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The XXL survey currently covers two 25 deg2 patches with XMM observations of ∼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 < 2) cluster, (z < 4) active galactic nuclei (AGN), and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi-λ observations, will lead to solid standalone cosmological constraints and provide a wealth of information on the formation and evolution of AGN, clusters, and the X-ray background. In particular, it will offer a unique opportunity to pinpoint the z > 1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions.

Pierre, M., Adami, C., Birkinshaw, M., Chiappetti, L., Ettori, S., Evrard, A., et al. (2017). The XXL survey: First results and future. ASTRONOMISCHE NACHRICHTEN, 338(2-3), 334-341 [10.1002/asna.201713352].

The XXL survey: First results and future

Pierre, M;Adami, C.;Birkinshaw, M.;Chiappetti, L.;Ettori, S.;Evrard, A.;Faccioli, L.;Gastaldello, F.;Giles, P.;Horellou, C.;Iovino, A.;Koulouridis, E.;Lidman, C.;Le Brun, A.;Maughan, B.;Maurogordato, S.;Mccarthy, I.;Miyazaki, S.;Pacaud, F.;Paltani, S.;Plionis, M.;Reiprich, T.;Sadibekova, T.;Smolcic, V.;Snowden, S.;Surdej, J.;Tsirou, M.;VIGNALI, CRISTIAN;Willis, J.;Alis, S.;Altieri, B.;Baran, N.;Benoist, C.;Bongiorno, A.;Bremer, M.;Butler, A.;Cappi, A.;Caretta, C.;Ciliegi, P.;Clerc, N.;Corasaniti, P. S.;Coupon, J.;Delhaize, J.;DELVECCHIO, IVAN;Democles, J.;Desai, S.h.;Devriendt, J.;Dubois, Y.;Eckert, D.;ELYIV, ANDRII;Farahi, A.;Ferraril, C.;Fotopoulou, S.;Forman, W.;Georgantopoulos, I.;Guglielmo, V.;Huynh, M.;Jerlin, N.;Jones, C.h.;Lavoie, S.;Le Fevre, J. P.;Lieu, M.;Kilbinger, M.;MARULLI, FEDERICO;Mantz, A.;Mcgee, S.;Melin, J. B.;Melnyk, O.;MOSCARDINI, LAURO;Novak, M.;Piconcelli, E.;Poggianti, B.;Pomarede, D.;Pompei, E.;Ponman, T.;Ramos Ceja, M. E.;Rana, P.;Rapetti, D.;Raychaudhury, S.;Ricci, M.;Rottgering, H.;Sahlen, M.;Sauvageot, J. L.;Schimd, C.;SERENO, MAURO;Smith, G. P.;Umetsu, K.;Valageas, P.;Valotti, A.;Valtchanov, I.;VEROPALUMBO, ALFONSO;Ascaso, B.;Barnes, D.;De Petris, M.;Durret, F.;Donahue, M.;Ithana, M.;Jarvis, M.;Johnston Hollitt, M.;Kalfountzou, E.;Kay, S.;La Franca, F.;Okabe, N.;Muzzin, A.;Rettura, A.;Ricci, F.;Ridl, J.;Risaliti, G.;Takizawa, M.;Thomas, P.;Truong, N.

2017

Abstract

The XXL survey currently covers two 25 deg2 patches with XMM observations of ∼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 < 2) cluster, (z < 4) active galactic nuclei (AGN), and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi-λ observations, will lead to solid standalone cosmological constraints and provide a wealth of information on the formation and evolution of AGN, clusters, and the X-ray background. In particular, it will offer a unique opportunity to pinpoint the z > 1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions.

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	Anno
	
				2017
			
	Rivista
	
				ASTRONOMISCHE NACHRICHTEN
			
	Codice DOI
	
				https://dx.doi.org/10.1002/asna.201713352
			
	Citazione
	
				Pierre, M., Adami, C., Birkinshaw, M., Chiappetti, L., Ettori, S., Evrard, A., et al. (2017). The XXL survey: First results and future. ASTRONOMISCHE NACHRICHTEN, 338(2-3), 334-341 [10.1002/asna.201713352].
			
	Tutti gli autori
	
				Pierre, M; Adami, C.; Birkinshaw, M.; Chiappetti, L.; Ettori, S.; Evrard, A.; Faccioli, L.; Gastaldello, F.; Giles, P.; Horellou, C.; Iovino, A.; Koulouridis, E.; Lidman, C.; Le Brun, A.; Maughan, B.; Maurogordato, S.; Mccarthy, I.; Miyazaki, S.; Pacaud, F.; Paltani, S.; Plionis, M.; Reiprich, T.; Sadibekova, T.; Smolcic, V.; Snowden, S.; Surdej, J.; Tsirou, M.; Vignali, C.; Willis, J.; Alis, S.; Altieri, B.; Baran, N.; Benoist, C.; Bongiorno, A.; Bremer, M.; Butler, A.; Cappi, A.; Caretta, C.; Ciliegi, P.; Clerc, N.; Corasaniti, P.S.; Coupon, J.; Delhaize, J.; Delvecchio, I.; Democles, J.; Desai, Sh.; Devriendt, J.; Dubois, Y.; Eckert, D.; Elyiv, A.; Farahi, A.; Ferraril, C.; Fotopoulou, S.; Forman, W.; Georgantopoulos, I.; Guglielmo, V.; Huynh, M.; Jerlin, N.; Jones, Ch.; Lavoie, S.; Le Fevre, J.-P.; Lieu, M.; Kilbinger, M.; Marulli, F.; Mantz, A.; Mcgee, S.; Melin, J.-B.; Melnyk, O.; Moscardini, L.; Novak, M.; Piconcelli, E.; Poggianti, B.; Pomarede, D.; Pompei, E.; Ponman, T.; Ramos Ceja, M.E.; Rana, P.; Rapetti, D.; Raychaudhury, S.; Ricci, M.; Rottgering, H.; Sahlen, M.; Sauvageot, J.-L.; Schimd, C.; Sereno, M.; Smith, G.P.; Umetsu, K.; Valageas, P.; Valotti, A.; Valtchanov, I.; Veropalumbo, A.; Ascaso, B.; Barnes, D.; De Petris, M.; Durret, F.; Donahue, M.; Ithana, M.; Jarvis, M.; Johnston-Hollitt, M.; Kalfountzou, E.; Kay, S.; La Franca, F.; Okabe, N.; Muzzin, A.; Rettura, A.; Ricci, F.; Ridl, J.; Risaliti, G.; Takizawa, M.; Thomas, P.; Truong, N.
			
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/588059

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