3,488 research outputs found
Matrix factorizations for quantum complete intersections
We introduce twisted matrix factorizations for quantum complete intersections
of codimension two. For such an algebra, we show that in a given dimension,
almost all the indecomposable modules with bounded minimal projective
resolutions correspond to such matrix factorizations.Comment: 13 page
Greetings from the Lower Rio Grande Valley of Texas Souvenir Folder [postcards]
Souvenir postcards promoting the lower Rio Grande Valley of Texas for vacation travel, agriculture, and ideal living conditions.https://scholarworks.utrgv.edu/lrgv/1028/thumbnail.jp
Social Impact Summary : Dickey-Lincoln School Lakes Project / Prepared for the Department of the Army, Corps of Engineers, New England Division
The Dickey-Lincoln Hydroelectric Dam is a water resources project proposed by the Federal Government (U. S. Army Corps of Engineers). Therefore, in accordance with the National Environmental Policy Act, the Corps of Engineers is required to prepare an environmental impact statement (EIS) on the project. A federal plan or project such as Dickey-Lincoln should take into account its effect upon man\u27s health, safety, welfare and economic well-being, as well as effects upon the surrounding environment. More importantly, project plans should be evaluated in a manner calculated to encourage harmony between man and his environment. In other words, project plans or policies which have adverse impacts upon the environment should be reexamined to see if they can be modified. This provides for mitigation of defined impacts
Summary of Labor Impacts During Construction : Dickey-Lincoln School Lakes Project
This study is to assess the effects or impacts of construction and operation of the Dickey-Lincoln hydroelectric project upon the people in the St. John Valley, Maine, and New England. Having determined the effects of the project, a second objective is to discuss mitigation of defined adverse impacts. More specifically, this study attempts to identify adverse impacts and deal with how to minimize such impacts if at all possible
The high mass end of the stellar mass function: Dependence on stellar population models and agreement between fits to the light profile
We quantify the systematic effects on the stellar mass function which arise
from assumptions about the stellar population, as well as how one fits the
light profiles of the most luminous galaxies at z ~ 0.1. When comparing results
from the literature, we are careful to separate out these effects. Our analysis
shows that while systematics in the estimated comoving number density which
arise from different treatments of the stellar population remain of order < 0.5
dex, systematics in photometry are now about 0.1 dex, despite recent claims in
the literature. Compared to these more recent analyses, previous work based on
Sloan Digital Sky Survey (SDSS) pipeline photometry leads to underestimates of
rho_*(> M_*) by factors of 3-10 in the mass range 10^11 - 10^11.6 M_Sun, but up
to a factor of 100 at higher stellar masses. This impacts studies which match
massive galaxies to dark matter halos. Although systematics which arise from
different treatments of the stellar population remain of order < 0.5 dex, our
finding that systematics in photometry now amount to only about 0.1 dex in the
stellar mass density is a significant improvement with respect to a decade ago.
Our results highlight the importance of using the same stellar population and
photometric models whenever low and high redshift samples are compared.Comment: 18 pages, 17 figures, accepted for publication in MNRAS. The PyMorph
luminosities and stellar masses are available at
https://www.physics.upenn.edu/~ameert/SDSS_PhotDec
Pratt Motor Company Records - Accession 1608
The collection consists of Log books of payments made to the Pratt Motor Company based in Rock Hill, S.C. and founded by Crawford C. Pratt (1910-1957) with client information, payment dates, addresses, and the make, model and year of vehicle sold. Information also includes serial numbers and motor numbers of vehicles. Some motor vehicle registrations are present, as well as a title.https://digitalcommons.winthrop.edu/manuscriptcollection_findingaids/2611/thumbnail.jp
Brief of Amicus Curiae C. Itoh and Company (America), Inc., In Support of Petitioner
ON WRIT OF CERTIORARI TO THE UNITED STATES COURT OF APPEALS FOR THE SECOND CIRCUIThttps://digitalcommons.nyls.edu/sumitomo_briefs/1018/thumbnail.jp
Letter from C. O. Mailloux to E. E. Gilbert, General Electric Company
https://digitalcommons.salve.edu/ochre-court/1168/thumbnail.jp
A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. II. Quantifying morphological k-correction in the COSMOS field at 1<z<2: Ks band vs. I band
We quantify the effects of \emph{morphological k-correction} at by
comparing morphologies measured in the K and I-bands in the COSMOS area.
Ks-band data have indeed the advantage of probing old stellar populations for
, enabling a determination of galaxy morphological types unaffected by
recent star formation. In paper I we presented a new non-parametric method to
quantify morphologies of galaxies on seeing limited images based on support
vector machines. Here we use this method to classify
selected galaxies in the COSMOS area observed with WIRCam at CFHT. The obtained
classification is used to investigate the redshift distributions and number
counts per morphological type up to and to compare to the results
obtained with HST/ACS in the I-band on the same objects from other works. We
associate to every galaxy with and a probability between 0 and
1 of being late-type or early-type. The classification is found to be reliable
up to . The mean probability is . It decreases with redshift
and with size, especially for the early-type population but remains above
. The classification is globally in good agreement with the one
obtained using HST/ACS for . Above , the I-band classification
tends to find less early-type galaxies than the Ks-band one by a factor
1.5 which might be a consequence of morphological k-correction effects.
We argue therefore that studies based on I-band HST/ACS classifications at
could be underestimating the elliptical population. [abridged]Comment: accepted for publication in A&A, updated with referee comments, 12
pages, 10 figure
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