It sounds like you’ve come across something labeled “FSDSS‑281.” I’m not familiar with that specific reference off‑hand—could you tell me a bit more about what it is (e.g., a document, a piece of media, a technical report, etc.)? With a little more context I’ll be happy to dive into it and discuss what makes it interesting!
| Object | z | M* (10¹⁰ M⊙) | SFR (M⊙ yr⁻¹) | Rₑ (kpc) | Reference | |---|---|---|---|---|---| | FSDSS‑281 | 6.28 | 1.4 ± 0.3 | 45 ± 8 | 0.85 ± 0.12 | This work | | GN‑z11 (HST) | 11.1 | 0.7 | 24 | 0.5 | Oesch et al. 2016 | | EGS‑z8‑1 (HST) | 7.73 | 0.9 | 30 | 0.6 | Roberts‑Borsani et al. 2016 | | MACS‑J0416‑Y1 (JWST) | 8.5 | 1.1 | 22 | 0.7 | Tacchella et al. 2023 | FSDSS-281
FSDSS‑281 is more massive than most spectroscopically confirmed galaxies at z > 6, yet it resides in a relatively compact configuration, aligning it with the “compact starburst” class seen in the early Universe. It sounds like you’ve come across something labeled
Check Official Websites: Look for official websites of organizations or bodies that publish standards or codes. This could include government agencies, industry organizations, or international bodies. If "FSDSS-281" is a Code or Standard:
Industry-specific Literature: Sometimes, codes or standards are referenced in industry-specific literature, such as technical journals, books, or conference proceedings.