HSC 1547

0.09 UTI

0.0

C_N

0.65

C_dens

0.38

C_C3

0.0

C_lit

0.44

C_dup

C3 classification CB

Number of members (P>50%) 20

Radius (P>50% members) 1.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.65 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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HSC 1547 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a large^* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~5.01 kpc) differs significantly from the median photometric distance (~8.78 kpc).

Very distant High extinction Massive Young

Data

🔍 Search references for HSC 1547 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	94.709	15.283	0.2	0.073	-0.401	–
Hunt & Reffert	2024	94.686	15.289	0.106	0.076	-0.452	–
Hunt & Reffert	2023	94.686	15.289	0.106	0.076	-0.452	–

💡 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]	Bfr	BSS
Hunt & Reffert	2024	–	–	–	–	–	1152*	–	–
Hunt & Reffert	2023	8.78	3.01	1.42	69	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 438	56.0	94.82	15.29	0.21	0.14	-0.41	32.2	0.51

💡 Note: The % column shows the percentage of members that HSC 1547 shares with each listed object.

Visualization

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