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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Prof Patrick Roche

Professor of Physics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
Pat.Roche@physics.ox.ac.uk
Telephone: 01865 (2)83133
Denys Wilkinson Building, room 765
  • About
  • Research
  • Teaching
  • Publications

A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data

Astronomy & Astrophysics EDP Sciences 666 (2022) l5

Authors:

I García-Bernete, D Rigopoulou, A Alonso-Herrero, FR Donnan, PF Roche, M Pereira-Santaella, A Labiano, L Peralta de Arriba, T Izumi, C Ramos Almeida, T Shimizu, S Hönig, S García-Burillo, DJ Rosario, MJ Ward, E Bellocchi, EKS Hicks, L Fuller, C Packham
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A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data

(2022)

Authors:

I García-Bernete, D Rigopoulou, A Alonso-Herrero, FR Donnan, PF Roche, M Pereira-Santaella, A Labiano, L Peralta de Arriba, T Izumi, C Ramos Almeida, T Shimizu, S Hönig, S García-Burillo, DJ Rosario, MJ Ward, E Bellocchi, EKS Hicks, L Fuller, C Packham
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A technique to select the most obscured galaxy nuclei

Astronomy & Astrophysics EDP Sciences 663 (2022) a46

Authors:

I García-Bernete, D Rigopoulou, S Aalto, HWW Spoon, A Hernán-Caballero, A Efstathiou, PF Roche, S König
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Probing computational methodologies in predicting mid-infrared spectra for large polycyclic aromatic hydrocarbons

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 513:3 (2022) 3663-3681

Authors:

B Kerkeni, I García-Bernete, D Rigopoulou, DP Tew, PF Roche, DC Clary
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Probing computational methodologies in predicting mid-infrared spectra for large polycyclic aromatic hydrocarbons

Monthly Notices of the Royal Astronomical Society Oxford University Press 513:3 (2022) 3663-3681

Authors:

Bouthena Kerkeni, Dimitra Rigopoulou, Ismael Garcia-Bernete, D Tew, Patrick Roche, D Clary

Abstract:

We extend the prediction of vibrational spectra to large sized polycyclic aromatic hydrocarbon (PAH) molecules comprising up to ∼1500 carbon atoms by evaluating the efficiency of several computational chemistry methodologies. We employ classical mechanics methods (Amber and Gaff) with improved atomic point charges, semi-empirical (PM3, and density functional tight binding), and density functional theory (B3LYP) and conduct global optimizations and frequency calculations in order to investigate the impact of PAH size on the vibrational band positions. We primarily focus on the following mid-infrared emission bands 3.3, 6.2, 7.7, 8.6, 11.3, 12.7, and 17.0 μm. We developed a general Frequency Scaling Function (⁠FSF⁠) to shift the bands and to provide a systematic comparison versus the three methods for each PAH. We first validate this procedure on IR scaled spectra from the NASA Ames PAH Database, and extend it to new large PAHs. We show that when the FSF is applied to the Amber and Gaff IR spectra, an agreement between the normal mode peak positions with those inferred from the B3LYP/4-31G model chemistry is achieved. As calculations become time intensive for large sized molecules Nc > 450, this proposed methodology has advantages. The FSF has enabled extending the investigations to large PAHs where we clearly see the emergence of the 17.0 μm feature, and the weakening of the 3.3 μm one. We finally investigate the trends in the 3.3 μm/17.0 μm PAH band ratio as a function of PAH size and its response following the exposure to fields of varying radiation intensities.
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