Browsing by Author "Dennefeld, M."

Now showing items 1-3 of 3

    • Erratum: On the diversity of superluminous supernovae: ejected mass as the dominant factor 
      Nicholl, M.; Smartt, S. J.; Jerkstrand, A.; Inserra, C.; Sim, S. A.; Chen, T. W.; Benetti, S.; Fraser, M.; Gal Yam, Avishay; Kankare, E.; Maguire, K.; Smith, K.; Sullivan, M.; Valenti, S.; Young, D. R.; Baltay, C.; Bauer, F. E.; Baumont, S.; Bersier, D.; Botticella, M.-T.; Childress, M.; Dennefeld, M.; Valle, M. Della; Elías-Rosa, N.; Feindt, U.; Galbany, Lluis; Hadjiyska, E.; Le Guillou, L.; Leloudas, G.; Mazzali, P.; McKinnon, R.; Polshaw, J.; Rabinowitz, D.; Rostami, S.; Scalzo, R.; Schmidt, B. P.; Schulze, Steve; Sollerman, J.; Taddia, F.; Yuan, F. (Royal Astronomical Society, 2016)
      This is an erratum to the paper ‘On the diversity of superluminous supernovae: ejected mass as the dominant factor’, published in MNRAS, 2015, 452.
    • On the diversity of superluminous supernovae: ejected mass as the dominant factor 
      Nicholl, M.; Smartt, S. J.; Jerkstrand, A.; Inserra, C.; Sim, S. A.; Chen, T. W.; Benetti, S.; Fraser, M.; Gal Yam, Avishay; Kankare, E.; Maguire, K.; Smith, K.; Sullivan, M.; Valenti, S.; Young, D. R.; Baltay, C.; Bauer, F. E.; Baumont, S.; Bersier, D.; Botticella, M. T.; Childress, M.; Dennefeld, M.; Della Valle, Massimo; Elias Rosa, N.; Feindt, U.; Galbany, Lluis; Hadjiyska, E.; Le Guillou, L.; Leloudas, G.; Mazzali, P.; McKinnon, R.; Polshaw, J.; Rabinowitz, D.; Rostami, S.; Scalzo, R.; Schmidt, B. P.; Schulze, S.; Sollerman, J.; Taddia, F.; Yuan, F. (Oxford University Press, 2015)
      We assemble a sample of 24 hydrogen-poor superluminous supernovae (SLSNe). Parameterizing the light-curve shape through rise and decline time-scales shows that the two are highly correlated. Magnetar-powered models can ...
    • Potential asteroid discoveries by the ESA gaia misión results from follow-up observations 
      Carry, B.; Thuillot, W.; Spoto, F.; David, P.; Berthier, J.; Tanga, P.; Mignard, F.; Bouquillon, S.; Méndez Bussard, René Alejandro; Rivet, J. P.; Le Van Suu, A.; Dell’Oro, A.; Fedorets, G.; Frezouls, B.; Granvik, M.; Guiraud, J.; Muinonen, K.; Panem, C.; Pauwels, T.; Roux, W.; Walmsley, G.; Petit, J. M.; Abe, L.; Ayvazian, V.; Baillié, K.; Baransky, A.; Bendjoya, P.; Dennefeld, M.; Desmars, J.; Eggl, S.; Godunova, V.; Hestroffer, D.; Inasaridze, R.; Kashuba, V.; Krugly, Y. N.; Molotov, I. E.; Robert, V.; Simon, A.; Sokolov, I.; Souami, D.; Tarady, V.; Taris, F.; Troianskyi, V.; Vasylenko, V.; Vernet, D. (EDP Sciences, 2021)
      Context. Since July 2014, the Gaia mission of the European Space Agency has been surveying the entire sky down to magnitude 20.7 in the visible. In addition to the millions of daily observations of stars, thousands of ...