Gaia data processing. SEAPipe: The source environment analysis pipeline
D. L. Harrison (1, 2), F. van Leeuwen (1), P. J. Osborne (1), P. W., Burgess (1), F. De Angeli (1), D. W. Evans (1) ((1) Institute of Astronomy,, Cambridge, (2) Kavli Institute for Cosmology, Cambridge)

TL;DR
This paper presents SEAPipe, a pipeline for Gaia data that detects new sources near known ones, comparing two methods and showing the image-subtraction approach is superior in performance.
Contribution
The paper introduces two options for the Gaia Source Environment Analysis pipeline, detailing their algorithms and performance, with the image-subtraction method outperforming the vanilla approach.
Findings
Image-subtraction pipeline has higher completeness and purity.
Performance metrics depend on source magnitude and separation.
The pipeline effectively identifies secondary sources near Gaia primaries.
Abstract
Aims. To describe two potential options for the Source Environment Analysis pipeline, SEAPipe, for the Gaia mission. This pipeline will enable the discovery of sources which are new to Gaia, in the sense that they were not found by the on-board detection algorithm. These additional sources (secondaries) are discoverable in the vicinity of those Gaia sources (primaries) that were found by the on-board detection. Methods. The main algorithmic steps required are described; the 2-dimensional image reconstruction of 1-dimensional transit data, the analysis of these images to find the additional sources present, and the determination of the mean positions, proper motions, parallaxes and brightness of these sources. Additionally, the Monte Carlo simulations used to characterise the performance of the pipelines are described. Results. The performance of the two options for SEAPipe, the…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Solar and Space Plasma Dynamics · Geophysics and Gravity Measurements
