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Planetary nebulae and how to find them: Color identification in big broadband surveys

TitlePlanetary nebulae and how to find them: Color identification in big broadband surveys
Publication TypeJournal Article
Year of Publication2019
AuthorsVejar G., Montez R., Morris M., Stassun K.G
Volume879
Date Published2019/07
Type of ArticleArticle
ISBN Number0004-637X
Accession NumberWOS:000473696200004
KeywordsAstronomy & Astrophysics; chemical abundances; evolution; galactic plane; h-alpha survey; halo; kinematics; origin; photometric; planetary nebulae: general; population; release; stars: evolution; Surveys; symbiotic stars; techniques:
Abstract

Planetary nebulae (PNe) provide tests of stellar evolution, can serve as tracers of chemical evolution in the Milky Way and other galaxies, and are also used as calibrators of the cosmological distance ladder. Current and upcoming large-scale photometric surveys have the potential to complete the census of PNe in our galaxy and beyond, but it is a challenge to disambiguate partially or fully unresolved PNe from the myriad other sources observed in these surveys. Here we carry out synthetic observations of nebular models to determine ugrizy color-color spaces that can successfully identify PNe among billions of other sources. As a primary result we present a grid of synthetic absolute magnitudes for PNe at various stages of their evolution, and we make comparisons with real PNe colors from the Sloan Digital Sky Survey. We find that the r - i versus g - r, and the r - i versus u - g, color-color diagrams show the greatest promise for cleanly separating PNe from stars, background galaxies, and quasars. Finally, we consider the potential harvest of PNe from upcoming large surveys. For example, for typical progenitor host star masses of similar to 3 M-circle dot, we find that the Large Synoptic Survey Telescope (LSST) should be sensitive to virtually all PNe in the Magellanic Clouds with extinction up to AV of similar to 5 mag; out to the distance of Andromeda, LSST would be sensitive to the youngest PNe (age less than similar to 6800 yr) and with AV up to 1 mag.

DOI10.3847/1538-4357/ab21ba
Student Publication: 
No