{"id":61,"date":"2018-02-07T13:35:58","date_gmt":"2018-02-07T18:35:58","guid":{"rendered":"https:\/\/science.clemson.edu\/ctagn\/?page_id=61"},"modified":"2025-02-03T12:51:03","modified_gmt":"2025-02-03T17:51:03","slug":"publications","status":"publish","type":"page","link":"https:\/\/science.clemson.edu\/ctagn\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"

These are the refereed publications related to the Clemson-INAF CT-AGN project. You can find an updated list on ADS<\/a> as well.<\/p>\n\n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Number<\/th>Title<\/th>Author<\/th>ADS<\/th>arXiv<\/th>\n<\/tr>\n<\/thead>\n
1<\/td>X-Ray Spectral Properties of Seven Heavily Obscured Seyfert 2 Galaxies<\/td>Marchesi et al. (2017)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
2<\/td>Chandra and NuSTAR Follow-up Observations of Swift-BAT-selected AGNs<\/td>Marchesi et al. (2017)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
3<\/td>Compton thick AGN in the NuSTAR era<\/td>Marchesi et al. (2018)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
4<\/td>Compton-thick AGN in the NuSTAR Era. II. A Deep NuSTAR and XMM-Newton View of the Candidate Compton-thick AGN in NGC 1358<\/td>Zhao et al. (2019a)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
5<\/td>Compton-thick AGN in the NuSTAR Era. III. A Systematic Study of the Torus Covering Factor<\/td>Marchesi et al. (2019a)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
6<\/td>Compton-thick AGN in the NuSTAR Era. IV. A Deep NuSTAR and XMM-Newton View of the Candidate Compton-thick AGN in ESO 116-G018<\/td>Zhao et al. (2019b)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
7<\/td>Compton-thick AGNs in the NuSTAR Era. V. Joint NuSTAR and XMM-Newton Spectral Analysis of Three \u201cSoft-gamma\u201d Candidate CT-AGNs in the Swift\/BAT 100-month Catalog<\/td>Marchesi et al. (2019b)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
8<\/td>A Broadband X-Ray Study of a Sample of AGNs with [O III] Measured Inclinations<\/td>Zhao et al. (2020)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
9<\/td>A New Observation-based Clumpy Torus Model for Active Galactic Nuclei<\/td>Zhao et al. (2021)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
10<\/td>Compton-Thick AGN in the NuSTAR era VI: The observed Compton-thick fraction in the Local Universe<\/td>Torres-Alb\u00e0 et al. (2021)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
11<\/td>Compton-Thick AGN in the NuSTAR era VII. A joint NuSTAR, Chandra and XMM-Newton analysis of two nearby, heavily obscured sources<\/td>Traina et al. (2021)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
12<\/td>Chandra Follow-up Observations of Swift-BAT-selected AGNs II<\/td>Silver et al. (2022)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
13<\/td>Compton-thick AGN in the NuSTAR Era. VIII. A joint NuSTAR-XMM-Newton Monitoring of the Changing-look Compton-thick AGN NGC 1358<\/td>Marchesi et al. (2022)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
14<\/td>A Multiepoch X-Ray Study of the Nearby Seyfert 2 Galaxy NGC 7479: Linking Column Density Variability to the Torus Geometry<\/td>Pizzetti et al. (2022)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
15<\/td>Compton-thick AGN in the NuSTAR Era. IX. A Joint NuSTAR and XMM-Newton Analysis of Four Local AGN<\/td>Silver et al. (2022)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
16<\/td>A machine learning algorithm for reliably predicting active galactic nucleus absorbing column densities<\/td>Silver et al. (2023)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
17<\/td>Compton-thick AGN in the NuSTAR Era X: Analysing seven local CT-AGN candidates<\/td>Sengupta et al. (2023)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
18<\/td>Hydrogen column density variability in a sample of local Compton-thin AGN<\/td>Torres-Alb\u00e0 et al. (2023)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
19<\/td>A Simple Method for Predicting N H Variability in Active Galactic Nuclei<\/td>Cox et al. (2023)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
20<\/td>An X-Ray Significantly Variable, Luminous, Type 2 Quasar at z = 2.99 with a Massive Host Galaxy<\/td>Zhao et al. (2024)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
21<\/td>Chandra Follow-up Observations of Swift-BAT-selected AGNs III<\/td>Cox et al. (2025)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
22<\/td>Hydrogen Column Density Variability in a Sample of Local Compton-thin AGN II<\/td>Pizzetti et al. (2025)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
23<\/td>Swift-XRT and NuSTAR Monitoring of Obscuration Variability in Mrk 477<\/td>Torres-Alb\u00e0 et al. (2025)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
24<\/td>A multiwavelength characterization of the obscuring medium at the center of NGC 6300<\/td>Sengupta et al. (2025)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
25<\/td>X-ray polarization observations of NGC 2110 with IXPE<\/td>Pal et al. (2025)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
26<\/td>A systematic search for AGN obscuration variability in the Chandra archive<\/td>Cox et al (2025)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n
27<\/td>Unveiling Obscured Accretion in the Local Universe<\/td>Pal et al. (2025)<\/td>ADS<\/a><\/td>arXiv<\/a><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n\n","protected":false},"excerpt":{"rendered":"

These are the refereed publications related to the Clemson-INAF CT-AGN project. You can find an updated list on ADS as well.<\/p>\n","protected":false},"author":6,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-61","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/pages\/61","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/users\/6"}],"replies":[{"embeddable":true,"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/comments?post=61"}],"version-history":[{"count":5,"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/pages\/61\/revisions"}],"predecessor-version":[{"id":823,"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/pages\/61\/revisions\/823"}],"wp:attachment":[{"href":"https:\/\/science.clemson.edu\/ctagn\/wp-json\/wp\/v2\/media?parent=61"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}