text: 63,25,1121780337061896192,3422471637,Elias Kammoun,"Here is our new paper on NGC 5347: a bona fide Compton-thick AGN just sitting in our backyard! More exciting results from our survey of nearby obscured AGN with @NASANuSTAR are coming soon..  <LINK> <LINK> @NASANuSTAR In ~12 years the @AthenaXIFU on board of @AthenaXobs will allow us to look at the finest details in X-ray spectra of obscured AGN, opening a whole new window in X-ray astronomy, going from the current data-quality (left) to the well-resolved emission lines with Athena (right). <LINK>",https://arxiv.org/abs/1904.11028,"Current measurements show that the observed fraction of Compton-thick (CT) 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 \rm ~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 ($N_{\rm H} > 2.23\times 10^{24}~\rm cm^{-2}$). Its 2-30~keV spectrum is dominated by reprocessed emission from distant material, characterized by a strong Fe K$\alpha$ line and a Compton hump. We found a large equivalent width of the Fe K$\alpha$ line ($\rm EW = 2.3 \pm 0.3$ keV) and a high intrinsic-to-observed flux ratio ($\sim 100$). All of these observations are typical for bona fide CTAGN. We estimate a bolometric luminosity of $L_{\rm bol} \simeq 0.014 \pm 0.005~L_{\rm Edd.}$. The $Chandra$ image of NGC 5347 reveals the presence of extended emission dominating the soft X-ray spectrum ($E < 2\,\rm keV$), which coincides with the [O III] emission detected in the $Hubble ~Space~ Telescope$ 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. ",A hard look at NGC 5347: revealing a nearby Compton-thick AGN,2,"['Here is our new paper on NGC 5347: a bona fide Compton-thick AGN just sitting in our backyard!\n\nMore exciting results from our survey of nearby obscured AGN with @NASANuSTAR are coming soon.. \n\n<LINK> <LINK>', '@NASANuSTAR In ~12 years the @AthenaXIFU on board of @AthenaXobs will allow us to look at the finest details in X-ray spectra of obscured AGN, opening a whole new window in X-ray astronomy, going from the current data-quality (left) to the well-resolved emission lines with Athena (right). https://t.co/ohySAjTJkl']",19,04,502