Bibcode
Cami, J.; Cox, N. L.; Farhang, A.; Smoker, J.; Elyajouri, M.; Lallement, R.; Bacalla, X.; Bhatt, N. H.; Bron, E.; Cordiner, M. A.; de Koter, A..; Ehrenfreund, P.; Evans, C.; Foing, B. H.; Javadi, A.; Joblin, C.; Kaper, L.; Khosroshahi, H. G.; Laverick, M.; Le Petit, F..; Linnartz, H.; Marshall, C. C.; Monreal-Ibero, A.; Mulas, G.; Roueff, E.; Royer, P.; Salama, F.; Sarre, P. J.; Smith, K. T.; Spaans, M.; van Loon, J. T..; Wade, G.
Bibliographical reference
The Messenger, vol. 171, p. 31-36
Advertised on:
3
2018
Citations
7
Refereed citations
7
Description
The ESO Diffuse Interstellar Band Large Exploration Survey (EDIBLES) is
a Large Programme that is collecting high-signal-to-noise (S/N) spectra
with UVES of a large sample of O and B-type stars covering a large
spectral range. The goal of the programme is to extract a unique sample
of high-quality interstellar spectra from these data, representing
different physical and chemical environments, and to characterise these
environments in great detail. An important component of interstellar
spectra is the diffuse interstellar bands (DIBs), a set of hundreds of
unidentified interstellar absorption lines. With the detailed
line-of-sight information and the high-quality spectra, EDIBLES will
derive strong constraints on the potential DIB carrier molecules.
EDIBLES will thus guide the laboratory experiments necessary to identify
these interstellar “mystery molecules”, and turn DIBs into
powerful diagnostics of their environments in our Milky Way Galaxy and
beyond. We present some preliminary results showing the unique
capabilities of the EDIBLES programme.