tests:astropars:challenge2
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===== Objectives ===== | ===== Objectives ===== | ||
- | * Employ high-resolution spectra from X-shooter | + | * Employ high-resolution spectra from X-shooter |
* Investigate GSP-Phot performance on X-shooter spectra. | * Investigate GSP-Phot performance on X-shooter spectra. | ||
===== Comparison to RVS and BP/RP spectra ===== | ===== Comparison to RVS and BP/RP spectra ===== | ||
- | {{:tests:discs:vlos_helio_axisym.jpeg?200|}} | + | * Gaia RVS spectra and corresponding segments of x-shooter spectra look very similar. Ca-Triplet lines are easily identified and other prominent lines are also in obvious correspondence. |
+ | * x-shooter spectra contain telluric bands around 760nm and 950nm. In fact, BP/RP shows prominent dips there, which are NOT reflected by space-based instrument models. That must be a problem when modelling those spectra with GSP-Phot. | ||
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+ | {{:tests:compare-spectra.png|}} | ||
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+ | ===== GSP-Phot performance on x-shooter spectra ===== | ||
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+ | * Paula compiled mean parameters for all stars from Pastel. (These are no " | ||
+ | * Paula' | ||
+ | * GSP-Phot performs very poorly on x-shooter spectra: Teff is loosely related for some stars, but logg looks rather random and GSP-Phot tends to assign too low [Fe/H]. | ||
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+ | {{: | ||
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+ | == Possible explanations for poor GSP-Phot performance == | ||
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+ | * x-shooter spectra are ground-based spectra, including telluric features, that are not part of the Gaia spectra. | ||
+ | * Lack of giants in GSP-Phot training data. | ||
+ | * x-shooter spectra were processed with GOG version 14, whereas GSP-Phot training data was processed with GOG version 8. | ||
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+ | ===== Andy's SICK performance on x-shooter spectra ===== |
tests/astropars/challenge2.1414748670.txt.gz · Last modified: 2022/10/24 12:26 (external edit)