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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.

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At least 847 records · Page 47
All sourcesNASA NTRSDOE OSTI
DOE OSTI2016

The COSMOS2015 Catalog: Exploring the 1 < z < 6 universe with half a million galaxies

We present the COSMOS2015{sup 24} catalog, which contains precise photometric redshifts and stellar masses for more than half a million objects over the 2deg{sup 2} COSMOS field. Including new YJHK{sub s} images from the UltraVISTA-DR2 survey, Y-band images from Subaru/Hyper-Suprime-Cam, and infrared data from the Spitzer Large Area Survey with the Hyper-Suprime-Cam Spitzer legacy program, this near-infrared-selected catalog is highly optimized for the study of galaxy evolution and environments in the early universe. To maximize catalog completeness for bluer objects and at higher redshifts, objects have been detected on a χ {sup 2} sum of the YJHK{sub s} and z {sup ++} images. The catalog contains ∼6×10{sup 5} objects in the 1.5 deg{sup 2} UltraVISTA-DR2 region and ∼1.5×10{sup 5} objects are detected in the “ultra-deep stripes” (0.62 deg{sup 2}) at K{sub s}⩽24.7 (3σ, 3″, AB magnitude). Through a comparison with the zCOSMOS-bright spectroscopic redshifts, we measure a photometric redshift precision of σ{sub Δz/(1+z{sub s)}} = 0.007 and a catastrophic failure fraction of η = 0.5%. At 3<z<6, using the unique database of spectroscopic redshifts in COSMOS, we find σ{sub Δz/(1+z{sub s)}} = 0.021 and η = 13.2%. The deepest regions reach a 90% completeness limit of 10{sup 10}M{sub ⊙} to z = 4. Detailed comparisons of the color distributions, number counts, and clustering show excellent agreement with the literature in the same mass ranges. COSMOS2015 represents a unique, publicly available, valuable resource with which to investigate the evolution of galaxies within their environment back to the earliest stages of the history of the universe. The COSMOS2015 catalog is distributed via anonymous ftp and through the usual astronomical archive systems (CDS, ESO Phase 3, IRSA).

79 ASTRONOMY AND ASTROPHYSICS↗
DOE OSTI2018

LAMOST DR1: Stellar Parameters and Chemical Abundances with SP-Ace

We present a new analysis of the LAMOST DR1 survey spectral database performed with the code SP-Ace, which provides the derived stellar parameters T{sub eff}, logg, [Fe/H], and [α/H] for 1,097,231 stellar objects. We tested the reliability of our results by comparing them to reference results from high spectral resolution surveys. The expected errors can be summarized as ∼120 K in T{sub eff}, ∼0.2 in logg, ∼0.15 dex in [Fe/H], and ∼0.1 dex in [α/Fe] for spectra with S/N > 40, with some differences between dwarf and giant stars. SP-Ace provides error estimations consistent with the discrepancies observed between derived and reference parameters. Some systematic errors are identified and discussed. The resulting catalog is publicly available at the LAMOST and CDS websites.

79 ASTRONOMY AND ASTROPHYSICS↗
NASA NTRS1969

Applied physics

Infrared converter, photoluminescence in CdS thin films, tunneling barriers, ionization gage and electrical-discharge machining studies

Anner, G. E.↗
NASA NTRS1970

Rf-sputtered cadmium sulfide 'thin crystals'

RF-sputtered CdS thin films structural and electrical characteristics from X ray diffractometer tracings, reflection electron diffraction and X ray double crystal spectrometry

Lagnado, I.↗
NASA NTRS1971

Effect of load voltage on thin film cuprous sulfide: Cadmium sulfide solar cells thermally cycled in a simulated space environment

Thin-film Cu2S-CdS solar cells, loaded at various fixed values of load resistance, were thermally cycled for 1429 cycles in a simulated space environment. Cell performance was measured under controlled conditions in air before and after thermal cycling. These data were used to determine the effect of load voltage on cell performance. The performance of the cells was relatively independent of load voltage up to about 0.39 volt. This appears to be a threshold voltage, beyond which there was a significant loss in cell performance. Fortunately, this threshold voltage appears to be sufficiently higher than the maximum power voltage of 0.33 volt so that it can be avoided in most applications.

Smithrick, J. J.↗
NASA NTRS1971

Simulated space environment tests on cadmium sulfide solar cells

Cadmium sulfide (Cu2s - CdS) solar cells were tested under simulated space environmental conditions. Some cells were thermally cycled with illumination from a Xenon-arc solar simulator. A cycle was one hour of illumination followed immediately with one-half hour of darkness. In the light, the cells reached an equilibrium temperature of 60 C (333 K) and in the dark the cell temperature dropped to -120 C (153 K). Other cells were constantly illuminated with a Xenon-arc solar simulator. The equilibrium temperature of these cells was 55 C (328 K). The black vacuum chamber walls were cooled with liquid nitrogen to simulate a space heat sink. Chamber pressure was maintained at 0.000001 torr or less. Almost all of the solar cells tested degraded in power when exposed to a simulated space environment of either thermal cycling or constant illumination. The cells tested the longest were exposed to 10.050 thermal cycles.

Clarke, D. R.↗
NASA NTRS1971

Ultrasonic attenuation in superconducting molybdenum-rhenium alloys.

Investigation of longitudinal sound attenuation in superconducting Mo-Re alloys as a function of temperature, magnetic field, and frequency. Evaporated thin film CdS transducers were used for the measurements at frequencies up to 3 GHz. The normal state attenuation coefficient was found to be proportional to the square of frequency over this frequency range. Measurements in zero magnetic field yielded a value of the energy gap parameter close to the threshold value of 3.56 kTc, appropriate to a weakly coupled dirty limit superconductor.

Ashkin, M.↗