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Recent Submissions

  • Nantais, JB; Van der Burge, RFJ; Lidman, C; Demarco, R; Noble, A; Wilson, G; Muzzin, A; Foltz, R; DeGroot, A; Cooper, MC (EDP SCIENCES, 2016-08)
    We present the stellar mass functions (SMFs) of passive and star-forming galaxies with a limiting mass of 10(10.1) M-circle dot in four spectroscopically confirmed Spitzer Adaptation of the Red-sequence Cluster Survey ...
  • Osorio, MRZ; Lodieu, N; Bejar, VJS; Martin, EL; Ivanov, VD; Bayo, A; Boffin, HMJ; Muzic, K; Minniti, D; Beamin, JC (EDP SCIENCES, 2016-08)
    Aims. We aim at obtaining near-infrared photometry and deriving the mass, age, temperature, and surface gravity of WISE J085510.74 071442.5 (J0855 0714), which is the coolest object beyond the solar system currently known. ...
  • Zarate, X; Schott, E; Escobar, CA; Lopez-Castro, R; Echeverria, C; Alvarado-Soto, L; Ramirez-Tagle, R (Sociedade Brasileira de Química, 2016-09)
    Chalcones are open chain molecules precursors of flavonoids and isoflavonoids, found spread in edible plants. Because they are easily accessible trough Claisen Shmidt condensation, a great variety of derivatives are ...
  • Romano, P; Bozzo, E; Esposito, P; Sbarufatti, B; Haberl, F; Ponti, G; D'Avanzo, P; Ducci, L; Segreto, A; Jin, C; Masetti, N; Del Santo, M; Campana, S; Mangano, V (EDP SCIENCES, 2016-09)
    Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival / serendipitous ...
  • Majaess, D; Turner, D; Dekany, I; Minniti, D; Gieren, W (EDP SCIENCES, 2016-09)
    Near-infrared color-excess and extinction ratios are essential for establishing the cosmic distance scale and probing the Galaxy, particularly when analyzing targets attenuated by significant dust. A robust determination ...
  • Bluhm, P; Jones, MI; Vanzi, L; Soto, MG; Voss, J; Wittenmyer, RA; Drass, H; Jenkins, JS; Olivares, F; Mennickent, RE; Vuckovic, M; Rojo, P; Melo, CHF (EDP SCIENCES, 2016-09)
    We report the discovery of 24 spectroscopic binary companions to giant stars. We fully constrain the orbital solution for 6 of these systems. We cannot unambiguously derive the orbital elements for the remaining stars ...
  • Braibant, L; Hutsemekers, D; Sluse, D; Anguita, T (EDP SCIENCES, 2016-07)
    We investigate the kinematics and ionization structure of the broad emission line region of the gravitationally lensed quasar QSO2237 + 0305 (the Einstein cross) using differential microlensing in the high-and low-ionization ...
  • Tissera, PB; Machado, REG; Sanchez-Blazquez, P; Pedrosa, SE; Sanchez, SF; Snaith, O; Vilchez, JM (EDP SCIENCES, 2016-08)
    Context. The stellar metallicity gradients of disc galaxies provide information on disc assembly, star formation processes, and chemical evolution. They also might store information on dynamical processes that could affect ...
  • Minniti, D; Ramos, RC; Zoccali, M; Rejkuba, M; Gonzalez, OA; Valenti, E; Gran, F (IOP PUBLISHING, 2016-10)
    Galactic nuclei, such as that of the Milky Way, are extreme regions with high stellar densities, and in most cases, the hosts of a supermassive black hole. One of the scenarios proposed for the formation of the Galactic ...
  • Ingallinera, A; Trigilio, C; Leto, P; Umana, G; Buemi, C; Bufano, F; Agliozzo, C; Riggi, S; Flagey, N; Silva, K; Cerrigone, L; Cavallaro, F (OXFORD UNIV PRESS, 2016-11)
    We present radio observations of 18 MIPSGAL bubbles performed at 5 GHz (6 cm) with the Karl G. Jansky Very Large Array in configuration B and BnA. The observations were aimed at understanding what kind of information ...
  • Molina, CN; Borissova, J; Catelan, M; Alonso-Garcia, J; Kerins, E; Kurtev, R; Lucas, PW; Medina, N; Minniti, D; Dekany, I (OXFORD UNIV PRESS, 2016-10)
    The Quintuplet cluster is one of the most massive star clusters in the Milky Way, situated very close to the Galactic Centre. We present a new search for variable stars in the vicinity of the cluster, using the five-year ...
  • Smartt, SJ; Chambers, KC; Smith, KW; Huber, ME; Young, DR; Cappellaro, E; Wright, DE; Coughlin, M; Schultz, ASB; Denneau, L; Flewelling, H; Heinze, A; Magnier, EA; Primak, N; Rest, A; Sherstyuk, A; Stalder, B; Stubbs, CW; Tonry, J; Waters, C; Willman, M; Anderson, JP; Baltay, C; Botticella, MT; Campbell, H; Dennefeld, M; Chen, TW; Della Valle, M; Elias-Rosa, N; Fraser, M; Inserra, C; Kankare, E; Kotak, R; Kupfer, T; Harmanen, J; Galbany, L; Gal-Yam, A; Le Guillou, L; Lyman, JD; Maguire, K; Mitra, A; Nicholl, M; Olivares, F; Rabinowitz, D; Razza, A; Sollerman, J; Smith, M; Terreran, G; Valenti, S; Gibson, B; Goggia, T (OXFORD UNIV PRESS, 2016-11)
    We searched for an optical counterpart to the first gravitational-wave source discovered by LIGO (GW150914), using a combination of the Pan-STARRS1 wide-field telescope and the Public ESO Spectroscopic Survey of Transient ...
  • Borissova, J.; Ramírez Alegría, S.; Alonso, J.; Lucas, P. W.; Kurtev, R.; Medina, N.; Navarro, C.; Kuhn, M.; Gromadzki, M.; Retamales, G.; Fernandez, M. A.; Agurto-Gangas, C.; Chené, A.-N.; Minniti, D.; Contreras Pena, C.; Catelan, M.; Decany, I.; Thompson, M. A.; Morales, E. F. E.; Amigo, P. (IOP PUBLISHING, 2016-09)
    The purpose of this research is to study the connections of the global properties of eight young stellar clusters projected in the Vista Variables in the Via Lactea (VVV) ESO Large Public Survey disk area and their young ...
  • Foley, Ryan J.; Pan, Yen-Chen; Brown, P.; Filippenko, A. V.; Fox, O. D.; Hillebrandt, W.; Kirshner, R. P.; Marion, G. H.; Milne, P. A.; Parrent, J. T.; Pignata, G.; Stritzinger, M. D. (OXFORD UNIV PRESS, 2016-06)
    Ultraviolet (UV) observations of Type Ia supernovae (SNe Ia) probe the outermost layers of the explosion, and UV spectra of SNe Ia are expected to be extremely sensitive to differences in progenitor composition and the ...
  • Casey, A. R.; Ruchti, G.; Masseron, T.; Randich, S.; Gilmore, G.; Lind, K.; Kennedy, G. M.; Koposov, S. E.; Hourihane, A.; Franciosini, E.; Lewis, J. R.; Magrini, L.; Morbidelli, L.; Sacco, G. G.; Worley, C. C.; Feltzing, S.; Jeffries, R. D.; Vallenari, A.; Bensby, T.; Bragaglia, A.; Flaccomio, E.; Francois, P.; Korn, A. J.; Lanzafame, A.; Pancino, E.; Recio-Blanco, A.; Smiljanic, R.; Carraro, G.; Costado, M. T.; Damiani, F.; Donati, P.; Frasca, A.; Jofre, P.; Lardo, C.; de Laverny, P.; Monaco, L.; Prisinzano, L.; Sbordone, L.; Sousa, S. G.; Tautvaisien, G.; Zaggia, S.; Zwitter, T.; Delgado Mena, E.; Chorniy, Y.; Martell, S. L.; Silva Aguirre, V.; Miglio, A.; Chiappini, C.; Montalban, J.; Morel, T.; Valentini, M. (OXFORD UNIV PRESS, 2016-07)
    The discovery of lithium-rich giants contradicts expectations from canonical stellar evolution. Here we report on the serendipitous discovery of 20 Li-rich giants observed during the Gaia-ESO Survey, which includes the ...
  • Carballo-Bello, Julio A.; Ramírez Alegría, S.; Borissova, J.; Smith, L. C.; Kurtev, R.; Lucas, P. W.; Moni Bidin, Ch.; Alonso-García, J.; Minniti, D.; Palma, T.; Dékány, I.; Medina, N.; Moyano, M.; Villanueva, V.; Kuhn, M. A. (OXFORD UNIV PRESS, 2016-10)
    We present deep near-infrared photometry and spectroscopy of the globular cluster 2MASS-GC 03 projected in the Galactic disc using MMT and Magellan Infrared Spectrograph on the Clay Telescope (Las Campanas Observatory) and ...
  • Delgado, A. J.; Sampedro, L.; Alfaro, E. J.; Costado, M. T.; Yun, J. L.; Frasca, A.; Lanzafame, A. C.; Drew, J. E.; Eislöffel, J.; Blomme, R.; Morel, T.; Lobel, A.; Semaan, T.; Randich, S.; Jeffries, R. D.; Micela, G.; Vallenari, A.; Kalari, V.; Gilmore, G.; Flaccomio, E.; Carraro, G.; Lardo, C.; Monaco, L.; Prisinzano, L.; Sousa, S. G.; Morbidelli, L.; Lewis, J.; Koposov, S.; Hourihane, A.; Worley, C.; Casey, A.; Franciosini, E.; Sacco, G.; Magrini, L. (OXFORD UNIV PRESS, 2016-05)
    The young open cluster NGC3293 is included in the observing program of the Gaia-ESO survey (GES). The radial velocity values provided have been used to assign cluster membership probabilities by means of a single-variable ...
  • Villanova, S.; Monaco, L.; Moni Bidin, C.; Assmann, P. (OXFORD UNIV PRESS, 2016-08)
    We present the abundance analysis for a sample of 18 red giant branch stars in the metal-poor globular cluster NGC 4147 based on medium- and high-resolution spectra. This is the first extensive spectroscopic study of this ...
  • Takáts, K.; Pignata, G.; Bersten, M.; Rojas Kaufmann, M. L.; Anderson, J. P.; Folatelli, G.; Hamuy, M.; Stritzinger, M.; Haislip, J. B.; LaCluyze, A. P.; Moore, J. P.; Reichart, D. (OXFORD UNIV PRESS, 2016-08)
    We present optical photometric and spectroscopic observations of the 1987A-like supernova (SN) 2009mw. Our BVRI and g ' r ' i ' z ' photometry covers 167 d of evolution, including the rise to the light-curve maximum, and ...
  • Folatelli, Gastón; Van Dyk, Schuyler D.; Kuncarayakti, Hanindyo; Maeda, Keiichi; Bersten, Melina C.; Nomoto, Ken'ichi; Pignata, Giuliano; Hamuy, Mario; Quimby, Robert M.; Zheng, WeiKang; Filippenko, Alexei V.; Clubb, Kelsey I.; Smith, Nathan; Elias-Rosa, Nancy; Foley, Ryan J.; Miller, Adam A. (IOP PUBLISHING, 2016-07)
    Supernova (SN) iPTF13bvn in NGC 5806 was the first Type Ib SN to have been tentatively associated with a progenitor in pre-explosion images. We performed deep ultraviolet (UV) and optical Hubble Space Telescope observations ...

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