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The 'VISTA Variables in the Vía Láctea eXtended (VVVX)' ESO Public Survey is a nearinfrared photometric sky survey that covers nearly 1700 deg2 towards the Galactic disc and bulge. It is well-suited to search for newopen clusters, hidden behind dust and gas. The pipeline processed and calibrated ...


Borissova, J.Ivanov, V.D.Lucas, P.W.Kurtev, R.Alonso-Garcia, J.Ramírez Alegría, S.Minniti, D.Froebrich, D.Hempel, M.Medina, N.Chené, A.-N.Kuhn, M.A.[New Galactic star clusters discovered in the disc area of the VVVX survey]New Galactic star clusters discovered in the disc area of the VVVX survey
Autor: Saito, R. K. Hempel, M. Minniti, D. Lucas, P. W. Rejkuba, M. Toledo, I. Gonzalez, O. A. Alonso-García, J. Irwin, M. 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. Dékány, I. Angeloni, R. Beamin, J. C. Catelan, M. Padilla, N. Zoccali, M. Pietrukowicz, P. Moni Bidin, C. Mauro, F. Geisler, D. Folkes, S. L. Sale, S. E. Borissova, J. Kurtev, R. Ahumada, A. V. Alonso, M. V. Adamson, A. Arias, J. I. Bandyopadhyay, R. M. Barbá, R. H. Barbuy, B. Baume, G. L. Bedin, L. R. Bellini, A. Benjamin, R. Bica, E. Bonatto, C. Bronfman Aguiló, Leonardo Carraro, Giovanni Chenè, A. N. Clariá, J. J. Clarke, J. R. A. Contreras, C. Corvillón, A. Grijs, R. de Dias, B. Drew, J. E. Fariña, C. Feinstein, C. Fernández Lajús, E. Gamen, R. Gieren, W. Goldman, B. González-Fernández, C. Grand, R. J. J. Gunthardt, G. Hambly, N. C. Hanson, M. M. Helminiak, K. G. Hoare, M. G. Huckvale, L. Jordán, A. Kinemuch, K. Longmore, A. López Corredoira, M. Maccarone, T. Majaess, D. Martín, E. L. Masetti, N. Mennickent, R. E. Mirabel, I. F. Monaco, L. Morelli, L. Motta, V. Palma, T. Parisi, M. C. Parker, Q. Peñaloza, F. Pietrzynski, G. Pignata Libralato, Giuliano Popescu, B. Read, M. A. Rojas, A. Roman-Lopes, A. Ruiz González, María Teresa Saviane, I. Schreiber, M. R. Schröder, A. C. Sharma, S. Smith, M. D. Sodré Jr., L. Stead, J. Stephens, A. W. Tamura, M. Tappert, C. Thompson, M. A. Valenti, E. Vanzi, L. Walton, N. A. Weidmann, W. Zijlstr, A.

Saito, R. K.Hempel, M.Minniti, D.Lucas, P. W.Rejkuba, M.Toledo, I.Gonzalez, O. A.Alonso-García, J.Irwin, M.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.Dékány, I.Angeloni, R.Beamin, J. C.Catelan, M.Padilla, N.Zoccali, M.Pietrukowicz, P.Moni Bidin, C.Mauro, F.Geisler, D.Folkes, S. L.Sale, S. E.Borissova, J.Kurtev, R.Ahumada, A. V.Alonso, M. V.Adamson, A.Arias, J. I.Bandyopadhyay, R. M.Barbá, R. H.Barbuy, B.Baume, G. L.Bedin, L. R.Bellini, A.Benjamin, R.Bica, E.Bonatto, C.Bronfman Aguiló, LeonardoCarraro, GiovanniChenè, A. N.Clariá, J. J.Clarke, J. R. A.Contreras, C.Corvillón, A.Grijs, R. deDias, B.Drew, J. E.Fariña, C.Feinstein, C.Fernández Lajús, E.Gamen, R.Gieren, W.Goldman, B.González-Fernández, C.Grand, R. J. J.Gunthardt, G.Hambly, N. C.Hanson, M. M.Helminiak, K. G.Hoare, M. G.Huckvale, L.Jordán, A.Kinemuch, K.Longmore, A.López Corredoira, M.Maccarone, T.Majaess, D.Martín, E. L.Masetti, N.Mennickent, R. E.Mirabel, I. F.Monaco, L.Morelli, L.Motta, V.Palma, T.Parisi, M. C.Parker, Q.Peñaloza, F.Pietrzynski, G.Pignata Libralato, GiulianoPopescu, B.Read, M. A.Rojas, A.Roman-Lopes, A.Ruiz González, María TeresaSaviane, I.Schreiber, M. R.Schröder, A. C.Sharma, S.Smith, M. D.Sodré Jr., L.Stead, J.Stephens, A. W.Tamura, M.Tappert, C.Thompson, M. A.Valenti, E.Vanzi, L.Walton, N. A.Weidmann, W.Zijlstr, A.[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 Via Lactea]

Deep near-IR images from the VISTA Variables in the Via Lactea (VVV) Survey were used to search for RR Lyrae stars in the Southern Galactic plane. A sizable sample of 404 RR Lyrae of type ab stars was identified across a thin slice of the fourth Galactic quadrant (295 degrees < l < 350 degrees, -...


Minniti, D.Dékány, I.Majaess, D.Palma, T.Pullen, J.Rejkuba, M.Alonso-García, J.Catelan, M.Contreras Ramos, R.Gonzalez, O.A.Hempel, M.Irwin, M.lLucas, P.W.Saito, R.K.Tissera, P.Valenti, E.Zoccali, M.[Characterization of the VVV Survey RR Lyrae Population across the Southern Galactic Plane]Characterization of the VVV Survey RR Lyrae Population across the Southern Galactic Plane

This paper is based on observations made with ESO telescopes at the La Silla Paranal Observatory under program ID 092.B-0104(A). We have made extensive use of the SIMBAD Database at CDS (Centre de Données astronomiques) Strasbourg, the NASA/IPAC Extragalactic Database (NED), which is operated by ...


Ivanov, V.D.Piatti, A.E.Beamín, J.-C.Minniti, D.Borissova, J.Kurtev, R.Hempel, M.Saito, R.K.[Candidate star clusters toward the inner Milky Way discovered on deep-stacked KS-band images from the VVV Survey]Candidate star clusters toward the inner Milky Way discovered on deep-stacked KS-band images from the VVV Survey

Context. The inner regions of the Galaxy are severely affected by extinction, which limits our capability to study the stellar populations present there. The Vista Variables in the Vía Láctea (VVV) ESO Public Survey has observed this zone at near-infrared wavelengths where reddening is highly dim...


Alonso-García, J.Saito, R.K.Hempel, M.Minniti, D.Pullen, J.Catelan, M.Ramos, R.C.Cross, N.J.G.Gonzalez, O.A.Lucas, P.W.Palma, T.Valenti, E.Zoccali, M.[Milky Way demographics with the VVV survey: IV. PSF photometry from almost one billion stars in the Galactic bulge and adjacent southern disk]Milky Way demographics with the VVV survey: IV. PSF photometry from almost one billion stars in the Galactic bulge and adjacent southern disk

We report the discovery of an enigmatic large-amplitude (ΔKs >10.5 mag) transient event in near-IR data obtained by the VISTA Variables in the Via Lactea (VVV) ESO Public Survey. The object (designated VVV-WIT- 06) is located at R.A.=17:07:18.917, decl.=-39:06:26.45 (J2000), corresponding to Gala...


Minniti, D.Saito, R.K.Forster, F.Pignata, G.Ivanov, V.D.Lucas, P.W.Beamin, J.C.Borissova, J.Catelan, M.Gonzalez, O.A.Hempel, M.Hsiao, E.Kurtev, R.Majaess, D.Masetti, N.Morrell, N.I.Phillips, M.M.Pullen, J.B.Rejkuba, M.Smith, L.Surot, F.Valenti, E.Zoccali, M.[The Emergence of the Infrared Transient VVV-WIT-06]The Emergence of the Infrared Transient VVV-WIT-06

We use deep, multi-epoch near-IR images of the VISTA Variables in the Via Lictea (VVV) Survey to measure proper motions (PMs) of stars in the Milky Way globular cluster (GC) FSR1716 = VVV-GC05. The colormagnitude diagram of this object, made by using PM-selected members, shows an extended horizon...


Ramos, R.C.Minniti, D.Fernández-Trincado, J.G.Alonso-Garcia, J.Catelan, M.Gran, F.Hajdu, G.Hanke, M.Hempel, M.Diaz, E.M.Pérez-Villegas, A.Rojas-Arriagada, A.Zoccali, M.[The Orbit of the New Milky Way Globular Cluster FSR1716 =VVV-GC05]The Orbit of the New Milky Way Globular Cluster FSR1716 =VVV-GC05

Interstellar extinction toward the Galactic Center (GC) is large and significantly differential. Its reddening and dimming effects in red clump (RC) stars in the Galactic Bulge can be exploited to better constrain the extinction law toward the innermost Galaxy. By virtue of a deep and complete ca...


Alonso-García, J.Minniti, D.Catelan, M.Contreras Ramos, R.Gonzalez, O.A.Hempel, M.Lucas, P.W.Saito, R.K.Valenti, E.Zoccali, M.[Extinction ratios in the inner Galaxy as revealed by the VVV survey]Extinction ratios in the inner Galaxy as revealed by the VVV survey

It is likely that a number of Galactic globular clusters remain to be discovered, especially toward the Galactic bulge. High stellar density combined with high and differential interstellar reddening are the two major problems for finding globular clusters located toward the bulge. We use the dee...


Minniti, D.Geisler, D.Alonso-Garcia, J.Palma, T.Beamin, J.C.Borissova, J.Catelan, M.Clariá, J.J.Cohen, R.E.Ramos, R.C.Dias, B.Fernández-Trincado, J.G.Gómez, M.Hempel, M.Ivanov, V.D.Kurtev, R.Lucas, P.W.Moni-Bidin, C.Pullen, J.Alegria, S.R.Saito, R.K.Valenti, E.[New VVV Survey Globular Cluster Candidates in the Milky Way Bulge]New VVV Survey Globular Cluster Candidates in the Milky Way Bulge

We present the first stellar density profile of the Milky Way bulge that reaches latitude b = 0 degrees. The profile was derived by counting red clump stars within the colour-magnitude diagram that was constructed using the new PSF-fitting photometry from VISTA Variables in the Via Lactea (VVV) s...


Valenti, E.Zoccali, M.Gonzalez, O. A.Minniti, D.Alonso-García, J.Marchetti, E.Hempel, M.Renzini, A.Rejkuba, M.[Stellar density profile and mass of the Milky Way bulge from VVV data]Stellar density profile and mass of the Milky Way bulge from VVV data

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