26 research outputs found
Letter from E. W. Reynolds to John Henry Jenks; September 2, 1863
A reproduction of the original and typed transcription of a letter from E. W. Reynolds Jenks to John Henry Jenks, written on September 2, 1863, from Swanzey, New Hampshire, during John Henry Jenks\u27 Civil War service with the 14th New Hampshire Volunteer Infantry
The X-ray Remnant of SN1987A
We present high resolution Chandra observations of the remnant of SN1987A in
the Large Magellanic Cloud. The high angular resolution of the Chandra X-ray
Observatory (CXO) permits us to resolve the X-ray remnant. We find that the
remnant is shell-like in morphology, with X-ray peaks associated with some of
the optical hot spots seen in HST images. The X-ray light curve has departed
from the linear flux increase observed by ROSAT, with a 0.5-2.0 keV luminosity
of 1.5 x 10^35 erg/s in January 2000. We set an upper limit of 2.3 x 10^34
ergs/s on the luminosity of any embedded central source (0.5 - 2 keV). We also
present a high resolution spectrum, showing that the X-ray emission is thermal
in origin and is dominated by highly ionized species of O, Ne, Mg, and Si.Comment: 16 pages, 3 figures, Accepted for publication in ApJ Letter
Monitoring the Evolution of the X-ray Remnant of SN 1987A
We report on the results of our monitoring program of the remnant of SN 1987A
with the Advanced CCD Imaging Spectrometer (ACIS) on board the {\it Chandra
X-ray Observatory}. Two new observations have been performed in AO2, bringing
the total to four monitoring observations over the past two years. Over this
time period, new techniques for correction of ``Charge Transfer Inefficiency
(CTI)'' and for use of charge spreading to provide angular resolution somewhat
better than the pixel size of the CCD detector have become available at Penn
State. We have processed all four observations using sub-pixel resolution to
obtain the highest possible angular resolution, and using our CTI correction
software to provide more reliable spectral analysis and flux estimations.
The high angular resolution images indicate that the X-ray bright knots are
convincingly correlated with the optical spots, primarily at \la1 keV, while
higher energy photons are very well correlated with radio images. Our data also
provide marginal evidence for radial expansion of the X-ray remnant at a rate
of 5200 2100 km s. The X-ray flux appears to linearly increase by
60% over the 18 month period of these observations. The spectrum is
dominated by broad complexes of atomic emission lines and can be fit with a
simple model of a plane-parallel shock with electron temperatures of
2 4 keV and a postshock electron density of 210
420 cm. The implied 0.5 10 keV band luminosity in 2001 April is
1.3 10 ergs s; as of that date, we still observe
no direct evidence for the central point source, with an upper limit on the
{\it observed} luminosity of 5.5 10 ergs
s in the 2 10 keV band.Comment: 29 pages, 5 figures (2 color images), Accepted for Ap
Creative destruction in science
Drawing on the concept of a gale of creative destruction in a capitalistic economy, we argue that initiatives to assess the robustness of findings in the organizational literature should aim to simultaneously test competing ideas operating in the same theoretical space. In other words, replication efforts should seek not just to support or question the original findings, but also to replace them with revised, stronger theories with greater explanatory power. Achieving this will typically require adding new measures, conditions, and subject populations to research designs, in order to carry out conceptual tests of multiple theories in addition to directly replicating the original findings. To illustrate the value of the creative destruction approach for theory pruning in organizational scholarship, we describe recent replication initiatives re-examining culture and work morality, working parents\u2019 reasoning about day care options, and gender discrimination in hiring decisions.
Significance statement
It is becoming increasingly clear that many, if not most, published research findings across scientific fields are not readily replicable when the same method is repeated. Although extremely valuable, failed replications risk leaving a theoretical void\u2014 reducing confidence the original theoretical prediction is true, but not replacing it with positive evidence in favor of an alternative theory. We introduce the creative destruction approach to replication, which combines theory pruning methods from the field of management with emerging best practices from the open science movement, with the aim of making replications as generative as possible. In effect, we advocate for a Replication 2.0 movement in which the goal shifts from checking on the reliability of past findings to actively engaging in competitive theory testing and theory building.
Scientific transparency statement
The materials, code, and data for this article are posted publicly on the Open Science Framework, with links provided in the article
The James Webb Space Telescope Mission
Twenty-six years ago a small committee report, building on earlier studies,
expounded a compelling and poetic vision for the future of astronomy, calling
for an infrared-optimized space telescope with an aperture of at least .
With the support of their governments in the US, Europe, and Canada, 20,000
people realized that vision as the James Webb Space Telescope. A
generation of astronomers will celebrate their accomplishments for the life of
the mission, potentially as long as 20 years, and beyond. This report and the
scientific discoveries that follow are extended thank-you notes to the 20,000
team members. The telescope is working perfectly, with much better image
quality than expected. In this and accompanying papers, we give a brief
history, describe the observatory, outline its objectives and current observing
program, and discuss the inventions and people who made it possible. We cite
detailed reports on the design and the measured performance on orbit.Comment: Accepted by PASP for the special issue on The James Webb Space
Telescope Overview, 29 pages, 4 figure