Published October 30, 2023
| Version 1
Dataset
Open
Observational Bias and Young Massive Cluster Characterisation II. Can Gaia accurately observe young clusters and associations?
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1.
University of Exeter
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2.
University of Geneva
Description
Field-of-View for synthetic Gaia observations of clusters Orion-type-3, Orion-type-5.5 and Wd2-type presented in Buckner et al. (2023).
Files contain both simulation and field stars along the Line-of-Sight (l = 270^o, b = 0^o) for the clusters when placed at 500pc, 2500pc and 4300pc distances.
The original simulation files are included for reference.
Included README files provide more detailed descriptions of the files.
Files
Orion_3MYR_FoV_2500pc.csv
Files
(4.6 GB)
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md5:77231b5e9607f4e91b39981476b12624
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md5:218441b4463f5fd6f2b796222677a3cc
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md5:2e744001776a652bcebac5c85a315cbf
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md5:65bdd5e5647efb88ebf18d98a115763f
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md5:201cf7dc35d7e79519286aa70f589d8d
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5.4 MB | Preview Download |
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md5:81d854608cffcc2ed54b294022976eda
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md5:8948d49a11007eb5135154e12ec0fc7b
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386.5 kB | Preview Download |
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md5:a2d21959b83015fdb9191ed683d31890
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626 Bytes | Preview Download |
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md5:91afc270d730a9c56037f3ea9dba5c57
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449 Bytes | Preview Download |
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md5:4b1ccc2191c255c681820234b340c23f
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59.9 MB | Preview Download |
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md5:59acf36242575de8f41691d6c9878653
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21.5 MB | Preview Download |
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md5:b225ab45a0ffed7bea3906288829585f
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3.0 GB | Preview Download |
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md5:64839d48da74c99a3e1bc331780b128b
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4.5 MB | Preview Download |
Additional details
Related works
- Is described by
- Publication: Buckner et al. (2023) (Other)
Funding
Dates
- Available
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2023-10-30
References
- Cluster simulations (sink form) taken from Dobbs et al. (2022).