I think this is interesting. I don't know whether Loeb's musing, that reconnaissance aircraft might be responsible for the transients, is a workable hypothesis,
but if it is then it's unlikely U-2 flights played a major part. if they did it would be reflected (no pun intended) in a greater frequency of transients in later plates, perhaps concentrated in the last 1% or so to be taken. "Oxcart" played no role whatsoever.
External Quote:
The first photographic plate was exposed on November 11, 1949. 99% of the plates were taken by June 20, 1956, but the final 1% was not completed until December 10, 1958.
Wikipedia,
https://en.wikipedia.org/wiki/National_Geographic_Society_–_Palomar_Observatory_Sky_Survey
But the first U-2 test flight wasn't until June 1955. Progress was fast, by March 1956 there were 9 planes and approx. 1000 flying hours logged
(
Unlimited Horizons- Design and Development of the U2, Peter W. Merlin, 2015, NASA
https://www.nasa.gov/wp-content/uploads/2015/07/unlimited-horizons.pdf)
By June 1956 the U-2 had attained altitudes of approx. 22,700 m, comfortably breaking the 20,080 m record set by a Canberra, August 1955.
The first "Oxcart" (YF-12) flight was in June 1963 (Wikipedia
https://en.wikipedia.org/wiki/Lockheed_YF-12), so not a possible cause of transients.
The Yak-25RV, a Russian aircraft sometimes described as performing a similar role to U-2, didn't fly until 1959. (Soviet claims about its performance may be unreliable, and it wasn't used in areas where we might expect a Soviet U-2 equivalent to be used).
And it's a pretty safe bet it was never visible from the Palomar Observatory. How would it get there? No Soviet aircraft carriers, no Communist Cuba until 31 December 1958.
Loeb may have been talking "off the cuff", but he seems to have been wondering if
high-altitude aircraft were responsible.
If pretty much
any fixed-wing aircraft might be the cause of large numbers of pseudo-transients, which are hard to distinguish from actual astronomical transients, I feel the wider astronomical community would have pointed this out to Villarroel
et al. pretty quickly, as it would be a familiar problem. Commercial aircraft must vastly outnumber secret military test flights in the skies around the observatory, and probably did in the 1950s. Area 51 is
relatively close to Mount Palomar (276 miles, 444 km) but only 104 U-2s were built over
34 years from 1955 (Wikipedia
https://en.wikipedia.org/wiki/Lockheed_U-2).
If altitude is a factor in hypothetical spy planes being transients, that sort of leaves us with the more modest Canberra, which entered UK service in January 1950.
The USAF adopted a heavily Americanised version, the Martin B-57 which was accepted into service in March 1953. But the B-57 was optimised for close air support, and had a ceiling of just 13,745 m (Wikipedia
https://en.wikipedia.org/wiki/Martin_B-57_Canberra).
The USAF further modified 20 aircraft as RB-57s for high-altitude (approx. 21,300 m) recce, Wikipedia
https://en.wikipedia.org/wiki/Martin_RB-57D_Canberra, which came into service from April 1956, again too late for the overwhelming majority of the POSS1 plates.
The direct Russian equivalent to the Canberra /B-57 was the Ilyushin Il-28, introduced 1950 but with a modest ceiling of 12,300 m, and like the Yak it wouldn't be troubling California.
So YF-12 (Oxcart) is too late to have played a role, U-2 entered service in modest numbers very much toward the end of the first 99% of the plates being produced. Likewise the twenty RB-57s. The main B-57 types used by the USAF were not high altitude machines.
Realistically, we can rule out Soviet aircraft or non-US Canberras (or any other foreign type, come to that).
I think it's unlikely that the small number of U-2s and RB-57s available while the last few percent of POSS1 plates were being taken had much impact. Whether aircraft more generally [
edited to add, not just high-altitude types] might be responsible for some, I don't know, but if they are I think astronomers would be well aware of the issue, perhaps with a rough idea of how many they might expect to see in any given exposure (taking time and area of sky being imaged into account).
(This is sort of apart from what we might read into why Loeb raised this possibility, and what it might indicate about his views on Villarroel
et al.'s claims; as pointed out by
@Andreas this could be very interesting).