Basit öğe kaydını göster

The XXL survey: First results and future

dc.contributor.authorAltieri, B.
dc.contributor.authorUmetsu, K.
dc.contributor.authorValageas, P.
dc.contributor.authorValotti, A.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVeropalumbo, A.
dc.contributor.authorAscaso, B.
dc.contributor.authorBarnes, D.
dc.contributor.authorDe Petris, M.
dc.contributor.authorDurret, F.
dc.contributor.authorDonahue, M.
dc.contributor.authorIthana, M.
dc.contributor.authorJarvis, M.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorKalfountzou, E.
dc.contributor.authorKay, S.
dc.contributor.authorLa Franca, F.
dc.contributor.authorOkabe, N.
dc.contributor.authorMuzzin, A.
dc.contributor.authorRettura, A.
dc.contributor.authorRicci, F.
dc.contributor.authorRidl, J.
dc.contributor.authorRisaliti, G.
dc.contributor.authorTakizawa, M.
dc.contributor.authorThomas, P.
dc.contributor.authorTruong, N.
dc.contributor.authorAlis, Sinan
dc.contributor.authorIovino, A.
dc.contributor.authorKoulouridis, E.
dc.contributor.authorPierre, M.
dc.contributor.authorAdami, C.
dc.contributor.authorBirkinshaw, M.
dc.contributor.authorChiappetti, L.
dc.contributor.authorEttori, S.
dc.contributor.authorEvrard, A.
dc.contributor.authorFaccioli, L.
dc.contributor.authorGastaldello, F.
dc.contributor.authorGiles, P.
dc.contributor.authorHorellou, C.
dc.contributor.authorLidman, C.
dc.contributor.authorLe Brun, A.
dc.contributor.authorMaughan, B.
dc.contributor.authorMaurogordato, S.
dc.contributor.authorMcCarthy, I.
dc.contributor.authorMiyazaki, S.
dc.contributor.authorPacaud, F.
dc.contributor.authorPaltani, S.
dc.contributor.authorPlionis, M.
dc.contributor.authorReiprich, T.
dc.contributor.authorSadibekova, T.
dc.contributor.authorSmolcic, V.
dc.contributor.authorSnowden, S.
dc.contributor.authorSurdej, J.
dc.contributor.authorTsirou, M.
dc.contributor.authorVignali, C.
dc.contributor.authorWillis, J.
dc.contributor.authorBaran, N.
dc.contributor.authorBenoist, C.
dc.contributor.authorBongiorno, A.
dc.contributor.authorBremer, M.
dc.contributor.authorButler, A.
dc.contributor.authorCappi, A.
dc.contributor.authorCaretta, C.
dc.contributor.authorCiliegi, P.
dc.contributor.authorClerc, N.
dc.contributor.authorCorasaniti, P. S.
dc.contributor.authorCoupon, J.
dc.contributor.authorDelhaize, J.
dc.contributor.authorDelvecchio, I.
dc.contributor.authorDemocles, J.
dc.contributor.authorDesai, Sh
dc.contributor.authorDevriendt, J.
dc.contributor.authorDubois, Y.
dc.contributor.authorEckert, D.
dc.contributor.authorElyiv, A.
dc.contributor.authorFarahi, A.
dc.contributor.authorFerraril, C.
dc.contributor.authorFotopoulou, S.
dc.contributor.authorForman, W.
dc.contributor.authorGeorgantopoulos, I.
dc.contributor.authorGuglielmo, V.
dc.contributor.authorHuynh, M.
dc.contributor.authorJerlin, N.
dc.contributor.authorJones, Ch.
dc.contributor.authorLavoie, S.
dc.contributor.authorLe Fevre, J. -P.
dc.contributor.authorLieu, M.
dc.contributor.authorKilbinger, M.
dc.contributor.authorMaruIli, F.
dc.contributor.authorMantz, A.
dc.contributor.authorMcGee, S.
dc.contributor.authorMelin, J. -B.
dc.contributor.authorMelnyk, O.
dc.contributor.authorMoscardini, L.
dc.contributor.authorNovak, M.
dc.contributor.authorPiconcelli, E.
dc.contributor.authorPoggianti, B.
dc.contributor.authorPomarede, D.
dc.contributor.authorPompei, E.
dc.contributor.authorPonman, T.
dc.contributor.authorCeja, M. E. Ramos
dc.contributor.authorRana, P.
dc.contributor.authorRapetti, D.
dc.contributor.authorRaychaudhury, S.
dc.contributor.authorRicci, M.
dc.contributor.authorRottgering, H.
dc.contributor.authorSahlen, M.
dc.contributor.authorSauvageot, J. -L.
dc.contributor.authorSchimd, C.
dc.contributor.authorSereno, M.
dc.contributor.authorSmith, G. P.
dc.date.accessioned2021-03-04T10:25:47Z
dc.date.available2021-03-04T10:25:47Z
dc.identifier.citationPierre M., Adami C., Birkinshaw M., Chiappetti L., Ettori S., Evrard A., Faccioli L., Gastaldello F., Giles P., Horellou C., et al., "The XXL survey: First results and future", ASTRONOMISCHE NACHRICHTEN, cilt.338, ss.334-341, 2017
dc.identifier.issn0004-6337
dc.identifier.othervv_1032021
dc.identifier.otherav_6d302f9e-477e-4f87-aa9e-21762ee5869e
dc.identifier.urihttp://hdl.handle.net/20.500.12627/75432
dc.identifier.urihttps://doi.org/10.1002/asna.201713352
dc.description.abstractThe XXL survey currently covers two 25 deg(2) patches with XMM observations of similar to 10 ks. We summarize the scientific results associated with the first release of the XXL dataset, which occurred in mid-2016. We review several arguments for increasing the survey depth to 40 ks during the next decade of XMM operations. X-ray (z 1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe XXL survey: First results and future
dc.typeMakale
dc.relation.journalASTRONOMISCHE NACHRICHTEN
dc.contributor.departmentINAF OAB , ,
dc.identifier.volume338
dc.identifier.startpage334
dc.identifier.endpage341
dc.contributor.firstauthorID241622


Bu öğenin dosyaları:

DosyalarBoyutBiçimGöster

Bu öğe ile ilişkili dosya yok.

Bu öğe aşağıdaki koleksiyon(lar)da görünmektedir.

Basit öğe kaydını göster