616 research outputs found
Obscuration by Gas and Dust in Luminous Quasars
We explore the connection between absorption by neutral gas and extinction by
dust in mid-infrared (IR) selected luminous quasars. We use a sample of 33
quasars at redshifts 0.7 < z < 3 in the 9 deg^2 Bo\"otes multiwavelength survey
field that are selected using Spitzer Space Telescope Infrared Array Camera
colors and are well-detected as luminous X-ray sources (with >150 counts) in
Chandra observations. We divide the quasars into dust-obscured and unobscured
samples based on their optical to mid-IR color, and measure the neutral
hydrogen column density N_H through fitting of the X-ray spectra. We find that
all subsets of quasars have consistent power law photon indices equal to 1.9
that are uncorrelated with N_H. We classify the quasars as gas-absorbed or
gas-unabsorbed if N_H > 10^22 cm^-2 or N_H < 10^22 cm^-2, respectively. Of 24
dust-unobscured quasars in the sample, only one shows clear evidence for
significant intrinsic N_H, while 22 have column densities consistent with N_H <
10^22 cm^-2. In contrast, of the nine dust-obscured quasars, six show evidence
for intrinsic gas absorption, and three are consistent with N_H < 10^22 cm^-2.
We conclude that dust extinction in IR-selected quasars is strongly correlated
with significant gas absorption as determined through X-ray spectral fitting.
These results suggest that obscuring gas and dust in quasars are generally
co-spatial, and confirm the reliability of simple mid-IR and optical
photometric techniques for separating quasars based on obscuration.Comment: 5 pages, 3 figure
Leave as an Accommodation: When is Enough, Enough?
The right to reasonable accommodations under the Americans with Disabilities Act includes leave that will enable an employee with a disability to return to work rather than being discharged. This right may seem unreasonable for an employer needing employees to be at work to be productive, raising the question of when leave as an accommodation becomes unreasonable or imposes an undue hardship on an employer. In the absence of specific guidance from the Supreme Court, the circuit courts apply a variety of approaches, ranging from individualized analysis to determinations that any leave exceeding some number of weeks is unreasonable. In this paper, three hundred and fifty-three decisions addressing this question have been analyzed to determine which factors are determinative of reasonableness, including factors identified in the various approaches of the circuit courts as well as those which economists would use to determine the value of an employee and the cost of replacing that employee
Resolving the unresolved cosmic X-ray background in the Chandra Deep Fields
We present a measurement of the surface brightness of the cosmic X-ray
background (CXB) in the Chandra Deep Fields, after excluding all detected
X-ray, optical and infrared sources. The work is motivated by a recent X-ray
stacking analysis by Worsley and collaborators, which showed that galaxies
detected by HST but not by Chandra may account for most of the unresolved CXB
at E>1 keV. We find that after excluding HST and Spitzer IRAC sources, some CXB
still remains, but it is marginally significant: (3.4+/-1.4)x10^-13 ergs cm^-2
s^-1 deg^2 in the 1-2 keV band and (4+/-9)x10^-13 ergs cm^-2 s^-1 deg^2 in the
2-5 keV band, or 7%+/-3% and 4%+/-9% of the total CXB, respectively. Of the 1-2
keV signal resolved by the HST sources, 34%+/-2% comes from objects with
optical colors typical of ``normal'' galaxies (which make up 25% of the HST
sources), while the remaining flux comes from objects with colors of starburst
and irregular galaxies. In the 0.65-1 keV band (just above the bright Galactic
O VII line) the remaining diffuse intensity is (1.0+/-0.2)x10^-12 ergs cm^-2
s^-1 deg^2. This flux includes emission from the Galaxy as well as from the
hypothetical warm-hot intergalactic medium (WHIM), and provides a conservative
upper limit on the WHIM signal that comes interestingly close to theoretical
predictions.Comment: 5 emulateapj pages, 4 figures, 1 table, accepted to ApJL (mostly
minor improvements in response to referee's comments, in particular further
treatment of uncertainties on resolved fluxes
A Tale of Two Narrow-Line Regions: Ionization, Kinematics, and Spectral Energy Distributions for a Local Pair of Merging Obscured Active Galaxies
We explore the gas ionization and kinematics, as well as the optical--IR
spectral energy distributions for UGC 11185, a nearby pair of merging galaxies
hosting obscured active galactic nuclei (AGNs), also known as SDSS
J181611.72+423941.6 and J181609.37+423923.0 (J1816NE and J1816SW, ). Due to the wide separation between these interacting galaxies ( kpc), observations of these objects provide a rare glimpse of the
concurrent growth of supermassive black holes at an early merger stage. We use
BPT line diagnostics to show that the full extent of the narrow line emission
in both galaxies is photoionized by an AGN and confirm the existence of a
10-kpc-scale ionization cone in J1816NE, while in J1816SW the AGN narrow-line
region is much more compact (1--2 kpc) and relatively undisturbed. Our
observations also reveal the presence of ionized gas that nearly spans the
entire distance between the galaxies which is likely in a merger-induced tidal
stream. In addition, we carry out a spectral analysis of the X-ray emission
using data from {\em XMM-Newton}. These galaxies represent a useful pair to
explore how the [\ion{O}{3}] luminosity of an AGN is dependent on the size of
the region used to explore the extended emission. Given the growing evidence
for AGN "flickering" over short timescales, we speculate that the appearances
and impact of these AGNs may change multiple times over the course of the
galaxy merger, which is especially important given that these objects are
likely the progenitors of the types of systems commonly classified as "dual
AGNs."Comment: 15 pages, 10 figures, accepted by the Astrophysical Journa
A Redline Starburst: Co(2-1) Observations of an Eddington-Limited Galaxy Reveal Star Formation at its Most Extreme
We report observations of the CO(2-1) emission of SDSSJ1506+54, a compact (r_e~135pc) starburst galaxy at z=0.6. SDSSJ1506+54 appears to be forming stars close to the limit allowed by stellar radiation pressure feedback models: the measured L_IR/L\u27_CO 1500 is one of the highest measured for any galaxy. With its compact optical morphology but extended low surface brightness envelope, post-starburst spectral features, high infrared luminosity (L_IR\u3e10^12.5 L_Sun), low gas fraction (M_H2/M_stars~15%), and short gas depletion time (tens of Myr), we speculate that this is a feedback- limited central starburst episode at the conclusion of a major merger. Taken as such, SDSSJ1504+54 epitomizes the brief closing stage of a classic model of galaxy growth: we are witnessing a key component of spheroid formation during what we term a \u27redline\u27 starburst
Variable Hard X-ray Emission from the Candidate Accreting Black Hole in Dwarf Galaxy Henize 2-10
We present an analysis of the X-ray spectrum and long-term variability of the
nearby dwarf starburst galaxy Henize 2-10. Recent observations suggest that
this galaxy hosts an actively accreting black hole with mass ~10^6 M_sun. The
presence of an AGN in a low-mass starburst galaxy marks a new environment for
active galactic nuclei (AGNs), with implications for the processes by which
"seed" black holes may form in the early Universe. In this paper, we analyze
four epochs of X-ray observations of Henize 2-10, to characterize the long-term
behavior of its hard nuclear emission. We analyze observations with Chandra
from 2001 and XMM-Newton from 2004 and 2011, as well as an earlier, less
sensitive observation with ASCA from 1997. Based on detailed analysis of the
source and background, we find that the hard (2-10 keV) flux of the putative
AGN has decreased by approximately an order of magnitude between the 2001
Chandra observation and exposures with XMM-Newton in 2004 and 2011. The
observed variability confirms that the emission is due to a single source. It
is unlikely that the variable flux is due to a supernova or ultraluminous X-ray
source, based on the observed long-term behavior of the X-ray and radio
emission, while the observed X-ray variability is consistent with the behavior
of well-studied AGNs.Comment: 7 pages, 4 figures, 2 tables; accepted for publication in Ap
A Spectroscopic Survey of Wise -Selected Obscured Quasars with the Southern African Large Telescope
We present the results of an optical spectroscopic survey of a sample of 40 candidate obscured quasars identified on the basis of their mid-infrared emission detected by the Wide-Field Infrared Survey Explorer (WISE). Optical spectra for this survey were obtained using the Robert Stobie Spectrograph on the Southern African Large Telescope. Our sample was selected with WISE colors characteristic of active galactic nuclei (AGNs), as well as red optical to mid-IR colors indicating that the optical/UV AGN continuum is obscured by dust. We obtain secure redshifts for the majority of the objects that comprise our sample (35/40), and find that sources that are bright in the WISE W4 (22 μm) band are typically at moderate redshift (z = 0.35) while sources fainter in W4 are at higher redshifts (z = 0.73). The majority of the sources have narrow emission lines with optical colors and emission line ratios of our WISE-selected sources that are consistent with the locus of AGN on the rest-frame g – z color versus [Ne III] λ3869/[O II] λλ3726+3729 line ratio diagnostic diagram. We also use empirical AGN and galaxy templates to model the spectral energy distributions (SEDs) for the objects in our sample, and find that while there is significant variation in the observed SEDs for these objects, the majority require a strong AGN component. Finally, we use the results from our analysis of the optical spectra and the SEDs to compare our selection criteria to alternate criteria presented in the literature. These results verify the efficacy of selecting luminous obscured AGNs based on their WISE colors
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