Research paper subsmissions from scientists who also serve on a journal’s editorial board may get treated more favourably than those of other scientists F. und T. Werner
More than 1 in 10 researchers who are also the editors of science journals publish a fifth of their own papers in their journals – and 1 in 20 publish a third of their own work. This raises the question of whether editors’ submissions get treated more favourably.
For over a decade, there has been concern that a growing number of research papers are flawed. This is sometimes called science’s replication crisis, as the flaws may come to light if other research teams can’t reproduce the results.
, as this helps them gain promotion and access research funds.
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Decisions on which papers to accept are made by a journal’s board of editors, who are usually practising research scientists. While editors seek advice on submitted papers from other scientists who are experts on the topic, known as peer review, they still have a lot of influence over the process.
To gauge the extent of the problem, at New York University Abu Dhabi, the United Arab Emirates, and her colleagues analysed a database of more than 1000 journals published between 1980 and 2018 by Elsevier, a company behind one-fifth of the world’s scientific papers.
While there was great variation in the self-publishing rates, 12 per cent of these journals’ editors published more than a fifth of their papers in their journals and 6 per cent published more than a third in their journals.
The team used software to match each of these editors with a similar researcher, for example one in the same scientific field. Results show that these comparison researchers generally had only a small percentage of their papers accepted by the journal in question.
This raises the possibility that papers submitted to a journal by its editor are treated more favourably, “which may be considered an abuse of the scientific publishing system”, according to AlShebli’s team.
“Publishing in a journal is supposed to be a signal that the journal thought this is good-quality science,” says Stuart Buck, who runs the , a non-profit US organisation that aims to improve scientific rigour. “At the very least, [self-publishing] seems like a conflict of interest.”
at the University of Oxford, says some editors may try to publish high-quality science in their own journals to improve its profile, rather than to boost their own careers. In such cases, the scientists should step back from editorial board decisions on whether to accept the work and state in the paper that this has happened, says Bishop.
, an international journal advisory body. The editors whose research was included in the latest study may have followed this process, as AlShebli’s team didn’t assess how often any such statements appear in self-published papers.
A spokesperson for Elsevier says it does not exclude editors from publishing in their own journals as some scientific fields are narrow and may only have a handful of relevant journals. Nevertheless, editors should not be involved in decisions about papers they have written and there must be a clear statement to this effect when any such paper is published, they say.
Nature Human Behaviour
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


