Dictionary of Nomenclature of Celestial Objects
(Last update: 21-Jan-2022)

Result of query: info cati XDCP J0338.7+0030$


Details on Acronym:   XDCP
   XDCP (XMM-Newton Distant Cluster Project) Write:<<XDCP JHHMM.m+DDMM>>
<<XDCP XHHMMa>> (not recognised by Simbad, but found in literature) N: about 100 Object:(X) + Cluster of G  (SIMBAD class: ClG = Cluster of Galaxies) Note:The XMM-Newton Distant Cluster Project (XDCP) is a serendipitous survey for distant (z>0.8) X-ray luminous galaxy clusters based in XMM-Newton archival data.
http://www.xray.mpe.mpg.de/theorie/cluster/XDCP/xdcp_index.html Ref:=2011NJPh...13l5014F byFASSBENDER R. , BOEHRINGER H., NASTASI A., SUHADA R., MUEHLEGGER M., DE HOON A., KOHNERT J., LAMER G., MOHR J.J., PIERINI D., PRATT G.W., QUINTANA H., ROSATI P., SANTOS J.S., SCHWOPE A.D. NJPh, 13l, 5014 (2011) The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project. oTable 5: <XDCP JHHMM.m+DDMM> N=17. Ref:=2011A&A...527L..10F byFASSBENDER R. , NASTASI A., BOEHRINGER H., SUHADA R., SANTOS J.S., ROSATI P., PIERINI D., MUEHLEGGER M., QUINTANA H., SCHWOPE A.D., LAMER G., DE HOON A., KOHNERT J., PRATT G.W., MOHR J.J. Astron. Astrophys., 527L, 10-10 (2011) The X-ray luminous galaxy cluster XMMU J1007.4+1237 at z = 1.56. The dawn of starburst activity in cluster cores. oText: <XDCP J1007.4+1237> N=1. Fig. 1, Table 1: <[FNB2011] N> (Nos 1-4). Ref:=2011A&A...530A.110S bySUHADA R. , FASSBENDER R., NASTASI A., BOEHRINGER H., DE HOON A., PIERINI D., SANTOS J.S., ROSATI P., MUEHLEGGER M., QUINTANA H., SCHWOPE A.D., LAMER G., KOHNERT J., PRATT G.W. Astron. Astrophys., 530A, 110-110 (2011) Exploring the galaxy cluster-group transition regime at high redshifts. Physical properties of two newly detected z > 1 systems. oParagr. 3.3: XMMU J0338.8-0030 is a msiprint for XMMU J0338.7+0030. oText: <XDCP JHHMM.m+DDMM> (Nos J0302.2-0001, J1532.2-0836). Table 3: <[SFN2011] XMMU JHHMM.m+DDMM N> (Nos XMMU J0302.2-0001 1 to 6, XMMU J1532.2-0836 1 to 3). Appendix A: <[SFN2011] XMMU J0302.1-0000> N=1. Ref:=2011A&A...532L...6N byNASTASI A. , FASSBENDER R., BOEHRINGER H., SUHADA R., ROSATI P., PIERINI D., VERDUGO M., SANTOS J.S., SCHWOPE A.D., DE HOON A., KOHNERT J., LAMER G., MUEHLEGGER M., QUINTANA H. Astron. Astrophys., 532L, 6-6 (2011) Discovery of the X-ray selected galaxy cluster XMMU J0338.8+0021 at z = 1.49. Indications of a young system with a brightest galaxy in formation. o<XDCP J0338.8+0021> N=1. Fig. 1, Table 2: <[NFB2011] N-A> (Nos 1-A), <[NFB2011] NN> (Nos 4 to 7, 11, 14). MPI for extraterrestrial Physics (MPE) Originof the Acronym: p = Pre-registered to IAU Comm.5

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