You can find my ADS author query here. It is likely to be updated more often than this page. Nevertheless, here you will find pdf versions of most things.

Selected talks

  • 2009, September: Final Thesis Talk, RSAA [pdf]
  • 2009, August: Testing 3D models against observations, IAU General Assembly, JD 10, Rio de Janeiro [pdf]
  • 2009, August: Comparing 3D models with solar observations at high-spatial-resolution, IAU General Assembly, Comm. 36, Rio de Janeiro [pdf]
  • 2009, July: Data visualization: easy and powerful tools, RSAA [interactive, together with W. Kerzendorf and S. Murphy]
  • 2009, June: Electric Cars, RSAA [online]
  • 2009, April: Using Cython to optimize Python and interface with C, Astroinformatics summer school, Univ. of Sydney [pdf]
  • 2008, July: Observing oxygen lines across the solar disk: a test of 3D atmospheric models, Astronomical Society of Australia - Annual Science Meeting, Perth [pdf]
  • 2008, May: PhD Thesis Mid-Term Review, RSAA [pdf]
  • 2008, April: Dude, where's my computer? - The dangers of DRM in a digital world, RSAA [pdf]
  • 2007, June: Observational tests of 3D solar model atmospheres, Institute of Theoretical Astrophysics, Oslo [pdf]
  • 2007, November: Observing with the Swedish Solar Telescope, Stromlo Students Xmas Seminars [pdf]
  • 2007, May: Observational tests of 3D solar model atmospheres, Uppsala Astronomical Observatory [pdf]
  • 2007, April: Confronting the new generation of stellar atmospheres with observations, Institute of Solar Physics, Stockholm [pdf]
  • 2006, December: Convection, Granulation, Entropy. A look at results from 3D solar model atmospheres, Stromlo Students Xmas Seminars [pdf]
  • 2006, July: Scientific use of Python, RSAA [pdf]

Refereed publications

  • Pereira, T. M. D., Asplund, M., Trampedach, R., Collet, R. 2009, How realistic are solar model atmospheres?, submitted to A&A
  • Pereira, T. M. D., Asplund, M., Kiselman, D. 2009, Oxygen lines in solar granulation. II. Centre-to-limb variation, NLTE line formation, blends and the solar oxygen abundance, A&A in press, [arXiv]
  • Pereira, T. M. D., Kiselman, D., Asplund, M. 2009, Oxygen lines in solar granulation. I. Testing 3D models against new observations with high spatial and spectral resolution, A&A in press, [arXiv]
  • Pereira, T. M. D., et al. 2007, Searching for signatures of stochastic excitation in stellar pulsations: a look at gamma Doradus stars, A&A, 464, 659 [ADS]
  • Pereira, T. M. D., Lopes, I. 2005, On the Nature of Stochastic Excited Oscillations: Subdwarf B Star PG 1605+072 as a Case Study, ApJ, 622, 1068 [ADS]
  • Pereira, T. M. D., Lopes, I. 2004, Amplitude variations in the sdBV star PG 1605+072: Another beating time scale?, A&A, 426, 213 [ADS]
  • O'Toole, S. J., et al. 2004, MSST observations of the pulsating sdB star PG 1605+072, ApSS, 291, 457 [ADS | arXiv]

Other publications

  • Pereira, T. M. D., Asplund, M., Kiselman, D. 2009, Testing 3D solar models against observations, Mem. S.A.It. in press, in IAU JD 10: 3D views on cool stellar atmospheres: theory meets observation, ed. K.N. Nagendra, H.-G. Ludwig, P. Bonifacio [pdf | arXiv]
  • Pereira, T. M. D., Asplund, M., & Trampedach, R. 2008, Comparing 3D solar model atmospheres with observations: Hydrogen lines and centre-to-limb variations, in Precision Spectroscopy in Astrophysics, ed. N. C. Santos, L. Pasquini, A. C. M. Correia, & M. Romaniello, 313–314 [ADS | pdf | poster]
  • O'Toole, S. J., et al. 2004, Multisite spectroscopic and photometric observations of the pulsating sdB star PG 1605+072 in Astronomical Society of the Pacific Conference Series, Vol. 310, IAU Colloq. 193: Variable Stars in the Local Group, ed. D. W. Kurtz \& K. R. Pollard, 230 [ADS]
  • Heber, U. et al. 2003, Photometric and Spectroscopic Monitoring of the sdBV star PG 1605+072: The Multi-Site Spectroscopic Telescope (MSST) Project, in White Dwarfs, proceedings of the conference held at the Astronomical Observatory of Capodimonte, Napoli, Italy. Eds. D. de Martino, R. Silvotti, J.-E. Solheim, and R. Kalytis. Kluwer Academic Publishers. NATO Science Series II – Mathematics, Physics and Chemistry, Vol. 105, p. 105. [ADS | arXiv]