Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Perri, Armando N"'
Autor:
Yurchenko, Sergei N., Bowesman, Charles A., Brady, Ryan P., Guest, Elizabeth R., Kefala, Kyriaki, Mitev, Georgi B., Owens, Alec, Perri, Armando N., Pezzella, Marco, Smola, Oleksiy, Sokolov, Andrei, Zhang, Jingxin, Tennyson, Jonathan
Publikováno v:
MNRAS, 533, 3442-3456 (2020)
A theoretical line list for $^{15}$NH$_3$ CoYuTe-15 is presented based on the empirical potential energy and ab initio dipole moments surfaces developed and used for the production of the ExoMol line list CoYuTe for $^{14}$NH$_3$. The ro-vibrational
Externí odkaz:
http://arxiv.org/abs/2410.04295
Autor:
McKemmish, Laura K., Bowesman, Charles A., Kefala, Kyriaki, Perri, Armando N., Syme, Anna-Maree, Yurchenko, Sergei N., Tennyson, Jonathan
The best molecular line lists for astrophysical applications today require both high accuracy of line positions for strong lines as well as high overall completeness. The former is required to enable, for example, molecular detection in high-resoluti
Externí odkaz:
http://arxiv.org/abs/2409.03984
Autor:
Tennyson, Jonathan, Yurchenko, Sergei N., Zhang, Jingxin, Bowesman, Charles A., Brady, Ryan P., Buldyreva, Jeanna, Chubb, Katy L., Gamache, Robert R., Gorman, Maire N., Guest, Elizabeth R., Hill, Christian, Kefala, Kyriaki, Lynas-Gray, A. E., Mellor, Thomas M., McKemmish, Laura K., Mitev, Georgi B., Mizus, Irina I., Owens, Alec, Peng, Zhijian, Perri, Armando N., Pezzella, Marco, Polyansky, Oleg L., Qu, Qianwei, Semenov, Mikhail, Smola, Oleksiy, Solokov, Andrei, Somogyi, Wilfrid, Upadhyay, Apoorva, Wright, Samuel O. M., Zobov, Nikolai F.
The ExoMol database (www.exomol.com) provides molecular data for spectroscopic studies of hot atmospheres. These data are widely used to model atmospheres of exoplanets, cool stars and other astronomical objects, as well as a variety of terrestrial a
Externí odkaz:
http://arxiv.org/abs/2406.06347
Autor:
Perri, Armando N., McKemmish, Laura K.
Publikováno v:
MNRAS 2024
Imidogen (NH) is a reactive molecule whose presence in astrochemical environments is of interest due to its role in the formation of nitrogen-containing molecules and as a potential probe of nitrogen abundance. Spectroscopic NH monitoring is useful f
Externí odkaz:
http://arxiv.org/abs/2405.14065
Zirconium monoxide (ZrO) absorption lines define rare S-type stars and are currently being sought on exoplanets. Successful detection is dependent on an accurate and comprehensive line list, with existing data not ideal for many applications. Specifi
Externí odkaz:
http://arxiv.org/abs/2308.03922
Autor:
Yurchenko, Sergei N, Bowesman, Charles A, Brady, Ryan P, Guest, Elizabeth R, Kefala, Kyriaki, Mitev, Georgi B, Owens, Alec, Perri, Armando N, Pezzella, Marco, Smola, Oleksiy, Sokolov, Andrei, Zhang, Jingxin, Tennyson, Jonathan
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 9/30/2024, Vol. 533 Issue 3, p3442-3456, 15p
Autor:
Perri, Armando N, McKemmish, Laura K
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jul2024, Vol. 531 Issue 3, p3023-3033, 11p
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Sep2023, Vol. 524 Issue 3, p4631-4641, 11p
Autor:
Yurchenko, Sergei N1 (AUTHOR) s.yurchenko@ucl.ac.uk, Bowesman, Charles A1 (AUTHOR), Brady, Ryan P1 (AUTHOR), Guest, Elizabeth R1 (AUTHOR), Kefala, Kyriaki1 (AUTHOR), Mitev, Georgi B1 (AUTHOR), Owens, Alec1 (AUTHOR), Perri, Armando N1 (AUTHOR), Pezzella, Marco1 (AUTHOR), Smola, Oleksiy1 (AUTHOR), Sokolov, Andrei1 (AUTHOR), Zhang, Jingxin1 (AUTHOR), Tennyson, Jonathan1 (AUTHOR) j.tennyson@ucl.ac.uk
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 9/30/2024, Vol. 533 Issue 3, p3442-3456. 15p.