1,724,324 research outputs found
K.3244+
K.3244 + K.11282 + K.15950 + K.12551 + K.12552 + K.16938 + K.19811 + K.22040 (+) K.9024 + K.11696 + K.16820 + K.17324 + K.17325
Photographs and reconstructions by the Shumma alu team (FNS projects nos. 175970 and 205122
Wolters, P L, 3244
This record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/426905Surname: WOLTERS. Given Name(s) or Initials: P L. Military Service Number or Last Known Location: 3244. Missing, Wounded and Prisoner of War Enquiry Card Index Number: 14754.248920
Item: [2016.0049.59166] "Wolters, P L, 3244
Galaxy And Mass Assembly (GAMA) : the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm
We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z <0.1) galaxy luminosity functions in FUV, NUV, ugriz and YJHK bands from within a single well-constrained volume of 3.4 × 10 (Mpc h). The derived luminosity distributions are normalized to the SDSS data release 7 (DR7) main survey to reduce the estimated cosmic variance to the 5 per cent level. The data are used to construct the cosmic spectral energy distribution (CSED) from 0.1 to 2.1 μm free from any wavelength-dependent cosmic variance for both the elliptical and non-elliptical populations. The two populations exhibit dramatically different CSEDs as expected for a predominantly old and young population, respectively. Using the Driver et al. prescription for the azimuthally averaged photon escape fraction, the non-ellipticals are corrected for the impact of dust attenuation and the combined CSED constructed. The final results show that the Universe is currently generating (1.8 ± 0.3) × 10h W Mpc of which (1.2 ± 0.1) × 10h W Mpc is directly released into the inter-galactic medium and (0.6 ± 0.1) × 10h W Mpc is reprocessed and reradiated by dust in the far-IR. Using the GAMA data and our dust model we predict the mid- and far-IR emission which agrees remarkably well with available data. We therefore provide a robust description of the pre- and post-dust attenuated energy output of the nearby Universe from 0.1μm to 0.6 mm. The largest uncertainty in this measurement lies in the mid- and far-IR bands stemming from the dust attenuation correction and its currently poorly constrained dependence on environment, stellar mass and morphology.Peer reviewe
Block Card 3244 Penrose Avenue
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Cape Cod Style | 3244 Penrose Avenue (Toledo, Ohio) | Dwelling | Milton Place 1st Addition (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Block Card 3244 Northwood Avenue
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Modern Colonial Style | Dwelling (Toledo, Ohio) | 3244 Northwood Avenue (Toledo, Ohio) | Dauer Gardens Addition (Toledo, Ohio) | Deveaux Area (Toledo, Ohio) | West Toledo (Toledo, Ohio
IO Islamic 3244. Ta'rîkh-i-Panjâb, History of the Panjâb
IO Islamic 3244. Ta’rîkh-i-Panjâb, History of the Panjâ
IO Islamic 3244. Ta'rîkh-i-Panjâb, History of the Panjâb
IO Islamic 3244. Ta’rîkh-i-Panjâb, History of the Panjâ
Laida, John David (SC 3244)
Finding aid only for Manuscripts Small Collection 3244. “Iraq and Bible History,” a sermon of Dr. John David Laida, delivered at First Baptist Church, Owensboro, Kentucky, on 17 January 1993. His historical perspective includes comments on modern Iraq and Kuwait and the recent Persian Gulf War. He also calls for peace and for prayers for outgoing President George H. W. Bush and incoming president Bill Clinton
- …
