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FLAMINGO precomputed matter and component power spectra (ASCII P(k), 123 redshift indices), units without h, and the FlamingoBaryonResponseEmulator. Use when loading FLAMINGO P(k), comparing to theory, or emulating baryonic suppression without full hydro.
用 Codex 或 Claude 帮你安装 复制这段 Prompt，粘贴到 Codex、Claude 或其他助手里，让它检查 Skill 页面并帮你完成安装。
基于 SOC 职业分类
Deep-read an academic paper and produce a durable, critical research note — not a loose summary. Use when given a paper title, DOI, arXiv ID, publisher/PDF/GitHub URL, or local PDF, or when asked to read closely, summarize, extract contributions, analyze experiments, critique, compare to related work, reproduce results, or maintain a paper-reading repository index. Works across fields (astro/physics, ML, bio, security, …); examples lean astro-ph but the workflow is general.
Remote, slice-level access to FLAMINGO HDF5 files on COSMA via the `hdfstream` Python module — no need to download whole snapshots. Covers install, server connection, navigation, dataset slicing, multi-slice batched reads, and integration with swiftsimio. Use when reading any FLAMINGO data product remotely.
FLAMINGO past-lightcone products: virtual observers, particle lightcones, HEALPix shell maps, integrated_maps, and halo lightcones. Use when building mock surveys, stacking Compton-y or lensing maps, or cross-correlating with observations.
Review code changes against requirements and quality standards before merge. Use when dispatching a review subagent, after major features, before merging, or when the user asks for a code review. Requires reading the actual diff.
Style and structure for research manuscript text: IMRaD, hourglass narrative, formal tone, topic sentences, reproducible Methods, captions that tell the story. Use when drafting or editing titles, abstracts, sections, captions, or reports.
Iterative VLM review of compiled LaTeX PDFs for layout clashes (text vs figures, tables, long equations). Use after the first compile or any float/equation edit; loop fix-recompile-recheck until no clashes remain.
| name | flamingo-power-spectra |
| description | FLAMINGO precomputed matter and component power spectra (ASCII P(k), 123 redshift indices), units without h, and the FlamingoBaryonResponseEmulator. Use when loading FLAMINGO P(k), comparing to theory, or emulating baryonic suppression without full hydro. |
Source of truth: Power spectra
Each simulation run directory contains ASCII text files under power_spectra/
(e.g. /FLAMINGO/L1_m9/L1_m9/power_spectra/).
Pattern: power_<type>_<index>.txt
0000–0122 — 123 output redshifts from z ≈ 30 down to 0 (full
table on the portal).Do not subtract shot noise again.
matter, cdm, gas, starBH, pressure (electron pressure P_e = n_e k_B T).
cdm-gas, cdm-neutrino, cdm-starBH, gas-matter, gas-neutrino,
gas-starBH, matter-pressure, starBH-neutrino, neutrino0-neutrino1
(neutrino cross used for shot-noise suppression).
pressure auto-spectrum, not gas density alone.Documented under Baryonic response emulator.
FlamingoBaryonResponseEmulator (pip; GitHub:
FLAMINGOproject/FlamingoBaryonResponseEmulator).Use paired hydro and _DMO runs when you need the full simulation P(k) rather than the emulator.
For loading examples, use the portal Python examples page rather than inventing parsers in chat.