A hyperluminous obscured quasar at a redshift of z \textasciitilde 4.3. Efstathiou, A., Malek, K., Burgarella, D., Hurley, P., Oliver, S., Buat, V., Shirley, R., Duivenvoorden, S., Papadopoulou Lesta, V., Farrah, D., Duncan, K. J., & Campos Varillas, M. d. C. arXiv e-prints, 2103:arXiv:2103.08032, March, 2021. ![A hyperluminous obscured quasar at a redshift of z \textasciitilde 4.3 [link]](https://bibbase.org/img/filetypes/link.svg "link")
Paper abstract bibtex In this work we report the discovery of the hyperluminous galaxy HELP_J100156.75+022344.7 at the photometric redshift of z \textasciitilde 4.3. The galaxy was discovered in the Cosmological Evolution Survey (COSMOS) field, one of the fields studied by the Herschel Extragalactic Legacy Project (HELP). We present the spectral energy distribution (SED) of the galaxy and fit it with the CYprus models for Galaxies and their NUclear Spectra (CYGNUS) multi-component radiative transfer models. We find that its emission is dominated by an obscured quasar with a predicted total 1-1000um luminosity of \$3.91{\textasciicircum}\{+1.69\}_\{-0.55\} {\textbackslash}times 10{\textasciicircum}\{13\} L_{\textbackslash}odot\$ and an active galactic nucleus (AGN) fraction of \textasciitilde89%. We also fit HELP_J100156.75+022344.7 with the Code Investigating GALaxy Emission (CIGALE) code and find a similar result. This is only the second z \textgreater 4 hyperluminous obscured quasar discovered to date. The discovery of HELP_J100156.75+022344.7 in the \textasciitilde 2deg\textasciicircum2 COSMOS field implies that a large number of obscured hyperluminous quasars may lie in the HELP fields which cover \textasciitilde 1300deg\textasciicircum2. If this is confirmed, tension between supermassive black hole evolution models and observations will be alleviated. We estimate the space density of objects like HELP_J100156.75+022344.7 at z \textasciitilde 4.5 to be \${\textbackslash}sim 1.8 {\textbackslash}times 10{\textasciicircum}\{-8\}\$Mpc\${\textasciicircum}\{-3\}\$. This is slightly higher than the space density of coeval hyperluminous optically selected quasars suggesting that the obscuring torus in z \textgreater 4 quasars may have a covering factor \${\textbackslash}gtrsim 50{\textbackslash}%\$.
@article{efstathiou_hyperluminous_2021,
title = {A hyperluminous obscured quasar at a redshift of z {\textasciitilde} 4.3},
volume = {2103},
url = {http://adsabs.harvard.edu/abs/2021arXiv210308032E},
abstract = {In this work we report the discovery of the hyperluminous galaxy HELP\_J100156.75+022344.7 at the photometric redshift of z {\textasciitilde} 4.3. The galaxy was discovered in the Cosmological Evolution Survey (COSMOS) field, one of the fields studied by the Herschel Extragalactic Legacy Project (HELP). We present the spectral energy distribution (SED) of the galaxy and fit it with the CYprus models for Galaxies and their NUclear Spectra (CYGNUS) multi-component radiative transfer models. We find that its emission is dominated by an obscured quasar with a predicted total 1-1000um luminosity of \$3.91{\textasciicircum}\{+1.69\}\_\{-0.55\} {\textbackslash}times 10{\textasciicircum}\{13\} L\_{\textbackslash}odot\$ and an active galactic nucleus (AGN) fraction of {\textasciitilde}89\%. We also fit
HELP\_J100156.75+022344.7 with the Code Investigating GALaxy Emission (CIGALE) code and find a similar result. This is only the second z {\textgreater} 4 hyperluminous obscured quasar discovered to date. The discovery of HELP\_J100156.75+022344.7 in the {\textasciitilde} 2deg{\textasciicircum}2 COSMOS field implies that a large number of obscured hyperluminous quasars may lie in the HELP fields which cover {\textasciitilde} 1300deg{\textasciicircum}2. If this is confirmed, tension between supermassive black hole evolution models and observations will be alleviated. We estimate the space density of objects like
HELP\_J100156.75+022344.7 at z {\textasciitilde} 4.5 to be \${\textbackslash}sim 1.8 {\textbackslash}times
10{\textasciicircum}\{-8\}\$Mpc\${\textasciicircum}\{-3\}\$. This is slightly higher than the space density of coeval hyperluminous optically selected quasars suggesting that the obscuring torus in z {\textgreater} 4 quasars may have a covering factor \${\textbackslash}gtrsim 50{\textbackslash}\%\$.},
urldate = {2021-03-23},
journal = {arXiv e-prints},
author = {Efstathiou, Andreas and Malek, Katarzyna and Burgarella, Denis and Hurley, Peter and Oliver, Seb and Buat, Veronique and Shirley, Raphael and Duivenvoorden, Steven and Papadopoulou Lesta, Vicky and Farrah, Duncan and Duncan, Kenneth J. and Campos Varillas, Maria del Carmen},
month = mar,
year = {2021},
keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
pages = {arXiv:2103.08032},
}
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We present the spectral energy distribution (SED) of the galaxy and fit it with the CYprus models for Galaxies and their NUclear Spectra (CYGNUS) multi-component radiative transfer models. We find that its emission is dominated by an obscured quasar with a predicted total 1-1000um luminosity of \\$3.91{\\textasciicircum}\\{+1.69\\}_\\{-0.55\\} {\\textbackslash}times 10{\\textasciicircum}\\{13\\} L_{\\textbackslash}odot\\$ and an active galactic nucleus (AGN) fraction of \\textasciitilde89%. We also fit HELP_J100156.75+022344.7 with the Code Investigating GALaxy Emission (CIGALE) code and find a similar result. This is only the second z \\textgreater 4 hyperluminous obscured quasar discovered to date. The discovery of HELP_J100156.75+022344.7 in the \\textasciitilde 2deg\\textasciicircum2 COSMOS field implies that a large number of obscured hyperluminous quasars may lie in the HELP fields which cover \\textasciitilde 1300deg\\textasciicircum2. If this is confirmed, tension between supermassive black hole evolution models and observations will be alleviated. We estimate the space density of objects like HELP_J100156.75+022344.7 at z \\textasciitilde 4.5 to be \\${\\textbackslash}sim 1.8 {\\textbackslash}times 10{\\textasciicircum}\\{-8\\}\\$Mpc\\${\\textasciicircum}\\{-3\\}\\$. This is slightly higher than the space density of coeval hyperluminous optically selected quasars suggesting that the obscuring torus in z \\textgreater 4 quasars may have a covering factor \\${\\textbackslash}gtrsim 50{\\textbackslash}%\\$.","urldate":"2021-03-23","journal":"arXiv e-prints","author":[{"propositions":[],"lastnames":["Efstathiou"],"firstnames":["Andreas"],"suffixes":[]},{"propositions":[],"lastnames":["Malek"],"firstnames":["Katarzyna"],"suffixes":[]},{"propositions":[],"lastnames":["Burgarella"],"firstnames":["Denis"],"suffixes":[]},{"propositions":[],"lastnames":["Hurley"],"firstnames":["Peter"],"suffixes":[]},{"propositions":[],"lastnames":["Oliver"],"firstnames":["Seb"],"suffixes":[]},{"propositions":[],"lastnames":["Buat"],"firstnames":["Veronique"],"suffixes":[]},{"propositions":[],"lastnames":["Shirley"],"firstnames":["Raphael"],"suffixes":[]},{"propositions":[],"lastnames":["Duivenvoorden"],"firstnames":["Steven"],"suffixes":[]},{"propositions":[],"lastnames":["Papadopoulou","Lesta"],"firstnames":["Vicky"],"suffixes":[]},{"propositions":[],"lastnames":["Farrah"],"firstnames":["Duncan"],"suffixes":[]},{"propositions":[],"lastnames":["Duncan"],"firstnames":["Kenneth","J."],"suffixes":[]},{"propositions":[],"lastnames":["Campos","Varillas"],"firstnames":["Maria","del","Carmen"],"suffixes":[]}],"month":"March","year":"2021","keywords":"Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics","pages":"arXiv:2103.08032","bibtex":"@article{efstathiou_hyperluminous_2021,\n\ttitle = {A hyperluminous obscured quasar at a redshift of z {\\textasciitilde} 4.3},\n\tvolume = {2103},\n\turl = {http://adsabs.harvard.edu/abs/2021arXiv210308032E},\n\tabstract = {In this work we report the discovery of the hyperluminous galaxy HELP\\_J100156.75+022344.7 at the photometric redshift of z {\\textasciitilde} 4.3. The galaxy was discovered in the Cosmological Evolution Survey (COSMOS) field, one of the fields studied by the Herschel Extragalactic Legacy Project (HELP). We present the spectral energy distribution (SED) of the galaxy and fit it with the CYprus models for Galaxies and their NUclear Spectra (CYGNUS) multi-component radiative transfer models. We find that its emission is dominated by an obscured quasar with a predicted total 1-1000um luminosity of \\$3.91{\\textasciicircum}\\{+1.69\\}\\_\\{-0.55\\} {\\textbackslash}times 10{\\textasciicircum}\\{13\\} L\\_{\\textbackslash}odot\\$ and an active galactic nucleus (AGN) fraction of {\\textasciitilde}89\\%. We also fit\nHELP\\_J100156.75+022344.7 with the Code Investigating GALaxy Emission (CIGALE) code and find a similar result. This is only the second z {\\textgreater} 4 hyperluminous obscured quasar discovered to date. The discovery of HELP\\_J100156.75+022344.7 in the {\\textasciitilde} 2deg{\\textasciicircum}2 COSMOS field implies that a large number of obscured hyperluminous quasars may lie in the HELP fields which cover {\\textasciitilde} 1300deg{\\textasciicircum}2. If this is confirmed, tension between supermassive black hole evolution models and observations will be alleviated. We estimate the space density of objects like\nHELP\\_J100156.75+022344.7 at z {\\textasciitilde} 4.5 to be \\${\\textbackslash}sim 1.8 {\\textbackslash}times\n10{\\textasciicircum}\\{-8\\}\\$Mpc\\${\\textasciicircum}\\{-3\\}\\$. 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