172 research outputs found
Infrared Imaging of the Gravitational Lens PG 1115+080 with the Subaru Telescope
We present high spatial resolution images of the gravitational-lens system PG
1115+080 taken with the near-infrared camera (CISCO) on the Subaru telescope.
The FWHM of the combined image is in the -band, yielding spatial
resolution of after a deconvolution procedure. This is a first
detection of an extended emission adjacent to the A1/A2 components, indicating
the presence of a fairly bright emission region with a characteristic angular
radius of 5 mas (40 pc). The near-infrared image of the Einstein ring
was extracted in both the and bands. The color is found to be
significantly redder than that of a synthetic model galaxy with an age of 3
Gyr, the age of the universe at the quasar redshift.Comment: 11 pages, 6 figures. Accepted for publication in PASJ(2000
A contribution to the selection of emission-line galaxies using narrow-band filters in the optical airglow windows
Emission line galaxies are an invaluable tool for our understanding of the
evolution of galaxies in the Universe. Imaging of deep fields with narrow-band
filters allows not only the selection of these objects, but also to infer the
line flux and the equivalent width of the emission line with some assumptions.
The narrow-band filter technique provides homogeneous samples of galaxies in
small comoving volumes in the sky. We present an analysis of the selection of
emission-line galaxies using narrow-band filters. Different methods of
observation are considered: broad-band -- narrow-band filters and two
broad-band and one narrow-band filters.
We study also the effect of several lines entering simultaneously inside the
filters (this is the case of Halpha). In each case the equations to obtain the
equivalent width and line flux from the photometry are obtained. Candidates to
emission-line objects are selected by their color excess in a magnitude-color
diagram. For different narrow-band filters, we compute the mean colors of stars
and galaxies, showing that, apart from galaxies, some types of stars could be
selected with certain filter sets. We show how to compute the standard
deviation of the colors of the objects even in the usual case when there are
not enough objects to determine the standard deviation from the data. We
present also helpful equations to compute the narrow-band and the broad-band
exposure times in order to obtain minimum dispersion in the ratio of fluxes of
both bands with minimum total exposure time.Comment: Accepted for publication in PASP 48 pages, 10 figures Corrected
typos, fixed references. Updated reference to T
Implications from the optical to UV flux ratio of FeII emission in quasars
We investigate FeII emission in Broad Line Region (BLR) of AGNs by analyzing
the FeII(UV), FeII(4570) and MgII emission lines in 884 quasars in the Sloan
Digital Sky Survey (SDSS) Quasar catalog in a redshift range of 0.727 < z <
0.804. FeII(4570)/FeII(UV) is used to infer the column density of FeII-emitting
clouds and explore the excitation mechanism of FeII emission lines. As
suggested before in various works, the classical photoionization models fail to
account for FeII(4570)/FeII(UV) by a factor of 10, which may suggest anisotropy
of UV FeII emission; otherwise, an alternative heating mechanism like shock is
working. The column density distribution derived from FeII(4570)/FeII(UV)
indicates that radiation pressure plays an important role in BLR gas dynamics.
We find a positive correlation between FeII(4570)/FeII(UV) and the Eddington
ratio. We also find that almost all FeII-emitting clouds are to be under
super-Eddington conditions unless ionizing photon fraction is much smaller than
that previously suggested. Finally we propose a physical interpretation of a
striking set of correlations between various emission-line properties, known as
``Eigenvector 1''.Comment: 10 pages, 10 figures, accepted for publication in MNRA
Detecting high redshift evolved galaxies as the hosts of optically faint hard X-ray sources
We combine deep Subaru near-infrared images of the massive lensing clusters
A2390 and A370 with Keck optical data to map the spectral energy distributions
(SEDs) of Chandra X-ray sources lying behind the clusters. The three sources
behind A2390 are found to have extremely red colors with SEDs consistent with
evolved galaxies at redshifts z>1.4. One source has extremely anomalous colors,
which we interpret as evidence for a type Sa SED at a redshift around 2.5. The
photometric redshift of another source has been confirmed at z=1.467 from
near-infrared spectroscopy using the CISCO spectrograph on Subaru. Mapping of
optically faint hard X-ray sources may prove to be an extremely efficient way
to locate luminous evolved galaxies at high redshifts.Comment: 5 pages, ApJ Letters, in pres
Measurement of [OIII] Emission in Lyman Break Galaxies
Measurements of [OIII] emission in Lyman Break galaxies (LBGs) at z>3 are
presented. Four galaxies were observed with narrow-band filters using the
Near-IR Camera on the Keck I 10-m telescope. A fifth galaxy was observed
spectroscopically during the commissioning of NIRSPEC, the new infrared
spectrometer on Keck II. The emission-line spectrum is used to place limits on
the metallicity. Comparing these new measurements with others available from
the literature, we find that strong oxygen emission in LBGs may suggest
sub-solar metallicity for these objects. The [OIII]5007 line is also used to
estimate the star formation rate (SFR) of the LBGs. The inferred SFRs are
higher than those estimated from the UV continuum, and may be evidence for dust
extinction.Comment: 25 pages, including 6 figures. Accepted for publication in Ap
The Subaru Deep Field Project: Lyman Emitters at Redshift of 6.6
We present new results of a deep optical imaging survey using a narrowband
filter () centered at 9196 \AA ~ together with , ,
, , and broadband filters in the sky area of the Subaru
Deep Field which has been promoted as one of legacy programs of the 8.2m Subaru
Telescope. We obtained a photometric sample of 58 Ly emitter candidates
at 6.5 -- 6.6 among strong -excess () objects together with a color criterion of . We then obtained optical spectra of 20 objects in our -excess
sample and identified at least nine Ly emitters at -- 6.6
including the two emitters reported by Kodaira et al. (2003). Since our
Ly emitter candidates are free from strong amplification of
gravitational lensing, we are able to discuss their observational properties
from a statistical point of view. Based on these new results, we obtain a lower
limit of the star formation rate density of yr Mpc at , being
consistent with our previous estimate. We discuss the nature of star-formation
activity in galaxies beyond .Comment: 49 pages, 16 figures, PASJ, Vol. 57, No. 1, in pres
ERO R1 in CL0939+4713 field - Evidence for an S0-like galaxy at z \sim 1.5
We present further observations of the extremely red object ERO
J094258+4659.2, identified by \citet{iye00} as ERO R1 in their deep images of
the cluster A851. We estimate its redshift independently by eight-band
photometric redshift determination and cross-correlation of a new H-band
spectrum with the optical spectra of local E/S0 galaxies, and conclude that it
lies at . Although its colors are consistent both with an
elliptical galaxy and an S0 galaxy at that redshift, its elongated shape and
exponential luminosity profile suggest the presence of an evolved stellar disk
component. We rule out the possibility that these properties are strongly
influenced by gravitational lensing by the foreground cluster, and therefore
conclude that this object is more likely to be an S0-like galaxy, rather than a
lensed elliptical. The H-band spectrum does not show strong H emission
and the star formation rate therefore appears to be very modest. The presence
of such a galaxy with an apparently relaxed disk of stars at this high redshift
provides a new and strong constraint on theoretical models which aim to explain
the formation and evolution of galaxies.Comment: 23 pages, 9 figures, Submitted to the Astrophysical Journa
- …