Magellan IMACS color-magnitude diagram for Tucana B

David J Sand (Creator)
Burçin Mutlu-Pakdil (Creator)
Michael G. Jones (Creator)
A. Karunakaran (Creator)
Feige Wang (Creator)
Jinyi Yang (Creator)
Anirudh Chiti (Creator)
P. Bennet (Creator)
D. Crnojević (Contributor)
K. Spekkens (Creator)

Dataset

Description

VizieR online Data Catalogue associated with article published in journal Astrophysical Journal with title ' Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at.' (bibcode: 2022ApJ...935L..17S)

Date made available	2024
Publisher	Centre de Donnees Strasbourg (CDS)

DOI
10.26093/cds/vizier.19359017

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Refer to CDS usage

Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at D ≈ 1.4 Mpc* * This paper includes data gathered with the 6.5 m Magellan Telescope at Las Campanas Observatory, Chile.
Sand, D. J., Mutlu-Pakdil, B., Jones, M. G., Karunakaran, A., Wang, F., Yang, J., Chiti, A., Bennet, P., Crnojević, D. & Spekkens, K., Aug 1 2022, In: Astrophysical Journal Letters. 935, 1, L17.
Research output: Contribution to journal › Article › peer-review

Open Access
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Magellan IMACS color-magnitude diagram for Tucana B

Description

DOI

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Research output

Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at D ≈ 1.4 Mpc* * This paper includes data gathered with the 6.5 m Magellan Telescope at Las Campanas Observatory, Chile.

Cite this