SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:su-80707"
 

Search: onr:"swepub:oai:DiVA.org:su-80707" > The ESO/VLT 3rd yea...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

The ESO/VLT 3rd year Type Ia supernova data set from the supernova legacy survey

Balland, C. (author)
Baumont, S. (author)
Basa, S. (author)
show more...
Mouchet, M. (author)
Howell, D. A. (author)
Astier, P. (author)
Carlberg, R. G. (author)
Conley, A. (author)
Fouchez, D. (author)
Guy, J. (author)
Hardin, D. (author)
Hook, I. M. (author)
Pain, R. (author)
Perrett, K. (author)
Pritchet, C. J. (author)
Regnault, N. (author)
Rich, J. (author)
Sullivan, M. (author)
Antilogus, P. (author)
Arsenijevic, V. (author)
Le Du, J. (author)
Fabbro, S. (author)
Lidman, Chris (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Mourao, A. (author)
Palanque-Delabrouille, N. (author)
Pecontal, E. (author)
Ruhlmann-Kleider, V. (author)
show less...
 (creator_code:org_t)
2009-08-27
2009
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 507:1, s. 85-103
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Aims. We present 139 spectra of 124 Type Ia supernovae (SNe Ia) that were observed at the ESO/VLT during the first three years of the Canada-France-Hawa Telescope (CFHT) supernova legacy survey (SNLS). This homogeneous data set is used to test for redshift evolution of SN Ia spectra, and will be used in the SNLS 3rd year cosmological analyses. Methods. Spectra have been reduced and extracted with a dedicated pipeline that uses photometric information from deep CFHT legacy survey (CFHT-LS) reference images to trace, at sub-pixel accuracy, the position of the supernova on the spectrogram as a function of wavelength. It also separates the supernova and its host light in similar to 60% of cases. The identification of the supernova candidates is performed using a spectrophotometric SN Ia model. Results. A total of 124 SNe Ia, roughly 50% of the overall SNLS spectroscopic sample, have been identified using the ESO/VLT during the first three years of the survey. Their redshifts range from z = 0.149 to z = 1.031. The average redshift of the sample is z = 0.63 +/- 0.02. This constitutes the largest SN Ia spectral set to date in this redshift range. The spectra are presented along with their best-fit spectral SN Ia model and a host model where relevant. In the latter case, a host subtracted spectrum is also presented. We produce average spectra for pre-maximum, maximum and post-maximum epochs for both z < 0.5 and z >= 0.5 SNe Ia. We find that z < 0.5 spectra have deeper intermediate mass element absorptions than z = 0.5 spectra. The differences with redshift are consistent with the selection of brighter and bluer supernovae at higher redshift.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

cosmology: observations
supernovae: general
methods: data analysis
techniques: spectroscopic

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view