scholarly article | Q13442814 |
P819 | ADS bibcode | 2016A&A...594A..73A |
P818 | arXiv ID | 1607.08069 |
P356 | DOI | 10.1051/0004-6361/201628711 |
P724 | Internet Archive ID | arxiv-1607.08069 |
P50 | author | Piero Ranalli | Q56562515 |
Amalia Corral | Q58374109 | ||
P2093 | author name string | I. Georgantopoulos | |
A. Akylas | |||
G. Lanzuisi | |||
E. Gkiokas | |||
P2860 | cites work | The Swift X-Ray Telescope | Q55952012 |
The Chandra Deep Field-South survey: 4 Ms source catalogs | Q56551834 | ||
The Faint‐End Slopes of Galaxy Luminosity Functions in the COSMOS Field | Q56567294 | ||
The SDSS-III Baryon Oscillation Spectroscopic Survey: the quasar luminosity function from Data Release nine | Q57630686 | ||
Suzakuobservation of the LINER NGC 4102 | Q57676296 | ||
Suzaku and SWIFT-BAT observations of a newly discovered Compton-thick AGN | Q57676298 | ||
TheXMM-Newtonlong look of NGC 1365: uncovering of the obscured X-ray source | Q57676331 | ||
The [O iii] emission line luminosity function of optically selected type-2 AGN from zCOSMOS$^{\rm,}$ | Q58035639 | ||
THE NuSTAR EXTRAGALACTIC SURVEY: FIRST DIRECT MEASUREMENTS OF THE ≳10 keV X-RAY LUMINOSITY FUNCTION FOR ACTIVE GALACTIC NUCLEI AT z > 0.1 | Q58358250 | ||
THE NuSTAR EXTRAGALACTIC SURVEYS: INITIAL RESULTS AND CATALOG FROM THE EXTENDED CHANDRA DEEP FIELD SOUTH | Q58358263 | ||
The 60 month all-sky burst alert telescope survey of active galactic nucleus and the anisotropy of nearby AGNs | Q58358309 | ||
Three-year Swift-BAT survey of active galactic nuclei: reconciling theory and observations? | Q58358331 | ||
IC 751: a new changing look AGN discovered by NuSTAR | Q58785991 | ||
THENuSTAREXTRAGALACTIC SURVEYS: OVERVIEW AND CATALOG FROM THE COSMOS FIELD | Q58786157 | ||
Broadband observations of the Compton-Thick nucleus of NGC 3393 | Q58786165 | ||
THE 2-79 keV X-RAY SPECTRUM OF THE CIRCINUS GALAXY WITHNuSTAR,XMM-Newton, ANDCHANDRA: A FULLY COMPTON-THICK ACTIVE GALACTIC NUCLEUS | Q58786197 | ||
Lifting the veil on obscured accretion: active galactic nuclei number counts and survey strategies for imaging hard X-ray missions | Q58786409 | ||
The space density of compton-thick active galactic nucleus and the X-ray background | Q58786558 | ||
Detailed shape and evolutionary behavior of the X-ray luminosity function of active galactic nuclei | Q58908278 | ||
Compton thick AGN in the XMM-COSMOS survey | Q58908327 | ||
Identifying luminous active galactic nuclei in deep surveys: revised IRAC selection criteria | Q58908640 | ||
A new extensive catalog of optically variable active galactic nuclei in the GOODS fields and a new statistical approach to variability selection | Q58908762 | ||
The Cosmic X‐Ray Background and the Population of the Most Heavily Obscured AGNs | Q58908830 | ||
Hard X-ray emission of the luminous infrared galaxy NGC 6240 as observed by NuSTAR | Q58909312 | ||
NuSTARcatches the unveiling nucleus of NGC 1068 | Q58909334 | ||
Compton-thick accretion in the local universe | Q58909364 | ||
NuSTAROBSERVATIONS OF THE COMPTON-THICK ACTIVE GALACTIC NUCLEUS AND ULTRALUMINOUS X-RAY SOURCE CANDIDATE IN NGC 5643 | Q58909367 | ||
THENuSTARVIEW OF REFLECTION AND ABSORPTION IN NGC 7582 | Q58909428 | ||
THENuSTARVIEW OF NEARBY COMPTON-THICK ACTIVE GALACTIC NUCLEI: THE CASES OF NGC 424, NGC 1320, AND IC 2560 | Q58909496 | ||
The variable hard X-ray emission of NGC 4945 as observed by NuSTAR | Q58909515 | ||
TheXMMDeep survey in the CDF-S | Q58909598 | ||
Mass without radiation: Heavily obscured AGNs, the X-ray background, and the black hole mass density | Q58912172 | ||
The XMM deep survey in the CDF-S. IV. Compton-thick AGN candidates | Q58912204 | ||
On theLx–L6 μmratio as a diagnostic for Compton-thick AGN | Q58912217 | ||
Suzaku observations of hard x-ray-selected Seyfert 2 galaxies | Q58912237 | ||
The synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era | Q58912291 | ||
A new measurement of the cosmic X-ray background | Q58913250 | ||
The 2–10 keV unabsorbed luminosity function of AGN from the LSS, CDFS, and COSMOS surveys | Q58981813 | ||
Toward the standard population synthesis model of the X-ray background: evolution of X-ray luminosity and absorption functions of active galactic nuclei including compton-thick populations | Q58983358 | ||
P407 | language of work or name | English | Q1860 |
P304 | page(s) | 73–73 | |
P577 | publication date | 2016-10-01 | |
P1433 | published in | Astronomy and Astrophysics | Q752075 |
P1476 | title | Compton-thick AGN in the 70-monthSwift-BAT All-Sky Hard X-ray Survey: A Bayesian approach | |
P478 | volume | 594 |
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