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ApJS · 21 HR AGO
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New Tool Makes Star Speed Measurements Twice as Accurate

By Space.Fan Editorial Desk

Scientists created a better way to clean up data from a major space survey, making it easier to track how stars move across our galaxy.

The Milky Way galaxy arching over mountains on Earth.
Image · Space.Fan

The Drop

Astronomers use something called radial velocity to figure out how fast s are moving toward or away from us. Think of it like measuring the pitch of a siren to know if an ambulance is coming closer or driving away. To get this data, scientists use the LAMOST telescope. It looks at millions of s by taking pictures of their light and splitting it into a rainbow-like spectrum. However, the telescope system has many parts. Because it uses different cameras, fibers, and exposure times, the data often had tiny errors. These errors made it hard to compare measurements taken at different times or by different parts of the machine. The researchers had to figure out how to balance these settings so all the measurements would match up. To fix this, the team looked at data from two other trusted sources: the Gaia and APOGEE missions. By comparing the LAMOST results to these gold-standard measurements, they created a two-step correction method. This acts like a filter to remove the accidental noise caused by the telescope equipment. After applying this new correction, the measurements became much more consistent. The team found that their data became about two times more precise than it was before. They have now shared a huge catalog containing over 11 million speed measurements that are ready for other scientists to use.
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Why It Matters

This improvement is a big deal because it lets astronomers study the movement of the Milky Way with much more detail. When researchers try to map our galaxy, they need to know exactly how s are racing through space. Even small errors in speed measurements can lead to wrong conclusions about where s come from or how they are grouped together. By cleaning up this massive set of data, scientists can now spot subtle patterns in stellar motion that were previously hidden by technical noise. This helps us build a much clearer picture of how our galaxy is put together and how it has changed over time.
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The Catch

This method relies on comparing LAMOST data to other existing catalogs. If those reference catalogs, like Gaia or APOGEE, have their own hidden biases or errors, those issues could potentially carry over into this new dataset. While the correction makes the LAMOST data much more consistent with other surveys, it does not mean the measurements are perfect or free from all physical limitations.

Put That in Perspective

Scientists have spent years gathering these millions of spectra, and this update turns that raw effort into a high-quality tool. Future researchers will likely use this corrected catalog to trace the paths of stars more accurately as they move in their giant orbits around the center of the Milky Way.

Source September 27, 2026
Jinming Zhang and Haibo Yuan
Beijing Normal University·The Astrophysical Journal Supplement Series·10.3847/1538-4365/ae985e

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