819 research outputs found
A New X-ray Selected Sample of Very Extended Galaxy Groups from the ROSAT All-Sky Survey
Some indications for tension have long been identified between cosmological
constraints obtained from galaxy clusters and primary CMB measurements.
Typically, assuming the matter density and fluctuations, as parameterized with
Omega_m and sigma_8, estimated from CMB measurements, many more clusters are
expected than those actually observed. One possible explanation could be that
certain types of galaxy groups or clusters were missed in samples constructed
in previous surveys, resulting in a higher incompleteness than estimated. We
aim to determine if a hypothetical class of very extended, low surface
brightness, galaxy groups or clusters have been missed in previous X-ray
cluster surveys based on the ROSAT All-Sky Survey (RASS). We applied a
dedicated source detection algorithm sensitive also to more unusual group or
cluster surface brightness distributions. We found many known but also a number
of new group candidates, which are not included in any previous X-ray / SZ
cluster catalogs. In this paper, we present a pilot sample of 13 very extended
groups discovered in the RASS at positions where no X-ray source has been
detected previously and with clear optical counterparts. The X-ray fluxes of at
least 5 of these are above the nominal flux-limits of previous RASS cluster
catalogs. They have low mass (; i.e., galaxy
groups), are at low redshift (z<0.08), and exhibit flatter surface brightness
distributions than usual. We demonstrate that galaxy groups were missed in
previous RASS surveys, possibly due to the flat surface brightness
distributions of this potential new population. Analysis of the full sample
will show if this might have a significant effect on previous cosmological
parameter constraints based on RASS cluster surveys. (This is a shortened
version of the abstract - full text in the article)Comment: 18 pages, 7 figures, accepted by A&
Discovery of a Galaxy Cluster via Weak Lensing
We report the discovery of a cluster of galaxies via its weak gravitational
lensing effect on background galaxies, the first spectroscopically confirmed
cluster to be discovered through its gravitational effects rather than by its
electromagnetic radiation. This fundamentally different selection mechanism
promises to yield mass-selected, rather than baryon or photon-selected, samples
of these important cosmological probes. We have confirmed this cluster with
spectroscopic redshifts of fifteen members at z=0.276, with a velocity
dispersion of 615 km/s. We use the tangential shear as a function of source
photometric redshift to estimate the lens redshift independently and find z_l =
0.30 +- 0.08. The good agreement with the spectroscopy indicates that the
redshift evolution of the mass function may be measurable from the imaging data
alone in shear-selected surveys.Comment: revised version with minor changes, to appear in ApJ
The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
We present a new measurement of the mass-concentration relation and the
stellar-to-halo mass ratio over the halo mass range to
. To achieve this, we use weak lensing measurements
from the CFHT Stripe 82 Survey (CS82), combined with the central galaxies from
the redMaPPer cluster catalogue and the LOWZ/CMASS galaxy sample of the Sloan
Digital Sky Survey-III Baryon Oscillation Spectroscopic Survey Tenth Data
Release. The stacked lensing signals around these samples are modelled as a sum
of contributions from the central galaxy, its dark matter halo, and the
neighboring halos, as well as a term for possible centering errors. We measure
the mass-concentration relation: with
for and for . These amplitudes and slopes are completely
consistent with predictions from recent simulations. We also measure the
stellar-to-halo mass ratio for our samples, and find results consistent with
previous measurements from lensing and other techniques.Comment: 10 pages, 3 figures, 3 table
ESO Imaging Survey VII. Distant Cluster Candidates over 12 square degrees
In this paper the list of candidate clusters identified from the I-band data
of the ESO Imaging Survey (EIS) is completed using the images obtained over a
total area of about 12 square degrees. Together with the data reported earlier
the total I-band coverage of EIS is 17 square degrees, which has yielded a
sample of 252 cluster candidates in the redshift range 0.2 \lsim z \lsim 1.3.
This is the largest optically-selected sample currently available in the
Southern Hemisphere. It is also well distributed in the sky thus providing
targets for a variety of VLT programs nearly year round.Comment: 5 pages, 3 figures, submitted to Astronomy & Astrophysic
Probing the Relation Between X-ray-Derived and Weak-Lensing-Derived Masses for Shear-Selected Galaxy Clusters: I. A781
We compare X-ray and weak-lensing masses for four galaxy clusters that
comprise the top-ranked shear-selected cluster system in the Deep Lens Survey.
The weak-lensing observations of this system, which is associated with A781,
are from the Kitt Peak Mayall 4-m telescope, and the X-ray observations are
from both Chandra and XMM-Newton. For a faithful comparison of masses, we adopt
the same matter density profile for each method, which we choose to be an NFW
profile. Since neither the X-ray nor weak-lensing data are deep enough to well
constrain both the NFW scale radius and central density, we estimate the scale
radius using a fitting function for the concentration derived from cosmological
hydrodynamic simulations and an X-ray estimate of the mass assuming
isothermality. We keep this scale radius in common for both X-ray and
weak-lensing profiles, and fit for the central density, which scales linearly
with mass. We find that for three of these clusters, there is agreement between
X-ray and weak-lensing NFW central densities, and thus masses. For the other
cluster, the X-ray central density is higher than that from weak-lensing by 2
sigma. X-ray images suggest that this cluster may be undergoing a merger with a
smaller cluster. This work serves as an additional step towards understanding
the possible biases in X-ray and weak-lensing cluster mass estimation methods.
Such understanding is vital to efforts to constrain cosmology using X-ray or
weak-lensing cluster surveys to trace the growth of structure over cosmic time.Comment: 14 pages, 7 figures, matches version in Ap
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