NuSTAR CALDB Release Version: 20131007

The CALDB patch contains the following files: 

fpm/caldb.indx
fpm/index/caldb.indx20131007
fpm/bcf/arf/nuA20100101v006.arf
fpm/bcf/arf/nuB20100101v006.arf
fpm/bcf/instrmap/nuAinstrprobmap20100101v001.fits
fpm/bcf/instrmap/nuBinstrprobmap20100101v001.fits
fpm/bcf/instrmap/nuAinstrmap20100101v004.fits
fpm/bcf/instrmap/nuBinstrmap20100101v004.fits
fpm/bcf/pixpos/nuApixpos20100101v007.fits
fpm/bcf/pixpos/nuBpixpos20100101v007.fits
fpm/bcf/psf/nuAgrppsf20100101v001.fits
fpm/bcf/psf/nuBgrppsf20100101v001.fits
fpm/bcf/psf/nuA2dpsfen2_20100101v001.fits
fpm/bcf/psf/nuA2dpsfen1_20100101v001.fits
fpm/bcf/psf/nuA2dpsfen3_20100101v001.fits
fpm/bcf/psf/nuA2dpsfen5_20100101v001.fits
fpm/bcf/psf/nuA2dpsfen4_20100101v001.fits
fpm/bcf/psf/nuB2dpsfen1_20100101v001.fits
fpm/bcf/psf/nuA2dpsfen6_20100101v001.fits
fpm/bcf/psf/nuB2dpsfen3_20100101v001.fits
fpm/bcf/psf/nuB2dpsfen2_20100101v001.fits
fpm/bcf/psf/nuB2dpsfen4_20100101v001.fits
fpm/bcf/psf/nuB2dpsfen6_20100101v001.fits
fpm/bcf/psf/nuB2dpsfen5_20100101v001.fits
fpm/bcf/clock/nuCclock20100101v019.fits
fpm/bcf/instrument/nuBhkrange01_20100101v007.fits
fpm/bcf/instrument/nuAhkrange01_20100101v007.fits
fpm/bcf/instrument/nuBhkrange06_20100101v005.fits
fpm/bcf/instrument/nuBhkrange05_20100101v005.fits
fpm/bcf/instrument/nuBhkrange04_20100101v005.fits
fpm/bcf/instrument/nuBhkrange03_20100101v005.fits
fpm/bcf/instrument/nuBhkrange02_20100101v005.fits
fpm/bcf/instrument/nuAhkrange06_20100101v005.fits
fpm/bcf/instrument/nuAhkrange05_20100101v005.fits
fpm/bcf/instrument/nuAhkrange04_20100101v005.fits
fpm/bcf/instrument/nuAhkrange03_20100101v005.fits
fpm/bcf/instrument/nuAhkrange02_20100101v005.fits

Summary of changes:

ARF:

The NuSTAR ARF has been adjusted to match observations from soft X-ray
observatories (XMM/Swift XRT/Chandra). The new ARFs contain an energy
independent increase in the effective area, resulting in fluxes that
decrease by about 15%.

INSTRMAP:

The instrmap files were updated and a new "probmap" file was included. These
changes were made to support the improved exposure map algorithm in the latest
version of the nupipeline nuexpomap task.

PIXPOS:

Adjusted the PDF for high grades for pixels near the outer edge of the detectors
that had noisy (poor quality) calibration data to have the "Grade 0" PDF.

PSF:

An energy-dependent PSF was included based on observations of bright X-ray point
sources. This energy-dependent PSF is used by the numkarf task and accounts for the
increased scattering of low-energy (<10 keV) photons. This effect is small (on the order
of 5%) and will only be seen for sources with high SNR and when small (<30 arcesecond radius)
extraction regions are used. 

CLOCK:

The clock file has been brought up-to-date and now supports all observations up to 
2013-07-06.

INSTRUMENT:

The hkrange files have been updated to allow for the pipeline to be run when the instrument
metrology system is out of range.