lensing of supernovae by galaxies and galaxy clusters
DESCRIPTION
Lensing of supernovae by galaxies and galaxy clusters. Edvard Mörtsell, Stockholm Jakob Jönsson, Oxford Ariel Goobar; Teresa Riehm, Stockholm. Outline. Lensing of supernovae by galaxies Lensing of supernovae by galaxy clusters. Supernova cosmology. Davis, EM et al (2007). - PowerPoint PPT PresentationTRANSCRIPT
Lensing of supernovae by galaxies and galaxy clusters
Edvard Mörtsell, Stockholm
Jakob Jönsson, Oxford
Ariel Goobar; Teresa Riehm, Stockholm
Edvard Mörtsell, Stockholm University
Outline
• Lensing of supernovae by galaxies
• Lensing of supernovae by galaxy clusters
Edvard Mörtsell, Stockholm University
Davis, EM et al (2007)
SN = Type Ia supernova = SN Ia
Supernova cosmology
Edvard Mörtsell, Stockholm University
Davis, EM et al (2007)
Distance modulus = m – m(empty universe)
Edvard Mörtsell, Stockholm University
Magnitude uncertainties
• Evolution (0.15 mag)
• Intrinsic dispersion (0.15 mag): Gaussian
• Dust (0.15 mag): Increases with redshift
• Gravitational lensing (0.15 mag)– Increases with redshift– Averages out– Can be corrected for
• We need to get down to 0.015 mag
Edvard Mörtsell, Stockholm University
Correcting for lensing
Credit: Riess, STScI
SN 1997ff: The most distant Type Ia supernova at z = 1.755
Relate dark matter to luminous matter:
Estimated magnification: 0.15 mag
Edvard Mörtsell, Stockholm University
Riess et al (2001)
Edvard Mörtsell, Stockholm University
Uncertainties in lensing estimates
• Magnitude limit
• Finite field size
• Redshift and position uncertainties
• Luminous matter to dark matter:– Faber-Jackson and Tully-Fisher relations– Dark matter halo profile and extent
Luminous matter
Edvard Mörtsell, Stockholm University
More supernovae in GOODS fields
Jönsson et al (2006)
Edvard Mörtsell, Stockholm University
Lensing vs Hubble residuals Jönsson et al (2006)
Tentative detection (90 % CL) of correlation
Edvard Mörtsell, Stockholm University
Impact on cosmological fits
• Corrections can decrease the scatter from gravitational lensing by a factor of a few
• The bias introduced is negligible [Jönsson et al (2008)]
• Cosmological constraints from supernovae can be improved by 5-10 %
Edvard Mörtsell, Stockholm University
Davis, EM et al (2007)
Edvard Mörtsell, Stockholm University
Supernovae and halo masses
Correct masses (circles)
Underestimated masses (squares)
Overestimated masses(triangles)
The slope can be used to estimate masseswith 50 % accuracy using 450 SN Ia (SNLS)
Edvard Mörtsell, Stockholm University
Supernovae and galaxy clusters
• Clusters as telescopes
• Explore supernova rates at high redshifts
• Increase leverage of Hubble diagram
• Possibility to measure time delay and absolute magnification
Edvard Mörtsell, Stockholm University
Pilot study
• Near-IR observations ISAAC/VLT (PI: Ariel Goobar)
• SZ and J-band matching archival data
• A1689, A1835, AC114 monitored in spring of 2007
• Magnitude limit SZ < 24 mag (Vega)
• Average magnification in ISAAC field:– A1689: -3 mag– A1835: -1,5 mag– AC114: -1 mag
Edvard Mörtsell, Stockholm University
Goobar et al (2008)
Edvard Mörtsell, Stockholm University
A transient candidate
A1689 archival ISAAC and FORS2 data
Goobar et al (2008)
Type IIp at z = 0.68 magnified > 2 mag
!!!Preliminary!!!
Edvard Mörtsell, Stockholm University
Edvard Mörtsell, Stockholm University
Summary and outlook
• Galaxy lenses harmless for SN Ia cosmology
• SN Ia potentially useful as probes of halo masses
• A successful pilot study looking for supernovae behind cluster telescopes
• Further observation using HAWK-I camera will help constraining supernova rates, dark matter distribution, Hubble constant, dark energy properties…