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kbastroutils

  • 2.6.2
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KBAstroUtils

This is a collection of modules for analyses related to astrophysics by Dr. Kornpob Bhirombhakdi. Contact: kbhirombhakdi@stsci.edu

Tasks include:

- dqmask.py = handle data quality (DQ) arrays

- container.py = handle declaring attibutes given keys and values

- segmentation.py = wrapper for making a segmentation map (used to be source.py in version < 1.2.0)

- sub2full.py = mapping a subarray image back to its full frame

- gnd.py = wrapper, and main class for grism reduction

- grismconf.py = read conf file for grism reduction

- grismsens.py = read sens file for grism reduction

- grismapcorr.py = read aperture correction table, and calculate aperture correction factor

- grismmeta.py = construct meta info

- make_sip.py = calculate Simple Imaging Polynomial (SIP)

- photapcorr.py = read photometric calibration table, and prepare calibration factors (i.e., encircled energy correction, and photometric AB zeropoint)

- mag2flux.py = converting ABmag to flam

Known issues:

- ACS photometric zeropoints are set to 0.

- Memory

- No description/documentation

- Handling other telescopes

- flux2mag.py

- AB2Vega.py

- Vega2AB.py

- WFC3 subarray

- drz gets brighter about 10%

- test new code with ACS-WFC, and other WFC3-IR

Next

- Combine 1D spectra

- Use assertion for error handling (http://swcarpentry.github.io/python-novice-inflammation/09-defensive/index.html)

- HST-ACS-WFC flux calibration

- Fix drz getting brigther

v.2.5.0

- Implement ACS subarray

- Implement ('HST','ACS','WFC') as identifier

- Implement grismcrclean.py, grismmodel.py, grismcalibpath.py, grismdrz.py

- Change grismconf.py, grismsens.py, gnd.py, dqmask.py

v.2.4.0

- Implement grismmeta.py

- HST-ACS-WFC is available for wavelength calibration, but not flux calibration

- HST-ACS-WFC subarray is applicable

- Change the construction of GrismCONF, and GrismSens

v.2.3.0

- GND.make_pairs(pairs=None) can automatically make pairs

- GND.make_xyd(xyd=None, init=init, inittype='radec') can automatically find a centroid given init

- GND.show(method='meta', output=True) returns the table instead of displaying it

- GND.make_drz() is deactivated

v.2.2.0

- GND.save takes filename

- Fix GND.show(method='flam') handling xmin, xmax

- GND.show(method='stamp') takes dqon

v.2.1.0

- Add functionalities in GND.show(method='clean', traceon=True, zoom=True)

- Implement: photapcorr.py, mag2flux.py

v.2.0.0

- New APIs: gnd.py

- Demo provided

- Implement: grismapcorr.py, make_sip.py

v.1.3.1

- Fix import

v.1.3.0

- Implement: grismconf.py, gnd.py, grismsens.py

v.1.2.0

- Implement: sub2full.py

- Change: source.py to segmentation.py

- Fix description: segmentation.py

v.1.1.0

- Implement: container.py, source.py

- Fix description: dqmask.py

v.1.0.2

- Fix description of dqmask.py

v.1.0.1

- Fix import modules in dqmask.py

v.1.0.0

- Implement dqmask.py

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