32,019 research outputs found
Extending the baseline: Spitzer Mid-Infrared Photometry of Globular Cluster Systems in the Centaurus A and Sombrero Galaxies
Spitzer IRAC mid-infrared photometry is presented for the globular cluster
(GC) systems of the NGC 5128 ("Centaurus A") and NGC 4594 ("Sombrero")
galaxies. Existing optical photometric and spectroscopic are combined with this
new data in a comprehensive optical to mid-IR colour catalogue of 260 GCs.
Empirical colour-metallicity relationships are derived for all optical to
mid-IR colour combinations.
These colours prove to be very effective quantities to test the photometric
predictions of simple stellar population (SSP) models. In general, four SSP
models show larger discrepancies between each other and the data at bluer
wavelengths, especially at high metallicities. Such differences become very
important when attempting to use colour-colour model predictions to constrain
the ages of stellar populations. Furthermore, the age-substructure determined
from colour-colour diagrams and 91 NGC 5128 GCs with spectroscopic ages from
Beasley et al. (2008) are inconsistent, suggesting any apparent GC system
age-substructure implied by a colour-colour analysis must be verified
independently.
Unlike blue wavebands, certain optical to mid-IR colours are insensitive to
the flux from hot horizontal branch stars and thus provide an excellent
metallicity proxy. The NGC 5128 GC system shows strong bimodality in the
optical R-band to mid-IR colour distributions, hence proving it is bimodal in
metallicity. In this new colour space, a colour-magnitude trend, a "blue tilt",
is found in the NGC 5128 metal-poor GC data. The NGC 5128 young GCs do not
contribute to this trend. [abridged]Comment: 16 pages, 12 colour figures. To be published in MNRAS. Catalogue
available from the first author. Full resolution copy available here
http://lee.spitler.googlepages.com/spitzer_spitler.pd
A gyroscope calibration analysis for the Gamma Ray Observatory (GRO)
Current documentation and software do not adequately address the calculation and use of the optimal weight matrices involved in calibrating inertial reference units (IRU). Several facets of the GRO IRU calibration as it relates to the bias and misalignment weighting matrices are investigated. The physical meaning and use of the bias and misalignment weight matrices in IRU calibration are examined. The relation of the weighting and the final biases, misalignments, and their corrections are pursued. Methods for determining reliable, realistic weighting matrices to be used in the GRO IRU calibration (IRUCAL) utility are determined. Possible correlations among observation uncertainties are also explored. For the undetermined case where the maneuvers are insufficient to identify all calibration parameters, the weighting matrices allow as much information as possible to be extracted from the measurements. Finally, applicable simulated flight data are used, incorporating the appropriate calibration maneuvers, to test the weighting matrices in the IRUCAL utility, and examine correlation effects
Separating weak lensing and intrinsic alignments using radio observations
We discuss methods for performing weak lensing using radio observations to
recover information about the intrinsic structural properties of the source
galaxies. Radio surveys provide unique information that can benefit weak
lensing studies, such as HI emission, which may be used to construct galaxy
velocity maps, and polarized synchrotron radiation; both of which provide
information about the unlensed galaxy and can be used to reduce galaxy shape
noise and the contribution of intrinsic alignments. Using a proxy for the
intrinsic position angle of an observed galaxy, we develop techniques for
cleanly separating weak gravitational lensing signals from intrinsic alignment
contamination in forthcoming radio surveys. Random errors on the intrinsic
orientation estimates introduce biases into the shear and intrinsic alignment
estimates. However, we show that these biases can be corrected for if the error
distribution is accurately known. We demonstrate our methods using simulations,
where we reconstruct the shear and intrinsic alignment auto and cross-power
spectra in three overlapping redshift bins. We find that the intrinsic position
angle information can be used to successfully reconstruct both the lensing and
intrinsic alignment power spectra with negligible residual bias.Comment: 17 pages, 10 figures, submitted to MNRA
Separate and Unequal: The Effect of Unequal Access to Employment-Based Health Insurance on Gay, Lesbian, and Bisexual People
Employers' standard practice of including legal spouses in health insurance is likely to place people in unmarried couples at a significant disadvantage for obtaining coverage. Data from married and unmarried couples in the Current Population Survey confirm that people with unmarried partners are two to three times more likely to lack health insurance than are people in married couples, even after controlling for factors that influence coverage. A requirement to provide the same benefits for partners as are provided to spouses would reduce the proportion of uninsured people in same-sex couples and different-sex couples by as much as 50%. We find no evidence of adverse selection. We predict that a typical employer offering domestic partner coverage will see a small increase in enrollment, ranging from 0.1% to 0.3% for same-sex partners and 1.3% to 2.1% for different-sex unmarried partners.health, health insurance, benefits, employment benefits, health disparities, domestic partners, minorities, discrimination, gender, sexuality, sexual orientation, gay, lesbian, marriage, same-sex couples
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