HSC 1353

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0.21 UTI
0.0
CN
0.21
Cdens
0.25
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.25 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1353 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 79.862 33.649 0.196 0.885 -0.015 -10.549
Hu & Soubiran 2025 79.846 33.648 – – – –
Zhang et al. 2024 79.858 33.641 – – – –
Hunt & Reffert 2024 79.858 33.641 0.208 0.894 -0.032 -6.925
Cavallo et al. 2024 79.846 33.648 0.208 – – –
Hunt & Reffert 2023 79.858 33.641 0.208 0.894 -0.032 -6.925

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 4.665 1.875 1.25 892 -0.290 277 – –
Hu & Soubiran 2025 – – – – -0.410(5) – – –
Zhang et al. 2024 – – – – -0.190(1) – – –
Hunt & Reffert 2024 – – – – – 277(1) – –
Cavallo et al. 2024 4.13 1.91 – 1023 -0.290 – – –
Hunt & Reffert 2023 5.20 1.84 1.25 760 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3415 92.0 79.87 33.65 0.2 0.88 -0.01 -10.55 0.03

💡 Note: The % column shows the percentage of members that HSC 1353 shares with each listed object.

Visualization

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