"Why downsize the study to 10×10 arcmin?"
My guess would be to reduce the numbers of transients to be talked about.
If the frequency of them in that 10 x 10 is multiplied by the number of 10 x 10's in the entire sky suddenly there are billions and billions of flying saucers circling the Earth.
Source?In some ways it's similar to my favourite comparison I like to do in "it's probably a fly" videos where we see a 4 second video with a small black dot across it, I always ask for them to watch my 10 hour cows in a field video and ask if all of the black dots in there are UAP.
If she can't specify the criterion used to distinguish between her 10 and the multitude of other trivially-findable datapoints in the source data set available to her, then we can deduce they are equivalent. (If there's no test to distinguish between things, they are definitionally indistinguishable, and indistinguishable things are equivalent as they can be used interchangably.) Her method has pointed us to thousands/millions of alien craft, whether she intended that or not. However, because she ignored those myriad other ones, we can deduce that they're instead uninteresting. Therefore we can deduce her 10 are uninteresting.So essentially - the potential detection of ten flying saucers over a number of years is more believable than the detection of a thousand every day.
I'd also argue the correlation with nuclear explosions is similar. There's no a priori reason to associate UAPs with nuclear test dates, only UFO lore that assumes it to be true. You also have to wonder at the association of the transients +/- 1 day of the tests being carried out (and in supposed geosynchronous orbits not related to the location of the tests), when the tests were occasionally postponed from the scheduled dates due to weather or other factors. So if the supposed aliens knew the schedules and were showing up in advance of the explosions, there should be other transient clusters associated with dates of scheduled tests.If she can't specify the criterion used to distinguish between her 10 and the multitude of other trivially-findable datapoints in the source data set available to her, then we can deduce they are equivalent. (If there's no test to distinguish between things, they are definitionally indistinguishable, and indistinguishable things are equivalent as they can be used interchangably.) Her method has pointed us to thousands/millions of alien craft, whether she intended that or not. However, because she ignored those myriad other ones, we can deduce that they're instead uninteresting. Therefore we can deduce her 10 are uninteresting.
Her own bad science is its own undoing.
So I'll happily stick the "Texas sharpshooter fallacy" label on this too: these points are the interesting ones only because they're the ones she selected.
Phew haha I thought I was going crazy, missing something extremely obvious. But that's also my bad for not reading the linked medium article first.As far as I can tell they don't and neither could Izabela Melamed
First off, welcome to the website! And second, your post still has value contributions on top of mine! It's great to have more stats folks around here.An analysis issue , aside from the technical aspects of the data, is a very basic stats point. When you have a very large sample size (i.e. < 2000 data points), you have massive statistical power to generate a small P-value. This means you can get low P (and reject the null hypothesis) even with small or modest effect sizes. While technically statistically significant, in real world terms the effect could be trivial. Look at their Mann-Whitney U tests for example. Huge U scores for a smallish effect size. I would not be surprised if you could pick many random events (e.g. UK bank holidays) and find an association with these and appearance of transients. P-values need to be interpreted with common sense. Could be a useful exercise for stats teaching if the dataset is released.
Update...oops @yoshy beat me to it. I agree with @yoshy
Releasing data and code should be the norm rather than the exception, as the world operates today sadly. (Except in cases where releasing data would be unethical, dangerous, etc, of course)Could be a useful exercise for stats teaching if the dataset is released.
External Quote:I had a read through this and word searched the Aug 2nd print a few times. There is not one single mention of cosmic ray strikes as a probable cause which i find astonishing in a paper where conclusions are being derived from photographic material.
Cosmic ray strikes produce exactly these kind of star-like objects. I've seen them many thousands of times in my ~30yrs as an astrophotographer. Typically you'll get between 1-10 per min though not all leave a defect in the image, but over long exposures you'll get plenty of them (and these POSS plates are 50min exposures.) Artificial alien objects have got to be right at the bottom of the list as a potential explanation.....yet here that seems to be at the top.
External Quote:
Figure 7. Examples of streaks found near the shadow center, from B/IV. The box sizes in the upper panels are (a) 46.3 ×
31.9 arcmin, and (b) 25.2 arcmin ×16.6; in the lower panels: (c) 1.7 ×1.4 arcmin and (d) 2.6 ×3.8 arcmin. The first three images (a)
through (c) are believed to be observations of real objects, while the fourth (d) is likely a cosmic ray due to the narrowness (FHWM of
∼1 arcsecond) and uniform width of the track in spite of brightness fluctuations.
I was wondering about this myself.
External Quote:I had a read through this and word searched the Aug 2nd print a few times. There is not one single mention of cosmic ray strikes as a probable cause which i find astonishing in a paper where conclusions are being derived from photographic material.
Cosmic ray strikes produce exactly these kind of star-like objects. I've seen them many thousands of times in my ~30yrs as an astrophotographer. Typically you'll get between 1-10 per min though not all leave a defect in the image, but over long exposures you'll get plenty of them (and these POSS plates are 50min exposures.) Artificial alien objects have got to be right at the bottom of the list as a potential explanation.....yet here that seems to be at the top.
Source: https://x.com/peachastro/status/1953506332671095071
It's an increasing concern in the earth sciences that you have people crunching data gathered by other researchers and drawing conclusions without a hands-on familiarity with the physical processes involved.
Aliens?All those tails are swishing for a reason...
Aliens?
The speculative nature and reliance on potentially flawed data make this paper unlikely to pass peer review without major revision.It doesn't matter where the artefacts come from at all, if you're cherry picking..
I wonder if the paper gets through the peer review.
There is another paper, with Beatriz as first author. I believe this is the paper she has been primarily discussing online and in interviews.
"Aligned, multiple-transient events in the First Palomar Sky Survey",
Beatriz Villarroel, Enrique Solano, Hichem Guergouri, Alina Streblyanska et al., dated as "Preprint July 2025", available via ResearchGate https://www.researchgate.net/public...nsient_events_in_the_First_Palomar_Sky_Survey,
PDF attached.
Beatriz Villarroel is a member of Gary Nolan's Sol Foundation...
/vascoproject.org/local-probes-and-asteroids/External Quote:
Some theories of the Milky Way Galaxy suggest that technological probes have been sent to stars to perform investigative functions, such as monitoring the local planets...
Traveling slower than 1% of light speed, probes could leisurely travel from one star to another. Robotic interstellar probes may be purposely stealthy, equipped with telescopes, and communicating with a Galactic Internet – at the speed of light.
This hypothetical model predicts that some probes may currently reside in the Solar System, either in orbit around the Sun or around the Earth (Benford 2019, Gertz 2018, 2021).
Probes may be detected by specular reflection of sunlight off any flat surfaces, as described by Lacki (2019) and Villarroel et al. (2022). Such "glints" are momentarily brilliant because the reflected light is concentrated into a narrow beam equal to the angular size of the Sun, roughly ½ degree across for mirrors at 1 AU. Probes as stand-alone machines may glint making them momentarily detectable at the Earth.
vascoproject.org/exo-lasers/External Quote:
Other advanced civilizations may also use powerful lasers. We are searching for such extraterrestrial lasers.
vascoproject.org/vanishing-stars/External Quote:
Second, vanishing stars may also be a sign of extra-terrestrial technology. For example, Dyson spheres could cause a star to vanish (for an overview see Villarroel al. 2016, Villarroel et al. 2020).
Since VASCO started up in 2017, we have been searching for vanishing stars in the Milky Way through citizen science and automated methods. We are comparing images from the 1950s with images from modern sky surveys. We have found thousands of objects visible in the 1950s that no longer are seen today. We ourselves, refer to these as "short-lived transients", as we think most represent the bright state of an astrophysical object that brightened up for a few minutes later to dim again, rather than a star that actually vanished.
Because the website is not HTTPSI get a "not secure connection" warning from Chrome when I visit vascoproject.org.
If these transients are (sometimes? often?) caused by cosmic ray events, might one expect to find fewer events in the dark side of the Earth's hemisphere, perhaps because the magnetosphere is elongated in that direction?We also find a highly significant (∼22σ) deficit of transients from Solano et al. 2022 within Earth's shadow, supporting the interpretation that sunlight reflection plays a key role in producing these events.
might one expect to find fewer events in the dark side of the Earth's hemisphere, perhaps because the magnetosphere is elongated in that direction?
Where is the evidence? I'd like to see the data and code that was used.Generally I'd like to see more discussion of the shadow deficit in this thread. It's the most interesting, most well evidenced claim being made.
As far as I could find, they haven't released code, only their methodologies.Where is the evidence? I'd like to see the data and code that was used.
As for the actual image data, I think this is where you get it.Where is the evidence? I'd like to see the data and code that was used.
I've downloaded all five candidate files using the DSS plate finder. You can download them from Google drive. They are all 60x60 arcmins. File name format: cn (candidate number) + palomar + date (dd-mm-yyyy) + epoch (first four digits) + 60x60 (arcmins) + nnnnnn (plate id). File size: 8,6 Mb each.As for the actual image data, I think this is where you get it.
I'm not entirely sure this is the data though and there doesn't seem to be a bulk download option. Again, you'd probably need to email someone to get access to the bulk data.
@Mick West as far as I know, they have not published detailed data or tools concerning the claims about transients within Earth's shadow.
<snip>
This hypothesis has not been tested against modern datasets. Should similar sunlight-dependent transients be present?The methodology for determining whether or not the object is determined to be a defect or transient technosignature is given in this paper:
https://www.researchgate.net/public...nsient_events_in_the_First_Palomar_Sky_Survey
So it seems to be that transients are short, sharp points that are roughly in a line but less that 10x10arcmin (ie the distance that a geosynchrounous object would be expected to transit during the exposure time)
@HoaxEye said:
The Solar Reflection Hypothesis is also discussed therein:
<snip>
So its essentially saying that (statistically) there's less defects/transients in the shadowed part of the sky - but if these were objects reflecting the Sun's light why would we expect any reflections in the shadow?
As for the actual image data, I think this is where you get it.
I'm not entirely sure this is the data though and there doesn't seem to be a bulk download option. Again, you'd probably need to email someone to get access to the bulk data.
Thank you for your question about DSS availability.
The agreement we made with the original observatories when it became possible to make the digitized survey plates publicly available, was to provide cutout access for the astronomical community for research and education. We are only allowed to bulk redistribute to other data centers who sign a formal agreement with the same conditions.
The way that the data is stored as tile-compressed data files requires a software layer to reconstruct the image for delivery.
Thanks for your understanding.
They want a formal Data Sharing Agreement (that stops us just sending the data to someone else)Hmmm... our community is dedicated to research and education, I suppose, but I guess we are not in the astronomical community. Unless one of y'all...?
Is that normal? "Don't share the data" seems contrary to the way I was taught science should work, but admittedly that was a LONG time ago! Perhaps there is a "don't share the data widely until published" clause we were not taught back then!They want a formal Data Sharing Agreement (that stops us just sending the data to someone else)
We find that a) the image profiles of the transients are significantly sharper than typical stellar images on the plates; b) that an ML decision–tree classifier badges the images as spurious with high probability; c) that similar examples of apparent transients are present on the copy plate of the adjacent field; and finally d) that there are many hundreds of similar images on both plates in the overlap region between the two fields. We suggest one likely mechanism for the origin of at least some of these apparent transients as being emulsion holes on the intermediate positive plates used during reproduction of the copy sets. We therefore caution that digitised all–sky survey catalogues derived from the POSSI glass copies are likely peppered with these isolated false detections and that great care must be exercised when interpreting the publicly available digitised images or when making samples of unpaired catalogue records derived from them.
I've asked. They said they are waiting for publicationAs far as I could find, they haven't released code, only their methodologies.
You might be able to convince them to share code if you email them however.
The point of the "less transients in the shadowed part of the sky" measure is to argue in favor of the "transients being real objects reflecting the sun rather than plate defects" hypothesis.if these were objects reflecting the Sun's light why would we expect any reflections in the shadow?