1,769 research outputs found
The Frequency and Radio Properties of Broad Absorption Line Quasars
A sample of 67 Broad Absorption Line quasars (BALQSOs) from the Large Bright
Quasar Survey (LBQS) is used to estimate the observed and intrinsic fraction of
BAL quasars in optically--selected samples at intermediate (B_J \simeq 18.5)
magnitudes. The observed BALQSO fraction in the redshift range 1.5 < z < 3.0 is
15\pm3%. A well--determined, empirical, k--correction, to allow for the
differences in the spectral energy distributions of non--BALQSOs and BALQSOs
shortward of \simeq 2100A in the restframe, is applied to the sample. The
result is an estimate of the intrinsic fraction of BALQSOs, in the redshift
range 1.5 < z < 3.0, of 22+/-4%. This value is twice that commonly cited for
the occurrence of BALQSOs in optically--selected samples and the figure is in
reasonable agreement with that from a preliminary analysis of the SDSS Early
Data Release. The fraction of BALQSOs predicted to be present in an optical
survey with flux limits equivalent to that of the FIRST Bright Quasar Survey
(FBQS) is shown to be \simeq 20%. The BALQSO fractions derived from the FBQS
and the LBQS suggest that optically--bright BALQSOs are half as likely as
non-BALQSOs to be detectable as S_1.4GHz > 1mJy radio sources.Comment: Accepted for publication in AJ, April 2003 Issu
Large-Scale Structure at z~2.5
We have made a statistically complete, unbiased survey of C IV systems toward
a region of high QSO density near the South Galactic Pole using 25 lines of
sight spanning . Such a survey makes an excellent probe of
large-scale structure at early epochs. We find evidence for structure on the
proper Mpc scale ( km Mpc) as
determined by the two point C IV - C IV absorber correlation function, and
reject the null hypothesis that C IV systems are distributed randomly on such
scales at the level. The structure likely reflects the
distance between two groups of absorbers subtending and Mpc at and respectively. There is also a marginal trend for the association of
high rest equivalent width C IV absorbers and QSOs at similar redshifts but
along different lines of sight. The total number of C IV systems detected is
consistent with that which would be expected based on a survey using many
widely separated lines of sight. Using the same data, we also find 11 Mg II
absorbers in a complete survey toward 24 lines of sight; there is no evidence
for Mg II - Mg II or Mg II - QSO clustering, though the sample size is likely
still small to detect such structure if it exists.Comment: 56 pages including 32 of figures, in gzip-ed uuencoded postscript
format, 1 long table not included, aastex4 package. Accepted for publication
in ApJ Supplement
BOOK REVIEW ISLAM AND ECOLOGY: A BESTOWED TRUST
The themes of this hefty tome, consisting of twenty-three essays, preceded by prefaces and introductions, are closely connected with the May 1998 conference on Islam and ecology, which was held in the framework of a series of gatherings on the stance of the worldâs religious traditions towards todayâs environmental crisis, hosted by the Center for the Study of World Religions at Harvard University between 1996 and 1998. The editors of this volume must be credited with giving the contributors opportunity to present the most up-to-date essays, which must have been quite a strain on the editing process of an ambitious project like this
Civic Chorale
Center for the Performing Arts Concert Hall November 14, 2017 8:00 p.m
Fabrication and characterization of silver- and copper-coated Nylon 6 forcespun nanofibers by thermal evaporation
Silver and copper nanoparticles were deposited as thin films onto substrates consisting of Nylon 6 nanofibers manufactured using forcespinningR equipment. Different rotational speeds were used to obtain continuous nanofibers of various diameters arranged as nonwoven mats. The Nylon 6 nanofibers were collected as successive layers on frames, and a high-vacuum thermal evaporation method was used to deposit the silver and copper thin films on the nanofibers. The structures were investigated using scanning electron microscopyâscanning transmission electron microscopy, atomic force microscopy, x-ray diffraction, and electrical resistance measurements. The results indicate that evaporated silver and copper nanoparticles were successfully deposited on Nylon 6 nanofibers as thin films that adhered well to the polymer substrate while the native morphology of the nanofibers were preserved, and electrically conductive nanostructures were achieved
Diurnal variation of the tropospheric energy balance
November 1976.Includes bibliographical references.Sponsored by NSF OCD 75-01424.Suggested physical mechanism for diurnal cycle of required warming / W. M. Gray
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Reasoning from multiple texts: An automatic analysis of readers' situation models
In reading multiple texts, a reader must integrate information from the texts with his or her background knowledge. The resulting situation model represents a rich elaborated structure of events, actions, objects, and people involved in the text organized in a manner consistent with the reader's knowledge. In order to evaluate a reader's situation model, a reader's summary must be analyzed in relation to texts the subject has read as well as to more general knowledge such as an expert's knowledge. However, this analysis can be both time-consuming and difficult. In this paper, we use an automatic approach called Latent Semantic Analysis (LSA) for evaluating the situation model of readers of multiple documents. LSA is a statistical model of word usage that generates a high-dimensional semantic space that models the semantics of the text. This paper describes three experiments. The first two describe methods for analyzing a subject's essay to determine from what text a subject learned the information and for grading the quality of information cited in the essay. The third experiment analyzes the knowledge structures of novice and expert readers and compares them to the knowledge structures generated by the model. The experiments illustrate a general approach to modeling and evaluating readers' situation models
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Behavior of Explosives Under Pressure in a Diamond Anvil Cell
Diamond anvil cell (DAC) studies can yield information about the pressure dependence of materials and reactions under conditions comparable to shock loading. The pressure gradient across the face of the diamonds is often deliberately minimized to create uniform pressure over much of the sample and a simplified data set. To reach very high pressures (30-40 GPa), however, it may be necessary to use ''softer'', high nitrogen content diamonds that are more susceptible to bending under pressure. The resulting enhanced pressure gradient then provides a view of high-pressure behavior under anisotropic conditions similar to those found at the burn front in a bulk sample. We discuss visual observations of pressure-induced changes relative to variations in burn rate of several explosives (Triaminotrinitrobenzene, Nitromethane, CL-20) in the DAC. The burn rate behavior of both Nitromethane (NM) and Triaminotrinitrobenzene (TATB) were previously reported for pressures up to {approx}40 GPa. Nitromethane showed a near monotonic increase in burn rate to a maximum at {approx}30 GPa after which the burn rate decreased, all without color change. At higher pressures, the TATB samples had shiny (metallic) polycrystalline zones or inclusions where the pressure was highest in the sample. Around the shiny zones was a gradation of color (red to yellow) that appeared to follow the pressure gradient. The color changes are believed related to disturbances in the resonance structure of this explosive as the intermolecular separations decrease with pressure. The color and type of residue found in unvented gaskets after the burn was complete also varied with pressure. The four polymorphs of CL-20 ({alpha}, {beta}, {gamma}, {var_epsilon}-Hexanitrohexaazaisowurtzitane, HNIW) did not change color up to the highest pressure applied ({approx}30 GPa), and each polymorph demonstrated a distinctly different burn rate signature. One polymorph {beta} was so sensitive to laser ignition over a narrow pressure range that the sample could not be aligned with a low power laser without ignition. The burn rate for that one polymorph could only be measured at pressures above and below that unique pressure. This anomalous ignition threshold is discussed with respect to the matrix of possible polymorphs, most of which have not been isolated in the laboratory. The changes in behavior, color and reaction rates of all samples are discussed with respect to possible implications to chemistry at high pressure
The FIRST Bright Quasar Survey. II. 60 Nights and 1200 Spectra Later
We have used the VLA FIRST survey and the APM catalog of the POSS-I plates as
the basis for constructing a new radio-selected sample of optically bright
quasars. This is the first radio-selected sample that is competitive in size
with current optically selected quasar surveys. Using only two basic criteria,
radio-optical positional coincidence and optical morphology, quasars and BL
Lacs can be identified with 60% selection efficiency; the efficiency increases
to 70% for objects fainter than magnitude 17. We show that a more sophisticated
selection scheme can predict with better than 85% reliability which candidates
will turn out to be quasars.
This paper presents the second installment of the FIRST Bright Quasar Survey
with a catalog of 636 quasars distributed over 2682 square degrees. The quasar
sample is characterized and all spectra are displayed. The FBQS detects both
radio-loud and radio-quiet quasars out to a redshift z>3. We find a large
population of objects of intermediate radio-loudness; there is no evidence in
our sample for a bimodal distribution of radio characteristics. The sample
includes ~29 broad absorption line quasars, both high and low ionization, and a
number of new objects with remarkable optical spectra.Comment: 41 pages plus 39 gifs which contain all quasar spectra. Accepted for
publication in the Astrophysical Journal Supplement Serie
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