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, C.; Willis, J.; Alis, Sinan; Altieri, B.; Baran, N.; Benoist, C.; Bongiorno, A.; Bremer, M.; Butler, A.; Cappi, A.; Caretta, C.; Ciliegi, P.; Clerc, N.; Corasaniti, P.; 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.; Lieu, M.; Kilbinger, M.; MaruIli, F.; Mantz, A.; McGee, S.; Melin, J.; Melnyk, O.; Moscardini, L.; Novak, M.; Piconcelli, E.; Poggianti, B.; Pomarede, D.; Pompei, E.; Ponman, T.; Ceja, M.; Rana, P.; Rapetti, D.; Raychaudhury, S.; Ricci, M.; Rottgering, H.; Sahlen, M.; Sauvageot, J.; Schimd, C.; Sereno, M.; Smith, G.; 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.

doi:10.1002/asna.201713352

The XXL survey: First results and future

Atıf İçin Kopyala

Pierre M., Adami C., Birkinshaw M., Chiappetti L., Ettori S., Evrard A., ...Daha Fazla

ASTRONOMISCHE NACHRICHTEN, cilt.338, ss.334-341, 2017 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 338
Basım Tarihi: 2017
Doi Numarası: 10.1002/asna.201713352
Dergi Adı: ASTRONOMISCHE NACHRICHTEN
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.334-341
Anahtar Kelimeler: X-ray: general, cosmological parameters, galaxies: clusters: general, galaxies: active, TEMPERATURE RELATION, CLUSTER
İstanbul Üniversitesi Adresli: Evet

Özet

The 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 < 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-lambda 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.