Sotiria Fotopoulou

Affiliations: 
2012 Technical University of Munich (TUM), München, Bayern, Germany 
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"Sotiria Fotopoulou"
Cross-listing: Physics Tree

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Guenther Hasinger grad student 2012 Technical University of Munich (Physics Tree)
 (The X-ray luminosity function of AGN in the Lockman Hole Deep Field)
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Publications

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Fawcett VA, Alexander DM, Rosario DJ, et al. (2020) Fundamental differences in the radio properties of red and blue quasars: enhanced compact AGN emission in red quasars Monthly Notices of the Royal Astronomical Society. 494: 4802-4818
Fumagalli M, Fotopoulou S, Thomson L. (2020) Detecting neutral hydrogen at z ≳ 3 in large spectroscopic surveys of quasars Monthly Notices of the Royal Astronomical Society
Šlaus B, Smolčić V, Novak M, et al. (2020) The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations Astronomy and Astrophysics. 638
Ricci M, Birkinshaw M, Bremer M, et al. (2020) The XXL Survey XLIV. Sunyaev-Zel'dovich mapping of a low-mass cluster at z~1: a multi-wavelength approach Astronomy and Astrophysics
Masoura VA, Georgantopoulos I, Mountrichas G, et al. (2020) The XXL Survey. XL. Obscuration properties of red AGNs in XXL-N Astronomy and Astrophysics. 638
Logan C, Fotopoulou S. (2020) Unsupervised star, galaxy, qso classification: Application of HDBSCAN Astronomy and Astrophysics. 633
Masters DC, Stern DK, Cohen JG, et al. (2019) The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Analysis and Data Release 2 The Astrophysical Journal. 877: 81
Klindt L, Alexander DM, Rosario DJ, et al. (2019) Fundamental differences in the radio properties of red and blue quasars: evolution strongly favoured over orientation Monthly Notices of the Royal Astronomical Society. 488: 3109-3128
Barnett R, Warren SJ, Mortlock DJ, et al. (2019) Euclid preparation: V. Predicted yield of redshift 7 < z < 9 quasars from the wide survey Astronomy and Astrophysics. 631
Guglielmo V, Poggianti BM, Vulcani B, et al. (2019) The XXL Survey. XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1 ≤ z ≤ 0.5 Astronomy and Astrophysics. 625
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