May 7 draft comments

From: Alex Conley (aconley@panisse.lbl.gov)
Date: Sat May 10 2003 - 20:22:46 PDT

  • Next message: Alex Conley: "Re: May 7 draft comments"

    I have started reading the may 7th draft. First, I'd like to say
    that this paper started out good and is getting better with each
    iteration. It is wonderfully thorough, especially when compared
    with the Tonry et al. (2003) paper which you are avoiding reading.

    My first, and most substantial comment is about the use of R_B=2.3 in the
    cosmological fits. I have no problem with it per se, but I don't think
    that the comparison should always be between your value of 2.3 and
    Phillips value of 3.5. Phillips value is of the exact same standing as
    your value -- a completely empirical result based only on SNe cosmology
    fitting. Once people have accepted the concept of using a value different
    than what we use in the Milky Way (4.1), they can't really object to you
    finding a different empirical value than Phillips. That is, the
    controversy should all be in departing from the Milky Way law, which
    is the only one we have studied in detail.

      Thus, in Figure 5, when you show the Hubble Diagram, I believe that
    your two panels should be R_B = 4.1 and R_B = 2.3, not 3.5 and 2.3, and
    except when you discuss Phillips directly, your comparisons should always
    be between 4.1 and 2.3.

      Additionally, I think you should add a panel to Figure 11 that shows
    the difference between 4.1 and 2.3 as a source of systematic uncertainty.

      Okay, on to more minor comments (typos and whatnot)

    Abstract: You say in the abstract that only one of the 11 SNe
     is significantly reddened, but in section 3 you say that there
     are two which are clearly reddened (sn1998aw and sn1998as).

    pg 6, column 1, first paragraph : I don't think STScI is ever defined
     as an acronym (although the Space Telescope Science Institute is
     mentioned in the footnote 1)

    pg 6, column 2, paragraph 2
      The 25 denoting footnote 25 has a funny spacing relative to the sentence
     it is in.

    pg 7, column 1, paragraph 1:
      There are a couple citations that should possibly be put in \citep --
      the citation of Holtzmann, Dolphin, and the citation of Fruchter.

    pg 7, column 2, paragraph 1:
      lessim appears -- add a \

    pg 8, column 1, paragraph 1 :
      You say that there are 7 SNe without a color measurement, then say
     this includes (list of 7). Say are, not include.

    pg 8, column 2, paragraph 1 :
      I think it should be 'The first 100 days of each of the three templates
     are listed in Table 2.' instead of 'is listed in Table 2.', but I could
     be wrong.

    pg 8, column 2, paragraph 2 :
      The same include should be are mistake as above for the zero-float
     SNe. That is include -> are, since you list all of them.

    pg 10, column 2, paragraph 2 :
      refsec:dirtylaundry

    pg 13, column 13, paragraph 1 :
      The intrinsic error bar should have units -- -0.04 mag

    pg 13, column 2, paragraph 1 :
    >~ should be replaced with just ~ -- the > is superfluous.

    pg 13, colum 2, paragraph 1 :
      teh -> the

    pg 16, column 1, paragraph 1 :
      timescale in timescale stretch is superfluous -- you have already
     made use of stretch several times in the paper, so if people don't
     already know it has to do with the timescale they are hopelessly
     confused by this point.
     
    pg 16, column 2, paragraph 2 :
     'This reproduction was performed by modifying the spectral template
     exactly as described above' It isn't clear from this sentence what
     you mean by above -- do you use the 'smooth multiplicative function'
     mentioned a few pages back (which, incidentally, should probably be
     described in slighly more detail) or the O'Donnell extinction law
     mentioned in the previous paragraph? People may mistakenly assume
     that the extinction law was used everywhere (which is, after all,
     what Nugent recommends in Nugent, Kim and Perlmutter).

    pg 17, column 2, paragraph 1 :
      Why were different parameter ranges used for extinction corrected
     and non-extinction corrected fits? A little farther down you claim
     that your ranges include 99.99 percent of the probability, so one
     might be led to guess that your expanded range is because your error
     ellipses are that extra bit fatter with extinction correction.
     Looking at the error ellipses, this does appear to be true, but
     it seems worth pointing out that the decision was made for this
     reason.

    pg 17, column 2 :
      /refsec:colorcor

    pg 18, column 1, paragraph 2 :
    > 5 sigma outlier, not outliers, since there is only one object

    pg 19, column 1, paragraph 2 :
      R99 supernovae are not from all a flux -> R99 supernovae are not all
     from a flux

    pg 21, column 1, paragraph 2:
     adpot -> adopt

    pg 23, Table 8
      Empty areas of table, two fit 8s. I'm sure you already know about
     this one.

    pg 27, column 1, paragraph 1 :
     <~ -> \lessim

    pg 27, column 1, paragraph 1 :
     'By itself, the supernova data sets a 99% confidence limit of w < -0.5
     for any positive value of \Omega_{M}. (When a fit with
     extinction corrections applied to the full primary subset
     gives a 95% confidence imit of w < -0.5.)'

     First, the second sentence isn't a sentence (When what?). Second,
     it isn't clear what the data sample in the first sentence is.
     Is is all SNe without extinction correction applied?

    pg 27, column 2, paragraph 2 :
     distance reduced distance

    Okay, that's as far as I have read. The downside to this being such
    a thorough paper is that it's hard to read straight through, so I'll
    take a break and look at the rest later.

    Alex



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