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Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts

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Lutz,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Pérez-González, P. G., Egami, E., Rex, M., Rawle, T. D., Kneib, J.-P., Richard, J., Johansson, D., Altieri, B., Blain, A. W., Bock, J. J., Boone, F., Bridge, C. R., Chung, S. M., Clément, B., Clowe, D., Combes, F., Cuby, J.-G., Dessauges-Zavadsky, M., Dowell, C. D., Espino-Briones, N., Fadda, D., Fiedler, A. K., Gonzalez, A., Horellou, C., Ilbert, O., Ivison, R. J., Jauzac, M., Lutz, D., Pelló, R., Pereira, M. J., Rieke, G. H., Rodighiero, G., Schaerer, D., Smith, G. P., Valtchanov, I., Walth, G. L., van der Werf, P., Werner, M. W., & Zemcov, M. (2010). Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts. Astronomy & Astrophysics, 518:, pp. 1-5. doi:10.1051/0004-6361/201014593.


引用: https://hdl.handle.net/11858/00-001M-0000-0010-929A-8
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