Table 2.

A summary of the properties of our Perseus UDG sample. Columns from left to right are as follows: 1) Designation used throughout this work; 2) Signal-to-noise ratio on the continuum; 3) UDG recessional velocity; 4) UDG velocity dispersion and 5) Dynamical mass within 3D, circularized half-light radius. Kinematic properties are measured from the KCWI spectra described in Section 3. When relevant, uncertainties are given in (brackets) after values.

NameS/NVrσM(< R1/2)
PUDG_−1][km s−1][km s−1][×108 M]
R16124679 (2)12 (3)4.70 (2.41)
R15154762 (2)10 (4)2.25 (1.82)
R24147784 (4)20 (5)11.9 (6.19)
R84184039 (2)19 (3)6.74 (2.16)
S74166215 (2)22 (2)16.0 (3.03)
NameS/NVrσM(< R1/2)
PUDG_−1][km s−1][km s−1][×108 M]
R16124679 (2)12 (3)4.70 (2.41)
R15154762 (2)10 (4)2.25 (1.82)
R24147784 (4)20 (5)11.9 (6.19)
R84184039 (2)19 (3)6.74 (2.16)
S74166215 (2)22 (2)16.0 (3.03)
Table 2.

A summary of the properties of our Perseus UDG sample. Columns from left to right are as follows: 1) Designation used throughout this work; 2) Signal-to-noise ratio on the continuum; 3) UDG recessional velocity; 4) UDG velocity dispersion and 5) Dynamical mass within 3D, circularized half-light radius. Kinematic properties are measured from the KCWI spectra described in Section 3. When relevant, uncertainties are given in (brackets) after values.

NameS/NVrσM(< R1/2)
PUDG_−1][km s−1][km s−1][×108 M]
R16124679 (2)12 (3)4.70 (2.41)
R15154762 (2)10 (4)2.25 (1.82)
R24147784 (4)20 (5)11.9 (6.19)
R84184039 (2)19 (3)6.74 (2.16)
S74166215 (2)22 (2)16.0 (3.03)
NameS/NVrσM(< R1/2)
PUDG_−1][km s−1][km s−1][×108 M]
R16124679 (2)12 (3)4.70 (2.41)
R15154762 (2)10 (4)2.25 (1.82)
R24147784 (4)20 (5)11.9 (6.19)
R84184039 (2)19 (3)6.74 (2.16)
S74166215 (2)22 (2)16.0 (3.03)
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