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Record W1635080848

Segmentation and Detection of Extended Structures in Low Frequency Astronomical Surveys using Hybrid Wavelet Decomposition

2011· article· en· W1635080848 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

aboutThe title or abstract carries a Canadian signal from the geographic lexicon.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Bibliographic record

VenueASPC · 2011
Typearticle
Languageen
FieldChemistry
TopicSpectroscopy and Chemometric Analyses
Canadian institutionsnot available
Fundersnot available
KeywordsArtificial intelligenceSegmentationWaveletBrightnessComputer scienceComputer visionGalactic planePattern recognition (psychology)PhysicsAstronomy
DOInot available

Abstract

fetched live from OpenAlex

The morphological complexity of extended real structures (such as SNRs, HII regions, bow shocks, etc.), and their wide variety in scale and surface brightness make their automatic detection and segmentation in large surveys a difficult task. We propose in this paper a segmentation method based on applying wavelet decomposition in the residual thresholded images. This strategy avoids the artifacts produced by strong sources in a straight wavelet decomposition. Our method successfully segments extended structures at different scales and therefore is suitable for further morphological analysis and object recognition processes. Results using images from radio and infrared wavelengths surveys show the validity of our approach. 1. Motivation and Objectives Large surveys reveal thousands of low spatial frequency objects, shown at different intensity scales. When imaging rich areas in the interstellar medium, many of the compact sources overlap with objects associated to extended, morphologically complex real structures, such as SNRs, HII regions, bow shocks, etc. The wide variety in spacial scale and surface brightness of these objects make their automatic detection and segmentation a difficult task. To illustrate these facts, we use in this paper the image corresponding to the high galactic longitude end of the Phase I Canadian Galactic Plane Survey (CGPS hereafter, see Taylor et al. 2003). Figure 1 shows, on the top, the image composition corresponding to mosaics V1, V2, W1, W2, X1, X2, Y1 and Y2 of the CGPS 1420 MHz, continuum. We have eliminated 0.1% of the intensity outliers in order to visualize some dozens of sources. Nevertheless, the data corresponding to these mosaics contain thousands of objects, as it is illustrated when we display the sub-image contained in the red square at different intensity scales. On the bottom left of the figure we show the sub-image with 2% of the outliers eliminated, whereas on the right 5% of them have been removed. In addition to a great number of compact sources, several extended structures and their surrounding emission have appeared (the zoomed area contains Lynds Bright Nebula 679). In previous work we focused our attention on the performance of techniques suitable for the detection of faint compact objects (see for example Peracaula et al. 2008). In the present work we focus on the automatic detection of extended and irregular structures for further cataloguing and morphological analysis. In this context, wavelet image decomposition has been proven as a tool that can detect and separate objects represented at different spatial frequencies. However, the high dynamic range in intensity of this kind of image diminishes the performance

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.

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: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.131
Threshold uncertainty score0.397

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 communication0.0000.000
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 head0.022
GPT teacher head0.279
Teacher spread0.257 · 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