The VVV near-IR galaxy catalogue beyond the Galactic disc

Author:

Baravalle Laura D1,Alonso María Victoria12,Minniti Dante345,Nilo Castellón José Luis67,Soto Mario8,Valotto Carlos12,Villalón Carolina1,Graña Darío1,Amôres Eduardo B9,Milla Castro Fernanda6

Affiliation:

1. Instituto de Astronomía Teórica y Experimental (IATE, CONICET-UNC), Laprida 854, Córdoba, X5000BGR, Argentina

2. Observatorio Astronómico de Córdoba, Universidad Nacional de Córdoba, Córdoba, X5000BGR, Argentina

3. Departamento de Física, Facultad de Ciencias Exactas, Universidad Andrés Bello, Av. Fernandez Concha 700, Las Condes, Santiago, Chile

4. Instituto Milenio de Astrofísica, Santiago, 7500912, Chile

5. Vatican Observatory, V-00120 Vatican City State, Italy

6. Departamento de Física y Astronomía, Facultad de Ciencias, Universidad de La Serena, Av. Juan Cisternas 1200 Norte, La Serena, Chile

7. Instituto de Investigación Multidisciplinario en Ciencia y Tecnología, Universidad de La Serena. Av. Juan Cisternas 1400, La Serena, Chile

8. Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama, Copayapu 485, Copiapó, Chile

9. Departamento de Física, Universidade Estadual de Feira de Santana (UEFS), Av. Trans. S/N, CEP 44036-900 Feira de Santana, BA, Brazil

Abstract

ABSTRACT Knowledge about the large-scale distribution of galaxies is far from complete in the Zone of Avoidance (ZoA), which is mostly due to high interstellar extinction and to source confusion at lower Galactic latitudes. Past near-infrared (NIR) surveys, such as the Two Micron All Sky Survey (2MASS), have shown the power of probing large-scale structure at these latitudes. Our aim is to map the galaxy distribution across the Southern Galactic plane using the VISTA Variables in the Vía Láctea Survey (VVV), which reach 2–4 mag deeper than 2MASS. We used SExtractor+PSFEx to identify extended objects and to measure their sizes, the light concentration index, magnitudes, and colours. Morphological and colour constraints and visual inspection were used to confirm galaxies. We present the resulting VVV NIR Galaxy Catalogue (VVV NIRGC) of 5563 visually confirmed galaxies, of which only 45 were previously known. This is the largest catalogue of galaxies towards the Galactic plane, with 99 per cent of these galaxies being new discoveries. We found that the galaxy density distribution closely resembled the distribution of low interstellar extinction of the existing NIR maps. We also present a description of the 185 2MASS extended sources observed in the region, of which 16 per cent of these objects had no previous description, which we have now classified. We conclude that interstellar extinction and stellar density are the main limitations for the detection of background galaxies in the ZoA. The VVV NIRGC is a new data set providing information for extragalactic studies in the Galactic plane.

Funder

Consejo Nacional de Investigaciones Científicas y Técnicas

Secretaría de Ciencia y Técnica, Universidad Nacional de Río Cuarto

European School of Oncology

Centro de Astrofísica y Tecnologías Afines

Fondo Nacional de Desarrollo Científico y Tecnológico

National Aeronautics and Space Administration

California Institute of Technology

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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