Publications

[1]Nandra, K., “The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission”, arXiv e-prints, 2013.
[2]Elvis, M., “The Chandra COSMOS Survey. I. Overview and Point Source Catalog”, The Astrophysical Journal Supplement Series, vol. 184, no. 1, pp. 158–171, 2009. doi:10.1088/0067-0049/184/1/158.
[3]Civano, F., “The Chandra Cosmos Legacy Survey: Overview and Point Source Catalog”, The Astrophysical Journal, vol. 819, no. 1, 2016. doi:10.3847/0004-637X/819/1/62.
[4]Cisternas, M., “The Bulk of the Black Hole Growth Since z ~ 1 Occurs in a Secular Universe: No Major Merger-AGN Connection”, The Astrophysical Journal, vol. 726, no. 2, 2011. doi:10.1088/0004-637X/726/2/57.
[5]Salvato, M., “Photometric Redshift and Classification for the XMM-COSMOS Sources”, The Astrophysical Journal, vol. 690, no. 2, pp. 1250–1263, 2009. doi:10.1088/0004-637X/690/2/1250.
[6]Hasinger, G., “The XMM-Newton Wide-Field Survey in the COSMOS Field. I. Survey Description”, The Astrophysical Journal Supplement Series, vol. 172, no. 1, pp. 29–37, 2007. doi:10.1086/516576.
[7]Brusa, M., “The XMM-Newton Wide-field Survey in the Cosmos Field (XMM-COSMOS): Demography and Multiwavelength Properties of Obscured and Unobscured Luminous Active Galactic Nuclei”, The Astrophysical Journal, vol. 716, no. 1, pp. 348–369, 2010. doi:10.1088/0004-637X/716/1/348.
[8]Lusso, E., “The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS”, Astronomy and Astrophysics, vol. 512, 2010. doi:10.1051/0004-6361/200913298.
[9]Finoguenov, A., “The XMM-Newton Wide-Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies”, The Astrophysical Journal Supplement Series, vol. 172, no. 1, pp. 182–195, 2007. doi:10.1086/516577.
[10]Cappelluti, N., “The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue”, Astronomy and Astrophysics, vol. 497, no. 2, pp. 635–648, 2009. doi:10.1051/0004-6361/200810794.
[11]Leauthaud, A., “A Weak Lensing Study of X-ray Groups in the Cosmos Survey: Form and Evolution of the Mass-Luminosity Relation”, The Astrophysical Journal, vol. 709, no. 1, pp. 97–114, 2010. doi:10.1088/0004-637X/709/1/97.
[12]Marchesi, S., “The Chandra COSMOS Legacy survey: optical/IR identifications”, The Astrophysical Journal, vol. 817, no. 1, 2016. doi:10.3847/0004-637X/817/1/34.
[13]Silverman, J. D., “Ongoing and Co-Evolving Star Formation in zCOSMOS Galaxies Hosting Active Galactic Nuclei”, The Astrophysical Journal, vol. 696, no. 1, pp. 396–410, 2009. doi:10.1088/0004-637X/696/1/396.
[14]Fiore, F., “Chasing Highly Obscured QSOs in the COSMOS Field”, The Astrophysical Journal, vol. 693, no. 1, pp. 447–462, 2009. doi:10.1088/0004-637X/693/1/447.
[15]Salvato, M., “Dissecting Photometric Redshift for Active Galactic Nucleus Using XMM- and Chandra-COSMOS Samples”, The Astrophysical Journal, vol. 742, no. 2, 2011. doi:10.1088/0004-637X/742/2/61.
[16]Civano, F., “The Chandra COSMOS Survey. III. Optical and Infrared Identification of X-Ray Point Sources”, The Astrophysical Journal Supplement Series, vol. 201, no. 2, 2012. doi:10.1088/0067-0049/201/2/30.
[17]Merloni, A., “The incidence of obscuration in active galactic nuclei”, Monthly Notices of the Royal Astronomical Society, vol. 437, no. 4, pp. 3550–3567, 2014. doi:10.1093/mnras/stt2149.
[18]Gabor, J. M., “Active Galactic Nucleus Host Galaxy Morphologies in COSMOS”, The Astrophysical Journal, vol. 691, no. 1, pp. 705–722, 2009. doi:10.1088/0004-637X/691/1/705.
[19]Jahnke, K., “Massive Galaxies in COSMOS: Evolution of Black Hole Versus Bulge Mass but not Versus Total Stellar Mass Over the Last 9 Gyr?”, The Astrophysical Journal, vol. 706, no. 2, pp. L215–L220, 2009. doi:10.1088/0004-637X/706/2/L215.
[20]Brusa, M., “The XMM-Newton Wide-Field Survey in the COSMOS Field. III. Optical Identification and Multiwavelength Properties of a Large Sample of X-Ray-Selected Sources”, The Astrophysical Journal Supplement Series, vol. 172, no. 1, pp. 353–367, 2007. doi:10.1086/516575.
[21]Wang, T., “Discovery of a Galaxy Cluster with a Violently Starbursting Core at z = 2.506”, The Astrophysical Journal, vol. 828, no. 1, 2016. doi:10.3847/0004-637X/828/1/56.
[22]Silverman, J. D., “The Impact of Galaxy Interactions on Active Galactic Nucleus Activity in zCOSMOS”, The Astrophysical Journal, vol. 743, no. 1, 2011. doi:10.1088/0004-637X/743/1/2.
[23]Vanzella, E., “Hubble Imaging of the Ionizing Radiation from a Star-forming Galaxy at Z=3.2 with fesc>50%”, The Astrophysical Journal, vol. 825, no. 1, 2016. doi:10.3847/0004-637X/825/1/41.
[24]Comastri, A., “The XMM Deep survey in the CDF-S. I. First results on heavily obscured AGN”, Astronomy and Astrophysics, vol. 526, 2011. doi:10.1051/0004-6361/201016119.
[25]Merlin, E., “T-PHOT: A new code for PSF-matched, prior-based, multiwavelength extragalactic deconfusion photometry”, Astronomy and Astrophysics, vol. 582, 2015. doi:10.1051/0004-6361/201526471.
[26]Allevato, V., “The XMM-Newton Wide Field Survey in the COSMOS Field: Redshift Evolution of AGN Bias and Subdominant Role of Mergers in Triggering Moderate-luminosity AGNs at Redshifts up to 2.2”, The Astrophysical Journal, vol. 736, no. 2, 2011. doi:10.1088/0004-637X/736/2/99.
[27]Trump, J. R., “The COSMOS Active Galactic Nucleus Spectroscopic Survey. I. XMM-Newton Counterparts”, The Astrophysical Journal, vol. 696, no. 2, pp. 1195–1212, 2009. doi:10.1088/0004-637X/696/2/1195.
[28]Smolčić, V., “Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution”, Astronomy and Astrophysics, vol. 548, 2012. doi:10.1051/0004-6361/201219368.
[29]Cappelluti, N., “The XMM-Newton Wide-Field Survey in the COSMOS Field. II. X-Ray Data and the logN-logS Relations”, The Astrophysical Journal Supplement Series, vol. 172, no. 1, pp. 341–352, 2007. doi:10.1086/516586.
[30]Predehl, P., “eROSITA on SRG”, in Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, 2010, vol. 7732. doi:10.1117/12.856577.
[31]Civano, F., “A Runaway Black Hole in COSMOS: Gravitational Wave or Slingshot Recoil?”, The Astrophysical Journal, vol. 717, no. 1, pp. 209–222, 2010. doi:10.1088/0004-637X/717/1/209.
[32]Brusa, M., “High-Redshift Quasars in the COSMOS Survey: The Space Density of z > 3 X-Ray Selected QSOs”, The Astrophysical Journal, vol. 693, no. 1, pp. 8–22, 2009. doi:10.1088/0004-637X/693/1/8.
[33]Castellano, M., “The ASTRODEEP Frontier Fields catalogues. II. Photometric redshifts and rest frame properties in Abell-2744 and MACS-J0416”, Astronomy and Astrophysics, vol. 590, 2016. doi:10.1051/0004-6361/201527514.
[34]Gilli, R., “The spatial clustering of X-ray selected AGN in the XMM-COSMOS field”, Astronomy and Astrophysics, vol. 494, no. 1, pp. 33–48, 2009. doi:10.1051/0004-6361:200810821.
[35]Mainieri, V., “The XMM-Newton Wide-Field Survey in the COSMOS Field. IV. X-Ray Spectral Properties of Active Galactic Nuclei”, The Astrophysical Journal Supplement Series, vol. 172, no. 1, pp. 368–382, 2007. doi:10.1086/516573.
[36]Rovilos, E., “GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection”, Astronomy and Astrophysics, vol. 546, 2012. doi:10.1051/0004-6361/201218952.
[37]Ajello, M., “Galaxy Clusters in the Swift/Burst Alert Telescope Era: Hard X-rays in the Intracluster Medium”, The Astrophysical Journal, vol. 690, no. 1, pp. 367–388, 2009. doi:10.1088/0004-637X/690/1/367.
[38]Sargent, M. T., “The VLA-COSMOS Perspective on the Infrared-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the Infrared/Radio Properties of Star-Forming and Active Galactic Nucleus Galaxies at Intermediate and High Redshift”, The Astrophysical Journal Supplement Series, vol. 186, no. 2, pp. 341–377, 2010. doi:10.1088/0067-0049/186/2/341.
[39]Silverman, J. D., “The Environments of Active Galactic Nuclei within the zCOSMOS Density Field”, The Astrophysical Journal, vol. 695, no. 1, pp. 171–182, 2009. doi:10.1088/0004-637X/695/1/171.
[40]Natarajan, P., “Unveiling the First Black Holes With JWST:Multi-wavelength Spectral Predictions”, The Astrophysical Journal, vol. 838, no. 2, 2017. doi:10.3847/1538-4357/aa6330.
[41]Merlin, E., “The ASTRODEEP Frontier Fields catalogues. I. Multiwavelength photometry of Abell-2744 and MACS-J0416”, Astronomy and Astrophysics, vol. 590, 2016. doi:10.1051/0004-6361/201527513.
[42]Miyaji, T., “Detailed Shape and Evolutionary Behavior of the X-Ray Luminosity Function of Active Galactic Nuclei”, The Astrophysical Journal, vol. 804, no. 2, 2015. doi:10.1088/0004-637X/804/2/104.
[43]Mainieri, V., “Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS”, Astronomy and Astrophysics, vol. 535, 2011. doi:10.1051/0004-6361/201117259.
[44]Cappelluti, N., “Cross-correlating Cosmic Infrared and X-Ray Background Fluctuations: Evidence of Significant Black Hole Populations among the CIB Sources”, The Astrophysical Journal, vol. 769, no. 1, 2013. doi:10.1088/0004-637X/769/1/68.
[45]Lanzuisi, G., “Compton thick AGN in the XMM-COSMOS survey”, Astronomy and Astrophysics, vol. 573, 2015. doi:10.1051/0004-6361/201424924.
[46]Brunner, H., “XMM-Newton observations of the Lockman Hole: X-ray source catalogue and number counts”, Astronomy and Astrophysics, vol. 479, no. 1, pp. 283–300, 2008. doi:10.1051/0004-6361:20077687.
[47]Cappelluti, N., “Searching for the 3.5 keV Line in the Deep Fields with Chandra: The 10 Ms Observations”, The Astrophysical Journal, vol. 854, no. 2, 2018. doi:10.3847/1538-4357/aaaa68.
[48]Vito, F., “The hard X-ray luminosity function of high-redshift (3 < z ≲ 5) active galactic nuclei”, Monthly Notices of the Royal Astronomical Society, vol. 445, no. 4, pp. 3557–3574, 2014. doi:10.1093/mnras/stu2004. [49]Puccetti, S., “The Chandra Survey of the COSMOS Field. II. Source Detection and Photometry”, The Astrophysical Journal Supplement Series, vol. 185, no. 2, pp. 586–601, 2009. doi:10.1088/0067-0049/185/2/586. [50]LaMassa, S. M., “The 31 Deg2 Release of the Stripe 82 X-Ray Survey: The Point Source Catalog”, The Astrophysical Journal, vol. 817, no. 2, 2016. doi:10.3847/0004-637X/817/2/172. [51]Elvis, M., “Spectral Energy Distributions of Type 1 Active Galactic Nuclei in the COSMOS Survey. I. The XMM-COSMOS Sample”, The Astrophysical Journal, vol. 759, no. 1, 2012. doi:10.1088/0004-637X/759/1/6. [52]Cappelluti, N., “The Chandra COSMOS Legacy Survey: Energy Spectrum of the Cosmic X-Ray Background and Constraints on Undetected Populations”, The Astrophysical Journal, vol. 837, no. 1, 2017. doi:10.3847/1538-4357/aa5ea4. [53]Vito, F., “The deepest X-ray view of high-redshift galaxies: constraints on low-rate black hole accretion”, Monthly Notices of the Royal Astronomical Society, vol. 463, no. 1, pp. 348–374, 2016. doi:10.1093/mnras/stw1998. [54]Allevato, V., “Occupation of X-Ray-selected Galaxy Groups by X-Ray Active Galactic Nuclei”, The Astrophysical Journal, vol. 758, no. 1, 2012. doi:10.1088/0004-637X/758/1/47. [55]Georgantopoulos, I., “The XMM deep survey in the CDF-S. IV. Compton-thick AGN candidates”, Astronomy and Astrophysics, vol. 555, 2013. doi:10.1051/0004-6361/201220828. [56]Cappelluti, N., “A candidate tidal disruption event in the Galaxy cluster Abell 3571”, Astronomy and Astrophysics, vol. 495, no. 2, pp. L9–L12, 2009. doi:10.1051/0004-6361/200811479. [57]Trump, J. R., “Observational Limits on Type 1 Active Galactic Nucleus Accretion Rate in COSMOS”, The Astrophysical Journal, vol. 700, no. 1, pp. 49–55, 2009. doi:10.1088/0004-637X/700/1/49. [58]Miyaji, T., “The XMM-Newton Wide-Field Survey in the COSMOS Field. V. Angular Clustering of the X-Ray Point Sources”, ¨C58C, vol. 172, no. 1, pp. 396–405, 2007. doi:10.1086/516579. [59]Pacucci, F., Natarajan, P., Volonteri, M., Cappelluti, N., and Urry, C. M., “Conditions for Optimal Growth of Black Hole Seeds”, ¨C59C, vol. 850, no. 2, 2017. doi:10.3847/2041-8213/aa9aea. [60]Erfanianfar, G., “Non-linearity and environmental dependence of the star-forming galaxies main sequence”, ¨C60C, vol. 455, no. 3, pp. 2839–2851, 2016. doi:10.1093/mnras/stv2485. [61]Morselli, L., “Primordial environment of super massive black holes: large-scale galaxy overdensities around z ~ 6 quasars with LBT”, ¨C61C, vol. 568, 2014. doi:10.1051/0004-6361/201423853. [62]Ranalli, P., “The XMM deep survey in the CDF-S. III. Point source catalogue and number counts in the hard X-rays”, ¨C62C, vol. 555, 2013. doi:10.1051/0004-6361/201321211. [63]LaMassa, S. M., “Finding rare AGN: XMM-Newton and Chandra observations of SDSS Stripe 82”, ¨C63C, vol. 436, no. 4, pp. 3581–3601, 2013. doi:10.1093/mnras/stt1837. [64]Cappelluti, N., “Active Galactic Nuclei Clustering in the Local Universe: An Unbiased Picture from Swift-BAT”, ¨C64C, vol. 716, no. 2, pp. L209–L213, 2010. doi:10.1088/2041-8205/716/2/L209. [65]Cappelluti, N., “X-ray source overdensities in Chandra distant cluster fields: A new probe to map the cosmic tapestry?”, ¨C65C, vol. 430, pp. 39–45, 2005. doi:10.1051/0004-6361:20041534. [66]Allevato, V., “Clustering of Moderate Luminosity X-Ray-selected Type 1 and Type 2 AGNS at Z ~ 3”, ¨C66C, vol. 796, no. 1, 2014. doi:10.1088/0004-637X/796/1/4. [67]Lanzuisi, G., “Active Galactic Nucleus X-Ray Variability in the XMM-COSMOS Survey”, ¨C67C, vol. 781, no. 2, 2014. doi:10.1088/0004-637X/781/2/105. [68]Cappelluti, N., “eROSITA on SRG. A X-ray all-sky survey mission”, ¨C68C, vol. 17, p. 159, 2011. [69]Kocevski, D. D., “X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field”, ¨C69C, vol. 236, no. 2, 2018. doi:10.3847/1538-4365/aab9b4. [70]Iwasawa, K., “The XMM deep survey in the CDF-S. II. A 9-20 keV selection of heavily obscured active galaxies at z > 1.7”, Astronomy and Astrophysics, vol. 546, 2012. doi:10.1051/0004-6361/201220036.
[71]Ananna, T. T., “AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey”, The Astrophysical Journal, vol. 850, no. 1, 2017. doi:10.3847/1538-4357/aa937d.
[72]Cappelluti, N., “The nature of the unresolved extragalactic cosmic soft X-ray background”, Monthly Notices of the Royal Astronomical Society, vol. 427, no. 1, pp. 651–663, 2012. doi:10.1111/j.1365-2966.2012.21867.x.
[73]Powell, M. C., “The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs”, The Astrophysical Journal, vol. 858, no. 2, 2018. doi:10.3847/1538-4357/aabd7f.
[74]Cappelluti, N., “Chandra Counterparts of CANDELS GOODS-S Sources”, The Astrophysical Journal, vol. 823, no. 2, 2016. doi:10.3847/0004-637X/823/2/95.
[75]Aird, J., “The Hot and Energetic Universe: The formation and growth of the earliest supermassive black holes”, arXiv e-prints, 2013.
[76]Tanaka, M., “An X-Ray Detected Group of Quiescent Early-Type Galaxies at z = 1.6 in the Chandra Deep Field South”, Publications of the Astronomical Society of Japan, vol. 65, 2013. doi:10.1093/pasj/65.1.17.
[77]Finoguenov, A., “Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field South”, Astronomy and Astrophysics, vol. 576, 2015. doi:10.1051/0004-6361/201323053.
[78]Kashlinsky, A., Arendt, R. G., Atrio-Barandela, F., Cappelluti, N., Ferrara, A., and Hasinger, G., “Looking at cosmic near-infrared background radiation anisotropies”, Reviews of Modern Physics, vol. 90, no. 2, 2018. doi:10.1103/RevModPhys.90.025006.
[79]Williams, C. C., “Morphology Dependence of Stellar Age in Quenched Galaxies at Redshift ∼1.2: Massive Compact Galaxies Are Older than More Extended Ones”, The Astrophysical Journal, vol. 838, no. 2, 2017. doi:10.3847/1538-4357/aa662f.
[80]Iwasawa, K., “Fe K emission from active galaxies in the COSMOS field”, Astronomy and Astrophysics, vol. 537, 2012. doi:10.1051/0004-6361/201118203.
[81]Gozaliasl, G., “Chandra centres for COSMOS X-ray galaxy groups: differences in stellar properties between central dominant and offset brightest group galaxies”, Monthly Notices of the Royal Astronomical Society, vol. 483, no. 3, pp. 3545–3565, 2019. doi:10.1093/mnras/sty3203.
[82]Ziparo, F., “Reversal or no reversal: the evolution of the star formation rate-density relation up to z ∼ 1.6”, Monthly Notices of the Royal Astronomical Society, vol. 437, no. 1, pp. 458–474, 2014. doi:10.1093/mnras/stt1901.
[83]Ajello, M., “Galaxy Clusters in the Swift/BAT Era. II. 10 More Clusters Detected Above 15 keV”, The Astrophysical Journal, vol. 725, no. 2, pp. 1688–1706, 2010. doi:10.1088/0004-637X/725/2/1688.
[84]LaMassa, S. M., “Finding rare AGN: X-ray number counts of Chandra sources in Stripe 82”, Monthly Notices of the Royal Astronomical Society, vol. 432, no. 2, pp. 1351–1360, 2013. doi:10.1093/mnras/stt553.
[85]Suh, H., “Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching”, The Astrophysical Journal, vol. 841, no. 2, 2017. doi:10.3847/1538-4357/aa725c.
[86]Ziparo, F., “The lack of star formation gradients in galaxy groups up to z ∼ 1.6”, Monthly Notices of the Royal Astronomical Society, vol. 434, no. 4, pp. 3089–3103, 2013. doi:10.1093/mnras/stt1222.
[87]Georgantopoulos, I., “On the Lx – L6 μm ratio as a diagnostic for Compton-thick AGN”, Astronomy and Astrophysics, vol. 534, 2011. doi:10.1051/0004-6361/201117400.
[88]Vito, F., “Discovery of the first heavily obscured QSO candidate at z > 6 in a close galaxy pair”, Astronomy and Astrophysics, vol. 628, 2019. doi:10.1051/0004-6361/201935924.
[89]Helgason, K., Cappelluti, N., Hasinger, G., Kashlinsky, A., and Ricotti, M., “The Contribution of z <~ 6 Sources to the Spatial Coherence in the Unresolved Cosmic Near-infrared and X-Ray Backgrounds”, The Astrophysical Journal, vol. 785, no. 1, 2014. doi:10.1088/0004-637X/785/1/38. [90]Cappelluti, N., Allevato, V., and Finoguenov, A., “Clustering of X-Ray-Selected AGN”, Advances in Astronomy, vol. 2012, 2012. doi:10.1155/2012/853701. [91]Erfanianfar, G., “X-Ray Groups of Galaxies in the AEGIS Deep and Wide Fields”, The Astrophysical Journal, vol. 765, no. 2, 2013. doi:10.1088/0004-637X/765/2/117. [92]Roncarelli, M., Cappelluti, N., Borgani, S., Branchini, E., and Moscardini, L., “The effect of feedback on the emission properties of the warm-hot intergalactic medium”, Monthly Notices of the Royal Astronomical Society, vol. 424, no. 2, pp. 1012–1025, 2012. doi:10.1111/j.1365-2966.2012.21277.x. [93]Nanni, R., “The 500 ks Chandra observation of the z = 6.31 QSO SDSS J1030 + 0524”, Astronomy and Astrophysics, vol. 614, 2018. doi:10.1051/0004-6361/201832694. [94]Balmaverde, B., “Primordial environment of supermassive black holes. II. Deep Y- and J-band images around the z 6.3 quasar SDSS J1030+0524”, Astronomy and Astrophysics, vol. 606, 2017. doi:10.1051/0004-6361/201730683. [95]Cappelluti, N., “Probing Large-scale Coherence between Spitzer IR and Chandra X-Ray Source-subtracted Cosmic Backgrounds”, The Astrophysical Journal, vol. 847, no. 1, 2017. doi:10.3847/2041-8213/aa8acd. [96]Fotopoulou, S., “The 5-10 keV AGN luminosity function at 0.01 < z < 4.0”, Astronomy and Astrophysics, vol. 587, 2016. doi:10.1051/0004-6361/201424763. [97]Lanzuisi, G., “The most obscured AGN in the COSMOS field”, Astronomy and Astrophysics, vol. 578, 2015. doi:10.1051/0004-6361/201526036. [98]Ranalli, P., “The 2-10 keV unabsorbed luminosity function of AGN from the LSS, CDFS, and COSMOS surveys”, Astronomy and Astrophysics, vol. 590, 2016. doi:10.1051/0004-6361/201527013. [99]Predehl, P., “eROSITA on SRG”, in X-ray Astronomy 2009; Present Status, Multi-Wavelength Approach and Future Perspectives, 2010, vol. 1248, pp. 543–548. doi:10.1063/1.3475336. [100]Vignali, C., “The XMM deep survey in the CDF-S. IX. An X-ray outflow in a luminous obscured quasar at z ≈ 1.6”, ¨C102C, vol. 583, 2015. doi:10.1051/0004-6361/201525852. [101]Branchesi, M., Gioia, I. M., Fanti, C., Fanti, R., and Cappelluti, N., “Chandra point-source counts in distant galaxy clusters”, ¨C103C, vol. 462, no. 2, pp. 449–458, 2007. doi:10.1051/0004-6361:20066196. [102]Allevato, V., “The Chandra COSMOS Legacy Survey: Clustering of X-Ray-selected AGNs at 2.9 ≤ z ≤ 5.5 Using Photometric Redshift Probability Distribution Functions”, ¨C104C, vol. 832, no. 1, 2016. doi:10.3847/0004-637X/832/1/70. [103]LaMassa, S. 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