The nature of the faint radio source population from observations of the Subaru/XMM-Newton Deep Field

The nature of the faint radio source population from observations of the Subaru/XMM-Newton Deep Field

Dades bibliogràfiques
Autors principals:	Simpson, C, Rawlings, S, Martinez-Sansigre, A
Format:	Journal article
Publicat:	2006

Ítems similars

Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source population
per: Simpson, C, et al.
Publicat: (2006)

Accretion indicators for the 37 brightest radio sources in the Subaru/XMM-Newton Deep Field
per: Vardoulaki, E, et al.
Publicat: (2007)

The Subaru/XMM-Newton Deep Field - II. The 37 brightest radio sources
per: Vardoulaki, E, et al.
Publicat: (2008)

Low-power radio galaxy environments in the Subaru/XMM-Newton Deep Field at z~0.5
per: Geach, J, et al.
Publicat: (2007)

The Subaru/XMM-Newton deep survey (SXDS). V. Optically faint variable object survey
per: Morokuma, T, et al.
Publicat: (2008)

The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey
per: Okumura, J, et al.
Publicat: (2014)

Evolution of faint radio sources in the VIDEO-XMM3 field
per: McAlpine, K, et al.
Publicat: (2013)

X-ray groups and clusters of galaxies in the Subaru-XMM Deep Field
per: Finoguenov, A, et al.
Publicat: (2009)

The SVBABU/XMM-Newton deep survey (SXDS). V. Optically faint variable object survey
per: Morokuma, T, et al.
Publicat: (2008)

The XMM-SERVS survey: new XMM–Newton point-source catalogue for the XMM-LSS field
per: Chen, C-TJ, et al.
Publicat: (2018)

BLACK HOLE MASS AND EDDINGTON RATIO DISTRIBUTION FUNCTIONS OF X-RAY-SELECTED BROAD-LINE AGNs AT z similar to 1.4 IN THE SUBARU XMM-NEWTON DEEP FIELD
per: Nobuta, K, et al.
Publicat: (2012)

Deep XMM–Newton observations of the most distant SPT-SZ galaxy cluster
per: Mantz, Adam B, et al.
Publicat: (2022)

Deep XMM–Newton observations of the most distant SPT-SZ galaxy cluster
per: Mantz, Adam B, et al.
Publicat: (2021)

TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
per: Yang, Jun, et al.
Publicat: (2020)

TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
per: Jun Yang, et al.
Publicat: (2019-10-01)

XMM-Newton observations of 1A 0535+262 in quiescence.
per: Doroshenko V., et al.
Publicat: (2014-01-01)

Understanding the nature of the faint radio-source population
per: Vardoulaki, E
Publicat: (2009)

The evolution of radio sources in the UKIDSS-DXS-XMM-LSS field
per: McAlpine, K, et al.
Publicat: (2011)

GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection
per: Rovilos, E, et al.
Publicat: (2012)

Observational constraints on the spin of the most massive black holes from radio observations
per: Martinez-Sansigre, A, et al.
Publicat: (2011)

NUSTAR and XMM-Newton Spectroscopy of Ark 564
per: Zhang, Rachel C.
Publicat: (2022)

Search and Characterization of Remnant Radio Galaxies in the XMM-LSS Deep Field
per: Sushant Dutta, et al.
Publicat: (2023-01-01)

DEEP OBSERVATIONS OF INFRARED-FAINT RADIO SOURCES: HIGH-REDSHIFT RADIO-LOUD ACTIVE GALACTIC NUCLEI?
per: Norris, R, et al.
Publicat: (2011)

An XMM-Newton view of the X-ray flat radio-quiet quasar PG 1416-129
per: Porquet, D, et al.
Publicat: (2006)

IXPE and XMM-Newton Observations of the Soft Gamma Repeater SGR 1806–20
per: Roberto Turolla, et al.
Publicat: (2023-01-01)

THE GAS DYNAMICS OF NGC 4472 REVEALED BY XMM-NEWTON
per: Kraft, Ralph P., et al.
Publicat: (2015)

LOFAR observations of the XMM-LSS field
per: Hale, C, et al.
Publicat: (2019)

Characterizing Superflares in HR 1099 Using Temporal and Spectral Analysis of XMM-Newton Observations
per: Shweta Didel, et al.
Publicat: (2024-01-01)

The Hot Circumgalactic Medium of the Milky Way: New Insights from XMM-Newton Observations
per: Joy Bhattacharyya, et al.
Publicat: (2023-01-01)

The Phoenix Deep Survey: X-ray properties of faint radio sources
per: Georgakakis, A, et al.
Publicat: (2003)

XMM-Newton Perspective of the Unique Magnetic Binary-ϵ Lupi
per: Ayan Biswas, et al.
Publicat: (2024-01-01)

The faint radio source population at 15.7 GHz – IV. The dominance of core emission in faint radio galaxies
per: IH Whittam, et al.
Publicat: (2020)

The radio spectral energy distribution of infrared-faint radio sources
per: Herzog, A, et al.
Publicat: (2016)

PROBING THE ACCRETION DISK AND CENTRAL ENGINE STRUCTURE OF NGC 4258 WITH SUZAKU AND XMM-NEWTON OBSERVATIONS
per: Reynolds, Christopher S., et al.
Publicat: (2015)

XMM-Newton observations of two hyperluminous IRAS galaxies: Compton-thick quasars with obscuring starbursts
per: Wilman, R, et al.
Publicat: (2003)

Analysis and characterization of X-ray flare of Mkn 421 using XMM-Newton observation 0658801301
per: Rajendra Neupane, et al.
Publicat: (2023-04-01)

ASCA and XMM-Newton observations of the galactic supernova remnant G311.5−0.3
per: Pannuti T.G., et al.
Publicat: (2017-01-01)

Analysis and characterization of X-ray flare of Mkn 421 using XMM-Newton observation 0658801301
per: Rajendra Neupane, et al.
Publicat: (2023-04-01)

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
per: Pierre, M, et al.
Publicat: (2016)

Tidal disruption events from the first XMM-Newton slew survey
per: Komossa S., et al.
Publicat: (2012-12-01)