et al. Spectral line shapes and frequencies of the molecular oxygen B-band R-branch transitions. J Quant Spectrosc Radiat Transf 2015;155:22-31. doi:10.1016/j.jqsrt.2014.12.015.

[330] Domysławska J, Wójtewicz S, Masłowski P, Cygan A, Bielska K, Trawiński RS, et al. A new approach to spectral line shapes of the weak oxygen transitions for atmospheric applications. J Quant Spectrosc Radiat Transf 2016;169:111-21. doi:10.1016/j.jqsrt.2015.10.019.

[331] Sung K, Wishnow EH, Crawford TJ, Nemchick D, Drouin BJ, Toon GC, et al. FTS measurements of O₂ collision-induced absorption in the 565-700 nm region using a high pressure gas absorption cell. J Quant Spectrosc Radiat Transf 2019;235:232-43. doi:10.1016/j.jqsrt.2019.06.016.

[332] Fanjoux G, Millot G, Saint-Loup R, Chaux R, Rosenmann L. Coherent anti-Stokes Raman spectroscopy study of collisional broadening in the O₂-H₂O Q-branch. J Chem Phys 1994;101(2):1061-71. doi:10.1063/1.467803.

[333] Vess EM, Wallace CJ, Campbell HM, Awadalla VE, Hodges JT, Long DA, et al. Measurement of H₂O Broadening of O₂ A-band transitions and implications for atmospheric remote sensing. J Phys Chem A 2012;116(16):4069-73. doi:10.1021/jp301194j.

[334] Drouin BJ, Payne V, Oyafuso F, Sung K, Mlawer E. Pressure broadening of oxygen by water. J Quant Spectrosc Radiat Transf 2014;133:190-8. doi:10.1016/j.jqsrt.2013.08.001.

[335] Koshelev MA, Vilkov IN, Tretyakov MY. Pressure broadening of oxygen fine structure lines by water. J Quant Spectrosc Radiat Transf 2015;154:24-7. doi:10.1016/j.jqsrt.2014.11.019.

[336] Delahaye T, Landsheere X, Pangui E, Huet F, Hartmann JM, Tran H. Measurements of H₂O-broadening coefficients of O₂ A-band lines. J Quant Spectrosc Radiat Transf 2016;184:316-21. doi:10.1016/j.jqsrt.2016.07.019.

[337] Koshelev M, Vilkov I, Makarov D, Tretyakov M, Rosenkranz P. Speed-dependent broadening of the O₂ fine-structure lines. J Quant Spectrosc Radiat Transf 2021;264:107546. doi:10.1016/j.jqsrt.2021.107546.

[338] Crutzen PJ. The role of NO and NO₂ in the chemistry of the troposphere and stratosphere. Ann Rev Earth Planet Sci 1979;7:443. doi:10.1146/annurev.ea.07.051790.020303.

[339] Logan JA. Nitrogen oxides in the troposphere: global and regional budgets. J Geophys Res 1983;88(C15) 10,785-10,807. doi:10.1029/JC088c15107875.

[340] Gardner JL, Funke B, Mlynczak MG, López-Puertas M, Martin-Torres FJ, Russell JM, et al. Comparison of nighttime nitric oxide 5.3 µm emissions in the thermosphere measured by MIPAS and SABER. J Geophys Res (Space Phys) 2007;112(A10). doi:10.1029/2006JA011984.

[341] Wong A, Yurchenko SN, Bernath P, Müller HSP, McConkey S, Tennyson J. Exo-Mol line list - XXI. Nitric oxide (NO). Mon Not R Astron Soc 2017;470:882-97. doi:10.1093/mnras/stx1211.

[342] Tennyson J, Yurchenko SN. ExoMol: molecular line lists for exoplanet and other atmospheres. Mon Not R Astron Soc 2012;425:21-33. doi:10.1111/j.1365-2966.2012.21440.x.

[343] Yurchenko SN, Lodi L, Tennyson J, Stolyarov AV. DUO: a general program for calculating spectra of diatonic molecules. Comput Phys Commun 2016;202:262-75. doi:10.1016/j.cpc.2015.12.021.

[344] Müller HSP, Kobayashi K, Takahashi K, Tomaru K, Matsushima F. Terahertz spectroscopy of N¹⁰O and isotopic invariant fit of several nitric oxide isop topologs. J Mol Spectrosc 2015;310:92-8. doi:10.1016/j.jms.2014.12.002.

[345] Spencer MN, Chackerian C, Giver LP, Brown LR. The nitric oxide fundamental band: frequency and shape parameters for rovibrational lines. J Mol Spectrosc 1994;165(2):506-24. doi:10.1006/jmsp.1994.1154.

[346] Hartmann JM, Boulet C. Line shape parameters for HF in a bath of argon as a test of classical path models. J Chem Phys 2000;113:9000-10. doi:10.1063/1.3193436.

[347] Heinrich K, Fritsch T, Hering P, Mürtz M. Infrared laser-spectroscopic analysis of ¹⁴NO and ¹⁵NO in human breath. Appl Phys B Lasers Opt 2009;95(2):281-6. doi:10.1007/s00340-009-3423-1.

[348] Qu Q, Cooper B, Yurchenko SN, Tennyson J. A spectroscopic model for the low-lying electronic states of NO. J Chem Phys 2021;154(7):074112. doi:10.1063/5.0038527.

[349] Qu Q, Yurchenko SN, Tennyson J. ExoMol molecular line lists - XLII: rovibrational molecular line list for the low-lying states of NO. Mon Not R Astron Soc 2021;504:5768-77. doi:10.1093/mnras/stab1154.

[350] Carn SA, Fioletov VE, Mclinden CA, Li C, Krotkova NA. A decade of global volcanic SO₂ emissions measured from space. Sci Rep 2017;7(1):1-12. doi:10.1038/srep44095.

[351] Lin CK, Lin RT, Chen PC, Wang P, De Marcellis-Warin N, Zigler C, et al. A global perspective on sulfur oxide controls in coal-fired power plants and cardiovascular disease. Sci Rep 2018;8(1):2611. doi:10.1038/s41598-018-20404-2.

[352] Vandaele AC, Korablev O, Belyaev D, Chamberlain S, Evdokimova D, Encrenaz T, et al. Sulfur dioxide in the venus atmosphere: I. Vertical distribution and variability. Icarus 2017;295:16-33. doi:10.1016/j.icarus.2017.05.003.

[353] Encrenaz T, Greathouse TK, Richter MJ, Lacy JH, Fouchet T, Bézard B, et al. A stringent upper limit to SO₂ in the Martian atmosphere. Astron Astrophys 2011;530:37. doi:10.1051/0004-6361/201116820.

[354] Krasnopolsky VA. Search for methane and upper limits to ethane and SO₂ on Mars. Icarus 2012;217(1):144-52. doi:10.1016/j.icarus.2011.10.019.

[355] Loftus K, Wordsworth RD, Morley CV. Sulfate aerosol hazes and SO₂ gas as constraints on rocky exoplanets' surface liquid water. Astrophys J 2019;887(2):231. doi:10.3847/1538-4357/ab58cc.

[356] Webster CR, Blacksberg J, Christensen LE, Flesch GJ, Forouhar S, Briggs R, et al. Digital tunable laser spectrometer for venus atmospheric isotope ratios.

In: Venus science priorities for laboratory measurements, 1838; 2015. p. 4012.

[357] Huang X, Schwenke DW, Lee TJ. Quantitative validation of Ames IR intensity and new line lists for ³²³/³⁴S¹⁶O₂, ³²S¹⁸O₂ and ¹⁶O³²S¹⁸O. J Quant Spectrosc Radiat Transf 2019;225:327-36. doi:10.1016/j.jqsrt.2018.11.039.

[358] Naumenko OV, Horneman V-M. ³²S¹⁶O₂ line list; 2019. Private communication.

[359] Tóbiás R, Furtenbacher T, Császár AG, Naumenko OV, Tennyson J, Flaud JM, et al. Critical evaluation of measured rotational-vibrational transitions of four sulphur isotopologues of S¹⁶O₂. J Quant Spectrosc Radiat Transf 2018;208:152-63. doi:10.1016/j.jqsrt.2018.01.006.

[360] Huang X, Schwenke DW, Lee TJ. Highly accurate potential energy surface, dipole moment surface, rovibrational energy levels, and infrared line list for ³²S¹⁶O₂ up to 8000 cm⁻¹. J Chem Phys 2014;140(11). doi:10.1063/1.4868327.

[361] Huang X, Schwenke DW, Lee TJ. Empirical infrared line lists for five SO₂ isotopologues: ³²³/³⁴S³⁶S¹⁶O₂ and ³²S¹⁸O₂. J Mol Spectrosc 2015;311:19-24. doi:10.1016/j.jms.2015.01.010.

[362] Huang X, Schwenke DW, Lee TJ. Ames ³²S¹⁶O¹⁸O line list for high-resolution experimental IR analysis. J Mol Spectrosc 2016;330:101-11. doi:10.1016/j.jms.2016.08.013.

[363] Huang X, Schwenke DW, Lee TJ. Isotopologue consistency of semi-empirical computed infrared line lists and further improvement for rare isotopologues: CO₂ and SO₂ case studies. J Quant Spectrosc Radiat Transf 2019;230:222-46. doi:10.1016/j.jqsrt.2019.03.002.

[364] Huang X, Schwenke DW, Lee TJ. Exploring the limits of the data-model-theory synergy: "Hot" MW transitions for rovibrational IR studies. J Mol Struct 2020;1217:128260. doi:10.1016/j.molstruc.2020.128260.

[365] Underwood DS, Tennyson J, Yurchenko SN, Huang X, Schwenke DW, Lee TJ, et al. ExoMol molecular line lists - XIV. The rotation-vibration spectrum of hot SO₂. Mon Not R Astron Soc 2016;459(4):3890-9. doi:10.1093/mnras/stw849.

[366] Ulenikov O, Bekhtereva E, Horneman V-M, Alanko S, Gromova O. High resolution study of the 3v₁ band of SO₂. J Mol Spectrosc 2009;255(2):111-21. doi:10.1016/j.jms.2009.03.009.

[367] Ulenikov O, Bekhtereva E, Alanko S, Horneman V, Gromova O, Leroy C. On the high resolution spectroscopy and intramolecular potential function of SO₂. J Mol Spectrosc 2009;257(2):137-56. doi:10.1016/j.jms.2009.07.005.

[368] Ulenikov O, Bekhtereva E, Gromova O, Alanko S, Horneman V-M, Leroy C. Analysis of highly excited 'hot' bands in the SO₂ molecule: v₂ + 3v₃ - v₂ and 2v₁ + v₂ + v₃ - v₂. Mol Phys 2010;108(10):1253-61. doi:10.1080/00268970903468297.

[369] Ulenikov O, Gromova O, Bekhtereva E, Bolotova I, Leroy C, Horneman V-M, et al. High resolution study of the v₁+2v₂-v₂ and 2v₂+v₃-v₂ "hot" bands and ro-vibrational re-analysis of the v₁+v₂+v₃/v₃v₂ polyad of the ³²SO₂ molecule. J Quant Spectrosc Radiat Transf 2011;112(3):486-512. doi:10.1016/j.jqsrt.2010.09.013.

[370] Ulenikov O, Gromova O, Bekhtereva E, Bolotova I, Konov I, Horneman V-M, et al. High resolution analysis of the SO₂ spectrum in the 2600-2900 cm⁻¹ region: 2v₃, v₂+v₃-v₂ and 2v₁+v₂ bands. J Quant Spectrosc Radiat Transf 2012;113(7):500-17. doi:10.1016/j.jqsrt.2012.01.006.

[371] Ulenikov O, Onopenko G, Gromova O, Bekhtereva E, Horneman V-M. Re-analysis of the (100), (001), and (020) rotational structure of SO₂ on the basis of high resolution FTIR spectra. J Quant Spectrosc Radiat Transf 2013;130:220-32. doi:10.1016/j.jqsrt.2013.04.011.

[372] Ulenikov O, Gromova O, Bekhtereva E, Belova A, Bauerecker S, Maul C, et al. High resolution analysis of the (111) vibrational state of SO₂. J Quant Spectrosc Radiat Transf 2014;144:1-10. doi:10.1016/j.jqsrt.2014.03.027.

[373] Ulenikov O, Bekhtereva E, Gromova O, Berezkin K, Horneman V, Sydow C, et al. First high resolution analysis of the 3v₂ and 3v₃-v₂ bands of ³²S¹⁶O₂. J Quant Spectrosc Radiat Transf 2017;202:1-5. doi:10.1016/j.jqsrt.2017.07.012.

[374] Blake T, Flaud J-M, Lafferty W. First analysis of the rotationally-resolved v₂ and 2v₂-v₂ bands of sulfur dioxide, ³³S¹⁶O₂. J Mol Spectrosc 2017;333:19-22. doi:10.1016/j.jms.2016.12.011.

[375] Flaud J-M, Blake T, Lafferty W. First high-resolution analysis of the v₁, v₃ and v₁ + v₃ bands of sulphur dioxide ³³S¹⁶O₂. Mol Phys 2017;115(4):447-53. doi:10.1080/002689766.2016.1269966.

[376] Ulenikov O, Gromova O, Bekhtereva E, Fomchenko A, Sydow C, Bauerecker S. First high resolution analysis of the 3v₁ band of ³⁴S¹⁶O₂. J Mol Spectrosc 2016;319:50-4. doi:10.1016/j.jms.2015.11.002.

[377] Ulenikov O, Bekhtereva E, Gromova O, Buttersack T, Sydow C, Bauerecker S. High resolution FTIR study of ³⁴S¹⁶O₂: the bands 2v₁, v₁ + v₃, v₁ + v₂ + v₃ - v₂ and v₁ + v₂ + v₃. J Quant Spectrosc Radiat Transf 2016;169:49-57. doi:10.1016/j.jqsrt.2015.09.015.

[378] Ulenikov O, Gromova O, Bekhtereva E, Krivchikova Y, Sklyarova E, Buttersack T, et al. High resolution FTIR study of ³⁴S¹⁶O₂: the bands 2v₃, 2v₁ + v₂ and 2v₁ + v₂ - v₂. J Mol Spectrosc 2015;318:26-33. doi:10.1016/j.jms.2015.09.009.

[379] Ulenikov O, Bekhtereva E, Gromova O, Buttersack T, Sydow C, Bauerecker S. High resolution FTIR study of ³⁴S¹⁶O₂: re-analysis of the bands v₁ + v₂, v₂ + v₃, and first analysis of the hot band 2v₂ + v₃ - v₂. J Mol Spectrosc 2016;319:17-25. doi:10.1016/j.jms.2015.11.003.

[380] Ulenikov O, Bekhtereva E, Krivchikova Y, Zamotaeva V, Buttersack T, Sydow C, et al. Study of the high resolution spectrum of ³²S¹⁶O¹⁸O: The v₁ and v₃ bands. J Quant Spectrosc Radiat Transf 2016;168:29-39. doi:10.1016/j.jqsrt.2015.08.010.

[381] Ulenikov O, Bekhtereva E, Gromova O, Zamotaeva V, Kuznetsov S, Sydow C,
et al. Spectral line shapes and frequencies of the molecular oxygen B-band R-branch transitions. J Quant Spectrosc Radiat Transf 2015;155:22–31. doi: 10.1016/j.jqsrt.2014.12.015.

[330] Domysławska J, Wójtewicz S, Masłowski P, Cygan A, Bielska K, Trawiński RS, et al. A new approach to spectral line shapes of the weak oxygen transitions for atmospheric applications. J Quant Spectrosc Radiat Transf 2016;169:111–21. doi:10.1016/j.jqsrt.2015.10.019.

[331] Sung K, Wishnow EH, Crawford TJ, Nemchick D, Drouin BJ, Toon GC, et al. FTS measurements of O₂ collision-induced absorption in the 565–700 nm region using a high pressure gas absorption cell. J Quant Spectrosc Radiat Transf 2019;235:232–43. doi:10.1016/j.jqsrt.2019.06.016.

[332] Fanjoux G, Millot G, Saint-Loup R, Chaux R, Rosenmann L. Coherent anti-Stokes Raman spectroscopy study of collisional broadening in the O₂–H₂O Q-branch. J Chem Phys 1994;101(2):1061–71. doi:10.1063/1.467803.

[333] Vess EM, Wallace CJ, Campbell HM, Awadalla VE, Hodges JT, Long DA, et al. Measurement of H₂O Broadening of O₂ A-band transitions and implications for atmospheric remote sensing. J Phys Chem A 2012;116(16):4069–73. doi:10.1021/jp301194j.

[334] Drouin BJ, Payne V, Oyafuso F, Sung K, Mlawer E. Pressure broadening of oxygen by water. J Quant Spectrosc Radiat Transf 2014;133:190–8. doi:10.1016/j.jqsrt.2013.08.001.

[335] Koshelev MA, Vilkov IN, Tretyakov MY. Pressure broadening of oxygen fine structure lines by water. J Quant Spectrosc Radiat Transf 2015;154:24–7. doi:10.1016/j.jqsrt.2014.11.019.

[336] Delahaye T, Landsheere X, Pangui E, Huet F, Hartmann JM, Tran H. Measurements of H₂O-broadening coefficients of O₂ A-band lines. J Quant Spectrosc Radiat Transf 2016;184:316–21. doi:10.1016/j.jqsrt.2016.07.019.

[337] Koshelev M, Vilkov I, Makarov D, Tretyakov M, Rosenkranz P. Speed-dependent broadening of the O₂ fine-structure lines. J Quant Spectrosc Radiat Transf 2021;264:107546. doi:10.1016/j.jqsrt.2021.107546.

[338] Crutzen PJ. The role of NO and NO₂ in the chemistry of the troposphere and stratosphere. Ann Rev Earth Planet Sci 1979;7:443. doi:10.1146/annurev.ea.07.051790.020303.

[339] Logan JA. Nitrogen oxides in the troposphere: global and regional budgets. J Geophys Res 1983;88(C15) 10,785–10,807. doi:10.1029/JC088c15107875.

[340] Gardner JL, Funke B, Mlynczak MG, López-Puertas M, Martin-Torres FJ, Russell JM, et al. Comparison of nighttime nitric oxide 5.3 µm emissions in the thermosphere measured by MIPAS and SABER. J Geophys Res (Space Phys) 2007;112(A10). doi:10.1029/2006JA011984.

[341] Wong A, Yurchenko SN, Bernath P, Müller HSP, McConkey S, Tennyson J. Exo-Mol line list - XXI. Nitric oxide (NO). Mon Not R Astron Soc 2017;470:882–97. doi:10.1093/mnras/stx1211.

[342] Tennyson J, Yurchenko SN. ExoMol: molecular line lists for exoplanet and other atmospheres. Mon Not R Astron Soc 2012;425:21–33. doi:10.1111/j.1365-2966.2012.21440.x.

[343] Yurchenko SN, Lodi L, Tennyson J, Stolyarov AV. DUO: a general program for calculating spectra of diatonic molecules. Comput Phys Commun 2016;202:262–75. doi:10.1016/j.cpc.2015.12.021.

[344] Müller HSP, Kobayashi K, Takahashi K, Tomaru K, Matsushima F. Terahertz spectroscopy of N¹⁰O and isotopic invariant fit of several nitric oxide isop topologs. J Mol Spectrosc 2015;310:92–8. doi:10.1016/j.jms.2014.12.002.

[345] Spencer MN, Chackerian C, Giver LP, Brown LR. The nitric oxide fundamental band: frequency and shape parameters for rovibrational lines. J Mol Spectrosc 1994;165(2):506–24. doi:10.1006/jmsp.1994.1154.

[346] Hartmann JM, Boulet C. Line shape parameters for HF in a bath of argon as a test of classical path models. J Chem Phys 2000;113:9000–10. doi:10.1063/1.3193436.

[347] Heinrich K, Fritsch T, Hering P, Mürtz M. Infrared laser-spectroscopic analysis of ¹⁴NO and ¹⁵NO in human breath. Appl Phys B Lasers Opt 2009;95(2):281–6. doi:10.1007/s00340-009-3423-1.

[348] Qu Q, Cooper B, Yurchenko SN, Tennyson J. A spectroscopic model for the low-lying electronic states of NO. J Chem Phys 2021;154(7):074112. doi:10.1063/5.0038527.

[349] Qu Q, Yurchenko SN, Tennyson J. ExoMol molecular line lists - XLII: rovibrational molecular line list for the low-lying states of NO. Mon Not R Astron Soc 2021;504:5768–77. doi:10.1093/mnras/stab1154.

[350] Carn SA, Fioletov VE, Mclinden CA, Li C, Krotkova NA. A decade of global volcanic SO₂ emissions measured from space. Sci Rep 2017;7(1):1–12. doi:10.1038/srep44095.

[351] Lin CK, Lin RT, Chen PC, Wang P, De Marcellis-Warin N, Zigler C, et al. A global perspective on sulfur oxide controls in coal-fired power plants and cardiovascular disease. Sci Rep 2018;8(1):2611. doi:10.1038/s41598-018-20404-2.

[352] Vandaele AC, Korablev O, Belyaev D, Chamberlain S, Evdokimova D, Encrenaz T, et al. Sulfur dioxide in the venus atmosphere: I. Vertical distribution and variability. Icarus 2017;295:16–33. doi:10.1016/j.icarus.2017.05.003.

[353] Encrenaz T, Greathouse TK, Richter MJ, Lacy JH, Fouchet T, Bézard B, et al. A stringent upper limit to SO₂ in the Martian atmosphere. Astron Astrophys 2011;530:37. doi:10.1051/0004-6361/201116820.

[354] Krasnopolsky VA. Search for methane and upper limits to ethane and SO₂ on Mars. Icarus 2012;217(1):144–52. doi:10.1016/j.icarus.2011.10.019.

[355] Loftus K, Wordsworth RD, Morley CV. Sulfate aerosol hazes and SO₂ gas as constraints on rocky exoplanets' surface liquid water. Astrophys J 2019;887(2):231. doi:10.3847/1538-4357/ab58cc.

[356] Webster CR, Blacksberg J, Christensen LE, Flesch GJ, Forouhar S, Briggs R, et al. Digital tunable laser spectrometer for venus atmospheric isotope ratios.

In: Venus science priorities for laboratory measurements, 1838; 2015. p. 4012.

[357] Huang X, Schwenke DW, Lee TJ. Quantitative validation of Ames IR intensity and new line lists for ³²³/³⁴S¹⁰O₂, ³²S¹⁰O₂ and ¹⁶O³²S¹⁸O. J Quant Spectrosc Radiat Transf 2019;225:327–36. doi:10.1016/j.jqsrt.2018.11.039.

[358] Naumenko OV, Horneman V-M. ³²S¹⁶O₂ line list; 2019. Private communication.

[359] Tóbiás R, Furtenbacher T, Császár AG, Naumenko OV, Tennyson J, Flaud JM, et al. Critical evaluation of measured rotational-vibrational transitions of four sulphur isotopologues of S¹⁶O₂. J Quant Spectrosc Radiat Transf 2018;208:152–63. doi:10.1016/j.jqsrt.2018.01.006.

[360] Huang X, Schwenke DW, Lee TJ. Highly accurate potential energy surface, dipole moment surface, rovibrational energy levels, and infrared line list for ³²S¹⁶O₂ up to 8000 cm⁻¹. J Chem Phys 2014;140(11). doi:10.1063/1.4868327.

[361] Huang X, Schwenke DW, Lee TJ. Empirical infrared line lists for five SO₂ isotopologues: ³²³/³³/³⁴S¹⁶O₂ and ³²S¹⁸O₂. J Mol Spectrosc 2015;311:19–24. doi:10.1016/j.jms.2015.01.010.

[362] Huang X, Schwenke DW, Lee TJ. Ames ³²S¹⁶O¹⁰O line list for high-resolution experimental IR analysis. J Mol Spectrosc 2016;330:101–11. doi:10.1016/j.jms.2016.08.013.

[363] Huang X, Schwenke DW, Lee TJ. Isotopologue consistency of semi-empirical computed infrared line lists and further improvement for rare isotopologues: CO₂ and SO₂ case studies. J Quant Spectrosc Radiat Transf 2019;230:222–46. doi:10.1016/j.jqsrt.2019.03.002.

[364] Huang X, Schwenke DW, Lee TJ. Exploring the limits of the data-model-theory synergy: "Hot" MW transitions for rovibrational IR studies. J Mol Struct 2020;1217:128260. doi:10.1016/j.molstruc.2020.128260.

[365] Underwood DS, Tennyson J, Yurchenko SN, Huang X, Schwenke DW, Lee TJ, et al. ExoMol molecular line lists - XIV. The rotation-vibration spectrum of hot SO₂. Mon Not R Astron Soc 2016;459(4):3890–9. doi:10.1093/mnras/stw849.

[366] Ulenikov O, Bekhtereva E, Horneman V-M, Alanko S, Gromova O. High resolution study of the 3v₁ band of SO₂. J Mol Spectrosc 2009;255(2):111–21. doi:10.1016/j.jms.2009.03.009.

[367] Ulenikov O, Bekhtereva E, Alanko S, Horneman V, Gromova O, Leroy C. On the high resolution spectroscopy and intramolecular potential function of SO₂. J Mol Spectrosc 2009;257(2):137–56. doi:10.1016/j.jms.2009.07.005.

[368] Ulenikov O, Bekhtereva E, Gromova O, Alanko S, Horneman V-M, Leroy C. Analysis of highly excited 'hot' bands in the SO₂ molecule: v₂ + 3v₃ - v₂ and 2v₁ + v₂ + v₃ - v₂. Mol Phys 2010;108(10):1253–61. doi:10.1080/00268970903468297.

[369] Ulenikov O, Gromova O, Bekhtereva E, Bolotova I, Leroy C, Horneman V-M, et al. High resolution study of the v₁ + 2v₂ - v₂ and 2v₂ + v₃ - v₂ "hot" bands and ro-vibrational re-analysis of the v₁ + v₂ + v₃/3v₃ polyad of the ³²SO₂ molecule. J Quant Spectrosc Radiat Transf 2011;112(3):486–512. doi:10.1016/j.jqsrt.2010.09.013.

[370] Ulenikov O, Gromova O, Bekhtereva E, Bolotova I, Konov I, Horneman V-M, et al. High resolution analysis of the SO₂ spectrum in the 2600–2900 cm⁻¹ region: 2v₃, v₂ + 2v₃ - v₂ and 2v₁ + v₂ bands. J Quant Spectrosc Radiat Transf 2012;113(7):500–17. doi:10.1016/j.jqsrt.2012.01.006.

[371] Ulenikov O, Onopenko G, Gromova O, Bekhtereva E, Horneman V-M. Re-analysis of the (100), (001), and (020) rotational structure of SO₂ on the basis of high resolution FTIR spectra. J Quant Spectrosc Radiat Transf 2013;130:220–32. doi:10.1016/j.jqsrt.2013.04.011.

[372] Ulenikov O, Gromova O, Bekhtereva E, Belova A, Bauerecker S, Maul C, et al. High resolution analysis of the (111) vibrational state of SO₂. J Quant Spectrosc Radiat Transf 2014;144:1–10. doi:10.1016/j.jqsrt.2014.03.027.

[373] Ulenikov O, Bekhtereva E, Gromova O, Berezkin K, Horneman V, Sydow C, et al. First high resolution analysis of the 3v₂ and 3v₃ - v₂ bands of ³²S¹⁶O₂. J Quant Spectrosc Radiat Transf 2017;202:1–5. doi:10.1016/j.jqsrt.2017.07.012.

[374] Blake T, Flaud J-M, Lafferty W. First analysis of the rotationally-resolved v₂ and 2v₂ - v₂ bands of sulfur dioxide, ³³S¹⁶O₂. J Mol Spectrosc 2017;333:19–22. doi:10.1016/j.jms.2016.12.011.

[375] Flaud J-M, Blake T, Lafferty W. First high-resolution analysis of the v₁, v₃ and v₁ + v₃ bands of sulphur dioxide ³³S¹⁶O₂. Mol Phys 2017;115(4):447–53. doi:10.1080/002689766.2016.1269966.

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J Quant Spectrosc Radiat Transf 2017;200:17–24. doi:10.1016/j.jqsrt.2017.05.017.

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[388] Vasilenko IA, Naumenko OV, Horneman V-M. Expert list of absorption lines of the SO₂ molecule in the 2000–3000 cm⁻¹ spectral region, 33; 2020. p. 443–8. doi:10.1134/S1024856020050188.

[389] Naumenko OV, Vasilenko IA, Horneman V-M. High-resolution FTIR spectroscopy of SO₂ molecule in the region of the $2v_1 + v_2$ band 2019;Book of abstracts:74.

[390] Borkov YG, Lyulin OM, Petrova TM, Solodov AM, Solodov A, Deichuli VM, et al. CO₂-broadening and shift coefficients of sulfur dioxide near 4 µm. J Quant Spectrosc Radiat Transf 2019;225:119–24. doi:10.1016/j.jqsrt.2018.12.030.

[391] Tan Y, Kochanov RV, Rothman LS, Gordon IE. The broadening coefficients of SO₂. In: Proceedings of the towards HITRAN 2016; 2016. p. 2. doi:10.5281/zenodo.163447.

[392] Hargreaves RJ, Bernath PF, Bailey J, Dulick M. Empirical line lists and absorption cross sections for methane at high temperatures. Astrophys J 2015;813(1). doi:10.1088/0004-637X/813/1/12.

[393] Wilzewski JS, Gordon IE, Kochanov RV, Hill C, Rothman LS. H₂, He, and CO₂ line-broadening coefficients, pressure shifts and temperature-dependence exponents for the HITRAN database. Part 1: SO₂, NH₃, HF, HCl, OCS and C₂H₂. J Quant Spectrosc Radiat Transf 2016;168:193–206. doi:10.1016/j.jqsrt.2015.09.003.

[394] Dudaryonok A, Lavrentieva N. Theoretical estimation of SO₂ line broadening coefficients induced by carbon dioxide in the 150–300 K temperature range. J Quant Spectrosc Radiat Transf 2018;219:360–5. doi:10.1016/j.jqsrt.2018.08.022.

[395] Vinken GCM, Boersma KF, Maasakkers JD, Adon M, Martin RV. Worldwide biogenic soil NOₓ emissions inferred from OMI NO₂ observations. Atmos Chem Phys 2014;14(18):10363–81. doi:10.5194/acp-14-10363-2014.

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[397] Misra P, Takigawa M, Khatri P, Dhaka SK, Dimri AP, Yamaji K, et al. Nitrogen oxides concentration and emission change detection during COVID-19 restrictions in North India. Sci Rep 2021;11. doi:10.1038/s41598-021-87673-2.

[398] Lukashevskaya AA, Lavrentieva NN, Dudaryonok AC, Perevalov VI. NDSD-1000: high-resolution, high-temperature nitrogen dioxide spectroscopic database. J Quant Spectrosc Radiat Transf 2016;184:205–17. doi:10.1016/j.jqsrt.2016.07.014.

[399] Lukashevskaya AA, Lavrentieva NN, Dudaryonok AS, Perevalov VI. Corrected version of the NDSD-1000 databank. J Quant Spectrosc Radiat Transf 2017;202:37. doi:10.1016/j.jqsrt.2017.07.011.

[400] Perrin A, Kassi S, Campargue A. First high-resolution analysis of the $4v_1 + v_3$ band of nitrogen dioxide near 1.5 µm. J Quant Spectrosc Radiat Transf 2010;111:2246–55. doi:10.1016/j.jqsrt.2010.03.004.

[401] Naumenko OV, Lukashevskaya AA, Kassi S, Béguéier S, Campargue A. The $v_1 + 3v_3$ absorption band of nitrogen dioxide ($^{14}N^{16}O_2$) by CRDS near 6000 cm⁻¹. J Quant Spectrosc Radiat Transf 2019;232:146–51. doi:10.1016/j.jqsrt.2019.04.029.

[402] Lukashevskaya AA, Naumenko OV, Mondelain D, Kassi S, Campargue A. High sensitivity cavity ring down spectroscopy of the $3v_1 + 3v_2 + v_3$ band of NO₂ near 7587 cm⁻¹. J Quant Spectrosc Radiat Transf 2016;177:225–33. doi:10.1016/j.jqsrt.2015.12.017.

[403] Lukashevskaya AA, Naumenko OV, Kassi S, Campargue A. First detection and analysis of the $3v_1 + v_2 + v_3$ band of NO₂ by CRDS near 6156 cm⁻¹. J Mol Spectrosc 2017;338:91–6. doi:10.1016/j.jms.2017.06.005.

[404] Lukashevskaya AA, Kassi S, Campargue A, Perevalov VI. High sensitivity cavity ring down spectroscopy of the $4v_3$ band of NO₂ near 1.59 µm. J Quant Spectrosc Radiat Transf 2017;202:302–7. doi:10.1016/j.jqsrt.2017.07.024.

[405] Lukashevskaya AA, Kassi S, Campargue A, Perevalov VI. High sensitivity cavity ring down spectroscopy of the $2v_1 + 3v_2 + v_3$ band of NO₂ near 1.57 µm.

J Quant Spectrosc Radiat Transf 2017;200:17–24. doi:10.1016/j.jqsrt.2017.05.017.

[406] Lukashevskaya AA, Mondelain D, Campargue A, Perevalov VI. High sensitivity cavity ring down spectroscopy of the $v_1 + 4v_3$ band of NO₂ near 1.34 µm. J Quant Spectrosc Radiat Transf 2018;219:393–8. doi:10.1016/j.jqsrt.2018.07.021.

[407] Lukashevskaya AA, Naumenko OV, Perrin A, Mondelain D, Kassi S, Campargue A. High sensitivity cavity ring down spectroscopy of NO₂ between 7760 and 7917 cm⁻¹. J Quant Spectrosc Radiat Transf 2013;130:249–59. doi:10.1016/j.jqsrt.2013.06.026.

[408] Mondelain D, Perrin A, Kassi S, Campargue A. First high-resolution analysis of the $5v_3$ band of nitrogen dioxide near 1.3 µm. J Quant Spectrosc Radiat Transf 2012;113(11):1058–65. doi:10.1016/j.jqsrt.2011.10.005.

[409] Bykov AD, Lavrentieva NN, Sinitsa LN. Semi-empiric approach to the calculation of H₂O and CO₂ line broadening and shifting. Mol Phys 2004;102(14):1653–8. doi:10.1080/00268970410001725765.

[410] Dudaryonok AS, Lavrentieva NN, Q M. The average energy difference method for calculation of line broadening of asymmetric tops. Atoms Ocean Opt 2015;28:503–9. doi:10.1134/S1024856015060056.

[411] Dana V, Mandin JY, Allout MY, Perrin A, Régalia L, Barbe A, et al. Broadening parameters of NO₂ lines in the 3.4 µm spectral region. J Quant Spectrosc Radiat Transf 1997;57(4):445–57. doi:10.1016/S0022-4073(96)00161-6.

[412] Benner DC, Blake TA, Brown LR, Malathy Devi V, Smith MAH, Toth RA. Air-broadening parameters in the $v_3$ band of $^{14}N^{16}O_2$ using a multispectrum fitting technique. J Mol Spectrosc 2004;228(2):593–619. doi:10.1016/j.jms.2004.07.006.

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[438] Vander Auwera J, Vanfleteren T. Line positions and intensities in the 7400-8600 cm⁻¹ region of the ammonia spectrum. J Quant Spectrosc Radiat Transf 2018;116:3621-30. doi:10.1080/00268976.2018.1467054.

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[440] Sung K, Brown LR, Huang X, Schwenke DW, Lee TJ, Coy SL, et al. Extended line positions, intensities, empirical lower state energies and quantum assignments of NH₃ from 6300 to 7000 cm⁻¹. J Quant Spectrosc Radiat Transf 2012;113(11):1066-83. doi:10.1016/j.jqsrt.2012.02.037.

[441] Barton EJ, Yurchenko SN, Tennyson J, Béguier S, Campargue A. A near infrared line list for NH₃: analysis of a Kitt Peak spectrum after 35 years. J Mol Spectrosc 2016;325:7-12. doi:10.1016/j.jqsrt.2016.05.001.

[442] Yurchenko SN. A theoretical room-temperature line list for ¹⁵NH₃. J Quant Spectrosc Radiat Transf 2015;152:28-36. doi:10.1016/j.jqsrt.2014.10.023.

[443] Nemtchinov V. Measurements of line intensities and half-widths in the 10-µm bands of ¹⁴NH₃. J Quant Spectrosc Radiat Transf 2004;83(3-4):243-65. doi:10.1016/S0022-4073(02)00354-0.

[444] Skinner FM, Hargreaves RJ, Gordon IE. Modeling planetary opacities with HI-TRAN and HAPI: test case of ammonia microwave absorption spectra under jovian condition. In: Proceedings of the AGU fall meeting abstracts. 2020. p. A076-08.

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[446] Canè E, Di Lonardo G, Fusina L, Tamassia A. The $v_2 = 1, 2$ and $v_4 = 1$ bending states of ¹⁵NH₃ and their analysis at experimental accuracy. J Chem Phys 2019;150(19). doi:10.1063/1.5088751.

[447] Canè E, Lonardo GD, Fusina L, Tamassia F, Predoi-Cross A. Spectroscopic characterization of the $v_2 = 3$ and $v_2 = v_4 = 1$ states for ¹⁵NH₃ from high resolution infrared spectra. J Quant Spectrosc Radiat Transf 2020;250. doi:10.1016/j.jqsrt.2020.106987.

[448] Pearson JC, Yu S, Pirali O. Modeling the spectrum of the $2v_2$ and $v_4$ states of ammonia to experimental accuracy. J Chem Phys 2016;145(12):124301. doi:10.1063/1.4961656.

[449] Pearson J, Yu S, Pearson J, Sung K, Drouin B, Pirali O. Extended measurements and an experimental accuracy effective hamiltonian model for the $3v_2$ and $v_4 + v_2$ states of ammonia. J Mol Spectrosc 2018;353:60-6. doi:10.1016/j.jms.2018.09.004.

[450] Zobov NF, Bertin T, Vander Auwera J, Civis S, Knizek A, Ferus M, et al. The spectrum of ammonia near 0.793 µm. J Quant Spectrosc Radiat Transf 2021. This issue

[451] Zobov NF, Coles PA, Ovsyannikov RI, Kyuberis AA, Hargreaves RJ, Bernath PF, et al. Analysis of the red and green optical absorption spectrum of gas phase ammonia. J Quant Spectrosc Radiat Transf 2018;209:224-31. doi:10.1016/j.jqsrt.2018.02.001.

[452] Irwin PGJ, Bowles N, Braude AS, Garland R, Calcutt S, Coles PA, et al. Analysis of gaseous ammonia (NH₃) absorption in the visible spectrum of Jupiter - update. Icarus 2019;321:572-82. doi:10.1016/j.icarus.2018.12.008.

[453] Pickett HM, Drouin BJ, Canty T, Salawitch RJ, Fuller RA, Perun VS, et al. Validation of aura microwave limb sounder OH and HO₂ measurements. J Geophys Res Atmos 2008;113(D16), doi:10.1029/2007JD008775.

[454] Carlotti M, Ade PAR, Carli B, Chipperfield M, Hamilton PA, Mencaraglia F, et al. Diurnal variability and night detection of stratospheric hydroxyl radical from far infrared emission measurements. J Atmos Sol Terr Phys 2001;63(14):1509-18. doi:10.1016/S1364-6826(01)00030-X.

[455] Noll S, Winkler H, Goussev O, Proxauf B. OH level populations and accuracies of Einstein-A coefficients from hundreds of measured lines. Atmos Chem Phys 2020;20(9):5269-92. doi:10.5194/acp-20-5269-2020.

[456] Cheung R, Fai Li K, Wang S, Pongetti TJ, Cageao RP, Sander SP, et al. At-

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[458] Goicoechea JR, Joblin C, Contursi A, Berné O, Cernicharo J, Gerin M, et al. OH emission from warm and dense gas in the Orion Bar PDR. Astron Astrophys 2011;530. doi:10.1051/0004-6361/201116977.

[459] Maillard JP, Chauville J, Mantz AW. High-resolution emission spectrum of OH in an oxyacetylene flame from 3.7 to 0.9 µm. J Mol Spectrosc 1976;63(1):120-41. doi:10.1016/0022-2852(67)90139-7.

[460] Western CM. PGOPHER: a program for simulating rotational, vibrational and electronic spectra. J Quant Spectrosc Radiat Transf 2017;186:221-42. doi:10.1016/j.jqsrt.2016.04.010.

[461] Brooke JSA, Bernath PF, Western CM, Sneden C, Afšar M, Li G, et al. Line strengths of rovibrational and rotational transitions in the X²Π ground state of OH. J Quant Spectrosc Radiat Transf 2016;168:142-57. doi:10.1016/j.jqsrt.2015.07.021.

[462] Bernath PF, Colin R. Revised molecular constants and term values for the X²Π and B²Σ⁺ states of OH. J Mol Spectrosc 2009;257(1):20-3. doi:10.1016/j.jms.2009.06.003.

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[485] Lavrentieva N, Dudaryonok A. OCS-CO2 line broadening coefficients and their temperature dependences for the Earth and Venus atmospheres. Icarus 2020;336:113452. doi:10.1016/j.icarus.2019.113452.

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[487] Barry HR, Corner L, Hancock G, Peverall R, Ranson TL, Ritchie GAD. Mea-
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2003;5(15):3106. doi:10.1039/B304139P.

[488] Wang L, Sharples TR. Intrapulse quantum cascade laser spectroscopy: pres-
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Appl Phys B Lasers Opt 2012;108(2):427-35. doi:10.1007/s00340-012-5085-7.

[489] Nadler S, Reuter DC, Daunt SJ. Tunable diode laser measurements of formaldehyde foreign-gas broadening parameters and line strengths in the 9-11 µm region. Appl Opt 1987;26(9):1641-6. doi:10.1364/AO.26.001641.

[490] Al-Derzi AR, Yurchenko SN, Tennyson J, Melosso M, Jiang N, Puzzarini C, et al. MARVEL analysis of the measured high-resolution spectra of formaldehyde. J Quant Spectrosc Radiat Transf 2021;266:107563. doi:10.1016/j.jqsrt.2021.107563.

[491] Al-Refaie AF, Yurchenko SN, Yachmenev A, Tennyson J. ExoMol line lists - VIII: a variationally computed line list for hot formaldehyde. Mon Not R Astron Soc 2015;448:1704-14. doi:10.1093/mnras/stv091.

[492] Hot D, Pedersen RL, Weng W, Zhang Y, Alden M, Li Z. Spatially and temporally resolved IR-DFWM measurement of HCN released from gasification of biomass pellets. Proc Combust Inst 2019;37:1337-44. doi:10.1016/j.proci.2018.07.105.

[493] Azhar M, Mandon J, Neerincx A, Liu Z, Mink J, Merkus P, et al. A widely tun-
able, near-infrared laser-based trace gas sensor for hydrogen cyanide (HCN)
detection in exhaled breath. Appl Phys B 2017;123(11):1-7. doi:10.1007/
s00340-017-6842-4.

[494] Lellouch E, Gurwell M, Butler B, Fouchet T, Lavvas P, Strobel D, et al. Detection of CO and HCN in Pluto's atmosphere with ALMA. Icarus 2017;286:289-307. doi:10.1016/j.icarus.2016.10.013.

[495] Tsiaras A, Rocchetto M, Waldmann IP, Venot O, Varley R, Morello G, et al. Detection of an atmosphere around the super-earth 55 Cancri e. Astrophys J 2016;820(2). doi:10.3847/0004-637X/820/2/99.

[496] Cordiner M, Palmer M, de Val-Borro M, Charnley S, Paganini L, Villanueva G, et al. ALMA autocorrelation spectroscopy of comets: the HCN/H$^{13}$CN ratio in C/2012 S1 (ISON). Astrophys J Lett 2019;870(2):L26. doi:10.3847/2041-8213/aafb05.

[497] Barber RJ, Strange JK, Hill C, Polyansky OL, Mellau GC, Yurchenko SN, et al. ExoMol line lists - III. An improved hot rotation-vibration line list for HCN and HNC. Mon Not R Astron Soc 2014;437:1828-35. doi:10.1093/mnras/stt2011.

[498] Harris GJ, Polyansky OL, Tennyson J. Opacity data for HCN and HCN from a newab initio linelist. Astrophys J 2002;578:657-63. doi:10.1086/342318.

[499] Mellau GC. Complete experimental rovibrational eigenenergies of HCN up to 6880 cm⁻¹ above the ground state. J Chem Phys 2011;134:234303. doi:10.1063/1.3598942.

[500] Mellau GC, Makhnev VY, Gordon IE, Zobov NF, Tennyson J, Polyan-
sky OL. An experimentally-accurate and complete room-temperature infrared
HCN line-list for the HITRAN database. J Quant Spectrosc Radiat Transf
2021;270:107666. doi:10.1016/j.jqsrt.2021.107666.

[501] Maki A, Mellau GC, Klee S, Winnewisser M, Quapp W. High-temperature infrared measurements in the region of the bending fundamental of H$^{12}$C$^{14}$N, H$^{12}$C$^{15}$N, and H$^{13}$C$^{14}$N. J Mol Spectrosc 2000;202(1):67-82. doi:10.1006/jmsp.2000.8113.

[502] Maiwald F, Lewen F, Ahrens V, Beaky M, Gendriesch R, Koroliev A, et al. Pure rotational spectrum of HCN in the Terahertz region: use of a new planar Schottky diode multiplier. J Mol Spectrosc 2000;1(202):166-8. doi:10.1006/jmsp.2000.8118.

[503] Makhnev VY, Kyuberis AA, Polyansky OL, Mizus T, Tennyson J, Zobov NF. A new spectroscopically-determined potential energy surface and ab initio dipole moment surface for high accuracy HCN intensity calculations. J Mol Spectrosc 2018;353:40-53. doi:10.1016/j.jms.2018.09.002.

[504] Hofmann JP, Eifert B, Mellau GC. Near infrared emission spectrum of H$^{13}$CN. J Mol Spectrosc 2010;262(2):75-81. doi:10.1016/j.jms.2010.05.005.

[505] Guay P, Genest J, Fleisher AJ. Precision spectroscopy of H$^{13}$CN using a free-running, all-fiber dual electro-optic frequency comb system. Opt Lett 2018;43(6):1407-10. doi:10.1364/OL.43.001407.

[506] Cohen JB, Wilson EB. Rotational energy transfer in pure HCN and in HCN-
rare gas mixtures by microwave double resonance and pressure broadening.
J Chem Phys 1973;58(2):442-55. doi:10.1063/1.1679224.

[507] Mehrotra SC, Mäder H, de Vreede JPM, Dijkerman HA. J-dependence of self-, H₂- and He-broadened linewidth parameters for l-type doublet transitions in the bending vibrational state (01¹⁰) of HCN. Chem Phys 1985;93(1):115-25. doi:10.1016/0301-0104(85)85053-9.

[508] Lemaire V, Babay A, Lemoine B, Rohart F, Bouanich JP. Self- and foreign-
gas-broadening and shifting of lines in the $v_2$ band of HCN. J Mol Spectrosc
1996;177(1):40-5. doi:10.1006/jmsp.1996.0115.

[509] D'Eu JF, Lemoine B, Rohart F. Infrared HCN lineshapes as a test of Galatry and

speed-dependent Voigt profiles. J Mol Spectrosc 2002;212(1):96-110. doi:10.1006/jmsp.2002.8520.

[510] Charrón M, Anderson TG, Steinfield JI. Measurements of $T_2$ in excited vibra-
tional states of HCN. J Chem Phys 1980;73(4):1494-7. doi:10.1063/1.440354.

[511] Landrain V, Blanquet G, Lepère M, Walrand J, Bouanich J-P. Diode-laser mea-
surements of H₂-broadening coefficients in the $v_2$ band of HCN. J Mol Spectro-
trosc 1997;182(1):184-8. doi:10.1006/jmsp.1996.7223.

[512] Rohart F, Nguyen L, Buldyreva J, Colmont JM, Wlodarczak G. Lineshapes of the 172 and 602 GHz rotational transitions of HC$^{15}$N. J Mol Spectrosc 2007;246(2):213-27. doi:10.1016/j.jms.2007.09.009.

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[559] Snellen IAG, Guzman-Ramirez L, Hogerheijde MR, Hygate APS, van der Tak FFS. Re-analysis of the 267 GHz ALMA observations of Venus, no statistically significant detection of phosphine. Astron Astrophys 2020;644. doi:10.1051/0004-6361/202039717.

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[537] Pine AS, Lafferty WJ. Torsional splittings and assignments of the Doppler-limited spectrum of ethane in the C-H stretching region. J Res Natl Bureau Stand 1982;83(3):1-20.

[538] Lattanzi F, Di Lauro C, Vander Auwera J. Toward the understanding of the high resolution infrared spectrum of $C_2H_6$ near 3.3 µm. J Mol Spectrosc 2011;267:71-9. doi:10.1016/j.jms.2011.02.003.

[539] Radeva YL, Mumma MJ, Villanueva GL, A'Hearn MF. A newly developed fluorescence model for $C_2H_6\nu_5$ and application to cometary spectra acquired with NIRSPEC at Keck II. Astrophys J 2011;729(2):135. doi:10.1088/0004-637X/729/2/135. http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ApJ..729.135R&link_type=ABSTRACT

[540] Pine AS, Lafferty WJ. Torsional splittings and assignments of the Doppler-limited spectrum of ethane in the C-H stretching region. J Res Natl Bureau Stand 1982;87:237-56. doi:10.6028/jres.087.017.

[541] Pine AS, Stone SC. Torsional tunneling and $A_1-A_2$ splittings and air broadening of the $\tau_0$ and $PQ_3$ subsubranches of the $\nu_7$ band of ethane. J Mol Spectrosc 1995;175:21-30. doi:10.1006/jmsp.1996.0004.

[542] Dang-Nhu M, Pine AS, Lafferty WJ. Intensities in the $\nu_5$, $\nu_7$, and $\nu_8 + \nu_{11}$ bands of ethane $^{12}C_2H_6$. Can J Phys 1984;62:512. doi:10.1139/p84-069. http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984CaJph.62.512D&link_type=REFERENCES

[543] Harrison JJ, Allen NDC, Bernath PF. Infrared absorption cross sections for ethane ($C_2H_6$) in the 3 µm region. J Quant Spectrosc Radiat Transf 2010;111:357. doi:10.1016/j.jqsrt.2009.09.010. http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010JQSRT.111.357H&link_type=EJOURNAL

[544] Hargreaves RJ, Buzan E, Dulick M, Bernath PF. High-resolution absorption cross sections of $C_2H_6$ at elevated temperatures. Mol Astrophys 2015;1:20-5. doi:10.1016/j.molap.2015.09.001.

[545] Doney KD, Kofman V, Villanueva G, Sung K. A new model of monodeuterated ethane ($C_2H_5D$) spectrum: enabling sensitive constraints on the D/H in ethane emission in comets. J Quant Spectrosc Radiat Transf 2020;255. doi:10.1016/j.jqsrt.2020.107225.

[546] Sung K, Mantz AW, Smith MAH, Brown LR, Crawford TJ, Devi VM, et al. Cryogenic absorption cells operating inside a Bruker IFS-125HR: first results for $^{13}CH_4$ at 7 µm. J Mol Spectrosc 2010;262(2):122-34. doi:10.1016/j.jms.2010.05.004.

[547] Mantz AW, Sung K, Brown LR, Crawford TJ, Smith MAH, Malathy Devi V, et al. A cryogenic Herrirot cell vacuum-coupled to a Bruker IFS-125HR. J Mol Spectrosc 2014;304:12-24. doi:10.1016/j.jms.2014.07.006.

[548] Devi VM, Rinsland CP, Benner DC, Sams RL, Blake TA. Multispectrum analysis of the $\nu_9$ band of $^{12}C_2H_6$: Positions, intensities, self- and $N_2$-broadened half-width coefficients. J Quant Spectrosc Radiat Transf 2010;111:1234-51. doi:10.1016/j.jqsrt.2009.10.017.

[549] Malathy Devi V, Chris Benner D, Rinsland C, Smith M, Sams R, Blake T, et al. Multispectrum measurements of spectral line parameters including temperature dependences of $N_2$- and self-broadened half-width coefficients in the region of the $\nu_9$ band of $^{12}C_2H_6$. J Quant Spectrosc Radiat Transf 2010;111(17):2481-504. doi:10.1016/j.jqsrt.2010.07.010.

[550] Moazzen-Ahmadi N, Norooz Oliaee J, Ozier I, Wishnow EH, Sung K, Crawford TJ, et al. An intensity study of the torsional bands of ethane at 35 µm. J Quant Spectrosc Radiat Transf 2015;151:123-32. doi:10.1016/j.jqsrt.2014.09.016.

[551] Pasek MA, Sampson JM, Atlas Z. Redox chemistry in the phosphorus biogeochemical cycle. Proc Natl Acad Sci 2014;111(43):15468-73. doi:10.1073/pnas.1408134111.

[552] Larson HP, Treffers RR, Fink U. Phosphine in Jupiter's atmosphere: the evidence from high-altitude observations at 5 micrometers. Astrophys J 1977;211:972-9. doi:10.1086/155009.

[553] Fletcher LN, Orton GS, Teanby NA, Irwin PGJ. Phosphine on Jupiter and Saturn from Cassini/CIRS. Icarus 2009;202(2):543-64. doi:10.1016/j.icarus.2009.03.023.

[554] Burgess JL, Burgess DJ. Phosphine exposure from a methamphetamine laboratory investigation. J Toxicol Clin Toxicol 2001;39(2):165-8. doi:10.1081/CLT-100103833.

[555] Sousa-Silva C, Seager S, Ranjan S, Petkowski JJ, Zhan Z, Hu R, et al. Phosphine as a biosignature gas in exoplanet atmospheres. Astrobiology 2020;20(2):235-68. doi:10.1089/ast.2018.1954.

[556] Greaves JS, Richards AMS, Bains W, Rimmer PB, Sagawa H, Clements DL, et al. Phosphine gas in the cloud decks of Venus. Nat Astron 2021;5:655-64. doi:10.1038/s41550-021-0174-2.

[557] Villanueva G., Cordiner M., Irwin P., de Pater I., Butler B., Gurwell M., et al. No phosphine in the atmosphere of Venus, Nat Astron 5, 2021, 631-635, doi:10.1038/s41550-021-01422-z.

[558] Encrenaz T, Greathouse TK, Marcq E, Widemann T, Bézard B, Fouchet T, et al. A stringent upper limit of the $\nu_3$ abundance of the $\nu_3$ band at the cloud top of Venus. Astron Astrophys 2020;643. doi:10.1051/0004-6361/202039559.

[559] Snellen IAG, Guzman-Ramirez L, Hogerheijde MR, Hygate APS, van der Tak FFS. Re-analysis of the 267 GHz ALMA observations of Venus, no statistically significant detection of phosphine. Astron Astrophys 2020;644. doi:10.1051/0004-6361/202039717.

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