Quote from: LouScheffer on 12/07/2022 11:51 pmI think science was actually advanced in this case. We're talking about the impact on scientists, not just "science". It makes little difference in the grand scheme whether a paper comes out this month or in 3 months. It does however make a big difference to someone's career if they get a paper in a big journal with global media attention. The original team missed out on that. Note that without the original team this result would have been delayed much further, because they are the ones who got the data taken in the first place.
I think science was actually advanced in this case.
All these people were scooped, someone published their project before them. That's what scooped means, this is a no-true scotsman fallacy.
If the manuscript was less developed then there would be no response and we simply wouldn't have heard about it. It is a survivorship bias.
And when things are rushed mistakes happen. If you want examples of rushed analyses which turned out false then we have BICEP2 and some of the high redshift pre-flight calibration JWST papers.
Quote from: LouScheffer on 12/07/2022 11:51 pmIt's not at all obvious that peer review contributes more to science than it hurts by delaying distribution of knowledge. Peer review absolutely contributes to science by screening obvious errors. You're putting so much emphasis on speed of publication but none on quality control, which is absolutely the wrong view in my opinion. [...] If you want to see what science looks like without peer review take a look on viXra. Peer review isn't perfect but it's the only filter against absolute nonsense.
It's not at all obvious that peer review contributes more to science than it hurts by delaying distribution of knowledge.
(b) The need to publish in major journals. This is a huge problem. Since these publications are so coveted, the journals get an enourmous number of submissions. A considerable majority are tossed by the editor without even sending out for peer review, so your entire career depends on the reactions of a single person to a quick reading of your article. Which ones even make it to peer review is (in my experience) a total crapshoot. This is a horrible way to run a gate-keeping system.
(c) The problem of getting credit for data generation. This too is broken, related to (b). Despite the fact that collecting the data is often by far the largest task of solving the problem, top journals show no such respect and require a "science story". This leads precisely to data sets (which could be used for many purposes) being held back until the one particular science question that concerns the main researcher is answerable.
This is exactly why I am asking for real examples. There are two possibilities: (a) It happens all the time, we just don't hear about it, and (b) it doesn't really happen often, if at all. I think it's largely (b), and the way to disprove my hypothesis is to show real examples.
These are good examples of haste makes garbage. But they were invalidated quite quickly, and the authors certainly did not gain reputation in the longer run - quite the opposite.
This statement is only true if you restrict "published" to mean "published in a journal". If you include pre-prints, they were not scooped. This is not a hypothetical distinction - in some fields, such as physics, an arxiv publication is perfectly good for claiming scientific priority.
I certainly agree there is a tradeoff between speed and accuracy. But requiring peer review before publication, in my mind, is way past the point of diminishing returns - other points on the speed-accuracy curve are better overall. And peer review is certainly not the only filter against nonsense. Arxiv, for example, does not have any peer review, but the content-to-garbage ratio is reasonable and the speed much faster than peer review. xiVra, on the other hand, is indeed a dumpster fire, but that's not since it lacks peer review, it's because it does no gatekeeping whatsoever. Arxiv instead (at least the last time I checked) requires a one-time certification by someone in the field that you are a serious researcher. That, plus researcher's own incentive not to publish trash, seems to be enough.
But I think this is getting rather off topic,
NASA's decisions about proprietary time isn't going to reform publishing. Astronomers are at the mercy of academia as it is today, not how we might want it to be.
At least some high redshift galaxies are getting confirmed now. Discovery and properties of the earliest galaxies with confirmed distanceshttps://arxiv.org/abs/2212.04480
The arXiv basically relies on the fact that most of the papers are submitted to be peer reviewed. They have in the past removed research notes published in RNAAS because they are not peer reviewed, their current policy is vague.
IIRC, wasn't the BICEP2 'scooping' based on data scraped from slides presented by the original team prior to publication? i.e. the data the original team gathered WAS embargoed, but an embargo does no good if you go and disseminate it anyway.
Extremely off topic: the ban didn't have anything to do with RNAAS not being peer reviewed; there are a lot of papers on arxiv that are not (and are not intended to be) peer reviewed. The reason was that they were afraid of being flooded by lots of very short papers so they enforced some minimum length limit (though I think shorter papers could still be accepted in special cases). I'm not sure if the policy changed.
NASA's James Webb Space Telescope has produced amazing images in its first 5 months, but amazing science as well. Roland hears from one of the leading astronomers on the JWST programme, Dr Heidi Hammel, as well as other experts on what they are already learning about the first galaxies in the Universe, the birth places of stars, the strange behaviour of some other stars, and the first view of Neptune's rings in over 30 years.
Quote from: Eric Hedman on 01/26/2023 11:10 pmQuote from: CuddlyRocket on 01/25/2023 12:12 amQuote from: deadman1204 on 01/23/2023 06:25 pmQuote from: sghill on 01/23/2023 04:06 pmThey are also going to try to image the zodiacal light. Question: Are trace CFC gases in the zodiacal light something they could register with the spectrometer at this distance? There are obvious world-shattering implications if they see any... How would CFC's in the zodiacal light be "world shattering". The zodiacal light is reflected light from sol inside the solar system.Observing CFCs in the atmospheres of exoplanets is considered by astronomers as compelling evidence of a technosignature as they are only produced in significant quantities on Earth by industrial processes. So, reasoning by analogy ...Zodiacal light is not from the atmosphere of a planet. It is light reflected from the dust floating in space around a star. In our solar system the figure I get for the dust that reflects zodiacal light is the particles have a total volume equivalent to a 30 km sphere broken down into dust, that is a reflective surface many orders of magnitude greater than Earth's surface. CFCs are an incredibly small percent of our atmosphere. I highly doubt you would be able to find the signature of CFCs in the atmosphere of a planet within that dust cloud within all that light noise from zodiacal light.CFCs in our atmosphere can be monitored by satellites. The Aura satellite uses a microwave limb sounder to build a vertical profile of the gasses in our atmosphere. The microwaves are emitted by the gasses and not part of reflected sunlight. But to do it at stellar distances, is more than likely going to be beyond our technical capabilities for a long time if ever. So looking for CFCs from a planet buried inside the cloud of dust reflecting sunlight isn't likely to find CFCs anytime soon.I obviously put it obscurely, so trying to be clearer: The (probably tongue-in-cheek) original suggestion seemed to be that there would be world-shattering implications if they see traces of CFCs in the zodiacal light generally - i.e. from the circum-stellar dust; not specifically from any exoplanets - as it would be taken as evidence of widespread in-space industrial activity in the stellar system.
Quote from: CuddlyRocket on 01/25/2023 12:12 amQuote from: deadman1204 on 01/23/2023 06:25 pmQuote from: sghill on 01/23/2023 04:06 pmThey are also going to try to image the zodiacal light. Question: Are trace CFC gases in the zodiacal light something they could register with the spectrometer at this distance? There are obvious world-shattering implications if they see any... How would CFC's in the zodiacal light be "world shattering". The zodiacal light is reflected light from sol inside the solar system.Observing CFCs in the atmospheres of exoplanets is considered by astronomers as compelling evidence of a technosignature as they are only produced in significant quantities on Earth by industrial processes. So, reasoning by analogy ...Zodiacal light is not from the atmosphere of a planet. It is light reflected from the dust floating in space around a star. In our solar system the figure I get for the dust that reflects zodiacal light is the particles have a total volume equivalent to a 30 km sphere broken down into dust, that is a reflective surface many orders of magnitude greater than Earth's surface. CFCs are an incredibly small percent of our atmosphere. I highly doubt you would be able to find the signature of CFCs in the atmosphere of a planet within that dust cloud within all that light noise from zodiacal light.CFCs in our atmosphere can be monitored by satellites. The Aura satellite uses a microwave limb sounder to build a vertical profile of the gasses in our atmosphere. The microwaves are emitted by the gasses and not part of reflected sunlight. But to do it at stellar distances, is more than likely going to be beyond our technical capabilities for a long time if ever. So looking for CFCs from a planet buried inside the cloud of dust reflecting sunlight isn't likely to find CFCs anytime soon.
Quote from: deadman1204 on 01/23/2023 06:25 pmQuote from: sghill on 01/23/2023 04:06 pmThey are also going to try to image the zodiacal light. Question: Are trace CFC gases in the zodiacal light something they could register with the spectrometer at this distance? There are obvious world-shattering implications if they see any... How would CFC's in the zodiacal light be "world shattering". The zodiacal light is reflected light from sol inside the solar system.Observing CFCs in the atmospheres of exoplanets is considered by astronomers as compelling evidence of a technosignature as they are only produced in significant quantities on Earth by industrial processes. So, reasoning by analogy ...
Quote from: sghill on 01/23/2023 04:06 pmThey are also going to try to image the zodiacal light. Question: Are trace CFC gases in the zodiacal light something they could register with the spectrometer at this distance? There are obvious world-shattering implications if they see any... How would CFC's in the zodiacal light be "world shattering". The zodiacal light is reflected light from sol inside the solar system.
They are also going to try to image the zodiacal light. Question: Are trace CFC gases in the zodiacal light something they could register with the spectrometer at this distance? There are obvious world-shattering implications if they see any...