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Record W1968727606 · doi:10.1051/0004-6361:20065258

Archeops in-flight performance, data processing, and map making

2007· article· en· W1968727606 on OpenAlexaff
J. F. Macías–Pérez, G. Lagache, B. Maffei, K. Ganga, A. Bourrachot, P. A. R. Ade, A. Amblard, R. Ansari, É. Aubourg, J. Aumont, S. Bargot, J. G. Bartlett, A. Benoı̂t, J.-P. Bernard, R. Bhatia, Alain Blanchard, J. J. Bock, A. Boscaleri, F. R. Bouchet, P. Camus, J.-F. Cardoso, F. Couchot, P. de Bernardis, F.–X. Désert, O. Doré, M. Douspis, L. Dumoulin, X. Dupac, P. Filliatre, P. Fosalba, F. Gannaway, Brice Gautier, M. Giard, Y. Giraud–Héraud, R. Gispert, L. Guglielmi, J.–Ch. Hamilton, Shaul Hanany, S. Henrot–Versillé, V. V. Hristov, J. Kaplan, J.–M. Lamarre, A. E. Lange, K. Madet, Ch. Magneville, Daniel P. Marrone, S. Masi, F. Mayet, J. A. Murphy, F. Naraghi, F. Nati, G. Patanchon, O. Perdereau, G. Perrin, S. Plaszczynski, M. Piat, N. Ponthieu, S. Prunet, J.‐L. Puget, C. Renault, C. Rosset, D. Santos, Alexei A. Starobinsky, I. A. Strukov, R. Sudiwala, Romain Teyssier, M. Tristram, C. Tucker, Jean‐Charles Vanel, D. Vibert, E. Wakui, D. Yvon

Bibliographic record

VenueAstronomy and Astrophysics · 2007
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsUniversity of British ColumbiaUniversity of Toronto
FundersCentre National d’Etudes Spatiales
KeywordsCosmic microwave backgroundSkyPhysicsBolometerPlanckAngular resolution (graph drawing)AstrophysicsAstronomyAnisotropyRemote sensingSatelliteMeasure (data warehouse)OpticsDetectorGeologyComputer science

Abstract

fetched live from OpenAlex

Aims. Archeops is a balloon-borne experiment inspired by the Planck satellite and its high frequency instrument (HFI). It is designed to measure the cosmic microwave background (CMB) temperature anisotropies at high angular resolution (12 arcmin) over a large fraction of the sky (around 30%) at 143, 217, 353, and 545 GHz. The Archeops 353 GHz channel consists of three pairs of polarized sensitive bolometers designed to detect the polarized diffuse emission of Galactic dust. Methods. In this paper we present an update of the instrumental setup, as well as the flight performance for the last Archeops flight campaign (February 2002 from Kiruna, Sweden). We also describe the processing and analysis of the Archeops time-ordered data for that campaign, which led to measurement of the CMB anisotropy power spectrum in the multipole range = 10-700 and to the first measurements of both the polarized emission of dust at large angular scales and its power spectra in the multipole range = 3-70 Results. We present maps covering approximately 30% of the sky. These maps contain Galactic emission, including the Galactic plane, in the four Archeops channels at 143, 217, 353, and 545 GHz and CMB anisotropies at 143 and 217 GHz. These are one of the first sub-degree-resolution maps in the millimeter and submillimeter ranges of the large angular-scale diffuse Galactic dust emission and CMB temperature anisotropies, respectively.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.683
Threshold uncertainty score0.955

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.001
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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.

Opus teacher head0.017
GPT teacher head0.248
Teacher spread0.231 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

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".

Quick stats

Citations30
Published2007
Admission routes1
Has abstractyes

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