GRB 050915a & the Virgo detector

The analysis can be divided into two main parts: the study of the abundance pattern in the host galaxy measured by the afterglow absorption lines, and the study of the ionised

The pres- ence of strong stellar absorption features coupled with a weak [O ii ] emission line in the X-Shooter spectrum suggest that the host galaxy candidate is a low-mass member

The overall observed tem- poral properties of this burst, including the broad X-ray bump detected at late times, could be explained in the context of a standard afterglow

9 As outlined in these brief summaries, the role of science in Professional Foul and Hapgood has much in common with Stoppard’s use of chaos theory in Arcadia, since catastrophe

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

As it will be explained, Virgo is not a bare Michelson interferometer; several optical components are used in addition to the classical 50% reflecting beam splitter (BS) and

Finally, section VI deals with the main software tools developed for the online detector monitoring which is a mandatory complement of data

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