216 research outputs found
High-fidelity indirect readout of trapped-ion hyperfine qubits
We propose and demonstrate a protocol for high-fidelity indirect readout of
trapped ion hyperfine qubits, where the state of a qubit ion is
mapped to a readout ion using laser-driven Raman
transitions. By partitioning the ground state hyperfine
manifold into two subspaces representing the two qubit states and choosing
appropriate laser parameters, the protocol can be made robust to spontaneous
photon scattering errors on the Raman transitions, enabling repetition for
increased readout fidelity. We demonstrate combined readout and back-action
errors for the two subspaces of and
with 68% confidence while avoiding decoherence
of spectator qubits due to stray resonant light that is inherent to direct
fluorescence detection.Comment: 7 + 6 pages, 3 + 1 figure
Quantifying the Effects of Known Unknowns on Inferred High-redshift Galaxy Properties: Burstiness, the IMF, and Nebular Physics
The era of the James Webb Space Telescope ushers stellar populations models
into uncharted territories, particularly at the high-redshift frontier. In a
companion paper, we apply the \texttt{Prospector} Bayesian framework to jointly
infer galaxy redshifts and stellar populations properties from broad-band
photometry as part of the UNCOVER survey. Here we present a comprehensive error
budget in spectral energy distribution (SED) modeling. Using a
sample, we quantify the systematic shifts stemming from various model choices
in inferred stellar mass, star formation rate (SFR), and age. These choices
encompass different timescales for changes in the star formation history (SFH),
non-universal stellar initial mass functions (IMF), and the inclusion of
variable nebular abundances, gas density and ionizing photon budget. We find
that the IMF exerts the strongest influence on the inferred properties: the
systematic uncertainties can be as much as 1 dex, 2--5 times larger than the
formal reported uncertainties in mass and SFR; and importantly, exceed the
scatter seen when using different SED fitting codes. This means that a common
practice in the literature of assessing uncertainties in SED-fitting processes
by comparing multiple codes is substantively underestimating the true
systematic uncertainty. Highly stochastic SFHs change the inferred SFH by much
larger than the formal uncertainties, and introduce dex systematics
in SFR and dex systematics in average age. Finally, employing a
flexible nebular emission model causes dex systematic increase in
mass, comparable to the formal uncertainty. This paper constitutes one of the
initial steps toward a complete uncertainty estimate in SED modeling.Comment: Submitted to ApJ. 18 pages, 8 figures, 2 table
BACH2 regulates CD8(+) T cell differentiation by controlling access of AP-1 factors to enhancers.
T cell antigen receptor (TCR) signaling drives distinct responses depending on the differentiation state and context of CD8(+) T cells. We hypothesized that access of signal-dependent transcription factors (TFs) to enhancers is dynamically regulated to shape transcriptional responses to TCR signaling. We found that the TF BACH2 restrains terminal differentiation to enable generation of long-lived memory cells and protective immunity after viral infection. BACH2 was recruited to enhancers, where it limited expression of TCR-driven genes by attenuating the availability of activator protein-1 (AP-1) sites to Jun family signal-dependent TFs. In naive cells, this prevented TCR-driven induction of genes associated with terminal differentiation. Upon effector differentiation, reduced expression of BACH2 and its phosphorylation enabled unrestrained induction of TCR-driven effector programs
UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of Galaxies
Observations of high-redshift galaxies provide a critical direct test to the
theories of early galaxy formation, yet to date, only four have been
spectroscopically confirmed at . Due to strong gravitational lensing over
a wide area, the galaxy cluster field Abell~2744 is ideal for searching for the
earliest galaxies. Here we present JWST/NIRSpec observations of two galaxies: a
robust detection at , and a plausible
candidate at . The galaxies are
discovered in JWST/NIRCam imaging and their distances are inferred with
JWST/NIRSpec spectroscopy, all from the JWST Cycle 1 UNCOVER Treasury survey.
Detailed stellar population modeling using JWST NIRCam and NIRSpec data
corroborates the primeval characteristics of these galaxies: low mass (), young, rapidly-assembling, metal-poor, and star-forming.
Interestingly, both galaxies are spatially resolved, having lensing-corrected
rest-UV effective radii on the order of 300-400 pc, which are notably larger
than other spectroscopically confirmed systems. The observed
dynamic range of size spans over an order of magnitude, implying
a significant scatter in the size-mass relation at early times. Deep into the
epoch of reionization, these discoveries elucidate the emergence of the first
galaxies.Comment: submitted to ApJL; 13 pages, 4 figures, 2 table
UNCOVER: The growth of the first massive black holes from JWST/NIRSpec -- spectroscopic confirmation of an X-ray luminous AGN at z=10.1
The James Webb Space Telescope is now detecting early black holes (BHs) as
they transition from "seeds" to supermassive BHs. Recently Bogdan et al. (2023)
reported the detection of an X-ray luminous supermassive BH, UHZ-1, with a
photometric redshift at . Such an extreme source at this very high
redshift provides new insights on seeding and growth models for BHs given the
short time available for formation and growth. Harnessing the exquisite
sensitivity of JWST/NIRSpec, here we report the spectroscopic confirmation of
UHZ-1 at . We find that the NIRSpec/Prism spectrum is
typical of recently discovered z~10 galaxies, characterized primarily by
star-formation features. We see no clear evidence of the powerful X-ray source
in the rest-frame UV/optical spectrum, which may suggest heavy obscuration of
the central BH, in line with the Compton-thick column density measured in the
X-rays. We perform a stellar population fit simultaneously to the new NIRSpec
spectroscopy and previously available photometry. The fit yields a stellar mass
estimate for the host galaxy that is significantly better constrained than
prior photometric estimates ().
Given the predicted BH mass (), the resulting
ratio of remains two to three orders of magnitude higher than
local values, thus lending support to the heavy seeding channel for the
formation of supermassive BHs within the first billion years of cosmic
evolution.Comment: 9 pages, 4 figures, submitted to ApJL. Minor text correction
UNCOVER: Candidate Red Active Galactic Nuclei at 3<z<7 with JWST and ALMA
The James Webb Space Telescope (JWST) is revolutionizing our knowledge of
galaxies and their actively accreting black holes. Using the JWST Cycle 1
Treasury program Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of
Reionization (UNCOVER) in the lensing field Abell 2744, we report the
identification of a sample of little red dots at that
likely contain highly-reddened accreting supermassive black holes. Using a
NIRCam-only selection to F444W mag, we find 26 sources over the
arcmin field that are blue in F115WF200W (or for ), red in F200WF444W =
(), and are dominated by a point-source like
central component. Of the 20 sources with deep ALMA 1.2-mm coverage, none are
detected individually or in a stack. For the majority of the sample, SED fits
to the JWST+ALMA observations prefer models with hot dust rather than obscured
star-formation to reproduce the red NIRCam colors and ALMA 1.2-mm
non-detections. While compact dusty star formation can not be ruled out, the
combination of extremely small sizes ( pc after
correction for magnification), red rest-frame optical slopes, and hot dust can
by explained by reddened broad-line active galactic nuclei (AGNs). Our targets
have faint mag but inferred
bolometric luminosities of erg/s, reflecting
their obscured nature. If the candidates are confirmed as AGNs with upcoming
UNCOVER spectroscopy, then we have found an abundant population of reddened
luminous AGN that are at least ten times more numerous than UV-luminous AGN at
the same intrinsic bolometric luminosity.Comment: submitted to Ap
UNCOVER: A NIRSpec Identification of a Broad-line AGN at z = 8.50
Deep observations with the James Webb Space Telescope (JWST) have revealed an emerging population of red pointlike sources that could provide a link between the postulated supermassive black hole seeds and observed quasars. In this work, we present a JWST/NIRSpec spectrum from the JWST Cycle 1 UNCOVER Treasury survey of a massive accreting black hole at z = 8.50 displaying a clear broad-line component as inferred from the Hβ line with FWHM = 3439 ± 413 km s−1, typical of the broad-line region of an active galactic nucleus (AGN). The AGN nature of this object is further supported by high ionization, as inferred from emission lines, and a point-source morphology. We compute a black hole mass of
and a bolometric luminosity of Lbol ∼ 6.6 × 1045 erg s−1. These values imply that our object is accreting at ∼40% of the Eddington limit. Detailed modeling of the spectral energy distribution in the optical and near-infrared, together with constraints from ALMA, indicate an upper limit on the stellar mass of , which would lead to an unprecedented ratio of black hole to host mass of at least ∼30%. This is orders of magnitude higher compared to the local QSOs but consistent with recent AGN studies at high redshift with JWST. This finding suggests that a nonnegligible fraction of supermassive black holes either started out from massive seeds and/or grew at a super-Eddington rate at high redshift. Given the predicted number densities of high-z faint AGN, future NIRSpec observations of larger samples will allow us to further investigate galaxy–black hole coevolution in the early Universe
UNCOVER: A NIRSpec Identification of a Broad Line AGN at z = 8.50
Deep observations with JWST have revealed an emerging population of red
point-like sources that could provide a link between the postulated
supermassive black hole seeds and observed quasars. In this work we present a
JWST/NIRSpec spectrum from the JWST Cycle 1 UNCOVER Treasury survey, of a
massive accreting black hole at , displaying a clear broad-line
component as inferred from the H line with FWHM = km
s, typical of the broad line region of an active galactic nucleus (AGN).
The AGN nature of this object is further supported by high ionization, as
inferred from emission lines, and a point-source morphology. We compute the
black hole mass of log, and a bolometric
luminosity of erg s. These values
imply that our object is accreting at of the Eddington limit.
Detailed modeling of the spectral energy distribution in the optical and
near-infrared, together with constraints from ALMA, indicate an upper limit on
the stellar mass of log, which would lead to an
unprecedented ratio of black hole to host mass of at least . This
is orders of magnitude higher compared to the local QSOs, but is consistent
with recent AGN studies at high redshift with JWST. This finding suggests that
a non-negligible fraction of supermassive black holes either started out from
massive seeds and/or grew at a super-Eddington rate at high redshift. Given the
predicted number densities of high- faint AGN, future NIRSpec observations
of larger samples will allow us to further investigate the galaxy-black hole
co-evolution in the early Universe.Comment: 14 pages, 6 figures, 2 tables. Submitted to ApJ
DUALZ: Deep UNCOVER-ALMA Legacy High-Z Survey
We present the survey design and initial results of the ALMA Cycle 9 program
of DUALZ, which aims to establish a joint ALMA and JWST public legacy field
targeting the massive galaxy cluster Abell 2744. DUALZ features a contiguous
ALMA 30-GHz-wide mosaic in Band 6, covering areas of down
to a sensitivity of Jy. Through a blind search, we identified
69 dust continuum sources at S/N with median redshift and
intrinsic 1.2-mm flux of and ~mJy. Of
these, 27 have been spectroscopically confirmed, leveraged by the latest
NIRSpec observations, while photometric redshift estimates are constrained by
the comprehensive HST, NIRCam, and ALMA data for the remaining sources. With
priors, we further identify a [CII]158 m line emitter at
, confirmed by the latest NIRSpec spectroscopy. The NIRCam
counterparts of the 1.2-mm continuum exhibit undisturbed morphologies, denoted
either by disk or spheroid, implying the triggers for the faint mm emission are
less catastrophic than mergers. We have identified 8 HST-dark galaxies
(F150W27mag, F150WF444W2.3) and 2 JWST-dark (F444W30mag) galaxy
candidates among the ALMA continuum sources. The former includes face-on disk
galaxies, hinting that substantial dust obscuration does not always result from
inclination. We also detect a marginal dust emission from an X-ray-detected
galaxy at , suggesting an active co-evolution of the
central black hole and its host. We assess the infrared luminosity function up
to and find it consistent with predictions from galaxy formation
models. To foster diverse scientific outcomes from the community, we publicly
release reduced ALMA mosaic maps, cubes, and the source catalog.Comment: 33 pages, 16 figures, and 5 tables. Submitted to ApJS. The ALMA
products are fully available from here:
https://jwst-uncover.github.io/DR2.html#DUAL
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