VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea

R. K. Saito; M. Hempel; D. Minniti; P. W. Lucas; M. Rejkuba; I. Toledo; O. A. Gonzalez; J. Alonso-García; M. J. Irwin; E. Gonzalez-Solares; S. T. Hodgkin; J. R. Lewis; N. Cross; V. D. Ivanov; E. Kerins; J. P. Emerson; M. Soto; E. B. Amôres; S. Gurovich; I. Dékány; R. Angeloni; J. C. Beamin; M. Catelan; N. Padilla; M. Zoccali; P. Pietrukowicz; C. Moni Bidin; F. Mauro; D. Geisler; S. L. Folkes; S. E. Sale; J. Borissova; R. Kurtev; A. V. Ahumada; M. V. Alonso; A. Adamson; J. I. Arias; R. M. Bandyopadhyay; R. H. Barbá; B. Barbuy; G. L. Baume; L. R. Bedin; A. Bellini; R. Benjamin; E. Bica; C. Bonatto; L. Bronfman; G. Carraro; A. N. Chenè; J. J. Clariá; J. R A Clarke; C. Contreras; A. Corvillón; R. De Grijs; B. Dias; J. E. Drew; C. Fariña; C. Feinstein; E. Fernández-Lajús; R. C. Gamen; W. Gieren; B. Goldman; C. González-Fernández; R. J J Grand; G. Gunthardt; N. C. Hambly; M. M. Hanson; K. G. Hełminiak; M. G. Hoare; L. Huckvale; A. Jordán; K. Kinemuchi; A. Longmore; M. López-Corredoira; T. MacCarone; D. Majaess; E. L. Martín; N. Masetti; R. E. Mennickent; I. F. Mirabel; L. Monaco; L. Morelli; V. Motta; T. Palma; M. C. Parisi; Q. Parker; F. Peñaloza; G. Pietrzyński; G. Pignata; B. Popescu; M. A. Read; A. Rojas; A. Roman-Lopes; M. T. Ruiz; I. Saviane; M. R. Schreiber; A. C. Schröder; S. Sharma; M. D. Smith; L. Sodré; J. Stead; A. W. Stephens; M. Tamura; C. Tappert; M. A. Thompson; E. Valenti; L. Vanzi; N. A. Walton; W. Weidmann; A. Zijlstra

doi:10.1051/0004-6361/201118407

VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea

R. K. Saito, M. Hempel, D. Minniti, P. W. Lucas, M. Rejkuba, I. Toledo, O. A. Gonzalez, J. Alonso-García, M. J. Irwin, E. Gonzalez-Solares, S. T. Hodgkin, J. R. Lewis, N. Cross, V. D. Ivanov, E. Kerins, J. P. Emerson, M. Soto, E. B. Amôres, S. Gurovich, I. DékányR. Angeloni, J. C. Beamin, M. Catelan, N. Padilla, M. Zoccali, P. Pietrukowicz, C. Moni Bidin, F. Mauro, D. Geisler, S. L. Folkes, S. E. Sale, J. Borissova, R. Kurtev, A. V. Ahumada, M. V. Alonso, A. Adamson, J. I. Arias, R. M. Bandyopadhyay, R. H. Barbá, B. Barbuy, G. L. Baume, L. R. Bedin, A. Bellini, R. Benjamin, E. Bica, C. Bonatto, L. Bronfman, G. Carraro, A. N. Chenè, J. J. Clariá, J. R A Clarke, C. Contreras, A. Corvillón, R. De Grijs, B. Dias, J. E. Drew, C. Fariña, C. Feinstein, E. Fernández-Lajús, R. C. Gamen, W. Gieren, B. Goldman, C. González-Fernández, R. J J Grand, G. Gunthardt, N. C. Hambly, M. M. Hanson, K. G. Hełminiak, M. G. Hoare, L. Huckvale, A. Jordán, K. Kinemuchi, A. Longmore, M. López-Corredoira, T. MacCarone, D. Majaess, E. L. Martín, N. Masetti, R. E. Mennickent, I. F. Mirabel, L. Monaco, L. Morelli, V. Motta, T. Palma, M. C. Parisi, Q. Parker, F. Peñaloza, G. Pietrzyński, G. Pignata, B. Popescu, M. A. Read, A. Rojas, A. Roman-Lopes, M. T. Ruiz, I. Saviane, M. R. Schreiber, A. C. Schröder, S. Sharma, M. D. Smith, L. Sodré, J. Stead, A. W. Stephens, M. Tamura, C. Tappert, M. A. Thompson, E. Valenti, L. Vanzi, N. A. Walton, W. Weidmann, A. Zijlstra

Research output: Contribution to journal › Article › peer-review

Abstract

Context. The ESO public survey VISTA variables in the Vía Láctea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for about five years. Aims. We describe the progress of the survey observations in the first observing season, the observing strategy, and quality of the data obtained. Methods. The observations are carried out on the 4-m VISTA telescope in the ZYJHK s filters. In addition to the multi-band imaging the variability monitoring campaign in the K s filter has started. Data reduction is carried out using the pipeline at the Cambridge Astronomical Survey Unit. The photometric and astrometric calibration is performed via the numerous 2MASS sources observed in each pointing. Results. The first data release contains the aperture photometry and astrometric catalogues for 348 individual pointings in the ZYJHK s filters taken in the 2010 observing season. The typical image quality is ∼0′′.9-1′′.0. The stringent photometric and image quality requirements of the survey are satisfied in 100% of the JHK s images in the disk area and 90% of the JHK s images in the bulge area. The completeness in the Z and Y images is 84% in the disk, and 40% in the bulge. The first season catalogues contain 1.28 × 10 8 stellar sources in the bulge and 1.68 × 10 8 in the disk area detected in at least one of the photometric bands. The combined, multi-band catalogues contain more than 1.63 × 10 8 stellar sources. About 10% of these are double detections because of overlapping adjacent pointings. These overlapping multiple detections are used to characterise the quality of the data. The images in the JHK s bands extend typically ∼4 mag deeper than 2MASS. The magnitude limit and photometric quality depend strongly on crowding in the inner Galactic regions. The astrometry for K s = 15-18 mag has rms ∼35-175 mas. Conclusions. The VVV Survey data products offer a unique dataset to map the stellar populations in the Galactic bulge and the adjacent plane and provide an exciting new tool for the study of the structure, content, and star-formation history of our Galaxy, as well as for investigations of the newly discovered star clusters, star-forming regions in the disk, high proper motion stars, asteroids, planetary nebulae, and other interesting objects. © 2012 ESO.

Original language	English
Article number	A107
Journal	Astronomy and Astrophysics
Volume	537
DOIs	https://doi.org/10.1051/0004-6361/201118407
Publication status	Published - 2012

Keywords

Galaxy: bulge
Galaxy: disk
Galaxy: stellar content
infrared: stars
stars: abundances
surveys

Access to Document

10.1051/0004-6361/201118407

Cite this

Saito, R. K., Hempel, M., Minniti, D., Lucas, P. W., Rejkuba, M., Toledo, I., Gonzalez, O. A., Alonso-García, J., Irwin, M. J., Gonzalez-Solares, E., Hodgkin, S. T., Lewis, J. R., Cross, N., Ivanov, V. D., Kerins, E., Emerson, J. P., Soto, M., Amôres, E. B., Gurovich, S., ... Zijlstra, A. (2012). VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea. Astronomy and Astrophysics, 537, Article A107. https://doi.org/10.1051/0004-6361/201118407

@article{ef5ca2e61af64037a36bd9596fa27949,

title = "VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the V{\'i}a L{\'a}ctea",

abstract = "Context. The ESO public survey VISTA variables in the V{\'i}a L{\'a}ctea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for about five years. Aims. We describe the progress of the survey observations in the first observing season, the observing strategy, and quality of the data obtained. Methods. The observations are carried out on the 4-m VISTA telescope in the ZYJHK s filters. In addition to the multi-band imaging the variability monitoring campaign in the K s filter has started. Data reduction is carried out using the pipeline at the Cambridge Astronomical Survey Unit. The photometric and astrometric calibration is performed via the numerous 2MASS sources observed in each pointing. Results. The first data release contains the aperture photometry and astrometric catalogues for 348 individual pointings in the ZYJHK s filters taken in the 2010 observing season. The typical image quality is ∼0′′.9-1′′.0. The stringent photometric and image quality requirements of the survey are satisfied in 100% of the JHK s images in the disk area and 90% of the JHK s images in the bulge area. The completeness in the Z and Y images is 84% in the disk, and 40% in the bulge. The first season catalogues contain 1.28 × 10 8 stellar sources in the bulge and 1.68 × 10 8 in the disk area detected in at least one of the photometric bands. The combined, multi-band catalogues contain more than 1.63 × 10 8 stellar sources. About 10% of these are double detections because of overlapping adjacent pointings. These overlapping multiple detections are used to characterise the quality of the data. The images in the JHK s bands extend typically ∼4 mag deeper than 2MASS. The magnitude limit and photometric quality depend strongly on crowding in the inner Galactic regions. The astrometry for K s = 15-18 mag has rms ∼35-175 mas. Conclusions. The VVV Survey data products offer a unique dataset to map the stellar populations in the Galactic bulge and the adjacent plane and provide an exciting new tool for the study of the structure, content, and star-formation history of our Galaxy, as well as for investigations of the newly discovered star clusters, star-forming regions in the disk, high proper motion stars, asteroids, planetary nebulae, and other interesting objects. {\textcopyright} 2012 ESO.",

keywords = "Galaxy: bulge, Galaxy: disk, Galaxy: stellar content, infrared: stars, stars: abundances, surveys",

author = "Saito, {R. K.} and M. Hempel and D. Minniti and Lucas, {P. W.} and M. Rejkuba and I. Toledo and Gonzalez, {O. A.} and J. Alonso-Garc{\'i}a and Irwin, {M. J.} and E. Gonzalez-Solares and Hodgkin, {S. T.} and Lewis, {J. R.} and N. Cross and Ivanov, {V. D.} and E. Kerins and Emerson, {J. P.} and M. Soto and Am{\^o}res, {E. B.} and S. Gurovich and I. D{\'e}k{\'a}ny and R. Angeloni and Beamin, {J. C.} and M. Catelan and N. Padilla and M. Zoccali and P. Pietrukowicz and {Moni Bidin}, C. and F. Mauro and D. Geisler and Folkes, {S. L.} and Sale, {S. E.} and J. Borissova and R. Kurtev and Ahumada, {A. V.} and Alonso, {M. V.} and A. Adamson and Arias, {J. I.} and Bandyopadhyay, {R. M.} and Barb{\'a}, {R. H.} and B. Barbuy and Baume, {G. L.} and Bedin, {L. R.} and A. Bellini and R. Benjamin and E. Bica and C. Bonatto and L. Bronfman and G. Carraro and Chen{\`e}, {A. N.} and Clari{\'a}, {J. J.} and Clarke, {J. R A} and C. Contreras and A. Corvill{\'o}n and {De Grijs}, R. and B. Dias and Drew, {J. E.} and C. Fari{\~n}a and C. Feinstein and E. Fern{\'a}ndez-Laj{\'u}s and Gamen, {R. C.} and W. Gieren and B. Goldman and C. Gonz{\'a}lez-Fern{\'a}ndez and Grand, {R. J J} and G. Gunthardt and Hambly, {N. C.} and Hanson, {M. M.} and He{\l}miniak, {K. G.} and Hoare, {M. G.} and L. Huckvale and A. Jord{\'a}n and K. Kinemuchi and A. Longmore and M. L{\'o}pez-Corredoira and T. MacCarone and D. Majaess and Mart{\'i}n, {E. L.} and N. Masetti and Mennickent, {R. E.} and Mirabel, {I. F.} and L. Monaco and L. Morelli and V. Motta and T. Palma and Parisi, {M. C.} and Q. Parker and F. Pe{\~n}aloza and G. Pietrzy{\'n}ski and G. Pignata and B. Popescu and Read, {M. A.} and A. Rojas and A. Roman-Lopes and Ruiz, {M. T.} and I. Saviane and Schreiber, {M. R.} and Schr{\"o}der, {A. C.} and S. Sharma and Smith, {M. D.} and L. Sodr{\'e} and J. Stead and Stephens, {A. W.} and M. Tamura and C. Tappert and Thompson, {M. A.} and E. Valenti and L. Vanzi and Walton, {N. A.} and W. Weidmann and A. Zijlstra",

note = "DOI: 10.1051/0004-6361/201118407; eprintid: arXiv:1111.5511",

year = "2012",

doi = "10.1051/0004-6361/201118407",

language = "English",

volume = "537",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Saito, RK, Hempel, M, Minniti, D, Lucas, PW, Rejkuba, M, Toledo, I, Gonzalez, OA, Alonso-García, J, Irwin, MJ, Gonzalez-Solares, E, Hodgkin, ST, Lewis, JR, Cross, N, Ivanov, VD, Kerins, E, Emerson, JP, Soto, M, Amôres, EB, Gurovich, S, Dékány, I, Angeloni, R, Beamin, JC, Catelan, M, Padilla, N, Zoccali, M, Pietrukowicz, P, Moni Bidin, C, Mauro, F, Geisler, D, Folkes, SL, Sale, SE, Borissova, J, Kurtev, R, Ahumada, AV, Alonso, MV, Adamson, A, Arias, JI, Bandyopadhyay, RM, Barbá, RH, Barbuy, B, Baume, GL, Bedin, LR, Bellini, A, Benjamin, R, Bica, E, Bonatto, C, Bronfman, L, Carraro, G, Chenè, AN, Clariá, JJ, Clarke, JRA, Contreras, C, Corvillón, A, De Grijs, R, Dias, B, Drew, JE, Fariña, C, Feinstein, C, Fernández-Lajús, E, Gamen, RC, Gieren, W, Goldman, B, González-Fernández, C, Grand, RJJ, Gunthardt, G, Hambly, NC, Hanson, MM, Hełminiak, KG, Hoare, MG, Huckvale, L, Jordán, A, Kinemuchi, K, Longmore, A, López-Corredoira, M, MacCarone, T, Majaess, D, Martín, EL, Masetti, N, Mennickent, RE, Mirabel, IF, Monaco, L, Morelli, L, Motta, V, Palma, T, Parisi, MC, Parker, Q, Peñaloza, F, Pietrzyński, G, Pignata, G, Popescu, B, Read, MA, Rojas, A, Roman-Lopes, A, Ruiz, MT, Saviane, I, Schreiber, MR, Schröder, AC, Sharma, S, Smith, MD, Sodré, L, Stead, J, Stephens, AW, Tamura, M, Tappert, C, Thompson, MA, Valenti, E, Vanzi, L, Walton, NA, Weidmann, W & Zijlstra, A 2012, 'VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea', Astronomy and Astrophysics, vol. 537, A107. https://doi.org/10.1051/0004-6361/201118407

TY - JOUR

T1 - VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea

AU - Saito, R. K.

AU - Hempel, M.

AU - Minniti, D.

AU - Lucas, P. W.

AU - Rejkuba, M.

AU - Toledo, I.

AU - Gonzalez, O. A.

AU - Alonso-García, J.

AU - Irwin, M. J.

AU - Gonzalez-Solares, E.

AU - Hodgkin, S. T.

AU - Lewis, J. R.

AU - Cross, N.

AU - Ivanov, V. D.

AU - Kerins, E.

AU - Emerson, J. P.

AU - Soto, M.

AU - Amôres, E. B.

AU - Gurovich, S.

AU - Dékány, I.

AU - Angeloni, R.

AU - Beamin, J. C.

AU - Catelan, M.

AU - Padilla, N.

AU - Zoccali, M.

AU - Pietrukowicz, P.

AU - Moni Bidin, C.

AU - Mauro, F.

AU - Geisler, D.

AU - Folkes, S. L.

AU - Sale, S. E.

AU - Borissova, J.

AU - Kurtev, R.

AU - Ahumada, A. V.

AU - Alonso, M. V.

AU - Adamson, A.

AU - Arias, J. I.

AU - Bandyopadhyay, R. M.

AU - Barbá, R. H.

AU - Barbuy, B.

AU - Baume, G. L.

AU - Bedin, L. R.

AU - Bellini, A.

AU - Benjamin, R.

AU - Bica, E.

AU - Bonatto, C.

AU - Bronfman, L.

AU - Carraro, G.

AU - Chenè, A. N.

AU - Clariá, J. J.

AU - Clarke, J. R A

AU - Contreras, C.

AU - Corvillón, A.

AU - De Grijs, R.

AU - Dias, B.

AU - Drew, J. E.

AU - Fariña, C.

AU - Feinstein, C.

AU - Fernández-Lajús, E.

AU - Gamen, R. C.

AU - Gieren, W.

AU - Goldman, B.

AU - González-Fernández, C.

AU - Grand, R. J J

AU - Gunthardt, G.

AU - Hambly, N. C.

AU - Hanson, M. M.

AU - Hełminiak, K. G.

AU - Hoare, M. G.

AU - Huckvale, L.

AU - Jordán, A.

AU - Kinemuchi, K.

AU - Longmore, A.

AU - López-Corredoira, M.

AU - MacCarone, T.

AU - Majaess, D.

AU - Martín, E. L.

AU - Masetti, N.

AU - Mennickent, R. E.

AU - Mirabel, I. F.

AU - Monaco, L.

AU - Morelli, L.

AU - Motta, V.

AU - Palma, T.

AU - Parisi, M. C.

AU - Parker, Q.

AU - Peñaloza, F.

AU - Pietrzyński, G.

AU - Pignata, G.

AU - Popescu, B.

AU - Read, M. A.

AU - Rojas, A.

AU - Roman-Lopes, A.

AU - Ruiz, M. T.

AU - Saviane, I.

AU - Schreiber, M. R.

AU - Schröder, A. C.

AU - Sharma, S.

AU - Smith, M. D.

AU - Sodré, L.

AU - Stead, J.

AU - Stephens, A. W.

AU - Tamura, M.

AU - Tappert, C.

AU - Thompson, M. A.

AU - Valenti, E.

AU - Vanzi, L.

AU - Walton, N. A.

AU - Weidmann, W.

AU - Zijlstra, A.

N1 - DOI: 10.1051/0004-6361/201118407; eprintid: arXiv:1111.5511

PY - 2012

Y1 - 2012

N2 - Context. The ESO public survey VISTA variables in the Vía Láctea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for about five years. Aims. We describe the progress of the survey observations in the first observing season, the observing strategy, and quality of the data obtained. Methods. The observations are carried out on the 4-m VISTA telescope in the ZYJHK s filters. In addition to the multi-band imaging the variability monitoring campaign in the K s filter has started. Data reduction is carried out using the pipeline at the Cambridge Astronomical Survey Unit. The photometric and astrometric calibration is performed via the numerous 2MASS sources observed in each pointing. Results. The first data release contains the aperture photometry and astrometric catalogues for 348 individual pointings in the ZYJHK s filters taken in the 2010 observing season. The typical image quality is ∼0′′.9-1′′.0. The stringent photometric and image quality requirements of the survey are satisfied in 100% of the JHK s images in the disk area and 90% of the JHK s images in the bulge area. The completeness in the Z and Y images is 84% in the disk, and 40% in the bulge. The first season catalogues contain 1.28 × 10 8 stellar sources in the bulge and 1.68 × 10 8 in the disk area detected in at least one of the photometric bands. The combined, multi-band catalogues contain more than 1.63 × 10 8 stellar sources. About 10% of these are double detections because of overlapping adjacent pointings. These overlapping multiple detections are used to characterise the quality of the data. The images in the JHK s bands extend typically ∼4 mag deeper than 2MASS. The magnitude limit and photometric quality depend strongly on crowding in the inner Galactic regions. The astrometry for K s = 15-18 mag has rms ∼35-175 mas. Conclusions. The VVV Survey data products offer a unique dataset to map the stellar populations in the Galactic bulge and the adjacent plane and provide an exciting new tool for the study of the structure, content, and star-formation history of our Galaxy, as well as for investigations of the newly discovered star clusters, star-forming regions in the disk, high proper motion stars, asteroids, planetary nebulae, and other interesting objects. © 2012 ESO.

AB - Context. The ESO public survey VISTA variables in the Vía Láctea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for about five years. Aims. We describe the progress of the survey observations in the first observing season, the observing strategy, and quality of the data obtained. Methods. The observations are carried out on the 4-m VISTA telescope in the ZYJHK s filters. In addition to the multi-band imaging the variability monitoring campaign in the K s filter has started. Data reduction is carried out using the pipeline at the Cambridge Astronomical Survey Unit. The photometric and astrometric calibration is performed via the numerous 2MASS sources observed in each pointing. Results. The first data release contains the aperture photometry and astrometric catalogues for 348 individual pointings in the ZYJHK s filters taken in the 2010 observing season. The typical image quality is ∼0′′.9-1′′.0. The stringent photometric and image quality requirements of the survey are satisfied in 100% of the JHK s images in the disk area and 90% of the JHK s images in the bulge area. The completeness in the Z and Y images is 84% in the disk, and 40% in the bulge. The first season catalogues contain 1.28 × 10 8 stellar sources in the bulge and 1.68 × 10 8 in the disk area detected in at least one of the photometric bands. The combined, multi-band catalogues contain more than 1.63 × 10 8 stellar sources. About 10% of these are double detections because of overlapping adjacent pointings. These overlapping multiple detections are used to characterise the quality of the data. The images in the JHK s bands extend typically ∼4 mag deeper than 2MASS. The magnitude limit and photometric quality depend strongly on crowding in the inner Galactic regions. The astrometry for K s = 15-18 mag has rms ∼35-175 mas. Conclusions. The VVV Survey data products offer a unique dataset to map the stellar populations in the Galactic bulge and the adjacent plane and provide an exciting new tool for the study of the structure, content, and star-formation history of our Galaxy, as well as for investigations of the newly discovered star clusters, star-forming regions in the disk, high proper motion stars, asteroids, planetary nebulae, and other interesting objects. © 2012 ESO.

KW - Galaxy: bulge

KW - Galaxy: disk

KW - Galaxy: stellar content

KW - infrared: stars

KW - stars: abundances

KW - surveys

U2 - 10.1051/0004-6361/201118407

DO - 10.1051/0004-6361/201118407

M3 - Article

SN - 0004-6361

VL - 537

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A107

ER -

VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea

Abstract

Keywords

Access to Document

Fingerprint

Cite this