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Supernovae and Gaia

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Abstract

Despite decades of dedicated efforts there are still basic questions to answer with regard to Supernova progenitor systems and explosion mechanisms. In particular, in the last years a number of exceptionally bright objects and extremely faint events have demonstrated an unexpected large Supernova variety.

The large number of Supernovae candidates at different redshifts provided by the next generation surveys, from ground and space, will allow to reach a better insight of the Supernova events in all their flavours. In particular it will be the possible to assess the systematics of type Ia Supernovae as distance indicator at any redshift.

The Gaia astrometric mission is expected to discover a huge number of transient events, including Supernovae, which will be immediately disseminated to the astronomical community by a transients alert system for a suitable follow up.

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Notes

  1. SN 1998bw & GRB 980425 (z=0.0085) (Galama et al. 1998); SN 2003dh & GRB 030329 (z=0.17) (Stanek et al. 2003; Hjorth et al. 2003; Matheson et al. 2003); SN 2003lw & GRB 031202 (z=0.1) (Malesani et al. 2004); SN 2006aj & GRB060218 (z=0.033) (Campana et al. 2006; Pian et al. 2006); SN 2008hw & GRB081007 (z=0.53) (Della Valle et al. 2008), SN2010bh & GRB100316D at z=0.0593 (Chornock et al. 2010; Starling et al. 2011).

  2. SN 2003fg SN 2006gz, SN 2007if, and SN 2009dc.

  3. to be noted that our estimate is based on the SN announced on CBETS and listed in http://www.cbat.eps.harvard.edu/lists/Supernovae.html. A not negligible number of SNe discovered by modern searches are not present in that list.

  4. http://pan-starrs.ifa.hawaii.edu/public/home.html.

  5. http://www.astro.caltech.edu/~avishay/zwicky1/ppts/-Price.pdf.

  6. http://ps1sc.org/transients/.

  7. http://www.lsst.org/lsst/.

  8. http://www.lsst.org/files/docs/aas/2006/WangL.pdf.

  9. http://www.lsst.org/lsst/science/scientist_transient.

  10. http://sci.esa.int/science-e/www/area/index.cfm?fareaid=26.

  11. And each observation consist on a transit on 9 CCD, with an integration time of 4.4 s per CCD.

  12. The precessional period is 63 days long.

  13. See the Gaia Science Alerts Working Group wiki http://www.ast.cam.ac.uk/ioa/research/gsawg.

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  1. INAF—Osservatorio Astronomico di Bologna, Bologna, Italy

    Giuseppe Altavilla

  2. INAF—Osservatorio Astronomico di Padova, Padova, Italy

    Maria Teresa Botticella & Enrico Cappellaro

  3. INAF—Osservatorio Astronomico di Trieste, Trieste, Italy

    Massimo Turatto

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Altavilla, G., Botticella, M.T., Cappellaro, E. et al. Supernovae and Gaia. Astrophys Space Sci 341, 163–178 (2012). https://doi.org/10.1007/s10509-012-1017-6

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