An excess of emission in the dark cloud LDN1111 with the Arcminute Microkelvin Imager[starf by Consortium, AMI, Scaife, AMM, Hurley-Walker, N, Green, DA, Davies, M L, Grainge, KJB, Hobson, M P, Lasenby, AN, Lopez-Caniego, M, Pooley, G G, Saunders, RDE, Scott, P F, Titterington, D J, Waldram, E M, Zwart, JTL

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The Arcminute Microkelvin Imagera by Zwart, JTL, Barker, R W, Biddulph, P, Bly, D, Boysen, R C, Brown, A R, Clementson, C, Crofts, M, Culverhouse, T L, Czeres, J, Dace, R J, Davies, M L, D'Alessandro, R, Doherty, P, Duggan, K, Ely, JA, Felvus, M, Feroz, F, Flynn, W, Franzen, TMO, Geisbuesch, J, Genova-Santos, R, Grainge, KJB, Grainger, W F, Hammett, D, Hills, R E, Hobson, M P, Holler, C M, Hurley-Walker, N, Jilley, R, Jones, ME, Kaneko, T, Kneissl, R, Lancaster, K, Lasenby, AN, Marshall, P J, Newton, F, Norris, O, Northrop, I, Odell, D M, Petencin, G, Pober, J C, Pooley, G G, Pospieszalski, M W, Quy, V, Rodriguez-Gonzalvez, C, Saunders, RDE, Scaife, AMM, Schofield, J, Scott, P F, Shaw, C, Shimwell, T W, Smith, H, Taylor, A C, Titterington, D J, Velic, M, Waldram, E M, West, S, Wood, BA, Yassin, G

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