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Wavelength dependence in the flux ratio of the double quasar SDSS J1650+4251 A.M. Mosquera (Universidad de Valencia) J.A. Muñoz (Universidad de Valencia)

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Presentation on theme: "Wavelength dependence in the flux ratio of the double quasar SDSS J1650+4251 A.M. Mosquera (Universidad de Valencia) J.A. Muñoz (Universidad de Valencia)"— Presentation transcript:

1 Wavelength dependence in the flux ratio of the double quasar SDSS J1650+4251 A.M. Mosquera (Universidad de Valencia) J.A. Muñoz (Universidad de Valencia) E. Mediavilla (Instituto de Astrofísica de Canarias) R. Barrena (Instituto de Astrofísica de Canarias)

2 Average extinction curves (MW, SMC, LMC) Sample average extinction curves plotted along with the “average” Milky Way curve (CCM with Rv=3.1) (Gordon et al. 2003) The 2175 Å bump is absent in the SMC bar sight lines while in other mesured extinction curves it is prominent. Gravitationally lensed QSOs can be used to determine the extinction law in galaxies where individual stars cannot be resolved.

3 Extinction in high redshift galaxies Z lens = 0.31 Z source = 1.72 Z lens = 0.68 Z source = 0.96 Z lens = 0.89 Z source = 2.51

4 Motta, Mediavilla, Muñoz et al. ApJ 2002 z=0.83

5 Muñoz et al. 2004, ApJ A Survey of Extinction Curves to Redshift z=1. Project provided by NASA through grant #GO-9896 from the STSI, 2003.

6 Observations and analysis Object of study: double quasar SDSS J1650 + 4251, with z = 1.547 (Morgan, Snyder, Reens 2003) Observations: NOT (2.56 m) Wavelength interval: 3510-8130 Å Performed PSF photometry fitting Derive the extinction law of the lens galaxy Discuss the 2175 Å feature I-band Image

7 SDSS J1650+4251 images in 8 different filters I- band (  = 8130Å) Iac#29 (  7015Å) H  6567Å  Iac#28 (  6062Å) Strömgren y (  = 5470Å) Strömgren b (  = 4670Å) Strömgren v (  = 4110Å) Strömgren u (  = 3510Å)

8 I-band image ( = 8130Å) SDSS J1650+4251 Modelled image without LG Residuals

9 Strömgren-u ( = 3510Å) SDSS J1650+4251 Modelled image Residuals

10 Strömgren-y ( = 5470Å) SDSS J1650+4251 Residuals Modelled image

11 SDSS J1650 + 4251 extinction curve

12 Conclusions The existence of the lens galaxy has been well determined in the I-band image. Our results are in agreement with those obtained by Morgan, Snyder, & Reens (2003) We have estimated de extinction law of the galaxy The absence of the 2175 Å feature is clearly confirmed with the strömgren-u data. We have found a galaxy which extinction law behaviour is similar to the SMC

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