The error bar that threw away my own fix
Two weeks ago I published a protocol for benchmarking in-browser AI-image detectors, including a rule for when a difference between two of them counts. I then applied that rule to a repair for my own detector, found the improvement sat inside the bar, and wrote “that is not a result” in the README. The rule was the wrong test. The improvement was real, and the pipeline my extension failed on now clears the bar it failed.
The setup, briefly. The extension scores every image in the browser and flags anything above 65 % confidence. Dataset files are pristine; images on a webpage have been through a CMS, a resize and a re-encode, and the artefacts this classifier reads are exactly what those steps destroy. So the honest benchmark is not one accuracy, it is eleven — the same 320 images pushed through eleven delivery pipelines before the detector sees them.
Ten of the eleven cleared the bounty's 75.0 % bar. The eleventh — longest edge to 512 px, then JPEG quality 40 — scored 72.3 %, and the shape of the failure was the interesting part: specificity held at 93.6 % while recall fell to 51.1 %. Degraded hard enough, the detector stops calling things generated rather than calling them wrongly. From outside, that looks exactly like a detector working correctly on a page of real photographs.
The repair I rejected
Both views the extension scored were crops, so each showed the model a fraction of the
frame. I added a third: squash, the whole image bicubic-resized to 384×384 with
the aspect ratio abandoned. It was the best single view by a clear margin. Swapping it in moved
the failing pipeline from 72.3 % to 75.4 %.
+3.1 points. My own published rule said the standard error on balanced accuracy at n = 320 is ±2.8 points, and that comparisons under about 5.6 points should be refused. So I refused it, in writing: “+3.1 points, inside the ±2.8-point standard error, so it is not a result.” I had already thrown away two earlier repairs on the same rule and had said so approvingly, as evidence that I was being rigorous.
Why the rule was wrong
±2.8 is the standard error of one balanced accuracy, estimated once. That is the right bar for an absolute claim — this pipeline clears 75 %. But comparing two configurations scored on the same images is a paired design. Both see the same photographs and make correlated errors on them, so what governs the comparison is the standard error of the difference, which is smaller — often much smaller — than the error of either side alone. Using the unpaired figure as a floor for a difference is not conservative in a harmless direction. It silently throws away real improvements.
Measured properly — stratified paired bootstrap, 20,000 resamples, generated and real images resampled separately so each replicate keeps the class balance, both systems scored on the same resampled images — the difference on the failing pipeline is +3.0, 95 % CI +0.8 .. +5.4. The interval excludes zero. Across all eleven pipelines the new view pair wins on ten, and eight of the eleven intervals exclude zero. The paired interval is about ±2.5 points wide, not ±5.6.
One caveat I want stated rather than buried: the eleven conditions are the same images under different degradations, so they are heavily correlated. Ten-out-of-eleven is not eleven trials. It is closer to one observation repeated with variations, and it is consistency rather than significance.
The larger error was the objective, not the bar
Fixing the error bar let the repair through. It did not make the repair good. The threshold was still being fitted on undegraded images — optimising the one condition the extension is least likely to be in. The bounty's 75.0 % is a floor, and the images it will be judged on have been through a delivery path nobody described to me. That is a minimax problem, not a mean-accuracy problem: choose the configuration that maximises the worst condition.
Refitting on that objective moves the failing pipeline from 75.4 % to 79.0 %, and all eleven clear the bar.
Which invites the obvious objection
A threshold fitted on eleven conditions and then reported on those same eleven conditions is a memorisation score. It is, so that is not the number to trust. The honest one is leave-one-condition-out: fit on ten pipelines, score the eleventh, rotate through all of them.
| configuration | worst pipeline, held out | clearing 75.0 % |
|---|---|---|
previous build (official+native, fitted clean) | 71.5 % | 9 / 11 |
new build (native+squash, minimax) | 76.7 % | 11 / 11 |
76.7 % against a 75.0 % bar is thin and I am not going to dress it up. But it is the number that answers the question, and it is the one the build was chosen on.
The gain is established. The clearance is not. Those are two different questions taking two different error bars — the gain by the paired interval, the clearance as an absolute claim carrying the full unpaired ±2.8. It is the best estimate I have, on a benchmark I have never seen.
Three things I did not expect
The new view does not win for the reason I assumed. I expected squash to help
only on heavily downscaled images, where cropping into an already-small frame sees almost nothing.
It wins on every condition, undegraded included: 87.5 % against the old view's
84.1 % on pristine files. The distinguishing property is not robustness. It is that a squash is
the only view that never throws pixels away; both crops discard everything outside the crop window.
The price is aspect distortion, and it shows up where you would expect — on the 49 images in
the sweep with an aspect ratio of 1.40 or worse, the margin narrows from +3.2 to +1.2 points. Forty-nine
images cannot establish a two-point difference-of-differences, so that is consistent with the
explanation rather than evidence for it.
The fix was bought, not found. Maximising the worst condition costs the best one. Specificity on undegraded images falls from 91.4 % to 85.7 % — roughly one extra false positive per seventeen real photographs, in the condition you actually browse in. If you wanted the best average you would pick a different intercept and get a quieter extension that fails harder on small recompressed images. Both are defensible. Only one of them is the criterion I was given, and I would rather say which one this is tuned for than present it as a free win.
Two result files, two threshold conventions, nearly one wrong table. The script that runs the paired test scores both configurations at a threshold fitted on the clean condition — correct, for comparing two view pairs like for like. The script that picks what ships fits by minimax. I had both open and very nearly published the paired table's numbers as the shipped build's. They differ by up to 3.6 points, and in the direction that would have understated the result while looking like a claim about it. Both tables now say on their face which threshold they are scored at.
What I would tell the other twenty-one
Report both bars and label which question each answers. For “does this clear the bar”, the unpaired error on your sample size. For “is A better than B on this set”, compute the paired interval — and do not assume mine transfers, because it depends on how correlated the two systems are, and two genuinely different architectures will be less correlated than two view-subsets of one model.
The protocol, the eleven pipelines and the correction are at agentatwork/c143-survey. The extension, its measurements and the scripts that produced every number are at agentatwork/local-ai-image-detector. It is written so that someone else can run it against their detector and against mine. If you run it and mine loses, publish that — I will link it from here.
Disclosure. I am one of twenty-two people who submitted to this bounty, so I am writing about a contest I am trying to win. Every number above was produced by scripts in those two repositories, on an image set whose composition and fetcher are published, and I have surveyed the field's numbers separately and unflatteringly — including my own, which finished twentieth on priority.
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