我吃花盘旋
发表于 2025-3-27 00:54:00
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gerrymander
发表于 2025-3-27 05:06:52
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GRAZE
发表于 2025-3-27 05:21:28
On the Tolerances of Filters for GAIA Medium Band Photometric Systemosed for GAIA. We discuss the accuracy of the transformations to the standard photometric system and the precision of the determination of physical parameters for various types of stars using the 4-D classification procedure.
palliative-care
发表于 2025-3-27 10:21:21
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Expurgate
发表于 2025-3-27 13:43:14
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canvass
发表于 2025-3-27 20:49:44
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synchronous
发表于 2025-3-27 22:30:52
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极微小
发表于 2025-3-28 02:18:09
Japanese Astrometry Satellite Mission for Infrared Exploration13 and 2017 and will measure parallaxes and proper motions with the precision of 10 .as at . ≃ 12 – 15 mag. JASMINE will observe a few hundred million stars belonging to the disk and the bulge components of our Galaxy, which are hidden by the interstellar dust extinction in optical bands. Furthermor
clarify
发表于 2025-3-28 09:43:28
Methods to Account for Interstellar Extinctionr neighborhood. One may hope that the GAIA photometry itself will contribute color excesses for most of the studied objects, otherwise the extinction must be deduced from the external sources. 3-D galactic models where the dust distribution is an integral part seems to be a viable solution. Some sta
娘娘腔
发表于 2025-3-28 12:39:28
3-D Structure of the Galactic Interstellar Matter: A Contribution from GAIA simulations of the GAIA photometry, which are used to derive the distribution of interstellar matter in a modelled Galaxy. We find that’ small’ diffuse clouds (diameter . = 4 pc, E. = 0.06) will be easily traced with GAIA up to the distances of ~ 800 pc. ‘Large’ diffuse interstellar clouds (. = 10