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Table 1.
Distributions of stellar mass (log M*, M⊙).
| HRS late-type | VCM | Field | H I-deficient | H I-normal | RPS | |
|---|---|---|---|---|---|---|
| (258) | (108) | (148) | (85) | (167) | (72) | |
| Min. | 8.46 | 8.56 | 8.46 | 8.53 | 8.46 | 7.39 |
| 1st Q. | 9.14 | 9.25 | 9.10 | 9.30 | 9.11 | 9.18 |
| Median | 9.49 | 9.60 | 9.46 | 9.69 | 9.42 | 9.48 |
| 3rd Q. | 9.98 | 10.14 | 9.88 | 10.14 | 9.88 | 10.08 |
| Max. | 11.12 | 11.00 | 11.12 | 11.00 | 11.12 | 11.34 |
Notes. The HRS sample is split into environmental classifications (see Section 2.1). The number of objects is given in parentheses. We excluded NGC4305 (HRS 116) and NGC4720 (HRS 265) because they lack W4 and W1 WISE band data, respectively.
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