[mbs-0021] SAT beams
まだ誰も着手していません。
評価
- 難易度
- 5/5
- 見積もり時間
- 1週間以上
- 初心者へのやさしさ
- 25/100
- issue の種類
- 機能追加
- 明瞭さ
- 説明が足りない
- 活発さ
- 活発
- 領域
- data
調査の方向性
Start with the issue's two beam-product options and inspect the listed products under /scratch/gpfs/SIMONSOBS/sat-iso/beams/planets/. Read the SO Wiki “Beams Metadata Version Log” and follow up on the broken strictly-SCR5 link. Done means deciding which granularity and normalization the simulations should use, then recording that decision in the project.
索引モデルが issue の本文から書いたものです。
説明
Context
We need to decide which SAT beam products to use in the map based simulations.
These are MEASUREMENTS, not simulations: the beams were measured on sky from radially binned planet maps (azimuthal symmetry of the beam assumed). The radial profile is obtained by fitting Bessel functions of the first kind to the beam core and a power-law wing to the tail, and the window functions come from numerical integration of the profiles (SO Wiki, "Beams Metadata Version Log").
Terminology
- SAT: Small Aperture Telescope. SO has three (satp1, satp2, satp3); beam products exist for satp1 and satp3.
- f090 / f150: frequency bands (~90 / ~150 GHz) of the SAT receivers.
- ws (wafer slot): position on the focal plane, 7 per SAT telescope (ws0..ws6).
- Beam radial profile: the measured beam brightness as a function of angle from the beam center (theta), assuming azimuthal symmetry.
- Window function W(ell): transfer function of the beam in harmonic space, by which the underlying sky is multiplied when simulating the observed map.
- solid angle (omega): integral of the beam over the sky, used to normalize.
- ell: multipole number (0..1999 in these products).
- SCR4 / SCR5: Site Cooldown Runs 4 and 5 (SAT-MF1 nomenclature), two successive observing campaigns of the SATs separated by cooldown/maintenance periods. Between them (around January 2025) the focal plane was reconfigured (detector retrofit / wafer swap): some wafers stayed, some were removed, some moved. SCR5 is the current configuration after the swap.
- Covariance matrices: estimates of the uncertainty of the window function, propagated from the measurement uncertainties (statistical, and from the core-to-wing transition and Bessel scaling parameters).
Two options (differ in granularity of the maps)
- Option 1 (per-frequency effective beams): 4 maps
one per telescope and frequency band: satp1_f090, satp1_f150, satp3_f090, satp3_f150 - Option 2 (per-wafer beams): 28 maps
one per telescope, band and wafer slot: satp1/satp3 x f090/f150 x ws0..ws6
Products live on Tiger3 under /scratch/gpfs/SIMONSOBS/sat-iso/beams/planets/ :
Option 1: per-frequency effective beams -> 4 maps
Directories:
- 20260521spline_effective_v4_paper_20260520_science/ (satp1)
- 20260521spline_effective_v4_paper_20260520_science_satp3/ (satp3)
Files: one beam window function per telescope and band, in two formats:
- satp1_science_v4_paper_f090.fits / .dat
- satp1_science_v4_paper_f150.fits / .dat
- satp3_science_v4_paper_f090.fits / .dat
- satp3_science_v4_paper_f150.fits / .dat
Contents: the effective beam window function W(ell) for the full telescope and band, combining all 7 wafer slots. .dat: two columns, ell and window function (ell = 0..1999). .fits: healpy table with the 2000 window function values. Normalized to 1 at ell = 0. This is the beam to use when the simulation produces one map per telescope and band (4 maps).
Option 2: per-wafer beams -> 28 maps
Directory:
- 20260602_bessel_analytic_cov/
Files: one npz per telescope, band and wafer slot: original_cov_fitted_peak_{telescope}{band}{ws}_bessel_analytic_cov.npz
Each npz contains:
- theta, profile: radial angle (arcmin) and peak-normalized radial beam profile
- Bl: window function, ell = 0..1999
- omega, sigma_omega: solid angle and its 1-sigma error
- analytic_cov_Bl: statistical ell-ell covariance matrix (bin = 1)
- theta1_cov_Bl: covariance from the core-to-wing transition location uncertainty
- lmax_cov_Bl: covariance from the Bessel scaling parameter uncertainty
- sigma_wn_fn_diag: diagonal 1-sigma error on the window function (the three covariance terms added in quadrature)
- fwhm: estimated FWHM (azimuthal symmetry assumed)
Window function to use: Bl^2 * (2*pi/omega)^2, normalized to 1 at ell = 0. This is the beam to use when the simulation produces one map per wafer slot (28 maps).
Other products in the same folder
- 20260602_bessel_analytic_cov_effective_v4_paper_20260520_science: per-frequency effective beams with a different (not normalized to 1 at ell = 0) normalization; only the satp3 _norm0 variants are normalized
- 20260521spline: per-wafer spline window functions (ell, wn_fn), not normalized to 1 at ell = 0, one wafer-slot file missing
Note from the wiki (Beams Metadata Version Log)
The 20260602 products combine beams measured during SCR4 and SCR5, so profiles are mixed between wafers that remained on the focal plane, those removed after SCR4, and those that moved. No large focal plane variation is seen in the profiles, but use with caution; a strictly-SCR5 product exists (the link in the wiki is broken, to follow up with the beam team). The metadata format is for analysis (post-processing of TODs) and may change.
- 主要言語
- Jupyter Notebook
- スター
- 6
- フォーク
- 3
- PR マージ指標
- 30日以内にマージされた PR はありません
環境構築
このプロジェクトには開発コンテナ、Dockerfile、コントリビューションガイドがありません。まず README を読み、一般的な手順ははじめてのコントリビューションガイドを参照してください。
はじめの一歩
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simonsobs/map_based_simulations のほかの issue
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難易度 4/5 3〜5日 初心者へのやさしさ 50/100
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難易度 3/5 1〜2日 初心者へのやさしさ 25/100
simonsobs/map_based_simulations#38 · コメント 1 件 ·
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Write SO map based simulations paper再び着手できるかも @zonca が 2554 日前に担当しましたが、オープン中のプルリクエストはありません。 オープン
simonsobs/map_based_simulations#25 · コメント 9 件 · 担当者 1 名 ·
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