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Reviewer Response #47

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15 of 23 tasks
djperrefort opened this issue Apr 21, 2020 · 0 comments
Open
15 of 23 tasks

Reviewer Response #47

djperrefort opened this issue Apr 21, 2020 · 0 comments

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@djperrefort
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djperrefort commented Apr 21, 2020

  • Apply spectroscopic classifications (Estimate effeciency of classification #45)

    • How many of these ~400 SN Ia are clearly normal SN Ia?
    • How many have spectra that look more like 91bg-like SN Ia?
    • How many look like SN Ia, but could be 91bg-like at other epochs?
    • What is the FOM?
    • Choose the classification approach (i.e., band v collective v SiFTO) quantitatviely by using the FOM.
  • Double check how SDSS flagged peculiar SNe and update the text accordingly.

  • Clarify which SNe are classificed as peculiar by SDSS and what their classifications are. If shown in the appendix, they should be highlighted in some way.

  • "After visually inspecting the light-curves of each selected target, we disregard any objects that are found to have significantly noisy light-curves, which leaves us with 15 remaining SNe": This should be a cut instead of a pure subjective decision that is not defined at all in the paper, e.g. use the median S/N or the cumulative S/N, or both.

  • Objects in Appendix A should be grouped into the passed and excluded. Excluded objects should include the reason.

  • "having an older average stellar age that the hosts of normal SNe Ia." -> "than the hosts"

  • Please replace LSST with VRO Response: We intend to refer to the survey, not the observatory

  • 2002cx-like SNe, also known as SNe Iax (Li et al. 2003;Jha et al. 2006): add more current references, this has been a topic of significant advances in the last few years.

  • Change "We here " to "We here..."

  • Figure 1: Remove SNeII and unknown classifications.

  • Fig. 4: A few outliers are driving the axis limits, and it is hard to see the details in the central region. In particular the histograms are too small.

  • Fig. 5: The blue and green line are difficult to distinguish.

  • Fig. 4 caption: Clarify how "better" is defined

  • Fig 4 and analysis: Clarify we consider all observed SNe, not just SNe Ia.

  • "We note that three of the four SNe that were visually flagged by the SDSS SN team as potential 91bg-like objects are also labeled as 91bg-like SNe by our classifier."

    • Clarify what "visual" means. From the light curve, or spectra?
    • Fig. 6 is not annotated using open symbols like in Fig. 4
    • What does labeled as 91bg like SNe by the classifier mean? Clarify the bounds.
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