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Two New Publications at the Open Journal of Astrophysics

Posted in OJAp Papers, Open Access, The Universe and Stuff with tags , , , , , , , , , on September 7, 2024 by telescoper

It’s Saturday morning again so here’s another report on activity at the  Open Journal of Astrophysics.  Since the last update we have published two more papers, taking  the count in Volume 7 (2024) up to 73 and the total published by OJAp up to 188.  We’ve still got a few in the pipeline waiting for the final versions to appear on arXiv so I expect we’ll reach the 200 mark fairly soon.

The first paper of the most recent pair, published on September 4th 2024,  and in the folder marked Astrophysics of Galaxies, is “Massive Black Hole Seeds”  by John Regan of the Department of Theoretical Physics at Maynooth University and Marta Volonteri (Sorbonne Université, Paris, France). This article presents a discussion of the pathways to the formation of massive black holes, including both light and heavy initial seeds.

Here is a screen grab of the overlay which includes the abstract:

 

 

You can click on the image of the overlay to make it larger should you wish to do so. Those of you who are paying attention will see that there is a bit of a glitch on the left hand side where software has thrown a line break in between the two author names. I have no idea what caused this so I raised a ticket with Scholastica and no doubt it will soon be fixed.  (Update: it is now fixed, 12th September 2024). You can find the officially accepted version of this paper on the arXiv here.

The second paper has the title “The future of cosmological likelihood-based inference: accelerated high-dimensional parameter estimation and model comparison” and was published on 5th September 2024. The authors are Davide Piras (Université de Genève), Alicja Polanska (MSSL) , Alessio Spurio Mancini (Royal Holloway, London), Matthew A. Price(UCL) & Jason D. McEwen (UCL); the latter four are all based in the UK. This paper, which is in  the folder marked Cosmology and NonGalactic Astrophysics, describes an accelerated approach to Bayesian inference in higher-dimensional settings, as required for cosmology, based on recent developments in machine learning and its underlying technology.

Here is a screen grab of the overlay which includes the abstract:

 

 

You can click on the image of the overlay to make it larger should you wish to do so. You can find the officially accepted version of the paper on the arXiv here.

That concludes this week’s update. More  next week!

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The Editorial Board of the Open Journal of Astrophysics

Posted in Open Access, The Universe and Stuff with tags , , on September 6, 2024 by telescoper

A couple of months ago, I issued a call for new Editors of the Open Journal of Astrophysics. That was very successful and we added a number of new Editors. The complete list (of 20 members) follows:

Peter Coles* (Department of Theoretical Physics, Maynooth University, Ireland). Cosmology, astrophysics, statistics and methodology.

Thierry Appourchaux (CNRS, Institut d’Astrophysique Spatiale, Orsay, France). Space instrumentation, astroseismology, helioseismology, statistics and methodology.

Emory (Ted) Bunn (Department of Physics, University of Richmond, USA). Relativity, cosmology.

Walter Dehnen (Astronomisches Rechen-Institut, University of Heidelberg, Germany). Stellar dynamics, galaxy dynamics, galaxies, bars, Milky-Way dynamics, Gaia, numerical methods, N-body techniques, smooth particle hydrodynamics (SPH).

Philipp Edelmann (Los Alamos National Laboratory, New Mexico, USA). Stellar astrophysics, hydrodynamics, high-performance computing, supernovae, internal waves, stellar evolution, numerical methods.

Pedro Ferreira (Department of Physics, University of Oxford, UK). Large-scale structure, general relativity, cosmic microwave background, early universe, cosmology.

Andrew Jaffe (Department of Physics, Imperial College, London, UK). Astrophysics, statistics and methodology, cosmology.

Harley Katz (Department of Astronomy and Astrophysics, University of Chicago, USA). Galaxy formation and evolution, numerical simulations

Lucyna Kedziora-Chudczer (School of Physics, University of New South Wales, Sydney, Australia). Active galactic nuclei, polarimetry, atmospheres of planets, exoplanets, solar system planets.

Julien Larena (Laboratoire Univers et Particules de Montpellier, Université de Montpellier, France). Cosmology, gravitation, lensing, large-scale structure, general relativity.

Manuela Magliocchetti (National Institute of Astrophysics, Rome, Italy). Cosmology, galaxies, active galactic nuclei (AGN).

Sean McGee (Department of Physics & Astronomy, University of Birmingham, UK). Galaxy formation, galaxy clusters, galaxy surveys.

Manolis Plionis (Department of Physics, Aristotle University of Thessaloniki, Greece). Observational cosmology, extragalactic astrophysics, large-scale structure, active galactic nuclei.

Alkistis Pourtsidou (Higgs Centre & Institute for Astronomy, Edinburgh, UK). Cosmology, large-scale structure of the Universe, radio astronomy, galaxy surveys.

Justin Read (School of Mathematics and Physics, University of Surrey, UK). Dark matter, cosmology, galaxy formation and evolution, dwarf galaxies, milky way, galactic dynamics, galactic archaeology, computational modeling.

Hanno Rein (Department of Physics and Environmental Sciences, University of Toronto at Scarborough, Canada). Numerical methods, in particular N-body codes and integration methods for planetary systems, planet formation, stochastic processes, planet migration, celestial mechanics, and Saturn’s rings.

Aleks Scholz (School of Physics & Astronomy, University of St Andrews, UK). Exoplanets, brown dwarfs, protoplanetary disks, stellar evolution, star formation.

Elena Sellentin (Sterrewacht Leiden, Leiden University, The Netherlands). Applied Mathematics, Cosmology, Statistics, Statistical Inference.

Elena Terlevich (Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico). Stellar populations in galaxies, observational cosmology, violent star formation, element abundances, dynamics of stellar systems.

Bingbing Wang (Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, USA.) Particle astrophysics, MHD turbulence, cosmic rays acceleration, cosmic ray propagation in the Galaxy and heliosphere.

Apologies to anyone who volunteered but has not yet received a reply from me. I’ve been a bit preoccupied these last weeks! The call is still open, though. Here are the areas of arXiv covered by the journal:

  1. 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
  2. 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
  3. 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
  4. 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
  5. 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
  6. 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 indeed be useful to have people who can cover a range of subjects (as some of our existing editors do), but there I think we’re still a bit short on High-Energy Astrophysics, Solar and Stellar Physics, and Galactic Astrophysics. I’d also like to see a better gender balance so applications from female scientists are particularly welcomed, as are astrophysicists from geographical areas not currently covered. The Open Journal of Astrophysics is intended to be a global enterprise!

Please follow the instructions here if you would like to volunteer!

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New Publication at the Open Journal of Astrophysics

Posted in OJAp Papers, Open Access, The Universe and Stuff with tags , , , , , on August 17, 2024 by telescoper

It’s Saturday morning and time for the usual weekly update of publications at the Open Journal of Astrophysics. This will be a short post because there is only one paper to report this week, being  the 68th paper in Volume 7 (2024)  and the 183rd  altogether. It was published on Thursday August 15th 2024.

The title of the latest paper is is “Spatial segregation of massive clusters in a simulation of colliding dwarf galaxies” and it  is in the folder marked Astrophysics of Galaxies. The authors are Bruce Elmegreen (IBM, NY, USA) and Natalia Lahen (MPA Garching, Germany);  the paper presents a numerical study of the properties and spatial distribution of star clusters resulting from a collision between dwarf galaxies.

Here is the overlay of the paper containing the abstract:

 

 

You can click on the image of the overlay to make it larger should you wish to do so. You can also find the officially accepted version of the paper on the arXiv here.

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Open Access Updates & Announcements

Posted in Open Access with tags , , , on August 3, 2024 by telescoper

When I wrote last week’s update on papers published at the Open Journal of Astrophysics, I was a little surprised that our publishing activity had not tailed off because of the summer vacations. Well, it has now because we haven’t publish any papers this week! Rather than not post an update at all, however, I thought I’d point out a few interesting things that have happened in the world of open access.

First. I draw your attention to an article in C&EN (Chemical & Engineering News) reflecting on the fact that the Gates Foundation (one of the largest research charities in the world) announced in March 2024 that, starting from Jan. 1, 2025, it would no longer cover publishing costs. I actually wrote about this decision here. The article is largely about the threat this poses to the Gold Open Access model, which in my opinion thoroughly deserves to be threatened. It does, however, talk briefly about Diamond Open Access which commercial publishers don’t like as it removes – or should do – their source of profits:

Another alternative model is diamond OA, in which all research papers and their associated peer-reviewed reports are published without fees for the author or the reader and are also freely available to read and reuse. 

It goes on to say:

Under diamond OA, publishers are no longer gatekeepers of research. Instead, they become service providers that handle manuscript submissions, typesetting, and copyediting. This is in contrast to the current publishing system, in which the publisher controls everything from the copyright to the production process.

I don’t really agree with even the limited role of “service providers” mentioned here, as much of what that role entails just involves a decent reviewing platform. Elsewhere the article says that moving to Diamond OA would entail a significant cost. That may be but, as I’ve said over and over again, the actual cost of online publishing is low compared to the level of profit extracted by commercial publishers. The cost to academia of moving to Diamond OA would be much less than not moving to Diamond OA.

The second item I’d like to draw your attention is called Choosing a publisher? It’s not all about the impact factor and is by Antigoni Messaritaki, a senior publisher at IOP Publishing,  When I saw the title I thought that it might be about the uselessness of Journal Impact Factors and a commitment by IOP Publishing to stop using them. Sadly it’s nothing of the sort. It tries to entice authors to look beyond journal impact factors when choosing a publisher, pushing Open Access as an important factor to consider. It admits that APCs are expensive, but never even mentions Diamond OA. It’s an entirely self-serving piece. I find the IOP’s stance on publishing, and the disingenuous way they try to excuse their own profiteering, unethical and unacceptable. That’s why I resigned my fellowship of the IOP.

Last, and by all means least, I should draw your attention that the 32nd General Assembly of the International Astronomical Union takes place next week in Cape Town. I’m not attending in person – I’ve done enough travelling this year! – but I have accepted an invitation to give a remote talk at a side event called Open Access Encounters on Wednesday 7th August:

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Four New Publications at the Open Journal of Astrophysics

Posted in OJAp Papers, Open Access, The Universe and Stuff with tags , , , , , , , , , , , , , , , , , , on July 27, 2024 by telescoper

It’s Saturday morning, so once again it’s time for an update of activity at the Open Journal of Astrophysics. This week we have published another batch of four papers, the same number as last week, which takes the count in Volume 7 (2024) up to 64 and the total published altogether by OJAp up to 179.

Before announcing the week’s papers I’ll add three other updates you might find interesting:

  1.  When I looked at NASA/ADS this morning to help construct this post I saw that papers published in OJAp have now garnered over 2500 citations between them;
  2. We had a good response to our recent call for new members of the Editorial Board and have added four new members here;
  3. Last week we received a significant (unsolicited) cash donation from a higher education institution based in Europe to help with our work in Diamond Open Access. If any other organizations or individuals would like to do similar then please contact me!

Now, in chronological order, the four papers published this week, with their overlays, are as follows. You can click on the images of the overlays to make them larger should you wish to do so.

First one up is: “Widespread disruption of resonant chains during protoplanetary disk dispersal by Bradley M S Hansen (UCLA), Tze-Yeung Yu (UCLA) and Yasuhiro Hasegawa (JPL), all based in California, USA.  The paper presents a discussion of the effect of a dispersing protoplanetary disk on the evolution of low-mass planets around a Solar mass star.  It was published on 21st July 2024 and is in the folder marked Earth and Planetary Astrophysics.

Here is a screen grab of the overlay, which includes the abstract:

 

You can find the officially accepted version of the paper on the arXiv here.

The second paper to announce is “Using A One-Class SVM To Optimize Transit Detection” by Jakob Roche of the University of South Florida, also in the USA (but not in California). This articles discusses the advantages of One-Class Support Vector Machines (SVMs) over Convolutional Neural Networks (CNN) in the context of exoplanet detection. Its in the folder called Instrumentation and Methods for Astrophysics and was published on 25th July 2024.

You can see the overlay here:

 

 

 

The accepted version of this paper can be found on the arXiv here.

The next paper, also published on 25th July 2024, is in the folder marked High-Energy Astrophysical Phenomena. Its primary classification on arXiv is General Relativity and Quantum Cosmology (gr-qc), but it is cross-listed on astro-ph so we considered it for publication and had it refereed, with favourable results. It is entitled “What no one has seen before: gravitational waveforms from warp drive collapse” and is by Katy Clough (QMUL, UK), Tim Dietrich (Potsdam, Germany) and Sebastian Khan (Cardiff, UK).  Looking at the title of this paper you might be tempted to dismiss it on the grounds that warp drives are the stuff of science fiction (which they are), but this paper is really a rigorous technical study of the dynamical evolution and stability of spacetimes that violate the null energy condition, inspired by the idea of a warp drive.

Here is the overlay:

 

 

You can find the full text for this one on the arXiv here.

Last, published on 26th July 2024, we have a paper with the title “A study of gamma-ray emission from OJ 287 using Fermi-LAT from 2015-2023” by Vibhavasu Pasumarti and Shantanu Desai of the Indian Institute of Technology, Hyderabad, India. It is an investigation of the properties of gamma-ray emission from OJ287 (a BL Lac object) using the Fermi Large Area Telescope (LAT).  This one is also in the folder marked High-Energy Astrophysical Phenomena; here is the overlay

You can find the officially accepted version of this paper on the arXiv here.

That’s all for this week. Stay tuned for another update next week.

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Academic Publishing is a Lucrative Scam

Posted in OJAp Papers, Open Access with tags , , , , , , , , on July 17, 2024 by telescoper

I saw an article in the Guardian yesterday with the title Academic journals are a lucrative scam – and we’re determined to change that. It’s written by Arash Abizadeh who is Professor of Political Science at McGill University in Canada. I urge you to read the piece if you’re interested in Open Access and the issues surrounding it.

I agree with virtually everything in the article. Indeed I’ve been saying much the same thing for about 15 years! I’m also determined to change things too, which is why we set up the Open Journal of Astrophysics, a “Diamond” Open Access Journal. Talking about the system of Gold Open Access, Prof. Abizadeh writes:

There is an obvious alternative: universities, libraries, and academic funding agencies can cut out the intermediary and directly fund journals themselves, at a far lower cost. This would remove commercial pressures from the editorial process, preserve editorial integrity and make research accessible to all. The term for this is “diamond” open access, which means the publishers charge neither authors, editors, nor readers (this is how our new journal will operate). Librarians have been urging this for years. So why haven’t academics already migrated to diamond journals?

I think the reason more academics haven’t already migrated to Diamond Open Access journals is that there are relatively few such journals. The reason for that is that although there are lots of people talking about Diamond Open Access there are many fewer actually taking steps to implement it. The initiative mentioned in the Guardian article is therefore very welcome. Although I think in the long run this transition is inevitable, it won’t happen by itself. It certainly won’t be helped by the Academic Publishing Industry either. We academics have to provide the push.

Here’s another excerpt:

Career advancement depends heavily on publishing in journals with established name recognition and prestige, and these journals are often owned by commercial publishers. Many academics – particularly early-career researchers trying to secure long-term employment in an extremely difficult job market – cannot afford to take a chance on new, untested journals on their own.

This is true, up to a point.

First of all any institution that has signed up to the San Francisco Declaration On Research Assessment (DORA) should not be relying on (often bogus) indicators of prestige such as the Journal Impact Factor or the journal’s presence in the Scopus index. If Diamond Open Access is to gain further traction it has to be accompanied to a wholesale change towards fairer research assessment practices.

Second, although it is true that it has taken some years to reach the volume it has now, I have been pleasantly surprised how many early career researchers in astrophysics have been keen to try out the Open Journal of Astrophysics. I think that’s because (a) early career researchers have not been indoctrinated into the absurdities of existing publishing practices and (b) they can see that the citation rates on OJAp are no worse than other allegedly more “prestigious” journals.

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Call for Editors at the Open Journal of Astrophysics

Posted in Open Access with tags , , , , , , , , , , , , , on July 7, 2024 by telescoper

Just over halfway into 2024 the number of papers submitted to the Open Journal of Astrophysics continues to rise, as demonstrated by this nice graphic which shows the submission stats for the last five years:

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! We’re therefore looking for 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:

  1. 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
  2. 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
  3. 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
  4. 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
  5. 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
  6. 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 indeed be useful to have people who can cover a range of subjects (as some of our existing editors do), but there are two specific topics that have seen a big increase recently: (a) galaxy formation simulations (especially involving hydrodynamics) covered by astro-ph.CO; and (b) galactic dynamics, covered by astro-ph.GA. The latter increase is driven Gaia data, an immensely rich source for discovery science.

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.

Please get in touch either through the Open Journal website here, or through a message Mastodon here, BlueSky here, or Facebook here. You could even send a message through this form:

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Thank you for your response. ✨

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Open Access in Ecology

Posted in Open Access with tags , , , , on May 6, 2024 by telescoper

My attention was drawn yesterday to the following blog post about Open Access in the field of ecology. I recommend you read it (and the comments, some of which are excellent).

The state of academic publishing in 3 graphs, 6 trends, and 4 thoughts

I will add a few comments of my own here.

First, whenever I read an article like this from a discipline different from my own it makes me not only feel grateful that we have arXiv but also wonder why so many fields don’t have the equivalent. On the other hand, there is EarthArxiv, but it doesn’t seem to have very many papers on it.

Second, I agree with the author of the post that far too many papers are being published. That is driven by the absurdity of a system that no longer regards the journal article as a means of disseminating scientific results but instead as a kind of epaulette to give status to the author. I also agree that scientists have largely got themselves to blame for this ridiculous situation.

Third, I disagree most strongly with this statement:

First, pipe dreaming academics who believed in the mirage of “Diamond OA” (nobody pays and it is free to publish). Guess what – publishing a paper costs money – $500-$2000 depending on how much it is subsidized by volunteer scientists. 

This is nonsense. It does not cost anything like $500-$2000 dollars to publish a paper. Of course it does cost something, but the true amount is trivial – tens of dollars, rather than hundreds or thousands – and can easily be absorbed. The entire annual running costs of OJAp are less than the typical Article Processing Charge for a single paper in a “prestigious” journal. Most money being paid in the form of APC goes directly into profit for the publishers, and the rest is largely wasted on administrative overhead. The Open Journal of Astrophysics is a Diamond Open Access journal, not a mirage. It may be a no-frills service, but it’s a reality. Why doesn’t someone set up an overlay journal on EarthArXiv?

The author of this blog post also spectacularly misses the point with “depending on how much it is subsidized by volunteer scientists”. Volunteer scientists are already subsidizing the profits of profit-making publishers! One of the commenters on the blog post has it right:

On Diamond OA and who pays; we’re already paying the big publishers with both our time and our money to publish in / review for / edit for their journals. Perhaps if we redirected that time to Diamond OA titles things would be somewhat different.

A final comment, only tangentially related to this post, is that I have been (pleasantly) surprised by the extent to which early career researchers have embraced the concept of the Open Journal of Astrophysics when you might have thought that they had more to lose by not publishing in mainstream journals rather than us oldies who don’t care any more. The explanation seems to be that younger people seem to see the absurdity and obvious unsustainability of the current publishing environment more easily than those who have put up with it for decades already.

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The Gates Foundation and Open Access

Posted in Open Access with tags , , , , , on April 9, 2024 by telescoper

There has been quite a lot of reaction (e.g. here) to the recent announcement of a new Open Access Policy by the Bill & Melinda Gates Foundation, which is one of the one of the world’s top funders of biomedical research. This mandates the distribution of research it funds as preprints and also states that it will not pay Article Processing Charges (APCs). The essentials of the policy, which comes into effect on 1st January 2025, are these:

  1. Funded Manuscripts Will Be Available. As soon as possible and to the extent feasible, Funded Manuscripts shall be published as a preprint in a preprint server recognized by the foundation or preapproved preprint server which applies a sufficient level of scrutiny to submissions. Accepted articles shall be deposited immediately upon publication in PubMed Central (PMC), or in another openly accessible repository, with proper metadata tagging identifying Gates funding. In addition, grantees shall disseminate Funded Manuscripts as described in their funding agreements with the foundation, including as described in any proposal or Global Access commitments.
  2. Dissemination of Funded Manuscripts Will Be On “Open Access” Terms. All Funded Manuscripts, including any subsequent updates to key conclusions, shall be available immediately, without any embargo, under the Creative Commons Attribution 4.0 International License (CC BY 4.0) or an equivalent license. This will permit all users to copy, redistribute, transform, and build on the material in any medium or format for any purpose (including commercial) without further permission or fees being required.
  3. Gates Grantees Will Retain Copyright. Grantees shall retain sufficient copyright in Funded Manuscripts to ensure such Funded Manuscripts are deposited into an open-access repository and published under the CC-BY 4.0 or equivalent license.
  4. Underlying Data Will Be Accessible Immediately. The Foundation requires that underlying data supporting the Funded Manuscripts shall be made accessible immediately and as open as possible upon availability of the Funded Manuscripts, subject to any applicable ethical, legal, or regulatory requirements or restrictions. All Funded Manuscripts must be accompanied by an Underlying Data Availability Statement that describes where any primary data, associated metadata, original software, and any additional relevant materials or information necessary to understand, assess, and replicate the Funded Manuscripts findings in totality can be found. Grantees are encouraged to adhere to the FAIR principles to improve the findability, accessibility, interoperability, and reuse of digital assets.
  5. The Foundation Will Not Pay Article Processing Charges (APC). Any publication fees are the responsibility of the grantees and their co-authors.
  6. Compliance Is A Requirement of Funding. This Open Access policy applies to all Funded Manuscripts, whether the funding is in whole or in part. Compliance will be continuously reviewed, and grantees and authors will be contacted when they are non-compliant.
    • As appropriate, Grantees should include the following acknowledgment and notice in Funded Manuscripts:
    • “This work was supported, in whole or in part, by the Bill & Melinda Gates Foundation [Grant number]. The conclusions and opinions expressed in this work are those of the author(s) alone and shall not be attributed to the Foundation. Under the grant conditions of the Foundation, a Creative Commons Attribution 4.0 License has already been assigned to the Author Accepted Manuscript version that might arise from this submission. Please note works submitted as a preprint have not undergone a peer review process.”

Reactions to this new policy are generally positive, except (unsurprisingly) for the academic publishing industry.

For what it’s worth, my view is that it is a good policy, and I wish more funders went along this route, but it falls short of being truly excellent. As it stands, the policy seems to encourage authors to put the “final” version of their articles in traditional journals, without these articles being freely available through Open Access. That falls short of goal establishing a global worldwide network of institutional and/or subject-based repositories, linked to peer review mechanisms such as overlays, that share research literature freely for the common good. To help achieve that aim, the Gates’ Foundation should to encourage overlays rather than traditional journals as the way to carry out peer review. Perhaps this will be the next step?

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Open Access Talk at UNSW

Posted in Biographical, Open Access, The Universe and Stuff with tags , , , on February 21, 2024 by telescoper

After an exciting start to the day involving a fire alarm and consequent evacuation of my hotel, I today ventured into the suburbs of Sydney via the Light Rail system (i.e. the tram) to the University of New South Wales. The tram ride took about 20 minutes from Central and, incidentally, took me right past the Sydney Cricket Ground. Anyway, the UNSW campus at Kensington is very impressive:

After a few gremlins with the WIFI connection, the talk I gave was a longer version of the one I did at the University of Sydney on Monday. In discussions with the Astrophysics group at UNSW, I found they were particularly unhappy about the decision of Monthly Notices of the Royal Astronomical Society to charge a high level of APC (Article Processing Artificial Profit Charge) so is looking at alternative journals that aren’t so exploitative. A journal has no right to call itself “open access” if it excludes researchers on grounds of cost. The problem with the Open Journal of Astrophysics in this case is that they need their publications to be in “high impact journals” for research assessment purposes, and OJAp doesn’t have an “official” journal impact factor yet. The fascination of bureaucrats with the obviously flawed journal impact factor disturbs me greatly but I hope we will have one soon so we may be able to help them out before too long.

Anyway, here are the slides from today’s talk:

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