Population-based identification of H{\alpha}-excess sources in the Gaia DR2 and IPHAS catalogues
M. Fratta (Durham University, Texas Tech University), S. Scaringi, (Durham University, Texas Tech University), J. E. Drew (University College, London), M. Monguio (Universitat de Barcelona, Universitat politecnica de, Catalunya), C. Knigge (University of Southampton)

TL;DR
This paper introduces a new Gaia-based method to identify Hα-excess sources in the Northern Galactic Plane, resulting in a catalogue of over 28,000 candidates with high confidence levels, aiding stellar population studies.
Contribution
The study develops a novel technique combining Gaia astrometry and photometry with IPHAS data to reliably detect Hα-bright outliers, reducing biases from stellar population mixing and extinction.
Findings
Identified 28,496 Hα-excess candidates with >3 significance.
Achieved a purity of 81.9% using a 5σ conservative cut.
Completeness of detection is between 3% and 5%.
Abstract
We present a catalogue of point-like H{\alpha}-excess sources in the Northern Galactic Plane. Our catalogue is created using a new technique that leverages astrometric and photomeric information from Gaia to select H{\alpha}-bright outliers in the INT Photometric H{\alpha} Survey of the Northern Galactic Plane (IPHAS), across the colour-absolute magnitude diagram. To mitigate the selection biases due to stellar population mixing and to extinction, the investigated objects are first partitioned with respect to their positions in the Gaia colour-absolute magnitude space, and in the Galactic coordinates space, respectively. The selection is then performed on both partition types independently. Two significance parameters are assigned to each target, one for each partition type. These represent a quantitative degree of confidence that the given source is a reliable H{\alpha}-excess…
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