To find and download HEASARC data in the cloud, you can use astroquery.heasarc or download our new tool, hark.
The HEASARC and NuSTAR teams are greatly saddened by the sudden passing of Katja Pottschmidt. Most recently Katja was the lead scientist for the NuSTAR Guest Observer Facility (GOF), a role she had supported for many years. During her science career she worked on many other high energy astrophysics missions and played an integral role in advancing our knowledge of the universe. She was a wonderful colleague and friend and will be keenly missed by all who knew her.
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acisabs: Chandra ACIS q.e. decay
This model accounts for the decay in the ACIS quantum efficiency most likely caused by molecular contamination of the ACIS filters. The user needs to supply the number of days between Chandra launch and observation. The acisabs parameters related to the composition of the hydrocarbon and the rate of decay should be frozen and not modified. The present version of acisabs is to be used for the analysis of bare ACIS I and ACIS S data. For the present version of acisabs one must use the standard qe file vN0003 instead of the optional vN0004 file.
Because of the present large uncertainty in the ACIS gain at energies below 350eV we recommend that events in the 0-350eV range be ignored in the spectral analysis until the gain issue is resolved.
acisabs calculates the mass absorption coefficients of the contaminant from atomic scattering factor files provided at
http://henke.lbl.gov/optical_constants/asf.html
| par1 | Days between Chandra launch and ACIS observation |
| par2 | Slope of linear quantum efficiency decay |
| par3 | Offset of linear quantum efficiency decay |
| par4 | Number of carbon atoms in hydrocarbon |
| par5 | Number of hydrogen atoms in hydrocarbon |
| par6 | Number of oxygen atoms in hydrocarbon |
| par7 | Number of nitrogen atoms in hydrocarbon |