Results 51 to 60 of about 210,924 (322)
Gaia data release 1: Principles of the photometric calibration of the G
band [PDF]
, 2016 Context. Gaia is an ESA cornerstone mission launched on 19 December 2013
aiming to obtain the most complete and precise 3D map of our Galaxy by
observing more than one billion sources.Altavilla, G., Balaguer-Núñez, L., Bellazzini, M., Bragaglia, A., Brown, A. G. A., Burgess, P., Busso, G., Cacciari, C., Carrasco, J. M., Cocozza, G., De Angeli, F., Evans, D. W., Fabricius, C., Federici, L., Galleti, S., Gebran, M., Holland, G., Jordi, C., Marinoni, S., Montegriffo, P., Osborne, P., Pancino, E., Ragaini, S., Riello, M., van Leeuwen, F., Voss, H., Weiler, M. +26 morecore +3 more sourcesMilky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant [PDF]
Astrophysical Journal, 2018 We present Hubble Space Telescope (HST) photometry of a selected sample of 50 long-period, low-extinction Milky Way Cepheids measured on the same WFC3 F555W-, F814W-, and F160W-band photometric system as extragalactic Cepheids in Type Ia supernova host ...A. Riess, A. Riess, S. Casertano, S. Casertano, W. Yuan, W. Yuan, L. Macri, B. Bucciarelli, M. Lattanzi, J. Mackenty, J. B. Bowers, Wei Zheng, A. Filippenko, Caroline D. Huang, R. Anderson +14 moresemanticscholar +1 more sourceEstimating the selection function of Gaia DR3 subsamples [PDF]
Astronomy & Astrophysics, 2023 Understanding which sources are present in an astronomical catalogue and which are not is crucial for the accurate interpretation of astronomical data.A. Castro-Ginard, A. Brown, Z. Kostrzewa-Rutkowska, T. Cantat-Gaudin, R. Drimmel, S. Oh, V. Belokurov, A. Casey, M. Fouesneau, S. Khanna, A. Price-Whelan, H. Rix +11 moresemanticscholar +1 more sourceGaia's Game [PDF]
communication +1, 2014 James Lovelock’s vision of Earth as a living cybernetic system is popular again. The surprising new preacher of Gaia is Bruno Latour. He uses the concept to refer to a holistic understanding of Earth, in which mankind is situated as integral part. Gaia becomes the catalyst and fundament for his philosophical attempt to design a new believe-system in ...openaire +3 more sourcesDiscovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry [PDF]
Astronomy & AstrophysicsGravitational waves from black-hole (BH) merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected based on most stellar evolution models -- and also higher than known ...Gaia Collaboration P. Panuzzo, T. Mazeh, F. Arenou, B. Holl, E. Caffau, A. Jorissen, C. Babusiaux, P. Gavras, J. Sahlmann, U. Bastian, L. Wyrzykowski, L. Eyer, N. Leclerc, N. Bauchet, A. Bombrun, N. Mowlavi, G. Seabroke, D. Teyssier, E. Balbinot, A. Helmi, A. Brown, A. Vallenari, T. Prusti, J. D. Bruijne, A. Barbier, M. Biermann, O. Creevey, C. Ducourant, D. Evans, R. Guerra, A. Hutton, C. Jordi, S. Klioner, U. Lammers, L. Lindegren, X. Luri, F. Mignard, C. Nicolas, S. Randich, P. Sartoretti, R. Smiljanic, P. Tanga, N. Walton, C. Aerts, C. Bailer-Jones, M. Cropper, R. Drimmel, F. Jansen, D. Katz, M. Lattanzi, C. Soubiran, F. Th'evenin, F. V. Leeuwen, R. Andrae, M. Audard, J. Bakker, R. Blomme, J. Castañeda, F. Angeli, C. Fabricius, M. Fouesneau, Y. Fr'emat, L. Galluccio, A. Guerrier, U. Heiter, E.Masana, R. Messineo, K. Nienartowicz, F. Pailler, F. Riclet, W. Roux, R. Sordo, G. Gracia-Abril, J. Portell, M. Altmann, K. Benson, J. Berthier, P. Burgess, D. Busonero, G. Busso, C. Cacciari, H. C'anovas, J. Carrasco, B. Carry, A. Cellino, N. Cheek, G. Clementini, Y. Damerdji, M. Davidson, P. D. Teodoro, L. Delchambre, A. Dell’Oro, E. F. Garcia, D. Garabato, P. Garc'ia-Lario, R. Haigron, N. Hambly, D. Harrison, D. Hatzidimitriou, J. Hern'andez, D. Hestroffer, S. Hodgkin, S. Jamal, G. D. Fombelle, S. Jordan, A. Krone-Martins, A. Lanzafame, W. Loffler, A. Lorca, O. Marchal, P. Marrese, A. Moitinho, K. Muinonen, M. N. Campos, I. Oreshina-Slezak, P. Osborne, E. Pancino, T. Pauwels, A. Recio-Blanco, M. Riello, L. Rimoldini, A. Robin, T. Roegiers, L. M. Sarro, M. Schultheis, M. Smith, A. Sozzetti, E. Utrilla, M. V. Leeuwen, K. Weingrill, U. Abbas, P. 'Abrah'am, A. Aramburu, S. Ahmed, G. Altavilla, M. A. Álvarez, F. Anders, R. I. Anderson, E. A. Varela, T. Antoja, S. Baig, D. Baines, S. Baker, L. Balaguer-N'unez, Z. Balog, C. Barache, M. Barros, M. Barstow, S. Bartolom'e, D. Bashi, J.-L. Bassilana, N. Baudeau, U. Becciani, L. Bedin, I. Bellas-Velidis, M. Bellazzini, William Beordo, M. Bernet, C. Bertolotto, S. Bertone, L. Bianchi, A. Binnenfeld, Sergi Blanco-Cuaresma, J. Bland-Hawthorn, A. Blazère, T. Boch, D. Bossini, S. Bouquillon, A. Bragaglia, J. Braine, E. Bratsolis, E. Breedt, A. Bressan, N. Brouillet, E. Brugaletta, B. Bucciarelli, A. Butkevich, R. Buzzi, A. Camut, R. Cancelliere, T. Cantat-Gaudin, D. C. Guilarte, R. Carballo, T. Carlucci, M. I. Carnerero, J. Carretero, S. Carton, L. Casamiquela, A. Casey, M. Castellani, A. Castro-Ginard, L. Ceraj, V. Cesare, P. Charlot, C. Chaudet, L. Chemin, A. Chiavassa, N. Chornay, D. Chosson, W. J. Cooper, T. Cornez, S. Cowell, M. Crosta, C. Crowley, M. C. Reyes, C. Dafonte, M. D. Ponte, M. David, P. Laverny, F. Luise, R. March, J. D. Ridder, A. Torres, E. F. D. Peloso, M. Delbo, A. Delgado, J. Delisle, C. Demouchy, E. Denis, T. Dharmawardena, F. D. Giacomo, C. Diener, E. Distefano, C. Dolding, K. Dsilva, H. Enke, C. Fabre, M. Fabrizio, S. Faigler, M. Fatovi'c, G. Fedorets, J. Fern'andez-Hern'andez, P. Fernique, F. Figueras, C. Fouron, F. Fragkoudi, M. Gai, M. Galinier, A. Garcia-Serrano, M. Garc'ia-Torres, A. Garofalo, E. Gerlach, R. Geyer, P. Giacobbe, G. Gilmore, S. Girona, G. Giuffrida, A. Gomboc, A. Gomez, I. Gonz'alez-Santamar'ia, E. Gosset, M. Granvik, V. G. Barrera, R. Guti'errez-S'anchez, M. Haywood, A. Helmer, S. L. Hidalgo, T. Hilger, D. Hobbs, C. Hottier, H. Huckle, 'O. Jim'enez-Arranz, J. Campillo, Z. Kaczmarek, P. Kervella, S. Khanna, M. Kontizas, G. Kordopatis, A. Korn, 'A. K'osp'al, Z. Kostrzewa-Rutkowska, K. Kruszy'nska, M. Kun, S. Lambert, A. Lanza, Y. Lebreton, T. Lebzelter, S. Leccia, G. Lecoutre, S. Liao, L. Liberato, E. Licata, E. Livanou, A. Lobel, J. L'opez-Miralles, C. Loup, M. Madar'asz, L. Mahy, R. G. Mann, M. Manteiga, S. Marinoni, C. Marcellino, D. J. Marshall, D. Mascarenhas, J. Marchant, J. M. Lozano, A. Masip, M. Marconi, D. Pina, L. M. Polo, J. Mart'in-Fleitas, A. Mastrobuono-Battisti, P. McMillan, J. Meichsner, J. Merc, S. Messina, N. Millar, A. Mints, D. Mohamed, D. Molina, R. Molinaro, M. Mongui'o, P. Montegriffo, L. Monti, A. Mora, R. Morbidelli, D. Morris, R. Mudimadugula, T. Muraveva, I. Musella, Z. Nagy, N. Nardetto, C. Navarrete, S. Oh, C. Ordenovic, O. Orenstein, C. Pagani, I. Pagano, L. Palaversa, P. Palicio, L. Pallas-Quintela, M. Pawlak, A. Penttila, P. Pesciullesi, M. Pinamonti, E. Plachy, L. Planquart, G. Plum, E. Poggio, D. Pourbaix, A. Price-Whelan, L. Pulone, V. Rabin, M. Rainer, C. Raiteri, P. Ramos, M. Ramos-Lerate, M. Ratajczak, P. Fiorentin, S. Regibo, C. Reyl'e, V. Ripepi, A. Riva, H. Rix, G. Rixon, G. Robert, N. Robichon, C. Robin, M. Romero-G'omez, N. Rowell, D. Mieres, K. Rybicki, G. Sadowski, A. S. Sell'es, N. Sanna, R. Santoveña, M. Sarasso, M. Sarmiento, C. S. Riera, E. Sciacca, D. S'egransan, M. Semczuk, S. Shahaf, A. Siebert, E. Slezak18, R. Smart, O. Snaith, E. Solano, F. Solitro, D. Souami, J. Souchay, E. Spitoni, F. Spoto, L. A. Squillante, I. Steele, H. Steidelmuller, J. Surdej, L. Szabados, F. Taris, M. B. Taylor, R. Teixeira, T. Tepper-García, W. Thuillot, L. Tolomei, N. Tonello, F. Torra, G. T. Elipe, M. Trabucchi, E. Trentin, M. Tsantaki, C. Turon, A. Ulla, N. Unger, I. Valtchanov, O. Vanel, A. Vecchiato, D. Vicente, E. Villar, M. Weiler, H. Zhao, J. Zorec, S. Zucker, A. vZupi'c, T. Zwitter +413 moresemanticscholar +1 more sourceGaia-DR2 asteroid observations and INPOP planetary ephemerides [PDF]
, 2022 We used the INPOP19a planetary ephemerides to perform the orbital adjustment
of 14099 asteroids based on Gaia-DR2 observations, and compare for 23 of them
the resulting orbits to radar data. As Gaia-DR2 has been processed using the
planetary ephemeris INPOP10e, the primary goal of this paper is to confirm the
portability of the data when using an ...arxiv +1 more source