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Photometric Catalogs Surrounding Nearby Core-Collapse Supernovae ("CCSNE")Williams et al. 2018, ApJ, 860, 39
![]() IntroductionCCSNE (HST Proposal #14786) is a high-precision, photometric survey of areas surrounding historic, nearby core-collapse supernovae. The catalogs are used to infer the initial masses of the progenitors by fitting stellar evolution models to the color-magnitude distributions of the resolved stellar populations near the supernovae. Each area is observed in two filters, either F606W+F814W, F435W+F606W, or F438W+F606W. The drizzled mosaics and source catalogs are provided for all the observed fields. You can refer to the full collection of CCSNE data products using the DOI https://doi.org/10.17909/T9X97R.Description of Data ProductsEach of the 18 regions have four files with the following naming convention:
hlsp_ccsne_hst_<ins>_<target>_<filter>_v1_<exten>.fits
where:
Data AccessUsing tools like wget and curl, you can download the CCSNE data products (following the naming convention above) from the url:
https://archive.stsci.edu/hlsps/ccsne/
For example, the following command will download the high confidence star catalog for the NGC 6946-2 primary field:
wget -v -nH -np https://archive.stsci.edu/hlsps/ccsne/hlsp_ccsne_hst_acs-wfc_14786-ngc6946-2_f435w-f606w_v1_st.fits
You can also browse the summary table below to download CCSNE data products and view preview images. |
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