# Planck 2013 results - VIII. HFI photometric calibration and mapmaking

@article{Ade2014Planck2R, title={Planck 2013 results - VIII. HFI photometric calibration and mapmaking}, author={P. C. P. Ade and N. Aghanim and C. Armitage-Caplan and M. Arnaud and M. Ashdown and F. Atrio-Barandela and J. Aumont and C. Baccigalupi and A. Banday and R. B. Barreiro and E. Battaner and K. Benabed and A. Benoit and A. Benoit-levy and J. Bernard and M. Bersanelli and B. Bertincourt and P. Bielewicz and J. Bobin and J. Bock and J. R. Bond and J. Borrill and F. Bouchet and F. Boulanger and M. Bridges and M. Bucher and C. Burigana and J. Cardoso and A. Catalano and A. Challinor and A. Chamballu and R. Chary and X. Chen and L. Chiang and H. Chiang and P. Christensen and S. Church and D. Clements and S. Colombi and L. Colombo and C. Combet and F. Couchot and A. Coulais and B. P. Crill and A. Curto and F. Cuttaia and L. Danese and R. Davies and P. Bernardis and A. Rosa and G. Zotti and J. Delabrouille and J. Delouis and F. D{\'e}sert and C. Dickinson and J. Diego and H. Dole and S. Donzelli and O. Dor'e and M. Douspis and X. Dupac and G. Efstathiou and T. A. Ensslin and H. Eriksen and C. Filliard and F. Finelli and O. Forni and M. Frailis and E. Franceschi and S. Galeotta and K. Ganga and M. Giard and G. Giardino and Y. Giraud-H'eraud and J. Gonz{\'a}lez-Nuevo and K. G{\'o}rski and S. Gratton and A. Gregorio and A. Gruppuso and F. Hansen and D. Hanson and D. Harrison and G. Helou and S. Henrot-Versill'e and C. Hernandez-Monteagudo and D. Herranz and S. Hildebrandt and E. Hivon and M. Hobson and W. Holmes and A. Hornstrup and W. Hovest and K. Huffenberger and T. Jaffe and A. Jaffe and W. Jones and M. Juvela and E. Keihanen and R. Keskitalo and T. Kisner and R. Kneissl and J. Knoche and L. Knox and M. Kunz and H. Kurki-Suonio and G. Lagache and J. Lamarre and A. Lasenby and R. Laureijs and C. Lawrence and M. L. Jeune and E. Lellouch and R. Leonardi and C. Leroy and J. Lesgourgues and M. Liguori and P. Lilje and M. Linden-Vornle and M. L{\'o}pez-Caniego and P. Lubin and J. Mac'ias-P'erez and B. Maffei and N. Mandolesi and M. Maris and D. P. Marshall and P. Martin and E. Martinez-Gonzalez and S. Masi and S. Matarrese and F. Matthai and L. Maurin and P. Mazzotta and P. McGehee and P. Meinhold and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and S. Mitra and M. Miville-Desch{\^e}nes and A. Moneti and L. Montier and R. Moreno and G. Morgante and D. Mortlock and D. Munshi and J. A. Murphy and P. Naselsky and F. Nati and P. Natoli and C. B. Netterfield and H. N{\o}rgaard-Nielsen and F. Noviello and D. Novikov and I. Novikov and S. Osborne and C. A. Oxborrow and F. Paci and L. Pagano and F. Pajot and R. Paladini and D. Paoletti and B. Partridge and F. Pasian and G. Patanchon and O. Perdereau and L. Perotto and F. Perrotta and F. Piacentini and M. Piat and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and N. Ponthieu and L. Popa and T. Poutanen and G. W. Pratt and G. Prezeau and S. Prunet and J. Puget and J. Rachen and M. Reinecke and M. Remazeilles and C. Renault and S. Ricciardi and T. Riller and I. Ristorcelli and G. Rocha and C. Rosset and G. Roudier and B. Rusholme and D. Santos and G. Savini and E. Shellard and L. Spencer and J. Starck and V. Stolyarov and R. Stompor and R. Sudiwala and R. Sunyaev and F. Sureau and D. Sutton and A. Suur-Uski and J. Sygnet and J. A. Tauber and D. Tavagnacco and S. T{\'e}chen{\'e} and L. Terenzi and M. Tomasi and M. Tristram and M. Tucci and G. Umana and L. Valenziano and J. Valiviita and B. Tent and P. Vielva and F. Villa and N. Vittorio and L. A. Wade and B. Wandelt and D. Yvon and A. Zacchei and A. Zonca}, journal={Astronomy and Astrophysics}, year={2014}, volume={571}, pages={1-25} }

This paper describes the methods used to produce photometrically calibrated maps from the Planck High Frequency Instrument (HFI) cleaned, time-ordered information. HFI observes the sky over a broad range of frequencies, from 100 to 857 GHz. To obtain the best calibration accuracy over such a large range, two different photometric calibration schemes have to be used. The 545 and 857 GHz data are calibrated by comparing flux-density measurements of Uranus and Neptune with models of their… CONTINUE READING

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