Dimitra Rigopoulou

1996-2002 Max-Planck-Institut für extraterrestrische Physik 
 2003- University of Oxford, Oxford, United Kingdom 
"Dimitra Rigopoulou"
Mean distance: (not calculated yet)
BETA: Related publications


You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.

Cheng C, Cao X, Lu N, et al. (2020) ALMA $[{\rm{N}}\,{\rm{II}}]$ 205 μm Imaging Spectroscopy of the Lensed Submillimeter Galaxy ID 141 at Redshift 4.24 The Astrophysical Journal. 898: 33
Zhao (赵应和) Y, Lu N, Díaz-Santos T, et al. (2020) ALMA Imaging of the CO (7–6) Line Emission in the Submillimeter Galaxy LESS 073 at z = 4.755 The Astrophysical Journal. 892: 145
Hernán-Caballero A, Spoon HWW, Alonso-Herrero A, et al. (2020) Extinction in the 11.2 µm PAH band and the low L11.2/LIR in ULIRGs Monthly Notices of the Royal Astronomical Society. 497: 4614-4625
Alonso-Herrero A, Pereira-Santaella M, Rigopoulou D, et al. (2020) Cold molecular gas and PAH emission in the nuclear and circumnuclear regions of Seyfert galaxies. Astronomy and Astrophysics. 639
Cortzen I, Magdis GE, Valentino F, et al. (2020) Deceptively cold dust in the massive starburst galaxy GN20 at z ∼ 4 Astronomy and Astrophysics. 634
D'Amato Q, Gilli R, Vignali C, et al. (2020) Dust and gas content of high-redshift galaxies hosting obscured AGN in the Chandra Deep Field-South Astronomy and Astrophysics. 636
Pereira-Santaella M, Rigopoulou D, Magdis GE, et al. (2019) Optical integral field spectroscopy of intermediate redshift infrared bright galaxies Monthly Notices of the Royal Astronomical Society. 486: 5621-5645
Marques-Chaves R, Pérez-Fournon I, Villar-Martín M, et al. (2019) Discovery of a giant and luminous Lyα+C IV+He II nebula at z = 3.326 with extreme emission line ratios Astronomy and Astrophysics. 629
Alonso-Herrero A, García-Burillo S, Pereira-Santaella M, et al. (2019) Nuclear molecular outflow in the Seyfert galaxy NGC 3227. Astronomy and Astrophysics. 628
Lu N, Cao T, Díaz-Santos T, et al. (2018) CO (7−6), [C i] 370 μm, and [N ii] 205 μm Line Emission of the QSO BRI 1335-0417 at Redshift 4.407 The Astrophysical Journal. 864: 38
See more...