CHIANTI—An Atomic Database for Emission Lines. IV. Extension to X-Ray Wavelengths

By K. Dere, E. Landi, Peter R. Young, G. D. Zanna. 2001

158 citations recorded by the source corpus.

Subfields: Atomic and Molecular Physics, and Optics, Mechanics of Materials, Radiation

View Paper: https://www.semanticscholar.org/paper/8e08174eb9e7a4b05e74994dd04ea4ea25f005a2

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atomic and Molecular Physics, and Optics

1. G. D. Zanna
2. Peter R. Young
3. K. Dere
4. E. Landi
5. Helen E. Mason
6. R. Sutherland
7. W. Abbett
8. Hirohisa Hara

In Mechanics of Materials

1. G. D. Zanna
2. Peter R. Young
3. K. Dere
4. E. Landi
5. Helen E. Mason
6. R. Sutherland
7. W. Abbett
8. Hirohisa Hara

In Radiation

1. K. Dere
2. Peter R. Young
3. Hirohisa Hara
4. Tetsuya Watanabe
5. E. Landi
6. S. Bianchi
7. M. Guainazzi
8. G. D. Zanna

Citations in the corpus

• CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines (2019, methodology): “In Version 3 of CHIANTI (Dere et al. 2001), the dielectronic lines were accounted for by a model that assumed that dielectronic recombination took place only from the ground level of the higher ionization stage.”
• High-precision density measurements in the solar corona I. Analysis methods and results for Fe XII and Fe XIII (2008, methodology): “…work, the CHIANTI team found an error in the CHIANTI electron collision strength file for Fexiii, which actually contained older data from Fawcett & Mason (1989) rather than the data of Gupta & Tayal (1998) that were supposed to have been added in version 3 of the database (Dere et al. 2001).”
• A comprehensive range of X-ray ionized-reflection models (2005, methodology): “Excitation and line energies of nonresonance lines, as well as collision strengths for all lines, are derived from the CHIANTI database (Dere et al. 2001).”
• Multiwavelength Observations of Flares on AD Leonis (2003, background): “The line identifications Flare 6 and formation temperatures (from Dere et al. 1997, 2001), together with the quiescent line fluxes measured from the quiet AD Leo spectrum (see x 2), are listed in Table 2.”
• Elemental Abundances and Post-Coronal Mass Ejection Current Sheet in a Very Hot Active Region (2002, methodology): “We use the collisional excitation rates from the CHIANTI database Version 3.02 (Dere et al. 2001) and the ionization equilibria of Mazzotta et al. (1998).”
• CHIANTI—An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements (2006, unknown): “Details can be found in Dere et al. (2001).”
• CHIANTI - An atomic database for Emission Lines. Version 8 (2015, background): “In particular the lines due to dielectronic recombination that are important at X-ray wavelengths are not modeled and so it was necessary to retain the dielectronic files for these ions (see Dere et al. 2001).”
• On the origin of soft X-rays in obscured AGN: answers from high-resolution spectroscopy with XMM–Newton (2006, methodology): “…A we list energies, fluxes and intrinsic widths (for the RRC only) of the transitions individually presented in this paper, and discuss the consistency of our measurements with the expected laboratory energies [laboratory energies are extracted from the CHIANTI database (Dere et al. 2001)].”