COSMOLOGICAL EVOLUTION OF THE HARD X-RAY AGN LUMINOSITY FUNCTION

By Y. Ueda, M. Akiyama, K. Ohta, T. Miyaji. 2004

313 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/8d4ac4ab8c21f0cb0738822cf454641b0ec4787b

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. P. Hopkins
2. D. M. Alexander
3. L. Hernquist
4. W. N. Brandt
5. T. Heckman
6. R. Somerville
7. R. Dav'e
8. A. Merloni

Citations in the corpus

• The Relation between Quasar and Merging Galaxy Luminosity Functions and the Merger-driven Star Formation History of the Universe (2006, methodology): “…of uncertainty, as we generally employ hard X-ray samples that are complete to luminosities well below those of interest in our analysis, especially at the moderate redshifts that we consider in detail (see, e.g., Ueda et al. 2003), and have been corrected for obscuring columns with NHP 1025 cm 2.”
• Present-Day Growth of Black Holes and Bulges: The Sloan Digital Sky Survey Perspective (2004, background): “More recently X-ray surveys (Ueda et al. 2003; Steffen et al. 2003) have shown that the peak in the comoving emissivity of the AGN population occurs at lower and lower redshift for AGNs of lower and lower luminosity.”
• Active galactic nuclei: what’s in a name? (2017, background): “Some authors have found that the fraction of obscured lines-of-sight diminishes with increasing luminosity of the accretion disk (Ueda et al. 2003; Hasinger 2004; Simpson 2005; Hatziminaoglou et al. 2008; Assef et al. 2013; Mateos et al. 2016), an effect typically referred to as the receding torus…”
• THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION (2013, background): “…and luminosity correspond to the peak epoch in the black hole accretion history of the Universe and the knee of the X-ray luminosity function (e.g., Ueda et al. 2003; La Franca et al. 2005; Aird et al. 2010); thus, NuSTAR should detect the AGN source population that dominates the cosmic growth of…”
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. I. Galaxy Mergers and Quasar Activity (2007, methodology): “…will be obscured, of course, but we find that, e.g., using the full dis- tribution of column densities as a function of quasar luminosity from Ueda et al. (2003) to attenuate a template AGN SED yields a very similar answer (see also Franceschini et al. 2005), as does using a mean X-ray to…”
• SELF-CONSISTENT MODELS OF THE AGN AND BLACK HOLE POPULATIONS: DUTY CYCLES, ACCRETION RATES, AND THE MEAN RADIATIVE EFFICIENCY (2007, background): “…Richards et al. 2005, 2006; Jiang et al. 2006; Cool et al. 2006; Bongiorno et al. 2007; Fontanot et al. 2007; Shankar & Mathur 2007) and X-ray surveys (Barger et al. 2003; Ueda et al. 2003; Barger & Cowie 2005; Barger et al. 2005; La Franca et al. 2005; Nandra et al. 2005; Silverman et al. 2008).”
• The bolometric quasar luminosity function at z = 0–7 (2020, methodology): “In the bottom panel of Figure 3, we show the NH distribution at log LX = 43.5, z = 0.05 comparing different models (Ueda et al. 2003; Gilli et al. 2007; Treister et al. 2009; Ueda et al. 2014; Aird et al. 2015a).”
• The incidence of obscuration in active galactic nuclei (2013, methodology): “…to corroborate claims of positive evolution of the fraction of obscured AGN with increasing redshift (La Franca et al. 2005; Ballantyne et al. 2006; Treister et al. 2006; Hasinger 2008) as well as counterclaims of no significant evolution (Ueda et al. 2003; Tozzi et al. 2006; Gilli et al. 2007).”
• OBSCURATION-DEPENDENT EVOLUTION OF ACTIVE GALACTIC NUCLEI (2015, methodology): “Previous studies also find that the fraction of obscured AGN decreases with increasing luminosity (e.g. Ueda et al. 2003; Akylas et al. 2006; Ueda et al. 2014).”
• BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog (2017, background): “…of obscured and unobscured AGN (e.g., Della Ceca et al. 2008; Burlon et al. 2011; Aird et al. 2015), and is consistent with the observed decrease of the fraction of obscured sources with increasing luminosity (e.g., Ueda et al. 2003; Treister & Urry 2006; Burlon et al. 2011; Ueda et al. 2014).”
• HST WFC3/IR OBSERVATIONS OF ACTIVE GALACTIC NUCLEUS HOST GALAXIES AT z ∼ 2: SUPERMASSIVE BLACK HOLES GROW IN DISK GALAXIES (2010, methodology): “These AGN host galaxies are a significant fraction of the total AGN population by number density and in terms of light emitted by accretion (Ueda et al. 2003; Hasinger et al. 2005).”
• The dust covering factor in active galactic nuclei (2016, background): “The decrease of the covering factor of the torus with increasing luminosity is systematically found in X-ray surveys (e.g. Ueda et al. 2003; Beckmann et al. 2009; Burlon et al. 2011; Ricci et al. 2013; Merloni et al. 2014; Ueda et al. 2014; Buchner et al. 2015).”
• THE CHANDRA COSMOS LEGACY SURVEY: OPTICAL/IR IDENTIFICATIONS (2015, background): “More recently, Ueda et al. (2003) confirmed the result in the 2-10 keV (rest frame) band: at low luminosities, LX≃10 42 erg s−1, almost the whole sample is composed of obscured AGN, while unobscured sources prevail moving towards high luminosities, i.e. LX>10 44 erg s−1.”
• AGN wind scaling relations and the co-evolution of black holes and galaxies (2017, background): “BALs are from z = 2–3 QSOs.”
• Universal bolometric corrections for active galactic nuclei over seven luminosity decades (2020, background): “…A73, page 1 of 16 correction is fundamental for converting the AGN luminosity function into the accretion rate history (Salucci & Persic 1999; Ueda et al. 2003; Volonteri et al. 2003; Shankar et al. 2004; Marconi et al. 2004; Vittorini et al. 2005; La Franca et al. 2005; Aversa et al. 2015)…”
• Unveiling Obscured Accretion in the Chandra Deep Field-South (2007, background): “…of AGN is luminosity dependent, with lower luminosity AGN peaking at a redshift lower than luminous QSOs (Hasinger 2003, 2005, Fiore et al. 2003, Ueda et al. 2003, La Franca et al. 2005, Brandt & Hasinger 2005, Bongiorno et al. 2007), a bimodal behavior recalling the evolution of star-forming…”
• MID-INFRARED SELECTION OF ACTIVE GALACTIC NUCLEI WITH THE WIDE-FIELD INFRARED SURVEY EXPLORER. II. PROPERTIES OF WISE-SELECTED ACTIVE GALACTIC NUCLEI IN THE NDWFS BOÖTES FIELD (2012, methodology): “Furthermore, Ueda et al. (2003) has shown that the distribution of neutral gas column densities obscuring the X-ray emission of AGN is independent of redshift.”
• The Relationship of Hard X-Ray and Optical Line Emission in Low-Redshift Active Galactic Nuclei (2005, background): “On the other hand, the deep X-ray surveys carried out by the Chandra X-ray Observatory have revolutionized our picture of the cosmic history of the AGN phenomenon and thus of the growth of supermassive black holes (e.g., Ueda et al. 2003; Barger et al. 2005, hereafter B05; Hasinger et al. 2005).”
• Cosmological simulations of black hole growth: AGN luminosities and downsizing (2013, methodology): “…ROSAT, ASCA, eRosita; e.g. Miyaji, Hasinger & Schmidt 2000; La Franca et al. 2002; Barger et al. 2003; Cowie et al. 2003; Fiore et al. 2003, 2012; Ueda et al. 2003; Sazonov & Revnivtsev 2004; Barger & Cowie 2005; Hasinger, Miyaji & Schmidt 2005; Nandra, Laird & Steidel 2005; Ebrero et al. 2009;…”