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Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters

Planck 2015 results: V. LFI calibration

Planck 2015 results: II. Low Frequency Instrument data processings

Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope-Zeldovich (SZ) sources with the Russian-Turkish 1.5 m telescope (RTT150), as a part of the optical follow

Planck intermediate results: XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories

Planck 2015 results: XII. Full focal plane simulations

Planck intermediate results: III. the relation between galaxy cluster mass and Sunyaev-Zeldovich signal âWe examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal

Planck intermediate results: X. Physics of the hot gas in the Coma cluster

Planck intermediate results: XI. the gas content of dark matter halos: The sunyaev-zeldovich-stellar mass relation for locally brightest galaxies the mean SZ signal down to M500 ∼ 2 × 1011 M⊙, with a clear indication of signal at even lower stellar mass

Planck intermediate results: VIII. Filaments between interacting clusters

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