Re: GL magnification of 97ff (fwd)

From: Ariel Goobar (ariel@physto.se)
Date: Sat Jun 11 2005 - 02:31:59 PDT

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    FYI: during the SCP-meeting last week Jakob and I mentioned that we had
    found an inconsistency in the Benitez et al lensing analysis of 97ff.
    Narciso has now confirmed that we were right. -Ariel

    ---------- Forwarded message ----------
    Date: Fri, 10 Jun 2005 18:10:21 +0200
    From: Narciso Benitez <benitez@iaa.es>
    To: Ariel Goobar <ariel@physto.se>
    Cc: txitxo@pha.jhu.edu, adam riess <ariess@stsci.edu>,
    Subject: Re: GL magnification of 97ff

    Dear Ariel,

       I am afraid that your suspicion is right, I multiplied the velocity
    dispersion obtained from Faber Jackson for the ellipticals by sqrt(2) to
    have the same kind of velocity for all galaxies and then forgot to
    divide by 2 in the formula for the Einstein radius. With the right
    formula the magnification is ~0.16+-0.06.
    Best regards,

      Txitxo

    Ariel Goobar wrote:

    >Dear Narciso and Adam,
    >
    >we are in the process of re-analyzing the GL magnification probability
    >distributions for all GOODS SNe + 97ff. Of course, we will cite your
    >work on 97ff. However, we have found that we are unable to reproduce
    >your result in astro-ph/020709. We think we have found a possible
    >reason for the discrepancy. In table 1 (col 11), you give _circular_
    >velocities for six galaxies, two of which are labeled as being
    >ellipticals. This seems also to be the measure of velocity you use in
    >your definition of the Einstein radius, where you refer to the
    >Bartelmann & Schneider 2001 paper. Now, the definition seems to us to
    >be in conflict with the quoted paper, in which the velocity used in
    >the same expression is the velocity _dispersion_. This equation
    >made us somewhat concerned that you may have mixed-up v_c and v_disp.
    >
    >As a test, we were able to
    >reproduce your results when using your quoted circular velocities as
    >the velocity dispersion. However, if we apply the sqrt(2) factor to the
    >values in col 11 v_c=sqrt(2)*v_disp (as we think one should do),
    >our results differ , and we find less magnification.
    >
    >So here is our question to you: can you specify which Tully-Fisher and
    >Faber-Jackson relations you used to get your final result (0.34 +/- 0.12)?
    >In the last paragraph of the left column in page 2, you say that you use
    >the velocity dispersion. Do you think it is possible that you mixed up
    >the two kinds of velocity? Or do you have some other clue that would
    >explain a lower magnification (~0.2 mag) than what you found?
    >
    >Best regards,
    >
    >Jakob, Christofer and Ariel
    >
    >
    >
    >

    -- 
    ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
    Narciso (Txitxo) Benítez                          |tel:(34)-958-230-606
    Investigador Ramón y Cajal/Ramón y Cajal Scientist|fax:(34)-958-814-530
    

    Instituto de Astrofísica de Andalucía (CSIC) Camino Bajo de Huétor, 24 Granada 18008 Spain ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~



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