of galaxy model fitting” by Xiangchong Li (Brookhaven National Laboratory, USA). This is in the folder marked Cosmology and Nongalactic Astrophysics: it explores how galaxy model fitting responds to weak-lensing shear distortions using a new algebraic system, quintuple numbers, within the AnaCal framework, keeping multiplicative bias low.
The overlay is here:
The officially-accepted version of the paper can be found on arXiv here and the Fediverse announcement here:
New Publication at the Open Journal of Astrophysics: "Analytical weak-lensing shear response of galaxy model fitting" by Xiangchong Li (Brookhaven National Laboratory, USA)
New Publication at the Open Journal of Astrophysics: "Evidence for inefficient dust production in a massive, metal-rich galaxy at z=7.13 uncovered by JWST and ALMA" by Kasper E. Heintz (Cosmic Dawn Center, Copenhagen, Denmark) and 19 others in Europe, UK and USA.
The 11th paper of the week is “Starbursts hiding in the main sequence: a pathway toward quenching?” by Florent Renaud (Observatoire Astronomique de Strasbourg, France) and 12 others based in France and UK. This article explores the “starbursts in the main sequence” (SBMSs) that intermittently appear in galaxy evolution, attributing their existence to earlier stellar mass assembly and frequent mergers. It was published on Friday 2nd October 2026, in the folder Astrophysics of Galaxies.
The overlay is here:
The officially accepted version is on arXiv here and the Mastodon announcement here:
New Publication at the Open Journal of Astrophysics: "Starbursts hiding in the main sequence: a pathway toward quenching?" by Florent Renaud (Observatoire Astronomique de Strasbourg, France) and 12 others based in France and UK.
New Publication at the Open Journal of Astrophysics: "Ring Position Angles and Spin in M87* and Sgr A*" by Nicholas S. Conroy (U. Illinois at Urbana-Champaign, USA) and 6 others all based in the USA.
And finally, on Monday 28th September we announced one (minor) correction to a previously published article. The overlay of the correction notice is here:
Correction Notice issued at the Open Journal of Astrophysics: "CORRECTION – TDCOSMO XXVI: Uniform Lens Modeling of Eight Doubly Imaged Quasars" by Brady et al. (originally published 7th August 2026).
The corrected version of this paper can be found on arXiv here.
That concludes this week’s update. As things are going we seem likely to publish over 300 papers this year, and may reach the 750 mark by the end of the year too. I’ll do another update next week.
Putting my community service hat on, I thought I would relay an announcement on the arXiv blog that it is introducing a limit on the rate that any individual can submit papers to arXiv. To start with, the limit will be two per month. This limit applies to the submitter, not to all the authors, so I think large collaborations will find a way around it by having different co-authors do the submissions.
The reason for this limit is very clear:
The rate of submissions is currently growing in an uncontrolled and alarming way. Most of this growth is driven by AI, which makes it very easy for authors to flood the arXiv with boilerplate papers. All this is making life impossible for the moderators. It will be very interesting to see if this move manages to stem the tide.
If you have any questions, please read the FAQ on the page here. One thing I’m not sure about is whether the limit applies to replacements as well as new submissions. It doesn’t seem to be addressed in the FAQs.
Today we published four papers at the Open Journal of Astrophysics all related to the Megatron Project which is co-led by Martin Rey of the University of Bath (UK), Harley Katz of the University of Chicago (USA) and Corentin Cadiou of the Institut d’Astrophysique de Paris in France. I will include this quartet in my regular weekly update on Saturday but there is a press release accompanying these publications so I thought I’d splash them a bit here too.
I’ll show the overlays on Saturday but in the meantime here are some pretty graphics from three of the papers:
New simulations connect the first stars to cosmic fingerprints still visible today
International MEGATRON project links space telescope observations of the infant Universe with the chemical fossil record of the Milky Way.
Researchers have used some of the most detailed simulations yet of the early Universe to investigate how the first stars and galaxies formed.
Led by researchers at the University of Bath, alongside collaborators at the University of Chicago in the US and the Institut d’Astrophysique de Paris in France, the MEGATRON project uses advanced simulations to explore how the first stars and galaxies lit up the previously dark cosmos and enriched it with the chemical elements that would later become the building blocks of everything around us.
Published today in the Open Journal of Astrophysics, four studies from the MEGATRON project combine cutting-edge cosmological simulations with sophisticated models of radiation, chemistry and galaxy formation. Together, these constitute the collaboration’s first substantial body of published results, with further papers expected to follow.
The findings from the study of the first stars show that accurately capturing the interplay between starlight, gas and newly forged elements is essential for connecting two previously separate views of the early Universe: observations of young galaxies by the James Webb Space Telescope (JWST) and the chemical clues preserved in ancient stars in and around the Milky Way – the galaxy that contains our Solar System.
JWST provides a direct view of galaxies in the infant Universe, while ancient stars act as a fossil record of cosmic history. By studying the chemical fingerprints of these ancient stars, astronomers can reconstruct the properties of the first stars and trace how they enriched the cosmos with the first chemical elements.
The simulations follow the evolution of a young galaxy that will eventually grow into a system similar in mass to the Milky Way. Using advanced computer models that simultaneously track the movement of gas, the propagation of starlight and the evolution of chemical concentrations, the team investigated how stars shape the gas in and around galaxies over billions of years.
The study suggests that simplified models may underestimate the influence of stellar radiation and complex chemical processes on the gas surrounding galaxies. By modelling these effects at exceptionally high resolution, the team resolved structures in the gas that are not captured by simpler models, helping to improve predictions for current and future astronomical observations.
A direct glimpse of the infant cosmos
Dr Martin Rey from the Department of Physics at the University of Bath and a lead contributor to the MEGATRON collaboration, said: “The James Webb Space Telescope gives us a direct glimpse of the infant cosmos, while stellar archaeology allows us to study the relics of those earliest times in our own Galactic neighbourhood. MEGATRON provides a physical bridge between the two.”
The simulations begin with pristine gas containing no heavy elements, mirroring conditions shortly after the Big Bang. They then follow the birth of the first stars, the radiation they emit, the supernova explosions that mark their deaths and the dispersal of newly forged elements into subsequent generations of stars and galaxies.
Understanding this process is central to one of astronomy’s most fundamental questions: where the elements that make up today’s Universe came from.
Dr Rey said: “The elements that make our world and life possible – carbon, oxygen, iron and many others – were forged by stars. To understand where those elements came from, we need to understand how the first stars formed and enriched their surroundings. MEGATRON allows us to test these ideas directly by comparing detailed simulations with observations from JWST and the chemical fingerprints preserved in ancient stars.”
Looking ahead, the team plans to use MEGATRON to strengthen links between theory and emerging observational data. As JWST continues to transform our understanding of the earliest galaxies, large-scale stellar surveys will provide increasingly detailed information about ancient stars in and around the Milky Way.
Dr Rey and his colleagues at Bath are already developing the next generation of simulations. The project has been awarded 40 million processor hours on the UK’s national supercomputers, equivalent to running five million laptops in parallel for a year. These resources will enable simulations with higher resolution and more complete physical models, allowing even more direct comparisons with JWST observations and the chemical fossil record preserved in ancient stars.
“MEGATRON provides a common physical framework for interpreting two of astronomy’s most exciting new datasets: JWST’s view of the earliest galaxies and the stellar fossil record,” said Dr Rey. “Together, these complementary observations allow us to test competing models of the first stars in ways that weren’t previously possible.”
The MEGATRON project started in 2023 and is scheduled to run until 2030.
It’s time once more for another Saturday update of activity at the Open Journal of Astrophysics. Since the last update we have published a further eight papers, including one correction to an article already published, bringing the number in Volume 9 (2026) to 217 and the total so far published by OJAp up to 664. This is the third week running that we have published 7 new papers.
I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also contain a clickable form of the DOI for each paper. Our Mastodon account has regular updates and other announcements from OJAp too, including posts from the OJAp blog.
The first paper this week was published on Monday 21st September in the folder Solar and Stellar Astrophysics. The title is “The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds” and it is by Yuan-Sen Ting (Ohio State U., USA) and Elliot M. Kim (Cornell U., USA). The study introduces Payne Zero, a tool that reorganizes stellar spectra calculations for GPU-native synthesis, significantly speeding up the process and enabling direct physical fitting and atomic-data calibration at survey scale.
The overlay for this one is here:
You can find the officially accepted version on arXiv here and the announcement on Fediverse here:
New Publication at the Open Journal of Astrophysics: "The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds" by Yuan-Sen Ting (Ohio State U., USA) and Elliot M. Kim (Cornell U., USA)
The second paper for this week, published on Tuesday 22nd September, is titled “RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9” and is in the folder Astrophysics of Galaxies. The authors are Nikko Cleri (Penn State U., USA) and 12 others based in the USA, Switzerland and Germany. The article involves an examination of the time evolution of the ionization parameter in galaxies, finding that it increases with redshift and specific star formation rate, and decreases with stellar mass.
The overlay looks like this:
The official version of the paper can be found on arXiv here and the Fediverse announcement here:
New Publication at the Open Journal of Astrophysics: "RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9" by Nikko Cleri (Penn State U., USA) and 12 others based in the USA, Switzerland and Germany
New Publication at the Open Journal of Astrophysics: "Kinematics of the Weak Cool-Core Cluster A3571 Observed with XRISM: Low Cooling Rate Balanced by Low Heating Rate?" by Hannah McCall (U. Chicago, USA) and 12 others based around the world.
New Publication at the Open Journal of Astrophysics: "The Simons Observatory: Development of a Pipeline to Detect Rapid Transients in Time-Ordered Data" by Justin Clancy (U. Melbourne, Australia) and 16 others from around the world.
The fifth paper of the week is “Fisher Forecasting for the DESC with Augur” by Paul Rogozenski (Carnegie Mellon U., USA) and 16 others on behalf of the The LSST Dark Energy Science CollaborationThis was also published on Wednesday 16th September, but in the folder Cosmology and Nongalactic Astrophysics. This paper introduces the Augur tool, designed to provide Fisher forecasts for cosmological inference for the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST).
The overlay for this one looks like this:
The officially-accepted version of this paper is on arXiv here and the Mastodon announcement on the fediverse here:
New Publication at the Open Journal of Astrophysics: "Fisher Forecasting for the DESC with Augur" by Paul Rogozenski (Carnegie Mellon U., USA) and 16 0thers on behalf of the The LSST Dark Energy Science Collaboration
The sixth paper of the week is “Profile Analysis of the Multiwavelength 2.1-year Oscillations of PG 1553+113” by Pablo Penil (Clemson U. USA) and 7 others based in the USA, Germany and Spain. This was also published on Wednesday 23rd September, in the Astrophysics of Galaxies. The study examines the oscillation profiles of blazar PG~1553+113, finding that its 2.1-year periodicity is not strictly sinusoidal and varies across energy bands.
The overlay is here:
The officially accepted version is on arXiv here and the Mastodon announcement here:
New Publication at the Open Journal of Astrophysics: "Profile Analysis of the Multiwavelength 2.1-year Oscillations of PG 1553+113" by Pablo Penil (Clemson U. USA) and 7 others based in the USA, Germany and Spain.
Our seventh, and last, new paper of the week is “Radial Pulsations in Polaris: A Secondary Science Application of Cherenkov Telescopes via Intensity Interferometry” by Km Nitu Rai (IISER, India), Prasenjit Saha (U. Zurich, Switzerland) and Subrata Sarangi (IUCAA, India). This study demonstrates how Cherenkov telescopes, typically unused during moonlit nights, can be used for advanced optical stellar measurements, particularly for characterizing bright stars such as Polaris.
The overlay is here:
The final version of this paper is on the arXiv here and the Mastodon announcement here:
New Publication at the Open Journal of Astrophysics: "Radial Pulsations in Polaris: A Secondary Science Application of Cherenkov Telescopes via Intensity Interferometry" by Km Nitu Rai (IISER, India), Prasenjit Saha (U. Zurich, Switzerland) and Subrata Sarangi (IUCAA, India)
Correction Notice issued at the Open Journal of Astrophysics: "CORRECTION: The Abundance of Thin Dwarf Galaxies: a Challenge for Cosmological Simulations" by Jose Benavides et al. (originally published 12th May 2026)
The corrected version of this paper can be found on arXiv here.
That concludes this week’s update. I’ll just add a mention of yesterday’s post announcing that the Open Journal of Astrophysics is a Q1 Journal. It will be interesting to see if that stimulates another increase in submissions. As things are going we seem likely to publish about 300 papers this year. I’ll also mention that an exciting development is in the pipeline for next week, but I can’t say more until it happens.
I was a meeting this morning about other things during the course of which I found out that, as of 2025, the Open Journal of Astrophysics is a Q1 journal. This means that according to certain bibliometric criteria, OJAp is in the first quartile (i.e. top 25%) of journals in its field. You can find a table with all journals in Astronomy and Astrophysics curated by SCImago here. I searched the list for all the journals that are classified as Diamond Open Access and found that we’re the only one:
As with many of these bibliometric things the data are incorrect. We actually published 212 papers in 2025. The number of citations is wildly wrong too – the true figure is much higher. I presume that the number of documents (3 years) is 2022+2023+2024, which is the correct number if that’s what it is meant to represent.
My main objection to journal indicators like this (apart from the fact that they’re usually riddled with errors) is that nowadays it is quite easy to extract citation information at the article level so there’s no reason to use a metric associated with the journal to judge the quality of a paper. It’s like judging a book by its cover. I hate Journal Impact Factor for similar reasons; see posts here.
For this reason I don’t personally care at all about whether OJAp is Q1 or Q2 or whatever. I do recognize, however, that many astronomers and astrophysicists work in countries where the funding agencies do not count papers unless they are in Q1 journals. I think that’s silly, but it’s a fact of life.
If the only reason you were not submitting papers to OJAp was that it wasn’t a Q1 journal then you can start submitting them now!
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