Markos Trichas
Affiliations: | 2007 | Imperial College, London, London, England, United Kingdom | |
| 2013- | Airbus |
Website:
https://www.linkedin.com/in/markos-trichas-80a43627/Google:
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Publications
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| Trichas M, Green PJ, Silverman JD, et al. (2017) Erratum: “The Chandra Multi-wavelength Project: Optical Spectroscopy and the Broadband Spectral Energy Distributions of X-ray-selected AGNs” (2012, ApJS, 200, 17) Astrophysical Journal Supplement Series. 231: 23 |
| Trichas M, Green PJ, Constantin A, et al. (2013) Empirical Links between XRB and AGN Accretion Using the Complete z < 0.4 Spectroscopic CSC/SDSS Catalog The Astrophysical Journal. 778: 188 |
| Page MJ, Symeonidis M, Vieira JD, et al. (2012) The suppression of star formation by powerful active galactic nuclei. Nature. 485: 213-6 |
| Roseboom IG, Ivison RJ, Greve TR, et al. (2012) The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts Monthly Notices of the Royal Astronomical Society. 419: 2758-2773 |
| Trichas M, Green PJ, Silverman JD, et al. (2012) The chandra multi-wavelength project: Optical spectroscopy and the broadband spectral energy distributions of X-ray-selected AGNs Astrophysical Journal, Supplement Series. 200 |
| Goulding AD, Alexander DM, Bauer FE, et al. (2012) Deep silicate absorption features in compton-thick active galactic nuclei predominantly arise due to dust in the host galaxy Astrophysical Journal. 755 |
| Dai YS, Bergeron J, Elvis M, et al. (2012) A population of dust-rich quasars at z ∼ 1.5 Astrophysical Journal. 753 |
| Kim DW, Protopapas P, Trichas M, et al. (2012) A refined QSO selection method using diagnostics tests: 663 QSO candidates in the Large Magellanic Cloud Astrophysical Journal. 747 |
| Mauduit JC, Lacy M, Farrah D, et al. (2012) The spitzer extragalactic representative volume survey (SERVS): Survey definition and goals Publications of the Astronomical Society of the Pacific. 124: 714-736 |
| Béthermin M, Le Floc'H E, Ilbert O, et al. (2012) HerMES: Deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background Astronomy and Astrophysics. 542 |