Identifying Galactic halo PN candidates in the imaging surveys: J-PLUS/S-PLUS and J-PAS

Gutiérrez-Soto, L.; Gonçalves, D. R.; Akras, S.; Cortesi, A.; Ederoclite, T.; Aparício-Villegas, T.; Borges-Fernandes, M.; Daflon, S.; Pereira, C. B.; Mendes de Oliveira, C.; Viironen, K.; J-PAS Collaboration
XV Latin American Regional IAU Meeting Cartagena 2016 (Eds. Mario Armando Higuera Garzón & Santiago Vargas Domínguez) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 49, pp. 162-162 (2017).


Halo planetary nebulae (HPNe) are able to reveal important information about stellar and chemical evolution in galaxies. Their characteristic low continuum and strong emission lines make them good objects to be searched by multi-filter imaging surveys. Given that only 14 HPNe are known in the Galaxy, we are exploring colour-colour diagrams to search for these sources in Javalambre/Southern Photometric Local Universe Survey (J-PLUS/S-PLUS) and the Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS). They are narrow- and broad-band imaging cosmological surveys, with 12 and 54 filters, respectively. The J-PAS survey will be able to observe 85002 of Northern sky, it will detect sources up to magnitude mAB˜23. In the case of the J-PLUS survey the limit magnitudes is around mAB˜21.5. The S-PLUS survey will observe more than 60002 and it will map the Southern sky. Other optical emission lines sources, such as Galactic and extragalactic symbiotic stars (SySts), cataclysmic variables (CVs), QSOs at different redshifts, star-forming galaxies (SFGs), extragalactic H II regions and supernova remnants (SNR) can mimic PNe. Therefore, we explore different colour-colour diagrams in order to highlight those that can better identify HPN candidates, separating them from these other objects.