Published November 25, 2016
| Version v1
Journal article
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HST/COS OBSERVATIONS OF IONIZED GAS ACCRETION AT THE DISK-HALO INTERFACE OF M33
- 1. Department of Astronomy, Columbia University
- 2. Space Telescope Science Institute
- 3. Department of Astronomy, University of Washington
Description
Supplementary coadded HST/COS spectra that were processed by three different programs other than the CalCOS (version 3.0). The three codes applied are (1) an IDL routine x1d coadd.pro by Danforth et al. (2010), (2) a spectral co-add code by Wakker et al. (2015), and (3) the PyCOS pipeline by Liang & Chen (2014; & private communication). The spectra of one of the targets, M33-FUV-016, are shown in Appendix B in the Corresponding paper.
Notes
We acknowledge support from the National Science Foundation under Grant No. AST-1410800. J.E.G. Peek and J.K. Werk were supported in part by Hubble Fellowship grants 51295 and 51332, respectively, provided by NASA to STScI.
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Zheng16_M33ACC_supplement.zip
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Additional details
Related works
- Is supplement to
- 10.17909/T9FG6R (DOI)
References
- Danforth et al. (2010). x1d_coadd.pro code, see http://adsabs.harvard.edu/abs/2010ApJ...720..976D
- Wakker et al. (2015). coadded code, see http://adsabs.harvard.edu/abs/2015ApJ...814...40W
- Liang & Chen (2014): PyCOS coadded code, see http://adsabs.harvard.edu/abs/2014MNRAS.445.2061L (and private communication)