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[PDF] Top 20 Optical Spectroscopic Atlas of the MOJAVE/2cm AGN Sample

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Optical Spectroscopic Atlas of the MOJAVE/2cm AGN Sample

Optical Spectroscopic Atlas of the MOJAVE/2cm AGN Sample

... The MOJAVE/2cm sample of 250 AGN is pre- sented in Table 5, together with the homogeneous photometric information at the ...lists the source name, Columns ... See full document

32

BAT AGN spectroscopic survey II  X ray emission and high ionization optical emission lines

BAT AGN spectroscopic survey II X ray emission and high ionization optical emission lines

... parent sample, we first remove the spectra coming from the 6dF survey because they lack flux ...in the Roma blazar catalog (BZCAT) v5.0 (Massaro et al. 2009) since the X-ray emission in ... See full document

13

Radio-optical scrutiny of compact AGN: Correlations between properties of pc-scale jets and optical nuclear emission

Radio-optical scrutiny of compact AGN: Correlations between properties of pc-scale jets and optical nuclear emission

... from the variability timescales of radio flares at different frequen- cies; see Hovatta et ...2009) of about 50% of the MOJAVE blazars were estimated with the total flux ... See full document

17

BAT AGN Spectroscopic Survey (BASS) – VI  The ΓX–L/LEdd relation

BAT AGN Spectroscopic Survey (BASS) – VI The ΓX–L/LEdd relation

... X-ray-selected AGN. Our sample is based on the first data release of the BAT AGN Spectroscopic Survey ...collection of X-ray and optical data for about 642 ... See full document

15

BAT AGN Spectroscopic Survey  I  Spectral Measurements, Derived Quantities, and AGN Demographics

BAT AGN Spectroscopic Survey I Spectral Measurements, Derived Quantities, and AGN Demographics

... compilations of AGNs, as long as they were fl ux- and wavelength-calibrated and the spectral resolution was well ...determined. The spectral resolutions were measured based on the FWHM ... See full document

31

Quasi stellar objects in the ALHAMBRA survey I  Photometric redshift accuracy based on 23 optical NIR filter photometry

Quasi stellar objects in the ALHAMBRA survey I Photometric redshift accuracy based on 23 optical NIR filter photometry

... in the lit- erature in other cosmological fields. Table 5 summarizes the main characteristics of the photo-z accuracy for several relevant cosmological surveys, including the wavelength ... See full document

17

BAT AGN Spectroscopic Survey  VIII  Type 1 AGN with Massive Absorbing Columns

BAT AGN Spectroscopic Survey VIII Type 1 AGN with Massive Absorbing Columns

... parent sample consists of all AGNs in the BAT AGN Spectroscopic Survey 10 ( BASS; Koss et .... The BASS team has analyzed both new and archival optical spectra for a large ... See full document

11

Unveiling the nature of INTEGRAL objects through optical spectroscopy  VI  A multi observatory identification campaign

Unveiling the nature of INTEGRAL objects through optical spectroscopy VI A multi observatory identification campaign

... in the northern and southern hemispheres, plus archival data from two on-line sky surveys, we performed a systematic optical spectroscopic study of 39 putative counterparts of ... See full document

20

Radio–Optical–Gamma-Ray properties of MOJAVE AGN detected by Fermi/LAT ⋆

Radio–Optical–Gamma-Ray properties of MOJAVE AGN detected by Fermi/LAT ⋆

... complete sample of 135 core- dominated AGN compiled from the MOJAVE sample and the VLBA 15 GHz monitoring survey (Kellermann et ...2009a). The com- plete ... See full document

13

The Swift/BAT AGN Spectroscopic Survey  IX  The Clustering Environments of an Unbiased Sample of Local agns

The Swift/BAT AGN Spectroscopic Survey IX The Clustering Environments of an Unbiased Sample of Local agns

... or optical classi fi cation ) have the same clustering statistics, in accordance with the uni fi ed model, or if they tend to reside in different environments due to different accretion modes or due to ... See full document

12

The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light

The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light

... advent of the Spitzer space telescope led to the dis- covery of new dust-shrouded galaxy populations with starbursts and/or active nuclei ...2008). The mid-IR where the dust ... See full document

16

Dynamical analysis of strong lensing galaxy groups at intermediate redshift

Dynamical analysis of strong lensing galaxy groups at intermediate redshift

... for the analysis using the brighter sample of members, with the difference that, regardless of the fraction of members used in the analysis, the ... See full document

18

Unveiling the nature of INTEGRAL objects through optical spectroscopy X  A new multi year, multi observatory campaign

Unveiling the nature of INTEGRAL objects through optical spectroscopy X A new multi year, multi observatory campaign

... at the Loiano telescope, and Roberto Gualandi for night assistance; Giorgio Martorana and Mauro Rebeschini for Service Mode observations at the Asiago telescope and Luciano Traverso for coordinating them; ... See full document

21

Unveiling the nature of INTEGRAL objects through optical spectroscopy  VII  Identification of 20 Galactic and extragalactic hard X ray sources

Unveiling the nature of INTEGRAL objects through optical spectroscopy VII Identification of 20 Galactic and extragalactic hard X ray sources

... to the impossibility of a simultaneous de- tection of H α and H β emission lines in the Seyfert 2 galaxies and the XBONGs of our sample, we are not able to provide an ... See full document

15

The properties of optical FeII emission lines of AGN with double-peaked broad emission lines

The properties of optical FeII emission lines of AGN with double-peaked broad emission lines

... at optical bands that have exactly the same line profile as that of the broaddouble-peaked Hβ line (Zhang, Dultzin-Hacyan, & Wang 2006a, hereafter Paper ...whole sample of ... See full document

21

Stellar populations analysis along the Hubble sequence

Stellar populations analysis along the Hubble sequence

... samples of nearby galax- ies. The ETGs sample is composed of galaxies belonging to the bright end of the color-magnitude relation of the Virgo cluster ... See full document

104

BAT AGN Spectroscopic Survey   XII  The relation between coronal properties of active galactic nuclei and the Eddington ratio

BAT AGN Spectroscopic Survey XII The relation between coronal properties of active galactic nuclei and the Eddington ratio

... for the corona (Bisnovatyi-Kogan, Zel’dovich & Syunyaev 1971; Svensson 1984; Zdziarski 1985; Fabian et ...2017). The region where there is runaway pair production is delimited by the pair line, ... See full document

12

The Neutral Counterpart of an Uncatalogued Nebula and a Probable Interstellar Bubble around WR 53 in the Centaurus Region

The Neutral Counterpart of an Uncatalogued Nebula and a Probable Interstellar Bubble around WR 53 in the Centaurus Region

... on the paper and ...acknowledge the anony- mous referee for valuable ...by the Consejo Nacional de Investigaciones Cient´ıficas y T´ecnicas (CONICET) of Argentina under project PIP 5886/05, ... See full document

13

The Obscured Fraction of Active Galactic Nuclei in the XMM COSMOS Survey: A Spectral Energy Distribution Perspective

The Obscured Fraction of Active Galactic Nuclei in the XMM COSMOS Survey: A Spectral Energy Distribution Perspective

... goal of the present study is to measure the covering factor of the AGN obscuring medium ...(i.e., the obscured fraction) and its dependence on luminosity and ...a ... See full document

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Unveiling the nature of INTEGRAL objects through optical spectroscopy VIII  Identification of 44 newly detected hard X ray sources

Unveiling the nature of INTEGRAL objects through optical spectroscopy VIII Identification of 44 newly detected hard X ray sources

... by the INTEGRAL satellite have discovered a conspicuous fraction (up to 30%) of unidentified objects among the detected ...program of identification of these objects by (i) selecting ... See full document

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