A machine that finds planets the way pharma finds drug candidates: scan millions, confirm a handful.
That is what Princeton's T16 team built. Their pipeline chewed through 83,717,159 light curves from NASA's Transiting Exoplanet Survey Satellite — TESS, the space telescope that watches stars for the dimming that signals a planet crossing in front — and surfaced 11,554 planet candidates in a single systematic pass. More than double the known TESS catalog. Then they used telescope time on the 6.5-meter Magellan telescope to confirm exactly one.
The ratio is the story.
TESS has accumulated roughly 7,800 planet candidates over its mission, of which approximately 760 had been confirmed as of March 2026 — a historical confirmation rate of about 9.7 percent. The T16 catalog, in one contribution, added more candidates than the entire confirmed population. The bottleneck is not detection. It is radial velocity follow-up: the method astronomers use to measure the wobble a planet induces in its host star. That requires a high-resolution spectrograph on a large telescope, and telescope time is a finite, oversubscribed resource. The T16 team used Magellan's PFS spectrograph to confirm one target, TIC 183374187, a metal-poor thick-disk star hosting a hot Jupiter. They chose it carefully: you confirm one, demonstrate the pipeline works, and hand the rest of the list to a community that does not have enough telescope time to work through it.
The comparison to pharma is not metaphorical. Drug discovery works the same way: screen millions of compounds, push a handful through validation. Screening is fast. Clinical trials are slow and expensive and do not scale with the library size. Exoplanet astronomy has arrived at the same inflection point. T16 processed 83.7 million light curves using machine learning-assisted transit searches, turning what used to require teams of astronomers years of focused staring into a semi-automated pipeline running on data already collected. The detrending and systematics-correction across the full TESS Cycle 1 dataset — removing instrumental noise and stellar variability to expose transit signals underneath — is genuinely difficult signal processing. The results demonstrate it works.
The ExoNet paper, published independently by a separate team, frames the same bottleneck from the other side: a multimodal deep learning system that vets TESS candidates with 86.3 percent accuracy, identifying 1,754 high-confidence signals out of 4,720 unconfirmed candidates, including 52 in the habitable zone and six Earth-sized candidates below 1.6 Earth radii. TOI-5728.01 and TOI-6716.01 emerge as the most Earth-like unconfirmed targets. T16 finds candidates at scale. ExoNet triages them for follow-up priority. Together they describe an astronomical community that can produce candidate planets much faster than it can confirm them.
The practical consequence is that the T16 catalog is a target list more than a planet list. The 11,554 candidates are signals. Some fraction are real planets. Most will sit as candidates indefinitely because there is not enough radial velocity telescope time to work through the queue. Doubling the catalog does not mean doubling the confirmed planets unless the confirmation infrastructure scales with it. It has not.
What the team has built is a planet-finding machine. What they have handed the community is a very long to-do list. Whether that list gets worked through in the next decade or the next generation depends on how many radial velocity telescopes the field is willing to build, buy, or borrow. As of now, that number has not changed.