output
19932026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2006Show all

236 papers · 1 filter

nucl-th2006★ 50 cited

What Do Electromagnetic Plasmas Tell Us about Quark-Gluon Plasma?

Stanislaw Mrowczynski, Markus H. Thoma

Since the quark-gluon plasma (QGP) reveals some obvious similarities to the well-known electromagnetic plasma (EMP), an accumulated knowledge on EMP can be used in the QGP studies.…

astro-ph2006★ 66 cited

Probing the Disk-jet Connection of the Radio Galaxy 3C120 Observed with Suzaku

Jun Kataoka, James N. Reeves, Kazushi Iwasawa +13

Broad line radio galaxies (BLRGs) are a rare type of radio-loud AGN, in which the broad optical permitted emission lines have been detected in addition to the extended jet emission…

astro-ph2006★ 1 cited

511 keV line from millisecond pulsars in the Galactic center

Wei Wang

Observations of a strong and extended positron-electron annihilation line emission in the Galactic center (GC) region by the SPI/INTEGRAL are challenging to the existing models of…

astro-ph2006

Discovery of an X-ray Nebula associated with PSR J2124-3358

C. Y. Hui, W. Becker

We report the discovery of an X-ray nebula associated with the nearby millisecond pulsar PSR J2124-3358. This is the first time that extended emission from a solitary millisecond p…

astro-ph2006★ 2 cited

A Fast-Moving Central Compact Object in Puppis-A

C. Y. Hui, W. Becker

Utilizing two Chandra High Resolution Camera (HRC-I) observations with an epoch separation of somewhat more than five years, we have measured the proper motion of the central compa…

astro-ph2006★ 94 cited

X-ray monitoring of optical novae in M31 from July 2004 to February 2005

W. Pietsch, F. Haberl, G. Sala +9

Optical novae have recently been identified as the major class of supersoft X-ray sources in M31 based on ROSAT and early XMM-Newton and Chandra observations. This paper reports on…

astro-ph2006★ 24 cited

XMM-Newton Observations of PSR B1957+20

H. H. Huang, W. Becker

We report on XMM-Newton observations of the Black Widow pulsar, PSR B1957+20. The pulsar's X-ray emission is non-thermal and best modeled with a single powerlaw spectrum of photon…

astro-ph2006

Multi-wavelength and black hole mass properties of Low Luminosity Active Nuclei

F. Panessa, L. Bassani, M. Cappi +6

We investigate the relation between the X-ray nuclear emission, optical emission line, radio luminosity and black hole mass for a sample of nearby Seyfert galaxies. Strong linear c…

astro-ph2006★ 23 cited

XMM-Newton observation of Mrk 110

Th. Boller, I. Balestra, W. Kollatschny

We report on the first XMM-Newton observation of the bright Narrow-Line Seyfert 1 galaxy Mrk 110. We find a narrow Fe K fluorescent line, a broad component FWHM ~ 16500 km/s of the…

astro-ph2006★ 5 cited

An XMM-Newton view of the X-ray flat radio-quiet quasar PG 1416-129

D. Porquet, J. N. Reeves, A. Markowitz +3

(abridged) The radio-quiet quasar PG1416-129 (z=0.129) exhibits atypical optical and X-ray properties. Between 1990 and 2000, in response to its optical continuum decrease, the ``c…

astro-ph2006★ 23 cited

IGR J08408--4503: a new recurrent Supergiant Fast X-ray Transient

D. Gotz, M. Falanga, F. Senziani +3

The supergiant fast X-ray transient IGR J08408-4503 was discovered by INTEGRAL on May 15, 2006, during a bright flare. The source shows sporadic recurrent short bright flares, reac…

astro-ph2006

The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines

I. Strateva, W. N. Brandt, M. Eracleous +2

We summarize the optical, UV, and X-ray properties of double-peaked emitters -- AGN with double-peaked Balmer emission lines believed to originate in the AGN accretion disk. We foc…

astro-ph2006★ 52 cited

The XMM-Newton wide-field survey in the COSMOS field: V. Angular Clustering of the X-ray Point Sources

Takamitsu Miyaji, Giovanni Zamorani, Nico Cappelluti +9

We present the first results of the measurements of angular auto-correlation functions (ACFs) of X-ray point sources detected in the XMM-Newton observations of the 2 deg2 COSMOS fi…

astro-ph2006★ 111 cited

The XMM-Newton wide-field survey in the COSMOS field. IV: X-ray spectral properties of Active Galactic Nuclei

V. Mainieri, G. Hasinger, N. Cappelluti +25

We present a detailed spectral analysis of point-like X-ray sources in the XMM-COSMOS field. Our sample of 135 sources only includes those that have more than 100 net counts in the…

astro-ph2006★ 315 cited

The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies

A. Finoguenov, L. Guzzo, G. Hasinger +30

We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the COSMOS field. We reach a depth for a total cluster flux in the 0.5-2 keV band of…

astro-ph2006★ 175 cited

The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources

M. Brusa, G. Zamorani, A. Comastri +31

[ABRIGED] We present the optical identification of a sample of 695 X-ray sources detected in the first 1.3 deg^2 of the XMM-COSMOS survey, down to a 0.5-2 keV (2-10 keV) limiting f…

astro-ph2006★ 16 cited

The XMM-Newton Survey in the Marano Field I. The X-ray data and optical follow-up

M. Krumpe, G. Lamer, A. D. Schwope +6

We report on a medium deep XMM-Newton survey of the Marano Field and optical follow-up observations. The mosaicked XMM-Newton pointings in this optical quasar survey field cover 0.…

astro-ph2006★ 55 cited

Detection of HNC and tentative detection of CN at z=3.9

M. Guelin, P. Salome, R. Neri +8

Molecular line emission from high-redshift galaxies holds great promise for the study of galaxy formation and evolution. The weak signals can only be detected with the largest mm-w…

astro-ph2006★ 151 cited

Photometric Redshifts of Galaxies in COSMOS

B. Mobasher, P. Capak, N. Z. Scoville +26

We measure photometric redshifts and spectral types for galaxies in the COSMOS survey. We use template fitting technique combined with luminosity function priors and with the optio…

astro-ph2006★ 135 cited

Candidate tidal disruption events from the XMM-Newton Slew Survey

P. Esquej, R. D. Saxton, M. J. Freyberg +4

In recent years, giant amplitude X-ray flares have been observed from a handful of non-active galaxies. The most plausible scenario of these unusual phenomena is tidal disruption o…

astro-ph2006★ 353 cited

The XMM-Newton wide-field survey in the COSMOS field: I. Survey description

G. Hasinger, N. Cappelluti, H. Brunner +21

We present the first set of XMM-Newton EPIC observations in the 2 square degree COSMOS field. The strength of the COSMOS project is the unprecedented combination of a large solid a…

astro-ph2006★ 2k cited

The Cosmic Evolution Survey (COSMOS) -- Overview

N. Scoville, H. Aussel, M. Brusa +19

The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated evolution of galaxies, star formation, active galactic nuclei (AGN) and dark matter (DM) with large-scale s…

astro-ph2006★ 367 cited

The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field

Y. Taniguchi, N. Scoville, T. Murayama +27

We present deep optical imaging observations of 2 square degree area, covered by the Cosmic Evolution Survey (COSMOS), made by the prime-focus Camera (Supreme-Cam) on the 8.2m Suba…

astro-ph2006★ 1k cited

zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

S. J. Lilly, O. Le Fevre, A. Renzini +42

zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to…