catalogue | Q2352616 |
scholarly article | Q13442814 |
P819 | ADS bibcode | 2011ApJS..195...10X |
P818 | arXiv ID | 1105.5643 |
P356 | DOI | 10.1088/0067-0049/195/1/10 |
P5875 | ResearchGate publication ID | 231107978 |
P50 | author | Andrew C. Fabian | Q363059 |
Günther Hasinger | Q1561503 | ||
Marcella Brusa | Q56551848 | ||
Paolo Tozzi | Q56551855 | ||
Andrea Comastri | Q56551860 | ||
Cristian Vignali | Q58914523 | ||
Teng Liu | Q58915202 | ||
David M. Alexander | Q58923396 | ||
John D. Silverman | Q59675243 | ||
Donald Schneider | Q59702023 | ||
Vincenzo Mainieri | Q67221136 | ||
Amanda Bauer | Q19720733 | ||
Ohad Shemmer | Q53952521 | ||
Anton Koekemoer | Q56482119 | ||
Ian Smail | Q56547452 | ||
Maurizio Paolillo | Q56551842 | ||
P2093 | author name string | W. N. Brandt | |
D. A. Rafferty | |||
P. Rosati | |||
P. S. Broos | |||
B. Luo | |||
R. Gilli | |||
Y. Q. Xue | |||
A. E. Hornschemeier | |||
B. D. Lehmer | |||
P433 | issue | 1 | |
P304 | page(s) | 10 | |
P577 | publication date | 2011-06-29 | |
P1433 | published in | The Astrophysical Journal Supplement Series | Q2984591 |
P1476 | title | The Chandra Deep Field-South survey: 4 Ms source catalogs | |
P478 | volume | 195 |
Q59783130 | A Catalog of X-Ray Point Sources in the Abell 133 Region |
Q93012906 | A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger |
Q58785794 | A new, faint population of X-ray transients |
Q57807626 | A search for variable and transient radio sources in the extended Chandra Deep Field South at 5.5 GHz |
Q58786276 | A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys |
Q58912181 | A wide search for obscured active galactic nuclei using XMM–Newton and WISE |
Q58983738 | ALMA observations of cold molecular gas in AGN hosts at z ∼ 1.5 – evidence of AGN feedback? |
Q56549122 | ALMA resolves extended star formation in high-zAGN host galaxies |
Q58910672 | ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z = 4.75 |
Q58981949 | An X-Ray Detected Group of Quiescent Early-Type Galaxies atz= 1.6 in the Chandra Deep Field South |
Q58911793 | An enhanced fraction of starbursting galaxies among high Eddington ratio AGNs |
Q58912189 | Black hole accretion preferentially occurs in gas-rich galaxies* |
Q58983337 | Chandra survey in the AKARI North Ecliptic Pole Deep Field – I. X-ray data, point-like source catalogue, sensitivity maps, and number counts |
Q59708911 | Compton Thick AGN |
Q58981819 | Compton-thick AGN in the 70-monthSwift-BAT All-Sky Hard X-ray Survey: A Bayesian approach |
Q59783132 | Connecting the X-ray properties of weak-line and typical quasars: testing for a geometrically thick accretion disk |
Q58694691 | Demography of High-Redshift AGN |
Q58911797 | Dust attenuation inz~ 1 galaxies fromHerscheland 3D-HST Hαmeasurements |
Q58913599 | Early BHs: simulations and observations |
Q58908416 | Evidence for two modes of black hole accretion in massive galaxies at z∼2 |
Q58916875 | Evidence for wide-spread active galactic nucleus-driven outflows in the most massive z ~ 1-2 star-forming galaxies |
Q58907769 | Faint AGNs atz>4 in the CANDELS GOODS-S field: looking for contributors to the reionization of the Universe |
Q58908665 | Faint high-redshift AGN in theChandradeep field south: the evolution of the AGN luminosity function and black hole demography |
Q58786295 | Finding rare AGN: X-ray number counts of Chandra sources in Stripe 82 |
Q58786248 | Finding rare AGN: XMM–Newton and Chandra observations of SDSS Stripe 82 |
Q56039594 | First identification of direct collapse black hole candidates in the early Universe in CANDELS/GOODS-S |
Q58909561 | GOODS-Herschel: the far-infrared view of star formation in active galactic nucleus host galaxies since z ≈ 3 |
Q58831058 | Galaxy Zoo: Are bars responsible for the feeding of active galactic nuclei at 0.2 < z < 1.0? |
Q58916248 | HerMES: disentangling active galactic nuclei and star formation in the radio source population |
Q56550900 | Herschel-PACS observations of [Oi]63 μm towards submillimetre galaxies atz∼ 1 |
Q58908052 | High-redshift AGN in the Chandra Deep Fields: the obscured fraction and space density of the sub-L* population |
Q58785723 | Inferring Compton-thick AGN candidates at z > 2 with Chandra using the >8 keV rest-frame spectral curvature |
Q58910636 | Limits on the LyC signal fromz~ 3 sources with secure redshift and HST coverage in the E-CDFS field |
Q61207001 | Low-mass black holes as the remnants of primordial black hole formation |
Q58909223 | Luminous and Obscured Quasars and Their Host Galaxies |
Q58909527 | Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star-forming galaxies at 2 < z < 3 |
Q58910654 | Mapping the average AGN accretion rate in the SFR–M* plane for Herschel★-selected galaxies at 0 < z ≤ 2.5 |
Q57686628 | Massive compact galaxies with high-velocity outflows: morphological analysis and constraints on AGN activity |
Q58909411 | Mid-infrared luminous quasars in the GOODS–Herschelfields: a large population of heavily obscured, Compton-thick quasars atz≈ 2 |
Q58908428 | Morphologies of z ∼ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity |
Q58035429 | Nebular excitation in z ~ 2 star-forming galaxies from the SINS and LUCI surveys: the influence of shocks and active galactic nuclei |
Q58909530 | Nuclear activity is more prevalent in star-forming galaxies |
Q105582762 | Obscured accretion from AGN surveys |
Q58912217 | On theLx–L6 μmratio as a diagnostic for Compton-thick AGN |
Q58910657 | Peering through the holes: the far-UV color of star-forming galaxies atz~ 3−4 and the escaping fraction of ionizing radiation |
Q58909486 | Reversal or no reversal: the evolution of the star formation rate–density relation up to z ∼ 1.6 |
Q58004763 | SUDARE-VOICE variability-selection of active galaxies in theChandraDeep Field South and the SERVS/SWIRE region |
Q58981853 | Searching for highly obscured AGNs in theXMM-Newtonserendipitous source catalog |
Q58908272 | Star formation and quenching among the most massive galaxies at z ∼ 1.7 |
Q58923537 | Star formation properties of sub-mJy radio sources |
Q58035389 | THE SINS/zC-SINF SURVEY OFz∼ 2 GALAXY KINEMATICS: EVIDENCE FOR POWERFUL ACTIVE GALACTIC NUCLEUS-DRIVEN NUCLEAR OUTFLOWS IN MASSIVE STAR-FORMING GALAXIES |
Q58981826 | The 5–10 keV AGN luminosity function at 0.01 |
Q58923559 | The AGN content of deep radio surveys and radio emission in radio-quiet AGN. Why every astronomer should care about deep radio fields |
Q63374736 | The KMOS3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6–2.7 |
Q68175397 | The KMOS^3D^ survey: design, first results, and the evolution of galaxy kinematics from 0.7 <= z <= 2.7 |
Q57712673 | The MUSE Hubble Ultra Deep Field Survey I. Survey description, data reduction, and source detection |
Q58908172 | The VIMOS Ultra Deep Survey: Lyαemission and stellar populations of star-forming galaxies at 2 < z < 2.5 |
Q58983718 | The WISSH quasars project |
Q58912176 | The XMM Deep Survey in the CDF-S |
Q58909376 | The XMM deep survey in the CDF-S |
Q58912178 | The XMM deep survey in the CDF-S |
Q58912201 | The XMM deep survey in the CDF-S |
Q58912206 | The XMM deep survey in the CDF-S |
Q58912213 | The XMM deep survey in the CDF-S |
Q58912204 | The XMM deep survey in the CDF-S. IV. Compton-thick AGN candidates |
Q58981836 | The XXL Survey |
Q58908548 | The ages, masses and star formation rates of spectroscopically confirmed z ∼ 6 galaxies in CANDELS |
Q58908111 | The deepest X-ray view of high-redshift galaxies: constraints on low-rate black hole accretion |
Q57710839 | The deepestHerschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations |
Q58909509 | The evolution of star formation activity in galaxy groups |
Q58908305 | The galaxy stellar mass function at 3.5 ≤ z ≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields |
Q58912193 | The hard X-ray luminosity function of high-redshift (3 < z ≲ 5) active galactic nuclei |
Q58908339 | The host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS |
Q58908218 | The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 |
Q58909544 | The lack of star formation gradients in galaxy groups up to z ∼ 1.6 |
Q58910712 | The nature of the unresolved extragalactic cosmic soft X-ray background |
Q58908584 | The spectral energy distributions, host galaxies and environments of variability-selected active galactic nuclei in GOODS-South |
Q58911805 | The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities |
Q58923566 | The sub-mJy radio sky in the Extended Chandra Deep Field-South: source population |
Q58786184 | The systematic search for z ≳ 5 active galactic nuclei in the Chandra Deep Field South |
Q58909271 | Tracing the accretion history of supermassive black holes through X-ray variability: results from the ChandraDeep Field-South |
Q58910687 | Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel |
Q58909440 | Ultra-deep catalog of X-ray groups in the ExtendedChandraDeep Field South |
Q58004790 | Variability-selected active galactic nuclei in the VST-SUDARE/VOICE survey of the COSMOS field |
Q58981842 | X-ray observations of dust obscured galaxies in theChandradeep field south |
Q58910714 | X-ray properties of radio-selected star forming galaxies in theChandra-COSMOS survey |
Q56553872 | XMM–Newton view of X-ray overdensities from nearby galaxy clusters: the environmental dependencies |
Q59268370 | ZFOURGE catalogue of AGN candidates: an enhancement of 160-μm-derived star formation rates in active galaxies toz = 3.2 |
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