photoD with Rubin’s Data Preview 1: First stellar photometric distances and faint blue star deficits
Aims. We investigate the utility of Rubin’s Data Preview 1 (DP1) for estimating stellar number density profiles across the Milky Way halo. Methods. We used stellar broad-band near-UV to near-IR ugrizy photometry released in Rubin’s DP1 to estimate distance and metallicity for blue main sequence star...
I tiakina i:
| Ngā kaituhi matua: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
EDP Sciences
2026-03-01
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| Rangatū: | Astronomy & Astrophysics |
| Ngā marau: | |
| Urunga tuihono: | https://www.aanda.org/articles/aa/full_html/2026/03/aa57219-25/aa57219-25.html |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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