114 research outputs found
Three Emission-Line Galaxies at z~2.4
We present Keck near-infrared and WIYN optical photometry of a sample of
galaxies detected by near-infrared narrowband imaging in the fields of quasar
metal absorption line systems at z~2.4. Wide separations (0.6-1.6/h Mpc) from
the quasars indicates that they are not directly responsible for the absorption
systems. From the color excess of the galaxies we derived line fluxes, star
formation rates, and equivalent widths. The data are consistent with one source
having an active nucleus and two sources containing regions of star formation.
The blue (R-K) colors for the sources suggest relatively lesser dust content.
We discuss possible projects using current wide-field infrared instruments,
which can cover an order of magnitude greater area with modest allocations of
telescope time.Comment: 9 Pages, 3 figures LaTeX/AASTeX. ApJ accepted (est. March 2003
An Optical/Near-Infrared Study of Radio-Loud Quasar Environments II. Imaging Results
We use optical and near-IR imaging to examine the properties of the
significant excess population of K>=19 galaxies found in the fields of 31 z=1-2
radio-loud quasars by Hall, Green & Cohen (1998). The excess occurs on two
spatial scales: a component at <40'' from the quasars significant compared to
the galaxy surface density at >40'' in the same fields, and a component roughly
uniform to ~100'' significant compared to the galaxy surface density seen in
random-field surveys in the literature. The r-K color distributions of the
excess galaxy populations are indistinguishable and are significantly redder
than the color distribution of the field population.
The excess galaxies are consistent with being predominantly early-type
galaxies at the quasar redshifts, and there is no evidence that they are
associated with intervening MgII absorption systems. The average excess within
0.5 Mpc (~65'') of the quasars corresponds to Abell richness class ~0 compared
to the galaxy surface density at >0.5 Mpc from the quasars, and to Abell
richness class ~1.5 compared to that from the literature.
We discuss the spectral energy distributions (SEDs) of galaxies in fields
with data in several passbands. Most candidate quasar-associated galaxies are
consistent with being 2-3 Gyr old early-types at the quasar redshifts of z~1.5.
However, some objects have SEDs consistent with being 4-5 Gyr old at z~1.5, and
a number of others are consistent with ~2 Gyr old but dust-reddened galaxies at
the quasar redshifts. These potentially different galaxy types suggest there
may be considerable dispersion in the properties of early-type cluster galaxies
at z~1.5. There is also a population of galaxies whose SEDs are best modelled
by background galaxies at z>2.5.Comment: Accepted to ApJ; 54 pages including 30 figures; 2 color GIF files
available separately; also available from
http://www.astro.utoronto.ca/~hall/thesis.htm
Optical dropout galaxies lensed by the cluster A2667
We investigate the nature and the physical properties of z, Y and J-dropout
galaxies selected behind the lensing cluster A2667. This field is part of our
project aimed at identifying z~7-10 candidates accessible to spectroscopic
studies, based on deep photometry with ESO/VLT HAWK-I and FORS2 (zYJH and
Ks-band images, AB(3 sigma)~26-27) on a sample of lensing clusters extracted
from our multi-wavelength combined surveys with SPITZER, HST, and Herschel. In
this paper we focus on the complete Y and J-dropout sample, as well as the
bright z-dropouts fulfilling the selection criteria by Capak et al. (2011). 10
candidates are selected within the common field of ~33 arcmin2 (effective area
once corrected for contamination and lensing dilution). All of them are
detected in H and Ks bands in addition to J and/or IRAC 3.6/4.5, with
H(AB)~23.4 to 25.2, and have modest magnification factors. Although best-fit
photometric redshifts place all these candidates at high-z, the contamination
by low-z interlopers is estimated at 50-75% level based on previous studies,
and the comparison with the blank-field WIRCAM Ultra-Deep Survey (WUDS). The
same result is obtained when photometric redshifts include a luminosity prior,
allowing us to remove half of the original sample as likely z~1.7-3 interlopers
with young stellar pulations and strong extinction. Two additional sources
among the remaining sample could be identified at low-z based on a detection at
24 microns and on the HST z_850 band. These low-z interlopers are not well
described by current templates given the large break, and cannot be easily
identified based solely on optical and near-IR photometry. Given the estimated
dust extinction and high SFRs, some of them could be also detected in the IR or
sub-mm bands. After correction for likely contaminants, the observed counts at
z>7.5 seem to be in agreement with an evolving LF. (abridged)Comment: 18 pages, 11 figures. Accepted for publication in A&
Measurements of the UV background at 4.6 < z < 6.4 using the quasar proximity effect
We present measurements of the ionising ultraviolet background (UVB) at z ~
5-6 using the quasar proximity effect. The fifteen quasars in our sample cover
the range 4.6 < z_q < 6.4, enabling the first proximity effect measurements of
the UVB at z > 5. The metagalactic hydrogen ionisation rate, Gamma_bkg, was
determined by modelling the combined ionisation field from the quasar and the
UVB in the proximity zone on a pixel-by-pixel basis. The optical depths in the
spectra were corrected for the expected effect of the quasar until the mean
flux in the proximity region equalled that in the average Ly-alpha forest, and
from this we make a measurement of Gamma_bkg. A number of systematic effects
were tested using synthetic spectra. Noise in the flux was found to be the
largest source of bias at z ~ 5, while uncertainties in the mean transmitted
Ly-alpha flux are responsible for the largest bias at z ~ 6. The impacts of
large-scale overdensities and Lyman limit systems on Gamma_bkg were also
investigated, but found to be small at z > 5. We find a decline in Gamma_bkg
with redshift, from log(Gamma_bkg) = -12.15 0.16 at z ~ 5 to
log(Gamma_bkg) = -12.84 0.18 at z ~ 6 (1 sigma errors). Compared to UVB
measurements at lower redshifts, our measurements suggest a drop of a factor of
five in the HI photoionisation rate between z ~ 4 and z ~ 6. The decline of
Gamma_bkg appears to be gradual, and we find no evidence for a sudden change in
the UVB at any redshift that would indicate a rapid change in the attenuation
length of ionising photons. Combined with recent measurements of the evolution
of the mean free path of ionising photons, our results imply decline in the
emissivity of ionising photons by roughly a factor of two from z ~ 5 to 6,
albeit with significant uncertainty due to the measurement errors in both
Gamma_bkg and the mean free path.Comment: 22 pages, 19 figures, 5 tables; accepted for publication in MNRA
z~7 galaxy candidates from NICMOS observations over the HDF South and the CDF-S and HDF-N GOODS fields
We use ~88 arcmin**2 of deep (>~26.5 mag at 5 sigma) NICMOS data over the two
GOODS fields and the HDF South to conduct a search for bright z>~7 galaxy
candidates. This search takes advantage of an efficient preselection over 58
arcmin**2 of NICMOS H-band data where only plausible z>~7 candidates are
followed up with NICMOS J-band observations. ~248 arcmin**2 of deep
ground-based near-infrared data (>~25.5 mag, 5 sigma) is also considered in the
search. In total, we report 15 z-dropout candidates over this area -- 7 of
which are new to these search fields. Two possible z~9 J-dropout candidates are
also found, but seem unlikely to correspond to z~9 galaxies. The present z~9
search is used to set upper limits on the prevalence of such sources. Rigorous
testing is undertaken to establish the level of contamination of our selections
by photometric scatter, low mass stars, supernovae (SNe), and spurious sources.
The estimated contamination rate of our z~7 selection is ~24%. Through careful
simulations, the effective volume available to our z>~7 selections is estimated
and used to establish constraints on the volume density of luminous (L*(z=3),
or -21 mag) galaxies from these searches. We find that the volume density of
luminous star-forming galaxies at z~7 is 13_{-5}^{+8}x lower than at z~4 and
>25x lower (1 sigma) at z~9 than at z~4. This is the most stringent constraint
yet available on the volume density of >~L* galaxies at z~9. The present
wide-area, multi-field search limits cosmic variance to <20%. The evolution we
find at the bright end of the UV LF is similar to that found from recent Subaru
Suprime-Cam, HAWK-I or ERS WFC3/IR searches. The present paper also includes a
complete summary of our final z~7 z-dropout sample (18 candidates) identified
from all NICMOS observations to date (over the two GOODS fields, the HUDF,
galaxy clusters).Comment: 13 pages, 6 figures, 6 tables, accepted for publication in the
Astrophysical Journal, replaced to match accepted version, see
http://firstgalaxies.org/astronomers-area/ for a link to a complete reduction
of the NICMOS observations over the two GOODS field
Evidence for a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field
We perform a deep search for galaxies in the redshift range 6.5<z<7.5, to
measure the evolution of the number density of luminous galaxies in this
redshift range and derive useful constraints on the evolution of their
Luminosity Function. We present here the first results of an ESO Large Program,
that exploits the unique combination of area and sensitivity provided in the
near-IR by the camera Hawk-I at the VLT. We have obtained two Hawk-I pointings
on the GOODS South field for a total of 32 observing hours, covering ~90
arcmin2. The images reach Y=26.7 mags for the two fields. We have used public
ACS images in the z band to select z-dropout galaxies with the colour criteria
Z-Y>1, Y-J<1.5 and Y-K<2. The other public data in the UBVRIJHK bands are used
to reject possible low redshift interlopers. The output has been compared with
extensive Monte Carlo simulations to quantify the observational effects of our
selection criteria as well as the effects of photometric errors. We detect 7
high quality candidates in the magnitude range Y=25.5-26.7. This interval
samples the critical range for M* at z>6 (M_1500 ~- 19.5 to -21.5). After
accounting for the expected incompleteness, we rule out at a 99% confidence
level a Luminosity Function constant from z=6 to z=7, even including the
effects of cosmic variance. For galaxies brighter than M_1500=-19.0 we derive a
luminosity density rho_UV=1.5^{+2.0}_{-0.9} 10^25 erg/s/Hz/Mpc3, implying a
decrease by a factor 3.5 from z=6 to z~6.8. On the basis of our findings, we
make predictions for the surface densities expected in future surveys surveys,
based on ULTRA-VISTA, HST-WFC3 or JWST-NIRCam, evaluating the best
observational strategy to maximise their impact.Comment: Accepted for publication in Astronomy & Astrophysic
Early star-forming galaxies and the reionization of the Universe
Star forming galaxies represent a valuable tracer of cosmic history. Recent
observational progress with Hubble Space Telescope has led to the discovery and
study of the earliest-known galaxies corresponding to a period when the
Universe was only ~800 million years old. Intense ultraviolet radiation from
these early galaxies probably induced a major event in cosmic history: the
reionization of intergalactic hydrogen. New techniques are being developed to
understand the properties of these most distant galaxies and determine their
influence on the evolution of the universe.Comment: Review article appearing in Nature. This posting reflects a submitted
version of the review formatted by the authors, in accordance with Nature
publication policies. For the official, published version of the review,
please see http://www.nature.com/nature/archive/index.htm
Structural Basis of BRCC36 Function in DNA Repair and Immune Regulation
In mammals, âŒ100 deubiquitinases act on âŒ20,000 intracellular ubiquitination sites. Deubiquitinases are commonly regarded as constitutively active, with limited regulatory and targeting capacity. The BRCA1-A and BRISC complexes serve in DNA double-strand break repair and immune signaling and contain the lysine-63 linkage-specific BRCC36 subunit that is functionalized by scaffold subunits ABRAXAS and ABRO1, respectively. The molecular basis underlying BRCA1-A and BRISC function is currently unknown. Here we show that in the BRCA1-A complex structure, ABRAXAS integrates the DNA repair protein RAP80 and provides a high-affinity binding site that sequesters the tumor suppressor BRCA1 away from the break site. In the BRISC structure, ABRO1 binds SHMT2α, a metabolic enzyme enabling cancer growth in hypoxic environments, which we find prevents BRCC36 from binding and cleaving ubiquitin chains. Our work explains modularity in the BRCC36 DUB family, with different adaptor subunits conferring diversified targeting and regulatory functions.ISSN:1097-2765ISSN:1097-416
Overcoming acculturation: physical education recruits' experiences of an alternative pedagogical approach to games teaching
© 2015 Association for Physical Education Background: Physical education teacher education (PETE) programmes have been identified as a critical platform to encourage the exploration of alternative teaching approaches by pre-service teachers. However, the socio-cultural constraint of acculturation or past physical education and sporting experiences results in the maintenance of the status quo of a teacher-driven, reproductive paradigm. Previous studies have reported successfully overcoming the powerful influence of acculturation, resulting in a change in PETE students' custodial teaching beliefs and receptiveness to alternative teaching approaches. However, to date, limited information has been reported about how PETE students' acculturation shaped their receptiveness to an alternative teaching approach. This is particularly the case for PETE recruits identified in the literature as most resistant to change. Purpose: To explore the features and experiences of an alternative games teaching approach that appealed to PETE recruits identified as most resistant to change, requiring a specific sample of PETE recruits with strong, custodial, traditional physical education teaching beliefs, and whom are high-achieving sporting products of this traditional culture. The alternative teaching approach explored in this study is the constraints-led approach (CLA), which is similar operationally to Teaching Games for Understanding, but distinguished by a neurobiological theoretical framework (nonlinear pedagogy) that informs learning design. Participants and setting: A purposive sample of 10 Australian PETE students was recruited for the study. All participants initially had strong, custodial, traditional physical education teaching beliefs, and were successful sporting products of this teaching approach. After experiencing the CLA as learners during a games unit, participants demonstrated receptiveness to the alternative pedagogy. Data collection and analysis: Semi-structured interviews and written reflections were sources of data collection. Each participant was interviewed separately, once prior to participation in the games unit to explore their positive physical education experiences, and then again after participation to explore the specific games unit learning experiences that influenced their receptiveness to the alternative pedagogy. Participants completed written reflections about their personal experiences after selected practical sessions. Data were qualitatively analysed using grounded theory. Findings: Thorough examination of the data resulted in establishment of two prominent themes related to the appeal of the CLA for the participants: (i) psychomotor (effective in developing skill) and (ii) inclusivity (included students of varying skill level). The efficacy of the CLA in skill development was clearly an important mediator of receptiveness for highly successful products of a traditional culture. This significant finding could be explained by three key factors: the acculturation of the participants, the motor learning theory underpinning the alternative pedagogy and the unit learning design and delivery. The inclusive nature of the CLA provided a solution to the problem of exclusion, which also made the approach attractive to participants. Conclusions: PETE educators could consider these findings when introducing an alternative pedagogy aimed at challenging PETE recruits' custodial, traditional teaching beliefs. To mediate receptiveness, it is important that the learning theory underpinning the alternative approach is operationalised in a research-informed pedagogical learning design that facilitates students' perceptions of the effectiveness of the approach through experiencing and or observing it working
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