The standard screen size market is so big that every year there are enough people looking for an upgrade. Apart from enthusiasts or the fashion-minded, most people upgrade every 2-3 years.
"Opus 4.6 often thinks more deeply and more carefully revisits its reasoning before settling on an answer. This produces better results on harder problems, but can add cost and latency on simpler ones. If you’re finding that the model is overthinking on a given task, we recommend dialing effort down from its default setting (high) to medium."[1]
Yeah, I think the company that opens up a bit of the black box and open sources it, making it easy for people to customize it, will win many customers. People will already live within micro-ecosystems before other companies can follow.
Currently everybody is trying to use the same swiss army knife, but some use it for carving wood and some are trying to make some sushi. It seems obvious that it's gonna lead to disappointment for some.
Models are become a commodity and what they build around them seem to be the main part of the product. It needs some API.
I agree that if there was more transparency it might have prevented the token spend concerns, which feels caused by a lack of knowledge about how the models work.
If you're familiar with the technical specs, I'd be interested in hearing what size of objects the star trackers can sense and at what range. In theory the fancier star trackers can see objects around 10 cm diameter hundreds of kilometers away, without needing to worry about a pesky atmosphere [1], but I don't know how sensitive the sensors on Starlink's current generation satellites are, and this web site isn't saying.
They're mostly touting the improvement in latency over existing tracking, from delays measured in hours to ones measured in minutes. Which is very nice, of course, but the lack of other technical detail is mildly frustrating.
Note from analysis in the paper: (CST = Commercial Star Tracker, for which they model several common ones flown on satellites)
>From Fig. 1, it is clear that many typical CSTs can be used to detect debris with characteristic length less than
10 cm at distances as far as roughly 50 km. These same sensors have the potential to detect debris as small as 1 cm
in diameter as far as 5 km away. Even space-limited CubeSats using nanosatellite-class CSTs can detect 10-cm-class
debris at roughly 25 km away or 1-cm-class debris at a distance of 2.5 km. Higher-performing imagers like the MOST
telescope can further characterize orbital debris of 10 cm diameter as far as 400 km away or be used to characterize
orbital debris smaller than 1 cm at ranges not exceeding 40 km.
"The gpt-audio model is our first generally available audio model. It accepts audio inputs and outputs, and can be used in the Chat Completions REST API."
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