[1] A. A. A. Azzam, J. Tennyson, S. N. Yurchenko, T. Furtenbacher, and A. G. Császár, MARVEL Analysis of High-Resolution Rovibrational Spectra of ¹⁶O¹³C¹⁸O, J. Comp. Chem. 2025, 46, e27541. https://doi.org/10.1002/jcc.27541 PDF

[2] T. Salomon, C. Baddeliyanage, C. Schladt, I. Simkó, A. G. Császár, W. G. D. P. Silva, S. Schlemmer, and O. Asvany, High-Resolution Leak-Out Spectroscopy of HHe₂⁺, Phys. Chem. Chem. Phys. 2025, 27, 4826-4828. https://doi.org/10.1039/d4cp04767b PDF

[3] S. Mahmoud, N. El-Kork, N. A. Elkher, M. Almehairbi, M. S. Khalil, T. Furtenbacher, and A. G. Császár, O. P. Yurchenko, S. N. Yurchenko, J. Tennyson, MARVEL Analysis of Measured High-Resolution Spectra of ¹²C¹⁶O, Astrophys. J. Suppl. Ser. 2025, 276, 66. https://doi.org/10.3847/1538-4365/ada3c9 PDF

[4] A. A. A. Azzam, D. Alatoom, B. M. J. Abou Doud, M. Q. A. Shersheer, B. K. M. Almasri, C. N. M. Bader, B. O. A. Kh. Musleh, A. M. H. Abu Khudair, A. W. M. Al Shatarat, B. I. M. Qattan, L. H. M. Hamamsy, A. O. G. Saafneh, M. N. A. ALso’ub, M. M. A. Alkashashneh, H. O. M. Al-Zawahra, M. T. I. Ibrahim, J. Tennyson, S. N. Yurchenko, T. Furtenbacher, and A. G. Császár, The 626M24 Dataset of Validated Transitions and Empirical Rovibrational Energy Levels of ¹⁶O¹²C¹⁶O, Sci. Data 2025, 12, 532. https://doi.org/10.1038/s41597-025-04755-w PDF

[5] S. A. M. Obaidat, A. A. A. Azzam, D. Alatoom, M. T. I. Ibrahim, J. Tennyson, A. G. Császár, and T. Furtenbacher, MARVEL Analysis of High-Resolution Rovibrational Spectra of ¹⁶O¹²C¹⁷O, J. Quant. Spectrosc. Radiat. Transf. 2025, 340, 109444. https://doi.org/10.1016/j.jqsrt.2025.109444 PDF

[6] A. A. A. Azzam, J. M. A. AlAlawin, J. Tennyson, T. Furtenbacher, and A. G. Császár, MARVEL Analysis of High-Resolution Rovibrational Spectra of ¹⁷O¹³C¹⁸O and ¹⁷O¹³C¹⁷O, J. Quant. Spectrosc. Radiat. Transf. 2025, 343, 109485. https://doi.org/10.1016/j.jqsrt.2025.109485 PDF

[7] T. Furtenbacher, S. Egbert, K. Sung, S. C. Coburn, B. J. Drouin, G. B. Rieker, and A. G. Császár, Improved Assessment of H₂¹⁶O Transitions in the Region 6600-7500 cm^-1, J. Quant. Spectrosc. Radiat. Transf. 2025, 344, 109513. https://doi.org/10.1016/j.jqsrt.2025.109513 PDF

[8] T. Turányi, I. Gy. Zsély, M. Papp, T. Nagy, T. Furtenbacher, R. Tóbiás, P. Árendás, and A. G. Császár, ReSpecTh: Reaction Kinetics, Spectroscopy, and Thermochemical Datasets, Sci. Data 2025, 12, 1021. https://doi.org/10.1038/s41597-025-05272-6 PDF

[9] R. Tóbiás, T. Furtenbacher, and A. G. Császár, Past, Present, and Future of Joint Utilization of Experimental, Empirical, and Computed Spectroscopic Data: Challenges, Advantages, and Recommendations, Adv. Quant. Chem. 2025, in press. https://doi.org/10.1016/bs.aiq.2025.01.002

[10] T. Furtenbacher, A. H. Harvey, and A. G. Császár, Improved Partition Functions and Related Thermochemical Quantities for the ¹⁶O₂ and H₂¹⁶O Molecules, J. Phys. Chem. Ref. Data 2025, 54, 033103. https://doi.org/10.1063/5.0273661 PDF

[11] A. G. Császár, R. Tóbiás, P. Árendás, and T. Furtenbacher, A Network Approach to High-Resolution and Precision Spectroscopy, ISTE Encyclopedia 2025, in press.

[12] M. H. I. Mansour, A. B. I. Al-Iter, A. A. A. Azzam, J. Tennyson, T. Furtenbacher, and A. G. Császár, MARVEL Analysis of High-Resolution Rovibrational Spectra of ¹⁶O¹³C¹⁷O and ¹⁷O¹²C¹⁷O, Mol. Phys. (Zlatko Bacic Special Issue) 2025, in press.

[13] R. Tóbiás, C. Fábri, M. Bosquez Fuentes, M. Kodrycka, K. Patkowski, and A. G. Császár, Rovibrational Dynamics of the Quasistructural N₂ dimer, Commun. Chem. 2025, under revision.

[14] A. Altman, R. Tóbiás, A. S. Bogomolov, M. L. Diouf, F. M. J. Cozijn, A. G. Császár, C. Lauzin, and W. Ubachs, Precise Frequencies of H₂¹⁶O Lines Protected for Radio Astronomy, Astrophys. J. Suppl. 2025, under review.

[15] T. Furtenbacher, M. Horváth, D. Koller, P. Sólyom, A. Balogh, I. Balogh, and A. G. Császár, Erratum: “MARVEL Analysis of the Measured High-Resolution Rovibronic Spectra and Definitive Ideal-Gas Thermochemistry of the ¹⁶O₂ Molecule” [J. Phys. Chem. Ref. Data 48, 023101 (2019)], J. Phys. Chem. Ref. Data 2025, under review.