Published March 6, 2019 | Version v0.0.2
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atomneb/AtomNeb-idl: AtomNeb-idl.0.0.2

  • 1. University of Michigan

Description

AtomNeb - IDL/GDL Library for Atomic Data of Ionized Nebulae

AtomNeb is a database containing atomic data stored in FITS file format generated for for spectral analysis. The AtomNeb IDL Library is equipped with several API functions developed in Interactive Data Language (IDL) or GNU Data Language (GDL), which can be usedto read atomic data from the AtomNeb FITS files. The API functions of the AtomNeb IDL Library, together with the proEQUIB IDL Library, can be used to carry out plasma diagnostics and abundance analysis of spectra emitted from ionized nebulae.

Citation

@article{Danehkar2019,
  author = {{Danehkar}, Ashkbiz},
  title = {AtomNeb: IDL Library for Atomic Data of Ionized Nebulae},
  journal = {Journal of Open Source Software},
  volume = {4},
  number = {35},
  pages = {898},
  year = {2019},
  doi = {10.21105/joss.00898}
}

 

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References

  • Arabas, S., Schellens, M., Coulais, A., Gales, J., & Messmer, P. (2010). GNU Data Language (GDL) - a free and open-source implementation of IDL. In EGU general assembly conference, Geophysical research abstracts (Vol. 12, p. 924).
  • Coulais, A., Schellens, M., Gales, J., Arabas, S., Boquien, M., Chanial, P., Messmer, P., et al. (2010). Status of GDL - GNU Data Language. In Y. Mizumoto, K.-I. Morita, & M. Ohishi (Eds.), Astronomical data analysis software and systems xix, Astronomical society of the pacific conference series (Vol. 434, p. 187).
  • Danehkar, A. (2014). Evolution of Planetary Nebulae with WR-type Central Stars (PhD thesis). Macquarie University, Australia.
  • Danehkar, A. (2018a). proEQUIB: IDL Library for Plasma Diagnostics and Abundance Analysis. The Journal of Open Source Software, 3, 899. doi:10.21105/joss.00899
  • Danehkar, A. (2018b). Bi-Abundance Ionisation Structure of the Wolf-Rayet Planetary Nebula PB 8. Publications of the Astronomical Society of Australia, 35, e005. doi:10.1017/pasa.2018.1
  • Danehkar, A., Parker, Q. A., & Ercolano, B. (2013). Observations and three-dimensional ionization structure of the planetary nebula SuWt 2. Monthly Notices of the Royal Astronomical Society, 434, 1513–1530. doi:10.1093/mnras/stt1116
  • Danehkar, A., Parker, Q. A., & Steffen, W. (2016). Fast, Low-ionization Emission Regions of the Planetary Nebula M2-42. The Astronomical Journal, 151, 38. doi:10.3847/0004-6256/151/2/38
  • Danehkar, A., Todt, H., Ercolano, B., & Kniazev, A. Y. (2014). Observations and three-dimensional photoionization modelling of the Wolf-Rayet planetary nebula Abell 48. Monthly Notices of the Royal Astronomical Society, 439, 3605–3615. doi:10.1093/mnras/stu203
  • Davey, A. R., Storey, P. J., & Kisielius, R. (2000). Recombination coefficients for C II lines. Astronomy and Astrophysicss, 142, 85–94. doi:10.1051/aas:2000139
  • Dere, K. P., Landi, E., Young, P. R., Del Zanna, G., Landini, M., & Mason, H. E. (2009). CHIANTI - an atomic database for emission lines. IX. Ionization rates, recombination rates, ionization equilibria for the elements hydrogen through zinc and updated atomic data. Astronomy and Astrophysics, 498, 915–929. doi:10.1051/0004-6361/200911712
  • Ercolano, B., Barlow, M. J., & Storey, P. J. (2005). The dusty MOCASSIN: fully self-consistent 3D photoionization and dust radiative transfer models. Monthly Notices of the Royal Astronomical Society, 362, 1038–1046. doi:10.1111/j.1365-2966.2005.09381.x
  • Ercolano, B., Barlow, M. J., Storey, P. J., & Liu, X.-W. (2003). MOCASSIN: a fully three-dimensional Monte Carlo photoionization code. Monthly Notices of the Royal Astronomical Society, 340, 1136–1152. doi:10.1046/j.1365-8711.2003.06371.x
  • Ercolano, B., Young, P. R., Drake, J. J., & Raymond, J. C. (2008). X-Ray Enabled MOCASSIN: A Three-dimensional Code for Photoionized Media. The Astrophysical Journal Supplement Series, 175, 534–542. doi:10.1086/524378
  • Escalante, V., & Victor, G. A. (1990). Effective recombination coefficients of neutral carbon and singly ionized nitrogen. The Astrophysical Journal Supplement Series, 73, 513–553. doi:10.1086/191479
  • Fang, X., Storey, P. J., & Liu, X.-W. (2011). New effective recombination coefficients for nebular N ii lines. Astronomy and Astrophysics, 530, A18. doi:10.1051/0004-6361/201116511
  • Fang, X., Storey, P. J., & Liu, X.-W. (2013). New effective recombination coefficients for nebular N II lines (Corrigendum). Astronomy and Astrophysics, 550, C2. doi:10.1051/0004-6361/201116511e
  • Ferland, G. J., Korista, K. T., Verner, D. A., Ferguson, J. W., Kingdon, J. B., & Verner, E. M. (1998). CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra. Publications of the Astronomical Society of the Pacific, 110, 761–778. doi:10.1086/316190
  • Hanisch, R. J., Farris, A., Greisen, E. W., Pence, W. D., Schlesinger, B. M., Teuben, P. J., Thompson, R. W., et al. (2001). Definition of the Flexible Image Transport System (FITS). Astronomy and Astrophysics, 376, 359–380. doi:10.1051/0004-6361:20010923
  • Howarth, I. D., & Adams, S. (1981). Program EQUIB. University College London.
  • Howarth, I. D., Adams, S., Clegg, R. E. S., Ruffle, D. P., Liu, X.-W., Pritchet, C. J., & Ercolano, B. (2016). EQUIB: Atomic level populations and line emissivities calculator. Astrophysics Source Code Library, ascl:1603.005.
  • Kallman, T., & Bautista, M. (2001). Photoionization and High-Density Gas. The Astrophysical Journal Supplement Series, 133, 221–253. doi:10.1086/319184
  • Kisielius, R., Storey, P. J., Davey, A. R., & Neale, L. T. (1998). Recombination coefficients for Ne Ii lines at nebular temperatures and densities. Astronomy and Astrophysicss, 133, 257–269. doi:10.1051/aas:1998319
  • Landi, E., Del Zanna, G., Young, P. R., Dere, K. P., & Mason, H. E. (2012). CHIANTI-An Atomic Database for Emission Lines. XII. Version 7 of the Database. The Astrophysical Journal, 744, 99. doi:10.1088/0004-637X/744/2/99
  • Landi, E., Del Zanna, G., Young, P. R., Dere, K. P., Mason, H. E., & Landini, M. (2006). CHIANTI-An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements. The Astrophysical Journal Supplement Series, 162, 261–280. doi:10.1086/498148
  • Landsman, W. B. (1993). The IDL Astronomy User's Library. In R. J. Hanisch, R. J. V. Brissenden, & J. Barnes (Eds.), Astronomical data analysis software and systems ii, Astronomical society of the pacific conference series (Vol. 52, p. 246).
  • Landsman, W. B. (1995). The IDL Astronomy User's Library. In R. A. Shaw, H. E. Payne, & J. J. E. Hayes (Eds.), Astronomical data analysis software and systems iv, Astronomical society of the pacific conference series (Vol. 77, p. 437).
  • Liu, X.-W., Storey, P. J., Barlow, M. J., & Clegg, R. E. S. (1995). The rich O II recombination spectrum of the planetary nebula NGC 7009: new observations and atomic data. Monthly Notices of the Royal Astronomical Society, 272, 369–388. doi:10.1093/mnras/272.2.369
  • Luridiana, V., Morisset, C., & Shaw, R. A. (2015). PyNeb: a new tool for analyzing emission lines. I. Code description and validation of results. Astronomy and Astrophysics, 573, A42. doi:10.1051/0004-6361/201323152
  • Pence, W. D., Chiappetti, L., Page, C. G., Shaw, R. A., & Stobie, E. (2010). Definition of the Flexible Image Transport System (FITS), version 3.0. Astronomy and Astrophysics, 524, A42. doi:10.1051/0004-6361/201015362
  • Pequignot, D., Petitjean, P., & Boisson, C. (1991). Total and effective radiative recom- bination coefficients. Astronomy and Astrophysics, 251, 680–688.
  • Porter, R. L., Ferland, G. J., Storey, P. J., & Detisch, M. J. (2012). Improved He I emissivities in the case B approximation. Monthly Notices of the Royal Astronomical Society, 425, L28–L31. doi:10.1111/j.1745-3933.2012.01300.x
  • Porter, R. L., Ferland, G. J., Storey, P. J., & Detisch, M. J. (2013). Erratum: "Improved He I emissivities in the Case B approximation". Monthly Notices of the Royal Astronomical Society, 433, L89–L90. doi:10.1093/mnrasl/slt049
  • Shaw, R. A., & Dufour, R. J. (1994). The FIVEL Nebular Modelling Package in STSDAS. In D. R. Crabtree, R. J. Hanisch, & J. Barnes (Eds.), Astronomical data analysis software and systems iii, Astronomical society of the pacific conference series (Vol. 61, p. 327).
  • Shaw, R. A., de La Pena, M. D., Katsanis, R. M., & Williams, R. E. (1998). Analysis Tools for Nebular Emission Lines. In R. Albrecht, R. N. Hook, & H. A. Bushouse (Eds.), Astronomical data analysis software and systems vii, Astronomical society of the pacific conference series (Vol. 145, p. 192).
  • Storey, P. J. (1994). Recombination coefficients for O II lines at nebular temperatures and densities. Astronomy and Astrophysics, 282, 999–1013.
  • Storey, P. J., & Hummer, D. G. (1995). Recombination line intensities for hydrogenic ions- IV. Total recombination coefficients and machine-readable tables for Z=1 to 8. Monthly Notices of the Royal Astronomical Society, 272, 41–48. doi:10.1093/mnras/272.1.41
  • Storey, P. J., Sochi, T., & Bastin, R. (2017). Recombination coefficients for O II lines in nebular conditions. Monthly Notices of the Royal Astronomical Society, 470, 379–389. doi:10.1093/mnras/stx1189
  • Wells, D. C., Greisen, E. W., & Harten, R. H. (1981). FITS - a Flexible Image Transport System. Astronomy and Astrophysics Supplement, 44, 363.