[PDF] Top 20 SDSS IV MANGA - PROPERTIES OF AGN HOST GALAXIES
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SDSS IV MANGA - PROPERTIES OF AGN HOST GALAXIES
... rich galaxies that leads to instabilities in the ...mation of a pressure-supported ...an AGN that expels and heats the remaining gas, thus quenching the SF from the inside-out (Lipari et ...that ... See full document
44
SDSS IV MaNGA: Dependence of Global and Spatially Resolved SFR M ∗ Relations on Galaxy Properties
... Thus what processes fundamentally drive the two strong sequences in the traditional H α( global )– M * ( global ) relation in Figure 1? From left to right, the four panels in Figure 5, respectively, present the H α ... See full document
8
THE ENVIRONMENTAL DEPENDENCE OF THE AGE OF ACTIVE GALAXIES AND THE DEPENDENCE OF THE CLUSTERING PROPERTIES OF ACTIVE GALAXIES ON AGE
... study of active galactic nuclei (AGNs) (Dressler et ...presence of AGNs and the local environment of AGN host ...tudes of both X-ray-selected and optically selected SDSS ... See full document
9
Type II supernovae in low luminosity host galaxies
... low-luminosity host sample of 30 objects are drawn from several ...faint host galaxies, and from the Las Cumbres Observatory (LCO; Brown et ...SN host galaxy information: recession ... See full document
22
Low surface brightness galaxies in the SDSS: the link between environment, star forming properties, and active galactic nuclei
... many of the properties also found in high surface brightness galaxies (HSBGs), they also present a signif- icant list of challenging observational ...(some of them will be explained ... See full document
13
Quasi stellar objects in the ALHAMBRA survey I Photometric redshift accuracy based on 23 optical NIR filter photometry
... solutions of BLAGN and QSOs, at least in the red- shift interval 0 < z < 4, if the optical regime is cov- ered by a continuous medium-band filter set such as that of ...design of fu- ture ... See full document
17
X ray spectral constraints for z approximate to 2 massive galaxies: the identification of reflection dominated active galactic nuclei
... all of the spectra are combined and binned to increase the signal-to-noise ...spectrum of the heavily obscured AGNs is shown in ...spectrum of the heavily obscured AGNs is reflec- tion ...that ... See full document
16
BAT AGN Spectroscopic Survey V X Ray Properties of the Swift/BAT 70 month AGN Catalog
... coordinates of the associated counterparts in the original BAT catalog do not accurately point to the nuclei of the systems, which in all cases are identi fi ed with a relatively bright WISE and 2MASS ...an ... See full document
38
Herschel ATLAS: The cosmic star formation history of quasar host galaxies?
... density of quasars (QSOs) at most redshifts ...drivers of black hole growth and stellar mass ...diagram of far-infrared-selected hy- perluminous starbursts also bears a striking similarity to the K − ... See full document
5
Environmental Effects on the physical properties of galaxies: Clues to the formation of S0 galaxies
... for galaxies: the KR , LSR , FJR , and the FP ...use of one-dimensional fittings for surface brightness analysis (Jedrzejewski ...regions of high density of galaxies. The CMR of ... See full document
229
Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured
... mergers of galaxies are able to effectively fuel ...which host the most luminous obscured AGN known ...excess of submillimetre galaxies as neighbours (Jones et ...mergers ... See full document
27
Study of intrinsic properties of HII galaxies at high redshift
... identification of a class of isolated dwarf emission-line galaxies, which showed them to be indistinguishable in their observed properties from giant HII regions in nearby galaxies, was ... See full document
105
Massive stars in the SDSS IV/APOGEE SURVEY I OB stars
... Department of Energy Of fi ce of Science, and the Participating ...Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the ... See full document
11
Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours?
... sample of 1686 sources with flux densities above 35 mJy at 350 μm and above 3σ at 250 and 500 μm, we find the average redshift to be ...redshift of 2.4 ± 0.4 for the radio- identified sub-mm galaxies ... See full document
5
Actividad nuclear en galaxias inducida por interacción gravitacional
... absence of type 1 AGN in these sam- ples of isolated galaxies is ...1.0 AGN among the 175 active galaxies in our sam- ...fraction of types ...fractions of type 1 ... See full document
101
GOODS Herschel: radio excess signature of hidden AGN activity in distant star forming galaxies
... luminous AGN heavily obscured at MIR wavelengths, and hosted in dusty star-forming galaxies, whose IR emission is thus overwhelmed by star formation and eludes our detec- tion capability ...amount of ... See full document
28
Radio–Optical–Gamma-Ray properties of MOJAVE AGN detected by Fermi/LAT ⋆
... cores of parsec-scale ...correlation of the 1FGL with the 20 GHz Australia Telescope Compact Array radio survey catalogue (Mahoni et ...delays of 1.2 months. This result sug- gests that the origin ... See full document
13
The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light
... the AGN bolometric frac- tions of a sample of submm-selected galaxies in the Lockman Hole East, taken from the SCUBA Half Degree Extragalactic Survey (SHADES), using mid-infrared photometry ... See full document
16
Tracing the Mass Dependent Star Formation History of Late Type Galaxies Using X Ray Emission: Results from the Chandra Deep Fields
... luminosity of normal star-forming galaxies with cosmic look-back time in response to the increasing global star formation rate density ...rate of a galaxy and LMXBs trace its star formation history ... See full document
20
Future virialized structures: an analysis of superstructures in the SDSS DR7
... clustering properties of dark matter haloes depend exclusively on their total mass, recent analy- ses of numerical simulations have shown that they can be strongly affected by their assembly history ... See full document
13
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