[1] E. Gatuzz, J. García, C. Mendoza, T. R. Kallman, M. A. Bautista, and T. W. Gorczyca. Physical properties of the interstellar medium using high-resolution Chandra spectra: O K-edge absorption. ArXiv e-prints, March 2014. [ bib | arXiv ]
Keywords: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
[2] O. K. Madej, J. Garcia, P. G. Jonker, M. L. Parker, R. Ross, A. C. Fabian, and J. Chenevez. X-ray reflection in oxygen-rich accretion discs of ultra-compact X-ray binaries. ArXiv e-prints, March 2014. [ bib | arXiv ]
Keywords: Astrophysics - High Energy Astrophysical Phenomena
[3] J. García, T. Dauser, A. Lohfink, T. R. Kallman, J. F. Steiner, J. E. McClintock, L. Brenneman, J. Wilms, W. Eikmann, C. S. Reynolds, and F. Tombesi. Improved Reflection Models of Black Hole Accretion Disks: Treating the Angular Distribution of X-Rays. , 782:76, February 2014. [ bib | DOI | arXiv ]
Keywords: accretion, accretion disks, black hole physics, galaxies: individual: Ark 120, line: formation, radiative transfer, X-rays: general
[4] T. W. Gorczyca, M. A. Bautista, M. F. Hasoglu, J. García, E. Gatuzz, J. S. Kaastra, T. R. Kallman, S. T. Manson, C. Mendoza, A. J. J. Raassen, C. P. de Vries, and O. Zatsarinny. A Comprehensive X-Ray Absorption Model for Atomic Oxygen. , 779:78, December 2013. [ bib | DOI | arXiv ]
Keywords: atomic processes, ISM: atoms, line: formation, line: profiles, X-rays: ISM
[5] F. Tombesi, J. N. Reeves, C. S. Reynolds, J. García, and A. Lohfink. An outburst scenario for the X-ray spectral variability in 3C 111. , 434:2707-2717, September 2013. [ bib | DOI | arXiv ]
Keywords: accretion, accretion discs, black hole physics, line: identification, plasmas, galaxies: active, X-rays: galaxies
[6] J. García, E. E. Elhoussieny, M. A. Bautista, and T. R. Kallman. Time-dependent Photoionization of Gaseous Nebulae: The Pure Hydrogen Case. , 775:8, September 2013. [ bib | DOI | arXiv ]
Keywords: galaxies: nuclei, galaxies: Seyfert, H II regions, methods: numerical, planetary nebulae: general, plasmas, quasars: general
[7] L. Gou, J. E. McClintock, R. A. Remillard, J. F. Steiner, M. J. Reid, J. A. Orosz, R. Narayan, M. Hanke, and J. García. Confirmation Via the Continuum-Fitting Method that the Spin of the Black Hole in Cygnus X-1 is Extreme. ArXiv e-prints, August 2013. [ bib | arXiv ]
Keywords: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, High Energy Physics - Theory
[8] E. Gatuzz, J. García, C. Mendoza, T. R. Kallman, M. Witthoeft, A. Lohfink, M. A. Bautista, P. Palmeri, and P. Quinet. Photoionization Modeling of Oxygen K Absorption in the Interstellar Medium: The Chandra Grating Spectra of XTE J1817-330. , 768:60, May 2013. [ bib | DOI | arXiv ]
Keywords: atomic data, atomic processes, ISM: general, stars: individual: XTE J1817-330, X-rays: binaries, X-rays: general
[9] J. García, T. Dauser, C. S. Reynolds, T. R. Kallman, J. E. McClintock, J. Wilms, and W. Eikmann. X-Ray Reflected Spectra from Accretion Disk Models. III. A Complete Grid of Ionized Reflection Calculations. , 768:146, May 2013. [ bib | DOI | arXiv ]
Keywords: accretion, accretion disks, atomic processes, black hole physics, line: formation, radiative transfer, X-rays: general
[10] T. Dauser, J. Garcia, J. Wilms, M. Böck, L. W. Brenneman, M. Falanga, K. Fukumura, and C. S. Reynolds. Irradiation of an accretion disc by a jet: general properties and implications for spin measurements of black holes. , 430:1694-1708, April 2013. [ bib | DOI | arXiv ]
Keywords: accretion, accretion discs, black hole physics, lines: profiles, galaxies: active, galaxies: nuclei
[11] M. F. Hasoglu, S. A. Abdel-Naby, E. Gatuzz, J. Garcia, T. R. Kallman, C. Mendoza, and T. W. Gorczyca. K-Shell Photoabsorption of Magnesium Ions. ArXiv e-prints, March 2013. [ bib | arXiv ]
Keywords: Physics - Atomic Physics
[12] M. C. Witthoeft, M. A. Bautista, J. García, T. R. Kallman, C. Mendoza, P. Palmeri, and P. Quinet. Photoionization and photoabsorption cross sections for the aluminum iso-nuclear sequence. Atomic Data and Nuclear Data Tables, 99:53-61, January 2013. [ bib | DOI ]
[13] P. Palmeri, P. Quinet, C. Mendoza, M. A. Bautista, J. García, M. C. Witthoeft, and T. R. Kallman. Atomic decay data for modeling K lines of iron peak and light odd-Z elements. , 543:A44, July 2012. [ bib | DOI ]
Keywords: atomic data, atomic processes, line: formation, X-rays: general
[14] M. C. Witthoeft, M. A. Bautista, J. García, T. R. Kallman, C. Mendoza, P. Palmeri, and P. Quinet. K-shell Photoionization of Nickel Ions using R-matrix. , 196:7, September 2011. [ bib | DOI | arXiv ]
Keywords: atomic data, atomic processes, line: formation, X-rays: general
[15] J. García, J. M. Ramírez, T. R. Kallman, M. Witthoeft, M. A. Bautista, C. Mendoza, P. Palmeri, and P. Quinet. Modeling the Oxygen K Absorption in the Interstellar Medium: An XMM-Newton View of Sco X-1. , 731:L15, April 2011. [ bib | DOI | arXiv ]
Keywords: atomic data, atomic processes, dust, extinction, line: formation, X-rays: general
[16] J. García, T. R. Kallman, and R. F. Mushotzky. X-ray Reflected Spectra from Accretion Disk Models. II. Diagnostic Tools for X-ray Observations. , 731:131, April 2011. [ bib | DOI | arXiv ]
Keywords: accretion, accretion disks, atomic processes, black hole physics, line: formation, radiative transfer, X-rays: general
[17] P. Palmeri, P. Quinet, C. Mendoza, M. A. Bautista, J. García, M. C. Witthoeft, and T. R. Kallman. Atomic decay data for modeling the Al K lines. , 525:A59, January 2011. [ bib | DOI ]
Keywords: atomic data, atomic processes, line: formation, X-rays: general
[18] M. C. Witthoeft, J. García, T. R. Kallman, M. A. Bautista, C. Mendoza, P. Palmeri, and P. Quinet. K-shell Photoionization of Na-like to Cl-like Ions of Mg, Si, S, Ar, and Ca. , 192:7, January 2011. [ bib | DOI | arXiv ]
Keywords: atomic data, atomic processes, line: formation, X-rays: general
[19] J. García and T. R. Kallman. X-ray Reflected Spectra from Accretion Disk Models. I. Constant Density Atmospheres. , 718:695-706, August 2010. [ bib | DOI | arXiv ]
Keywords: accretion, accretion disks, atomic processes, black hole physics, line: formation, radiative transfer, X-rays: general
[20] J. García, T. R. Kallman, M. Witthoeft, E. Behar, C. Mendoza, P. Palmeri, P. Quinet, M. A. Bautista, and M. Klapisch. Nitrogen K-Shell Photoabsorption. , 185:477-485, December 2009. [ bib | DOI | arXiv ]
Keywords: atomic data, atomic processes, line: formation, X-rays: general
[21] J. García, N. Sánchez, and R. Velásquez. Quantitative Stellar Spectral Classification. IV. Application to the Open Cluster IC 2391. , 45:13-24, April 2009. [ bib | arXiv ]
Keywords: methods: data analysis, open clusters and associations: individual (IC 2391), stars: fundamental parameters, classification
[22] P. Palmeri, P. Quinet, C. Mendoza, M. A. Bautista, J. García, M. C. Witthoeft, and T. R. Kallman. Radiative and Auger Decay Data for Modeling Nickel K Lines. , 179:542-552, December 2008. [ bib | DOI | arXiv ]
Keywords: Atomic Data, Atomic Processes, Line: Formation, X-Rays: General
[23] P. Palmeri, P. Quinet, C. Mendoza, M. A. Bautista, J. García, and T. R. Kallman. Radiative and Auger Decay of K-Vacancy Levels in the Ne, Mg, Si, S, Ar, and Ca Isonuclear Sequences. , 177:408-416, July 2008. [ bib | DOI ]
Keywords: Atomic Processes, Atomic Data, Line: Formation, X-Rays: General
[24] J. García, C. Mendoza, M. A. Bautista, T. W. Gorczyca, T. R. Kallman, and P. Palmeri. K-Shell Photoabsorption of Oxygen Ions. , 158:68-79, May 2005. [ bib | DOI | arXiv ]
Keywords: Atomic Data, Atomic Processes, Line: Formation, X-Rays: General
[25] J. García, J. Stock, M. J. Stock, and N. Sánchez. Quantitative Stellar Spectral Classification. III. Spectral Resolution. , 41:31-40, April 2005. [ bib | arXiv ]
Keywords: STARS: FUNDAMENTAL PARAMETERS, CLASSIFICATION
[26] M. J. Stock, J. Stock, J. García, and N. Sánchez. Quantitative Stellar Spectral Classification. II. Early Type Stars. , 38:127-140, October 2002. [ bib | arXiv ]
Keywords: Stars: Fundamental Parameters

This file was generated by bibtex2html 1.97.