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by lutusp 4802 days ago
Thanks for posting. I would have thought narrow lines would produce the problem that those specific lines would become unavailable for study, or would be freely mixed with the "real" data in confusing ways. It didn't occur to me that they could simply be subtracted in a deterministic way.

On that basis, I might have argued for high pressure sodium (to smear the lines) instead of low pressure, and I would have been quite wrong.

Given these issues, it's no wonder that a mountaintop in Hawaii, and another one in the Atacama desert, are now the preferred locations for optical astronomy.

1 comments

> Thanks for posting. I would have thought narrow lines would produce the problem that those specific lines would become unavailable for study, or would be freely mixed with the "real" data in confusing ways. It didn't occur to me that they could simply be subtracted in a deterministic way.

Your original thought is basically correct: we do lose the ability to do any meaningful work at the wavelengths of the lamp emission lines. But the damage is concentrated at a few wavelengths. So we trade having noise over the entire spectrum for a few really, really noisy pieces of spectrum. It's generally a excellent tradeoff.

But even low pressure sodium lamps have some emission spread over a large wavelength range, so it is becoming increasingly difficult to do optical work near major urban areas. In the long run most of those sites will probably transition to mostly IR work.