SEVEN-YEAR <i>WILKINSON MICROWAVE ANISOTROPY PROBE</i> ( <i>WMAP</i> ) OBSERVATIONS: GALACTIC FOREGROUND EMISSION
Bibliographic record
Abstract
We present updated estimates of Galactic foreground emission using seven years of WMAP data. Using the power \nspectrum of differences between multi-frequency template-cleaned maps, we find no evidence for foreground \ncontamination outside of the updated (KQ85y7) foreground mask.We place a 15μK upper bound on rms foreground \ncontamination in the cleaned maps used for cosmological analysis. Further, the cleaning process requires only three \npower-law foregrounds outside of the mask. We find no evidence for polarized foregrounds beyond those from soft \n(steep-spectrum) synchrotron and thermal dust emission; in particular we find no indication in the polarization data \nof an extra “haze” of hard synchrotron emission from energetic electrons near the Galactic center. We provide an \nupdated map of the cosmic microwave background (CMB) using the internal linear combination method, updated \nforeground masks, and updates to point source catalogs using two different techniques. With additional years of \ndata, we now detect 471 point sources using a five-band technique and 417 sources using a three-band CMB-free \ntechnique. In total there are 62 newly detected point sources, a 12% increase over the five-year release. Also new \nare tests of theMarkov chain Monte Carlo foreground fitting procedure against systematics in the time-stream data, \nand tests against the observed beam asymmetry. Within a few degrees of the Galactic plane, the behavior in total \nintensity of low-frequency foregrounds is complicated and not completely understood. WMAP data show a rapidly \nsteepening spectrum from 20 to 40 GHz, which may be due to emission from spinning dust grains, steepening \nsynchrotron, or other effects. Comparisons are made to a 1 deg 408 MHz map (Haslam et al.) and the 11 deg \nARCADE 2 data (Singal et al.).We find that spinning dust or steepening synchrotron models fit the combination of \nWMAP and 408 MHz data equally well. ARCADE data appear inconsistent with the steepening synchrotron model \nand consistent with the spinning dust model, though some discrepancies remain regarding the relative strength \nof spinning dust emission. More high-resolution data in the 10–40 GHz range would shed much light on these \nissues.
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How this classification was reachedexpand
Full frame machine prediction
Teacher imitationNot calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.
Distilled classifier scores by category (both heads)
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.001 | 0.002 |
| Meta-epidemiology (narrow) | 0.001 | 0.000 |
| Meta-epidemiology (broad) | 0.000 | 0.001 |
| Bibliometrics | 0.003 | 0.003 |
| Science and technology studies | 0.000 | 0.000 |
| Scholarly communication | 0.001 | 0.001 |
| Open science | 0.001 | 0.001 |
| Research integrity | 0.000 | 0.001 |
| Insufficient payload (model declined to judge) | 0.003 | 0.002 |
Machine scores (provisional)
The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.
Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from itClassification
machine, unvalidatedMachine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.
How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".