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[PDF] Top 20 BROADBAND OBSERVATIONS OF THE COMPTON THICK NUCLEUS OF NGC 3393

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BROADBAND OBSERVATIONS OF THE COMPTON THICK NUCLEUS OF NGC 3393

BROADBAND OBSERVATIONS OF THE COMPTON THICK NUCLEUS OF NGC 3393

... by the ASDC. Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and ...NASA. The Cornell Atlas of ... See full document

18

The Space Density of Compton Thick Active Galactic Nucleus and the X Ray Background

The Space Density of Compton Thick Active Galactic Nucleus and the X Ray Background

... constrain the number density and evolution of Compton-thick (CT) active galactic nuclei ...In the local universe, we use the wide-area surveys from the Swift and INTEGRAL ... See full document

11

The NuSTAR Extragalactic Surveys: Source Catalog and the Compton thick Fraction in the UDS Field

The NuSTAR Extragalactic Surveys: Source Catalog and the Compton thick Fraction in the UDS Field

... presented the NuSTAR survey of the UDS fi eld, consisting of 35 observations performed in two separate passes on the fi ...eld. The total observing time is ...area of ... See full document

19

A new population of compton thick AGNs identified using the spectral curvature above 10 keV

A new population of compton thick AGNs identified using the spectral curvature above 10 keV

... spectra of the nine NuSTAR-observed Swift / BAT AGNs selected based on ...SC. The best- fi t MYT ORUS -based model ( Model M ; described in Section ...match the unfolded ...represent the ... See full document

18

WEAK HARD X RAY EMISSION FROM TWO BROAD ABSORPTION LINE QUASARS OBSERVED WITH NuSTAR: COMPTON THICK ABSORPTION OR INTRINSIC X RAY WEAKNESS?

WEAK HARD X RAY EMISSION FROM TWO BROAD ABSORPTION LINE QUASARS OBSERVED WITH NuSTAR: COMPTON THICK ABSORPTION OR INTRINSIC X RAY WEAKNESS?

... nature of intrinsic X-ray weakness remains ...destroy the X-ray emitting accretion-disk corona (see, e.g., the discussions in Leighly et ...part of the accretion-disk outflow ...for ... See full document

17

A spectroscopic study of the globular Cluster NGC 4147

A spectroscopic study of the globular Cluster NGC 4147

... First of all, we considered only stars with temperature hotter than 4400 ...around the mean value with no sign of any trend. However, the two coldest targets show an Na content much lower than ... See full document

9

An Iwasawa Taniguchi effect for Compton thick active galactic nuclei

An Iwasawa Taniguchi effect for Compton thick active galactic nuclei

... in the large dust and gas reservoirs that are rapidly being accreted, which absorb optical to X-ray emission and reprocess this at infrared ...on the spatial separation of the merging ... See full document

16

Multiwavelength Study of Massive Galaxies at z ~ 2  II  Widespread Compton thick Active Galactic Nuclei and the Concurrent Growth of Black Holes and Bulges

Multiwavelength Study of Massive Galaxies at z ~ 2 II Widespread Compton thick Active Galactic Nuclei and the Concurrent Growth of Black Holes and Bulges

... aim of Paper I is to investigate the nature of star for- mation at high redshift and to identify the best means to estimate the ongoing SFR ...activity. The work thus mostly ... See full document

17

On the Chemical Abundances of Miras in Clusters: V1 in the Metal rich Globular NGC 5927

On the Chemical Abundances of Miras in Clusters: V1 in the Metal rich Globular NGC 5927

... present the fi rst spectroscopic abundance determination of iron, α -elements ( Si, Ca, and Ti ) , and sodium for the Mira variable V1 in the metal-rich globular cluster NGC  ... See full document

7

TítuloA realistic computational model of the local circuitry of the cuneate nucleus

TítuloA realistic computational model of the local circuitry of the cuneate nucleus

... within the circuitry developed so far (Fig. 4)? The results are shown in ...interval, the cuneothalamic neurons stop firing. If the stimulus persists, the neurons enter in an oscillatory ... See full document

9

The abundance of nitrogen in starburst nucleus galaxies

The abundance of nitrogen in starburst nucleus galaxies

... source of excitation. This, in fact, was the solution preferred by Kenni- cutt et ...as the extra ...do the trick. However, the extra excitation hypothesis is in con- tradiction with ... See full document

14

The pragmatic function of theme: the case of the conditional subordinates

The pragmatic function of theme: the case of the conditional subordinates

... So lar, there are two points that I have tried to address: (i) the choice of Theme by the addresser is meaningful and, therefore, together with the textual meaning, it portrays an iate[r] ... See full document

15

Globular Clusters and X Ray Point Sources in Centaurus A (NGC 5128)

Globular Clusters and X Ray Point Sources in Centaurus A (NGC 5128)

... Chandra observations of Centaurus A ( NGC 5128), the nearest giant early-type galaxy, and correlate this point-source population with the largest available ensemble of confirmed ... See full document

13

The influence of the English language on the description of cosmetic products

The influence of the English language on the description of cosmetic products

... use of technology has grown exponentially worldwide and it is contributing to the gradual expansion of English; moreover, this specialized area provides more borrowings from English to other ...from ... See full document

27

The NGC 404 Nucleus: Star Cluster and Possible Intermediate mass Black Hole

The NGC 404 Nucleus: Star Cluster and Possible Intermediate mass Black Hole

... comparison of the SB profiles of all the NIR data, with the NIFS K-band image scaled to fit the SB profile of the NICMOS F160W images at r > 1 ...Within ... See full document

19

The impact of broadband quality standards on internet services market structure in Colombia

The impact of broadband quality standards on internet services market structure in Colombia

... THE IMPACT OF BROADBAND QUALITY STANDARDS ON INTERNET SERVICES MARKET STRUCTURE.. IN COLOMBIA.[r] ... See full document

36

Wittman y Gotelli, 2011

Predicting community structure of ground-foraging ant assemblages with Markov models of behavioral dominance

... for the Southeast site included eight different states (=species), representing the eight species that were present, and thus its dimensions are 8 9 ...8. The regional model (=6 species) consisted ... See full document

13

Predictive value of the number of symptoms during pH monitoring for the diagnosis of Gastroesophageal Reflux Disease

Predictive value of the number of symptoms during pH monitoring for the diagnosis of Gastroesophageal Reflux Disease

... ratio of only ...On the other side, we theorized that hypersen- sitivity, hypervigilance and psychiatric disorders would bring a higher number of symptoms during the test in GERD - ...number ... See full document

5

“I am not one of his followers”: The Rewriting of the Cultural Icon of the Virgin in Colm Tóibín’s The Testament of Mary

“I am not one of his followers”: The Rewriting of the Cultural Icon of the Virgin in Colm Tóibín’s The Testament of Mary

... art, the Devil is often associated with darkness and putrefaction, one of the penalties of the ...stench of death, its most terrifying signal, is constantly used in Christian ... See full document

12

Heavily Obscured AGN in Star Forming Galaxies at z sime 2

Heavily Obscured AGN in Star Forming Galaxies at z sime 2

... study the average X-ray properties of a sample of individually undetected sources, thus achieving an effective exposure time of many megaseconds ...both the web-based CSTACK code 16 ... See full document

18

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