We provide download links to fits files containing our <i>y</i> maps created from our NILC on Planck NPIPE data presented in
<a href="https://arxiv.org/abs/2307.01043">McCarthy and Hill (2023) I</a> and <a href="https://arxiv.org/abs/2308.16260">McCarthy and Hill (2023) II</a>. Please refer to paper I for detailed descriptions of the maps. Note that all maps are convolved with a 10 arcminute beam. We provide ILC maps created with three different frequency coverage specification; in all cases, we use all the low-frequency channels of the  <i>Planck</i> instrument (30, 44, 70) GHz, and the (100, 143, 217, 353) GHz channels of the high-frequency instrument. Additionally, our ``standard frequency coverage'' specification includes 545 GHz. We also include maps made with all of these frequencies and the 857 GHz information, as well as separate maps made without the 545 GHz information (these maps also do not include the 857 GHz information).
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We provide <i>y</i> maps made both with the full season maps and with two independent Ring-half splits. 
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We also provide several different configurations for the deprojected foregrounds, in particular the CMB; the CIB; and the first moments of the CIB's SED; see <a href="https://arxiv.org/abs/2307.01043">McCarthy and Hill (2023) I</a> and  <a href="https://arxiv.org/abs/2308.16260">McCarthy and Hill (2023) II</a> for the details of the different components we deproject. 
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Unless otherwise noted, all CIB (and CIB-moment) deprojections are done with a default modified-black-body SED with the parameters beta = 1.7 and T = 10.71 K. We also provide our CIB deprojections with beta = 1.2 and T = 24 K. Maps with different SEDs deprojected can be very easily provided upon request (send me an email!)
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The code used to create these maps is publically available: <a href="https://github.com/jcolinhill/pyilc">https://github.com/jcolinhill/pyilc</a>.

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<a href="./ymap_standard/">Standard frequency coverage: Including 545 GHz, no 857 GHz</a>
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<a href="./ymap_no545/">No 545 GHz (also no 857 GHz)</a>
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<a href="./ymap_with857/">Plus 857 GHz (including 545 and 857 GHz)</a>
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Additionally, we provide our inpainted, monopole- and dipole-subtracted single frequency maps. We created these by downloading the NPIPE single frequency maps; subtracting the kinematic dipole as provided by the NPIPE release; subtracting the remaining monopole from each map(*); and masking a small region of each map close to the galactic plane, along with the point sources; and iteratively inpainting the masked regions with our diffusive_inpaint code that replaces masked regions with the mean of the unmasked neighbouring pixels. As we provide the masks (in the Masks) folder, and make our diffusive_inpaint code public, these steps should be reproducible, however we include the maps here as they may be useful to anyone who wants to use pyilc to isolate any components that we have not released.
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<a href="./masks/">Masks</a>
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<a href="./inpainted_input_maps/">Inpainted input maps</a>
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email me: fiona dot mccarthy 0 at gmail dot com 
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Visit <a href="https://fionamccarthy0.wixsite.com/fionamccarthy">my website</a>
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