1,288 research outputs found
SDSS AGNs with X-ray Emission from ROSAT PSPC Pointed Observations
We present a sample of 1744 type 1 active galactic nuclei (AGNs) from the
Sloan Digital Sky Survey (SDSS DR4) spectroscopic catalog with X-ray
counterparts in the White-Giommi-Angelini Catalog (WGACAT) of ROSAT PSPC
pointed observations. Of 1744 X-ray sources, 1410 (80.9%) are new AGN
identifications. Of 4574 SDSS DR4 AGNs for which we found radio matches in the
catalog of radio sources from the FIRST catalog, 224 turned up in our sample of
SDSS X-ray AGNs. The sample objects are given in a catalog that contains
optical and X-ray parameters along with radio emission parameters where
available. We illustrate the content of our catalog and its potential for AGN
science by providing statistical relationships for the catalog data. The
potential of the morphological information is emphasized by confronting the
statistics of optically resolved and unresolved AGNs. The immediate properties
of the catalog objects include significant correlation of X-ray and optical
fluxes, which is consistent with expectations. Also expected is the decrease of
X-ray flux toward higher redshifts. The X-ray to optical flux ratio for the
unresolved AGNs exhibits a decline toward higher redshifts, in agreement with
previous results. The resolved AGNs, however, display the opposite trend. At a
given optical brightness, X-ray fluxes of radio-quiet AGNs by a factor of 2. We
caution, however, that because of the variety of selection effects present in
both the WGACAT and the SDSS, the interpretation of any relationships based on
our sample of X-ray AGNs requires a careful analysis of these effects.Comment: 34 pages, 18 figure
The RASS-SDSS galaxy cluster survey
Solid observational evidences indicate a strong dependence of the galaxy
formation and evolution on the environment. In order to study in particular the
interaction between the intracluster medium and the evolution of cluster
galaxies, we have created a large database of clusters of galaxies based on the
largest available X-ray and optical surveys: the ROSAT All Sky Survey (RASS),
and the Sloan Digital Sky Survey (SDSS). We analyzed the correlation between
the total optical and the X-ray cluster luminosity. The resulting correlation
of L_X and L_{op} shows a logarithmic slope of 0.6, a value close to the
self-similar correlation. We analysed also the cluster mass to light ratio, by
finding a significant dependence of M/L on the cluster mass with a logarithmic
slope ranging from 0.27 in the i and r bands to 0.22 in the z band.Comment: proceedings of 'Multiwavelength mapping of galaxy evolution'
conference held in Venice (Italy), October 2003, A. Renzini and R. Bender
(Eds.), 2 pages, 1 figur
FUSE Observations of Galactic and Intrinsic Absorption in the Spectrum of the Seyfert 1 Galaxy 2MASX J21362313-6224008
We present the far-ultraviolet spectrum of the Seyfert 1 galaxy 2MASX
J21362313-6224008 obtained with the Far Ultraviolet Spectroscopic Explorer
(FUSE). The spectrum features absorption from Galactic OVI at two velocities
and redshifted HI Lyman beta and gamma, CII, CIII, and O VI. The redshifted
absorption features represent a single kinematic component blueshifted by ~310
km/s relative to the AGN. We use photoionization models to derive constraints
on the physical parameters of the absorbing gas. An alternative interpretation
for the absorption lines is also proposed, whereby the absorbing gas is
associated with an intervening galaxy cluster.Comment: Astrophysical Journal, in pres
ROSAT All-Sky Survey observations of IRAS galaxies; I. Soft X-ray and far-infrared properties
The 120,000 X-ray sources detected in the RASS II processing of the ROSAT
All-Sky Survey are correlated with the 14,315 IRAS galaxies selected from the
IRAS Point Source Catalogue: 372 IRAS galaxies show X-ray emission within a
distance of 100 arcsec from the infrared position. By inspecting the structure
of the X-ray emission in overlays on optical images we quantify the likelihood
that the X-rays originate from the IRAS galaxy. For 197 objects the soft X-ray
emission is very likely associated with the IRAS galaxy. Their soft X-ray
properties are determined and compared with their far-infrared emission. X-ray
contour plots overlaid on Palomar Digitized Sky Survey images are given for
each of the 372 potential identifications. All images and tables displayed here
are also available in electronic form.Comment: accepted for publication in A&AS, complete version including all
figures and tables available at
http://www.rosat.mpe-garching.mpg.de/~bol/iras_rassI
Search for GRB afterglows in the ROSAT all-sky survey
We report on the status of our search for X-ray afterglows of gamma-ray
bursts (GRBs) using the ROSAT all-sky survey data. The number of potential
X-ray afterglow candidates with respect to the expected number of beamed GRBs
allows to constrain the relative beaming angles of GRB emission and afterglow
emission at about 1-5 hrs after the GRB.Comment: 3 pages A&A style, 1 color ps-figure; To appear in A&A Suppl. Series,
Proc. of Rome 1998 GRB workshop, also available from
http://www.aip.de/~jcg/publis.htm
Stars in the USNO-B1 Catalog with Proper Motions Between 1.0 and 5.0 arcseconds per year
This paper examines a subset of objects from the USNO-B1 catalogue with
listed proper motions between 1.0 and 5.0 arcseconds per year. We look at the
degree of contamination within this range of proper motions, and point out the
major sources of spurious high proper motion objects. Roughly 0.1% of the
objects in the USNO-B1 catalogue with listed motions between 1.0 and 5.0
arcseconds per year are real. Comparison with the revised version of Luyten's
Half Second catalogue indicates that USNO-B1 is only about 47% complete for
stars in this range. Preliminary studies indicate that there may be a dip in
completeness in USNO-B1 for objects with motions near 0.1 arcseconds per year.
We also present two new stars with motions between 1.0 and 5.0 arcseconds per
year, 36 new stars with confirmed motions between 0.1 and 1.0 arcseconds per
year, several new common proper motion pairs, and the recovery of LHS237a
(VBs3).Comment: 42 pages, 16 figures, uses AASTeX v5.2, accepted by A
On the Evidence for Axion-like Particles from Active Galactic Nuclei
Burrage, Davis, and Shaw recently suggested exploiting the correlations
between high and low energy luminosities of astrophysical objects to probe
possible mixing between photons and axion-like particles (ALP) in magnetic
field regions. They also presented evidence for the existence of ALP's by
analyzing the optical/UV and X-ray monochromatic luminosities of AGNs. We
extend their work by using the monochromatic luminosities of 320 unobscured
Active Galactic Nuclei from the Sloan Digital Sky Survey/Xmm-Newton Quasar
Survey (Young et al., 2009), which allows the exploration of 18 different
combinations of optical/UV and X-ray monochromatic luminosities. However, we do
not find compelling evidence for the existence of ALPs. Moreover, it appears
that the signal reported by Burrage et al. is more likely due to X-ray
absorption rather than to photon-ALP oscillation.Comment: 16 pages, 12 figures. Updated to reflect the minor changes introduced
in the published versio
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