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  1. Anderson, P. W. (1949), Pressure Broadening in the Microwave and Infra-Red RegionsPhys. Rev., 76(5), 647–661.
  2. Baranger, M. (1958), General Impact Theory of Pressure BroadeningPhys. Rev., 112(3), 855–865.
  3. Ben-Reuven, A. (1966), Impact Broadening of Microwave SpectraPhys. Rev., 145(1), 7–22.
  4. Hartmann, J.-M. and H. Tran G. C. Toon (2009), Influence of line mixing on the retrievals of atmospheric CO2 from spectra in the 1.6 and 2.1 μm regionsAtmos. Chem. Phys., 9(19), 7303–7312, doi:10.5194/acp-9-7303-2009.
  5. Makarov, D. S., M. Yu. Tretyakov, and P. W. Rosenkranz (2011), 60-GHz oxygen band: Precise experimental profiles and extended absorption modeling in a wide temperature rangeJ. Quant. Spectrosc. Radiat. Transfer, 112(9), 1420–1428, doi:10.1016/j.jqsrt.2011.02.018.
  6. Makarov, D. S., M. Yu. Tretyakov, and C. Boulet (2013), Line mixing in the 60-GHz atmospheric oxygen band: Comparison of the MPM and ECS modelJ. Quant. Spectrosc. Radiat. Transfer, 124, 1–10, doi:10.1016/j.jqsrt.2013.02.019.
  7. Niro, F., C. Boulet, and J.-M. Hartmann (2004), Spectra calculations in central and wing regions of CO2 IR bands between 10 and 20 μm. I: model and laboratory measurementsJ. Quant. Spectrosc. Radiat. Transfer, 88(4), 483–498, doi:10.1016/j.jqsrt.2004.04.003.
  8. Niro, F., F. Hase, C. Camy-Peyret, S. Payan, and J.-M. Hartmann (2005), Spectra calculations in central and wing regions of CO2 IR bands between 10 and 20 μm. II. Atmospheric solar occultation spectraJ. Quant. Spectrosc. Radiat. Transfer, 90(1), 43–59, doi:10.1016/j.jqsrt.2004.04.004.
  9. Niro, F., T. von Clarmann, K. Jucks, and J.-M. Hartmann (2005), Spectra calculations in central and wing regions of CO2 IR bands between 10 and 20 μm. III: atmospheric emission spectraJ. Quant. Spectrosc. Radiat. Transfer, 90(1), 61–76, doi:10.1016/j.jqsrt.2004.04.005.
  10. Niro, F., K. Jucks, and J.-M. Hartmann (2005), Spectra calculations in central and wing regions of CO2 IR bands between 10 and 20 μm. IV: software and database for the computation of atmospheric spectraJ. Quant. Spectrosc. Radiat. Transfer, 95(4), 469–481, doi:10.1016/j.jqsrt.2004.11.011.
  11. Rodrigues, R., K. W. Jucks, N. Lacome, Gh. Blanquet, J. Walrand, W. A. Traub, B. Khalil, R. Le Doucen, A. Valentin, C. Camy-Peyret, L. Bonamy, and J.-M. Hartmann (1999), Model, software, and database for computation of line-mixing effects in infrared Q branches of atmospheric CO2— I. Symmetric isotopomersJ. Quant. Spectrosc. Radiat. Transfer, 61(2), 153–184, doi:10.1016/S0022-4073(97)00208-2.
  12. Stähli, O., A. Murk, N. Kämpfer, C. Mätzler, and P. Eriksson (2013), Microwave radiometer to retrieve temperature profiles from the surface to the stratopauseAtmos. Chem. Phys. Discuss., 6, 2857–2905, doi:10.5194/amtd-6-2857-2013.
  13. Tretyakov, M. Yu., M. A. Koshelev, V.V. Dorovskikh, D. S. Makarov, and P. W. Rosenkranz (2005), 60-GHz oxygen band: precise broadening and central frequencies of fine-structure lines, absolute absorption profile at atmospheric pressure, and revision of mixing coefficientsJ. Molec. Struct., 231, 1–14, doi:10.1016/j.jms.2004.11.011.
  14. Turbet, M and H Tran (2017), Comment on "Radiative Transfer in CO 2-Rich Atmospheres: 1. Collisional Line Mixing Implies a Colder Early Mars"J. Geophys. Res.: Planets, 122(11), 2362–2365, doi:10.1002/2017JE005373.