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Table 4.
Estimates of M★, Mdust and SFR for NGC 3521 for the distance D0 = 10.7 Mpc.
| Authors, spectral range / software / original values | log M★ | log Mdust | logSFR |
|---|---|---|---|
| Skibba et al. (2011): log M★ from g − i colors and H-band luminosity using Zibetti et al. (2009); | 10.65 | – | 0.46 |
| logSFR from Hα+24 μm (Sect. 4.4.1). D = 9.2 Mpc, log M★ = 10.52, logSFR = 0.33 | |||
| Hunt et al. (2019) FUV to sub-mm (0.1–1000 μm); multi-code SED fitting (CIGALE, GRASIL, | 10.64 | 7.89 | 0.24 |
| MAGPHYS), D = 11.2 Mpc, log M★ = 10.68, log Mdust = 7.93, logSFR = 0.28 | |||
| Erroz-Ferrer et al. (2019) optical IFS (MUSE) + ancillary UV–IR SEDs (MAD project), D = 14.2 Mpc, | 10.90 | – | 0.22 |
| log M★ = 11.15, logSFR = 0.47 | |||
| Chang et al. (2020) IR to sub-mm (Herschel+JCMT; global cold-dust properties), D = 7.9 Mpc, | – | 7.91 | – |
| log Mdust = 7.65 | |||
| Pastoven et al. (2024) 135 nm to 21 cm (UV to radio), CIGALE (model A), D = 10.7 Mpc | 10.33 | 7.93 | 0.25 |
| This work, Model 1 (Appendix C) UV to radio cm, CIGALE+radio module, D = 10.7 Mpc | 10.76 | 7.99 | 0.29 |
| This work, Model 2, UV to radio decameter, CIGALE+radio_extra module, D = 10.7 Mpc | 10.78 | 8.12 | 0.22 |
Notes. A precise spectrophotometry of the SN 2024aecx event, which was recently recorded (Stevance et al. 2024) and classified as a type IIb SN (Andrews et al. 2024), allowed Xi et al. (2026) to define the distance to NGC 3521 as 11.3 ±1.1 Mpc.
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