1,727,608 research outputs found
Block Card 5347 Oldham Drive
No full textThis 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: dwelling | 5347 Oldham Drive (Toledo, Ohio) | Bungalow Style | McLains Jackman Place Plat 1 | Greenwood Area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | Washington Townshi
Inscribed Objects from Well P.5347
No full textEditions of the cuneiform and Luwian texts from Well P.5347 at Karkemis
The pottery assemblage from well P.5347
No full textThe pottery assemblage from well P.5347 consists of a total of 5707 collected sherds, 558 of which are diagnostic (rims, body sherds and bases), and are discussed here
Block Card 5347 Jackman Road
No full textThis 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: dwelling | 5347 Jackman Road (Toledo, Ohio) | Folk House Style | McLains Jackman Place Plat 1 | Greenwood Area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | Washington Townshi
Block Card 5347 Sanders Drive
No full textThis 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: Ranch houses | 5347 Sanders Drive (Toledo, Ohio) | Dwelling | Rancamp Place Addition (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Radio source J1402+5347 1.4GHz light curves
No full textVizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Extreme intra-hour variability of the radio source J1402+5347 discovered with Apertif.' (bibcode: 2020A&A...641L...4O
VPRS 6872 Police Magistrate's Register (Microfilm Copy of VPRS 5347)
No full textThis record series consists of a microfilm copy of VPRS 5347 Police Magistrate's Register
A hard look at NGC 5347: revealing a nearby Compton-thick AGN
Get PDFInternational audienceCurrent measurements show that the observed fraction of Compton-thick (CT) active galactic nuclei (AGN) is smaller than the expected values needed to explain the cosmic X-ray background. Prior fits to the X-ray spectrum of the nearby Seyfert-2 galaxy NGC 5347 (z = 0.00792, D = 35.5 Mpc ) have alternately suggested a CT and Compton-thin source. Combining archival data from Suzaku, Chandra, and—most importantly—new data from NuSTAR, and using three distinct families of models, we show that NGC 5347 is an obscured CTAGN (N H > 2.23 × 1024 cm−2). Its 2–30 keV spectrum is dominated by reprocessed emission from distant material, characterized by a strong Fe Kα line and a Compton hump. We found a large equivalent width of the Fe Kα line (EW = 2.3 ± 0.3 keV) and a high intrinsic-to-observed flux ratio (∼100). All of these observations are typical for bona fide CTAGN. We estimate a bolometric luminosity of L bol ≃ 0.014 ± 0.005 L Edd.. The Chandra image of NGC 5347 reveals the presence of extended emission dominating the soft X-ray spectrum (E < 2 keV), which coincides with the [O iii] emission detected in Hubble Space Telescope images. Comparison to other CTAGN suggests that NGC 5347 is broadly consistent with the average properties of this source class. We simulated XRISM and Athena/X-IFU spectra of the source, showing the potential of these future missions in identifying CTAGN in the soft X-rays
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