Planck intermediate results

@inproceedings{Ade2018PlanckIR,
  title={Planck intermediate results},
  author={Peter A. R. Ade and Nabila Aghanim and Francisco Arg{\"u}eso and M. Arnaud and Mark Ashdown and Fernando Atrio-Barandela and J. Aumont and Carlo Baccigalupi and Amedeo Balbi and Anthony J. Banday and Rita Bel{\'e}n Barreiro and Eduardo Battaner and Karim Benabed and Alain Beno{\^i}t and J. Bernard and M. Bersanelli and Matthieu B{\'e}thermin and Rajendra Bhatia and Anna Bonaldi and J. Richard Bond and Julian Borrill and François R. Bouchet and C. Burigana and Paolo Cabella and J I Cardoso and Allison Catalano and Laura Cay{\'o}n and A. Chamballu and R. Prasanth Chary and Xuhui Chen and L. Chiang and P. R. Christensen and D L Clements and Sergio Colafrancesco and St{\'e}phane Colombi and Loris P. L. Colombo and A. Coulais and Brendan P. Crill and F. Cuttaia and Luigi Danese and Richard J. Davis and Paolo de Bernardis and Giancarlo de Gasperis and G. de Zotti and Jacques Delabrouille and Caitlin Dickinson and Jos{\'e} Miguel De Diego and Herv{\'e} Dole and Simona Donzelli and Olivier Dor{\'e} and U. D{\"o}rl and Marian Douspis and Xavier Dupac and George P. Efstathiou and Torsten A. Ensslin and Hans Kristian Eriksen and Fabio Finelli and Olivier Forni and Pablo Fosalba and Marco Frailis and Enrico Franceschi and S. Galeotta and Ken Ganga and Martin Giard},
  year={2018}
}
We make use of the Planck all-sky survey to derive number counts and spectral indices of extragalactic sources – infrared and radio sources – from the Planck Early Release Compact Source Catalogue (ERCSC) at 100 to 857 GHz (3 mm to 350 μm). Three zones (deep, medium and shallow) of approximately homogeneous coverage are used to permit a clean and controlled… CONTINUE READING