First deep images catalogue of extended IPHAS PNe

Author:

Sabin L1ORCID,Guerrero M A2ORCID,Ramos-Larios G3ORCID,Boumis P4ORCID,Zijlstra A A56ORCID,Awang Iskandar D N F7ORCID,Barlow M J8ORCID,Toalá J A9ORCID,Parker Q A10ORCID,Corradi R M L1112ORCID,Morris R A H13

Affiliation:

1. Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 106, Ensenada, B.C. 22800, Mexico

2. Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía S/N, Granada 18008, Spain

3. Instituto de Astronomía y Meteorología, CUCEI, Universidad de Guadalajara, Av. Vallarta 2602, Arcos Vallarta, Guadalajara 44130, Mexico

4. Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, National Observatory of Athens, Penteli, Athens 15236, Greece

5. Jodrell Bank Centre for Astrophysics, The University of Manchester, Oxford Road, Manchester M13 9PL, UK

6. Laboratory for Space Research, University of Hong Kong, Pokfulam Road, Hong Kong

7. Faculty of Computer Science and Information Technology, Universiti Malaysia Sarawak, Sarawak 94300, Malaysia

8. Department of Physics & Astronomy, University College London, Gower St, London WC1E 6BT, UK

9. Instituto de Radioastronomía y Astrofísica, UNAM, Campus Morelia, C.P. 58089, Morelia, Mexico

10. Department of Physics, The University of Hong Kong, Chong Yuet Ming Physics Building Pokfulam Road, Hong Kong

11. GRANTECAN, Cuesta de San José s/n, E-38712, Breña Baja, La Palma, Spain

12. Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain

13. School of Physics, Bristol University, Tyndall Avenue, Bristol, BS8 1TL, UK

Abstract

ABSTRACT We present the first instalment of a deep imaging catalogue containing 58 True, Likely, and Possible extended PNe detected with the Isaac Newton Telescope Photometric H α Survey (IPHAS). The three narrow-band filters in the emission lines of H α, [N ii] λ6584 Å, and [O iii] λ5007 Å used for this purpose allowed us to improve our description of the morphology and dimensions of the nebulae. In some cases even the nature of the source has been reassessed. We were then able to unveil new macro- and micro-structures, which will without a doubt contribute to a more accurate analysis of these PNe. It has been also possible to perform a primary classification of the targets based on their ionization level. A Deep Learning classification tool has also been tested. We expect that all the PNe from the IPHAS catalogue of new extended planetary nebulae will ultimately be part of this deep H α, [N ii], and [O iii] imaging catalogue.

Funder

FEDER

CONACYT

UNAM

STFC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Morphologies and Central Stars of Planetary Nebulae in the Galactic bulge from VLT, HST and Pan-STARRS imaging;Monthly Notices of the Royal Astronomical Society;2022-11-30

2. Interacting planetary nebulae III: verification and galactic population based on the measurements of Gaia EDR3;Astrophysics and Space Science;2022-06

3. Hot white dwarf candidates from the IGAPS-GALEX cross-match;Monthly Notices of the Royal Astronomical Society;2022-05-20

4. Exploitation of the IPHAS to Investigate Planetary Nebulae;Frontiers in Astronomy and Space Sciences;2022-05-10

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