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1. J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX

Author

Whitten, D. D., primary, Placco, V. M., additional, Beers, T. C., additional, Chies-Santos, A. L., additional, Bonatto, C., additional, Varela, J., additional, Cristóbal-Hornillos, D., additional, Ederoclite, A., additional, Masseron, T., additional, Lee, Y. S., additional, Akras, S., additional, Borges Fernandes, M., additional, Caballero, J. A., additional, Cenarro, A. J., additional, Coelho, P., additional, Costa-Duarte, M. V., additional, Daflon, S., additional, Dupke, R. A., additional, Lopes de Oliveira, R., additional, López-Sanjuan, C., additional, Marín-Franch, A., additional, Mendes de Oliveira, C., additional, Moles, M., additional, Orsi, A. A., additional, Rossi, S., additional, Sodré, L., additional, and Vázquez Ramió, H., additional

Published
2019
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2. J-PLUS: The Javalambre Photometric Local Universe Survey

Author

Cenarro, A. J., primary, Moles, M., additional, Cristóbal-Hornillos, D., additional, Marín-Franch, A., additional, Ederoclite, A., additional, Varela, J., additional, López-Sanjuan, C., additional, Hernández-Monteagudo, C., additional, Angulo, R. E., additional, Vázquez Ramió, H., additional, Viironen, K., additional, Bonoli, S., additional, Orsi, A. A., additional, Hurier, G., additional, San Roman, I., additional, Greisel, N., additional, Vilella-Rojo, G., additional, Díaz-García, L. A., additional, Logroño-García, R., additional, Gurung-López, S., additional, Spinoso, D., additional, Izquierdo-Villalba, D., additional, Aguerri, J. A. L., additional, Allende Prieto, C., additional, Bonatto, C., additional, Carvano, J. M., additional, Chies-Santos, A. L., additional, Daflon, S., additional, Dupke, R. A., additional, Falcón-Barroso, J., additional, Gonçalves, D. R., additional, Jiménez-Teja, Y., additional, Molino, A., additional, Placco, V. M., additional, Solano, E., additional, Whitten, D. D., additional, Abril, J., additional, Antón, J. L., additional, Bello, R., additional, Bielsa de Toledo, S., additional, Castillo-Ramírez, J., additional, Chueca, S., additional, Civera, T., additional, Díaz-Martín, M. C., additional, Domínguez-Martínez, M., additional, Garzarán-Calderaro, J., additional, Hernández-Fuertes, J., additional, Iglesias-Marzoa, R., additional, Iñiguez, C., additional, Jiménez Ruiz, J. M., additional, Kruuse, K., additional, Lamadrid, J. L., additional, Lasso-Cabrera, N., additional, López-Alegre, G., additional, López-Sainz, A., additional, Maícas, N., additional, Moreno-Signes, A., additional, Muniesa, D. J., additional, Rodríguez-Llano, S., additional, Rueda-Teruel, F., additional, Rueda-Teruel, S., additional, Soriano-Laguía, I., additional, Tilve, V., additional, Valdivielso, L., additional, Yanes-Díaz, A., additional, Alcaniz, J. S., additional, Mendes de Oliveira, C., additional, Sodré, L., additional, Coelho, P., additional, Lopes de Oliveira, R., additional, Tamm, A., additional, Xavier, H. S., additional, Abramo, L. R., additional, Akras, S., additional, Alfaro, E. J., additional, Alvarez-Candal, A., additional, Ascaso, B., additional, Beasley, M. A., additional, Beers, T. C., additional, Borges Fernandes, M., additional, Bruzual, G. R., additional, Buzzo, M. L., additional, Carrasco, J. M., additional, Cepa, J., additional, Cortesi, A., additional, Costa-Duarte, M. V., additional, De Prá, M., additional, Favole, G., additional, Galarza, A., additional, Galbany, L., additional, Garcia, K., additional, González Delgado, R. M., additional, González-Serrano, J. I., additional, Gutiérrez-Soto, L. A., additional, Hernandez-Jimenez, J. A., additional, Kanaan, A., additional, Kuncarayakti, H., additional, Landim, R. C. G., additional, Laur, J., additional, Licandro, J., additional, Lima Neto, G. B., additional, Lyman, J. D., additional, Maíz Apellániz, J., additional, Miralda-Escudé, J., additional, Morate, D., additional, Nogueira-Cavalcante, J. P., additional, Novais, P. M., additional, Oncins, M., additional, Oteo, I., additional, Overzier, R. A., additional, Pereira, C. B., additional, Rebassa-Mansergas, A., additional, Reis, R. R. R., additional, Roig, F., additional, Sako, M., additional, Salvador-Rusiñol, N., additional, Sampedro, L., additional, Sánchez-Blázquez, P., additional, Santos, W. A., additional, Schmidtobreick, L., additional, Siffert, B. B., additional, Telles, E., additional, and Vilchez, J. M., additional

Published
2019
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4. Massive open star clusters using the VVV survey

Author

Ramírez Alegría, S., primary, Borissova, J., additional, Chené, A.-N., additional, Bonatto, C., additional, Kurtev, R., additional, Amigo, P., additional, Kuhn, M., additional, Gromadzki, M., additional, and Carballo-Bello, J. A., additional

Published
2016
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5. Massive open star clusters using the VVV survey

Author

Chené, A.-N., primary, Ramírez Alegría, S., additional, Borissova, J., additional, O’Leary, E., additional, Martins, F., additional, Hervé, A., additional, Kuhn, M., additional, Kurtev, R., additional, Consuelo Amigo Fuentes, P., additional, Bonatto, C., additional, and Minniti, D., additional

Published
2015
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6. New galactic star clusters discovered in the VVV survey. Candidates projected on the inner disk and bulge

Author

Borissova, J., primary, Chené, A.-N., additional, Ramírez Alegría, S., additional, Sharma, S., additional, Clarke, J. R. A., additional, Kurtev, R., additional, Negueruela, I., additional, Marco, A., additional, Amigo, P., additional, Minniti, D., additional, Bica, E., additional, Bonatto, C., additional, Catelan, M., additional, Fierro, C., additional, Geisler, D., additional, Gromadzki, M., additional, Hempel, M., additional, Hanson, M. M., additional, Ivanov, V. D., additional, Lucas, P., additional, Majaess, D., additional, Moni Bidin, C., additional, Popescu, B., additional, and Saito, R. K., additional

Published
2014
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9. Massive open star clusters using the VVV survey

Author

Ramírez Alegría, S., primary, Borissova, J., additional, Chené, A. N., additional, O’Leary, E., additional, Amigo, P., additional, Minniti, D., additional, Saito, R. K., additional, Geisler, D., additional, Kurtev, R., additional, Hempel, M., additional, Gromadzki, M., additional, Clarke, J. R. A., additional, Negueruela, I., additional, Marco, A., additional, Fierro, C., additional, Bonatto, C., additional, and Catelan, M., additional

Published
2014
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10. Investigating potential planetary nebula/cluster pairs

Author

Moni Bidin, C., primary, Majaess, D., additional, Bonatto, C., additional, Mauro, F., additional, Turner, D., additional, Geisler, D., additional, Chené, A.-N., additional, Gormaz-Matamala, A. C., additional, Borissova, J., additional, Kurtev, R. G., additional, Minniti, D., additional, Carraro, G., additional, and Gieren, W., additional

Published
2014
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11. Anchors for the cosmic distance scale: the Cepheids U Sagittarii, CF Cassiopeiae, and CEab Cassiopeiae

Author

Majaess, D., primary, Carraro, G., additional, Moni Bidin, C., additional, Bonatto, C., additional, Berdnikov, L., additional, Balam, D., additional, Moyano, M., additional, Gallo, L., additional, Turner, D., additional, Lane, D., additional, Gieren, W., additional, Borissova, J., additional, Kovtyukh, V., additional, and Beletsky, Y., additional

Published
2013
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12. Massive open star clusters using the VVV survey

Author

Chené, A.-N., primary, Borissova, J., additional, Bonatto, C., additional, Majaess, D. J., additional, Baume, G., additional, Clarke, J. R. A., additional, Kurtev, R., additional, Schnurr, O., additional, Bouret, J.-C., additional, Catelan, M., additional, Emerson, J. P., additional, Feinstein, C., additional, Geisler, D., additional, de Grijs, R., additional, Hervé, A., additional, Ivanov, V. D., additional, Kumar, M. S. N., additional, Lucas, P., additional, Mahy, L., additional, Martins, F., additional, Mauro, F., additional, Minniti, D., additional, and Moni Bidin, C., additional

Published
2013
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13. Massive open star clusters using the VVV survey

Author

Chené, A.-N., primary, Borissova, J., additional, Clarke, J. R. A., additional, Bonatto, C., additional, Majaess, D. J., additional, Moni Bidin, C., additional, Sale, S. E., additional, Mauro, F., additional, Kurtev, R., additional, Baume, G., additional, Feinstein, C., additional, Ivanov, V. D., additional, Geisler, D., additional, Catelan, M., additional, Minniti, D., additional, Lucas, P., additional, de Grijs, R., additional, and Kumar, M. S. N., additional

Published
2012
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15. Strengthening the open cluster distance scale via VVV photometry

Author

Majaess, D., primary, Turner, D., additional, Moni Bidin, C., additional, Geisler, D., additional, Borissova, J., additional, Minniti, D., additional, Bonatto, C., additional, Gieren, W., additional, Carraro, G., additional, Kurtev, R., additional, Mauro, F., additional, Chené, A.-N., additional, Forbes, D., additional, Lucas, P., additional, Dékány, I., additional, Saito, R. K., additional, and Soto, M., additional

Published
2012
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16. 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

Author

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

Published
2012
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17. New Galactic star clusters discovered in the VVV survey

Author

Borissova, J., primary, Bonatto, C., additional, Kurtev, R., additional, Clarke, J. R. A., additional, Peñaloza, F., additional, Sale, S. E., additional, Minniti, D., additional, Alonso-García, J., additional, Artigau, E., additional, Barbá, R., additional, Bica, E., additional, Baume, G. L., additional, Catelan, M., additional, Chenè, A. N., additional, Dias, B., additional, Folkes, S. L., additional, Froebrich, D., additional, Geisler, D., additional, de Grijs, R., additional, Hanson, M. M., additional, Hempel, M., additional, Ivanov, V. D., additional, Kumar, M. S. N., additional, Lucas, P., additional, Mauro, F., additional, Moni Bidin, C., additional, Rejkuba, M., additional, Saito, R. K., additional, Tamura, M., additional, and Toledo, I., additional

Published
2011
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49. Probing embedded star clusters in the HII complex NGC6357 with VVV.

Author

Lima, E. F., Bica, E., Bonatto, C., and Saito, R. K.

Subjects
BINARY stars, STAR clusters, STELLAR mass, STELLAR magnitudes, STELLAR photometry
Abstract

Context. NGC6357 is an active star-forming region located in the Sagittarius arm that displays several star clusters, which makes it a very interesting target to investigate star formation and early cluster evolution. Aims. We explore NGC6357 with the VISTA Variables in the Vía Láctea (VVV) photometry of seven embedded clusters (ECs), and one open cluster projected in the outskirts of the complex. Methods. Photometric and structural properties (age, reddening, distance, core, and total radii) of the star clusters were derived. VVV saturated stars were replaced by their 2MASS counterparts. Field-decontaminated VVV photometry was used to analyse colour– magnitude diagrams (CMDs) and stellar radial density profiles and determine astrophysical parameters. Results. We report the discovery of four ECs and one intermediate-age cluster in the complex area. We derive a revised distance estimate for NGC6357 of 1.78 ± 0.1 kpc based on the cluster CMD morphologies. Of the ECs, one contains the binary star WR93, while the remaining ones are dominated by pre-main sequence stars, young stellar objects, and/or and have a developed main sequence. These features reflect a significant age spread among the clusters. Evidence is found that the relatively populous cluster Pismis 24 hosts two subclusters. [ABSTRACT FROM AUTHOR]

Published
2014
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50. Investigating potential planetary nebula/cluster pairs.

Author

Bidin, C. Moni, Majaess, D., Bonatto, C., Mauro, F., Turner, D., Geisler, D., Chené, A.-N., Gormaz-Matamala, A. C., Borissova, J., Kurtev, R. G., Minniti, D., Carraro, G., and Gieren, W.

Subjects
PLANETARY nebulae, INTERSTELLAR medium, UBV system (Astronomy), OPEN clusters of stars, ASTROPHYSICS
Abstract

Context. Fundamental parameters characterizing the end-state of intermediate-mass stars may be constrained by discovering planetary nebulae (PNe) in open clusters (OCs). Cluster membership may be exploited to establish the distance, luminosity, age, and physical size for PNe, and the intrinsic luminosity and mass of its central star. Aims. Four potential PN-OC associations were investigated to assess the cluster membership for the PNe. Methods. Radial velocities were measured from intermediate-resolution optical spectra, complemented with previous estimates in the literature. When the radial velocity study supported the PN/OC association, we analyzed whether other parameters (e.g., age, distance, reddening, central star brightness) were consistent with this conclusion. Results. Our measurements imply that the PNe VBe 3 and HeFa 1 are not members of the OCs NGC5999 and NGC6067, respectively, and that they very likely belong to the background bulge population. Conversely, consistent radial velocities indicate that NGC2452/NGC 2453 could be associated, but our results are not conclusive so additional observations are warranted. Finally, we demonstrate that all the available information point to He 2-86 being a young, highly internally obscured PN member of NGC4463. New near-infrared photometry acquired via the Vista Variables in the Via Lactea ESO public survey was used in tandem with existing UBV photometry to measure the distance, reddening, and age of NGC4463, finding d = 1.55 ± 0.10 kpc, E(B - V) = 0.41 ± 0.02, and t = 65 ± 10 Myr, respectively. The same values should be adopted for the PN if the proposed cluster membership is confirmed. [ABSTRACT FROM AUTHOR]

Published
2014
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