Now showing items 1-2 of 2

    • The Chandra COSMOS Survey III : Optical and infrared identification of X-ray point sources 

      Civano, F.; Elvis, M.; Aldcroft, T.; Fruscione, A.; Hao, H.; Lanzuisi, G.; Wright, N.J.; Brusa, M.; Salvato, M.; Bongiorno, A.; Comastri, A.; Zamorani, G.; Cappelluti, N.; Gilli, R.; Lusso, E.; Vignali, C.; Fiore, F.; Capak, P.; Scoville, N.Z.; Cisternas, M.; Kartaltepe, J.; Koekemoer, A. M.; Impey, C.D.; Trump, J.; Mainieri, V.; Miyaji, T.; Lilly, S.; Masters, D.; Puccetti, S.; Schawinski, K.; Urry, M.; Silverman, J. (2012-08-01)
      The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central 0.9 deg2 of the COSMOS field down to limiting depths of 1.9×10−16 erg cm−2 s−1 in the soft (0.5–2 keV) band, 7.3×10−16 ...
    • The Second Radio Synchrotron Background Workshop: Conference Summary and Report 

      Singal, J.; Fornengo, N.; Regis, M.; Bernardi, G.; Bordenave, D.; Branchini, E.; Cappelluti, N.; Caputo, A.; Carucci, I. P.; Chluba, J.; Cuoco, A.; DiLullo, C.; Fialkov, A.; Hale, C.; Harper, S. E.; Heston, S.; Holder, G.; Kogut, A.; Krause, M. G. H.; Leahy, J. P.; Mittal, S.; Monsalve, R. A.; Piccirilli, G.; Pinetti, E.; Recchia, S.; Taoso, M.; Todarello, E. (2023-03-20)
      We summarize the second radio synchrotron background workshop, which took place on 2022 June 15–17 in Barolo, Italy. This meeting was convened because available measurements of the diffuse radio zero level continue to ...