| scholarly article | Q13442814 |
| P819 | ADS bibcode | 2017MNRAS.471.4398P |
| P818 | arXiv ID | 1707.05332 |
| P356 | DOI | 10.1093/MNRAS/STX1761 |
| P50 | author | Amanda Bauer | Q19720733 |
| Ohad Shemmer | Q53952521 | ||
| Anton Koekemoer | Q56482119 | ||
| Maurizio Paolillo | Q56551842 | ||
| Paolo Tozzi | Q56551855 | ||
| Andrea Comastri | Q56551860 | ||
| Viola Allevato | Q58375748 | ||
| Cristian Vignali | Q58914523 | ||
| Fabio Vito | Q58914893 | ||
| Teng Liu | Q58915202 | ||
| P2093 | author name string | G. Yang | |
| W. N. Brandt | |||
| I. Papadakis | |||
| B. Luo | |||
| R. Gilli | |||
| Y. Q. Xue | |||
| J. X. Wang | |||
| X. C. Zheng | |||
| P2860 | cites work | First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters | Q22066135 |
| An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30. | Q34043274 | ||
| Black Hole Models for Active Galactic Nuclei | Q56335817 | ||
| The Chandra Deep Field-South survey: 4 Ms source catalogs | Q56551834 | ||
| TheChandraDeep Field–South Survey: 2 Ms Source Catalogs | Q56556106 | ||
| TheXMM-Newtonlong look of NGC 1365: uncovering of the obscured X-ray source | Q57676331 | ||
| PRIMUS: an observationally motivated model to connect the evolution of the active galactic nucleus and galaxy populations out to z ~ 1 | Q57686763 | ||
| PRIMUS: the dependence of AGN accretion on host stellar mass and color | Q57686933 | ||
| On the Estimation of Confidence Intervals for Binomial Population Proportions in Astronomy: The Simplicity and Superiority of the Bayesian Approach | Q58490567 | ||
| A new, faint population of X-ray transients | Q58785794 | ||
| A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys | Q58786276 | ||
| Measuring X-ray variability in faint/sparsely sampled active galactic nuclei | Q58907723 | ||
| The deepest X-ray view of high-redshift galaxies: constraints on low-rate black hole accretion | Q58908111 | ||
| Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey | Q58908589 | ||
| Prevalence of X‐Ray Variability in the Chandra Deep Field–South | Q58909073 | ||
| ChandraDeep Field South: The 1 Ms Catalog | Q58909113 | ||
| Variability-selected low-luminosity active galactic nuclei in the 4 Ms Chandra Deep Field-South | Q58909580 | ||
| Deep‐Survey Constraints on X‐Ray Outbursts from Galactic Nuclei | Q58909645 | ||
| Tracing the Large‐Scale Structure in theChandraDeep Field South | Q58910836 | ||
| Active galactic nucleus X-ray variability in the XMM-COSMOS survey | Q58912185 | ||
| X-ray variability in a deep, flux-limited sample of QSOs | Q58915714 | ||
| Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies | Q58921815 | ||
| The sub-mJy radio sky in the Extended Chandra Deep Field-South: source population | Q58923566 | ||
| The radio-X-ray relation as a star formation indicator: results from the Very Large Array-Extended Chandra Deep Field-South | Q58923576 | ||
| Pan-STARRS1 variability of XMM-COSMOS AGN | Q58980737 | ||
| Active galactic nuclei as scaled-up Galactic black holes | Q59064045 | ||
| P433 | issue | 4 | |
| P407 | language of work or name | English | Q1860 |
| P921 | main subject | black hole | Q589 |
| supermassive black hole | Q40392 | ||
| P1104 | number of pages | 14 | |
| P304 | page(s) | 4398–4411 | |
| P577 | publication date | 2017-07-14 | |
| P1433 | published in | Monthly Notices of the Royal Astronomical Society | Q1536490 |
| P1476 | title | Tracing the accretion history of supermassive black holes through X-ray variability: results from the ChandraDeep Field-South | |
| P478 | volume | 471 |
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