IPP Software Navigation Tools IPP Links Communication Pan-STARRS Links

Ignore:
Timestamp:
Mar 20, 2020, 10:46:42 AM (6 years ago)
Author:
eugene
Message:

various referee comments

File:
1 edited

Legend:

Unmodified
Added
Removed
  • trunk/doc/release.2015/ps1.analysis/response.txt

    r41310 r41312  
    518518are averaged.
    519519
     520** We agree that the organization of this section could be improved,
     521but we disagree a bit with the proposal.  We consider all of these
     522analyses to be forced in that the fits are highly constrained by the
     523stack priors, with their positions (for PSFs and the lensing anaysis)
     524and most of the structural parameters fixed.  In the extended galaxy
     525analysis, each of the grid steps is completely forced, just like in
     526forced PSF photometry.  By using the term 'forced' to describe this
     527process, we would like to make it clear that, for each grid position,
     528the parameters (except normalization) are completely constrained.
     529
     530We have renamed Section 6 as Forced Warp Analysis and split out the
     531PSF vs extended source analysis sections as recommended.  We added
     532some explanation at the end of the section to explain what we mean by
     533'forced'.
     534
    520535- The general description of the section should end with "variant of psphot",
    521536with the motivation being written such that it applies to both the
    522537averaged forced photometry on stars and the averaged single-epoch fits
    523538for galaxies
     539** see previous
    524540
    525541Sec 6.1 (now 6.2):
     
    532548- The terms "skycell" and "warp image" are first used here without
    533549definition. Are warp images the same as CAMERA and CHIP?
    534 **
     550** Updated Section 2 to outline the relevant processing stages and
     551define 'warp', 'skycell', and 'stack' more cleanly.
    535552
    536553- For the forced photometry on single epoch images, is this a joint
    537554fit for overlapping objects?
    538 Are overlapping galaxy models subtracted first? "The PSF model is
    539 fitted..." -> "The amplitude of the PSF model is fitted as the flux..."
     555** for the galaxy models, no.  The galaxy model fits are measured on
     556each object with the other objects subtracted.  Text added to this
     557effect in Section 6.1
     558
     559Are overlapping galaxy models subtracted first?
     560** yes, see above.
     561
     562"The PSF model is fitted..." -> "The amplitude of the PSF model is fitted as the flux..."
     563** fixed the wording here and also clarified below that we measure
     564Kron and aperture fluxes as well.
    540565
    541566Sec 6.2 (now 6.3):
     
    543568parameters are an average of all of the single-epoch measurements.
    544569This should be stated upfront, and then again at the end of the subsection
    545 clarifying how the PSF systematics are removed. Phrases like
     570clarifying how the PSF systematics are removed.
     571
     572Phrases like
    546573"interpolated PSF ellipticities" are confusing, when I *think* what's
    547574being used are "interpolated star ellipticities".
     575** reworded this to make the analysis clearer
    548576
    549577- Was this lensing code used in any of the GREAT challenge papers,
     
    554582- "ie,," -> "ie,"
    555583" absoluate" -> "absolute"
     584** fixed both
    556585
    557586Sec 7:
     
    561590If these questions are covered in other Pan-STARRS papers, please reference
    562591them here.
     592****
    563593
    564594- A basic piece of information that should be given is whether the differencing
    565595is performed on pairs of images, or single (warp) images compared to
    566596image stacks.
     597****
    567598
    568599- "model from is" -> "model is"
     600** fixed
    569601
    570602Conclusions:
Note: See TracChangeset for help on using the changeset viewer.