Observing planet-driven dust spirals with ALMA

<b>Dataset and image gallery </b>supplementing the publication:Speedie, J., Booth R.A. &amp; Dong, R. (2022). Observing Planet-driven Dust Spirals with ALMA. <i>ApJ</i>, 930:40 (22pp).<br>--------------------------------------------------------------------------------<b>data.zip</b> contains fits files of synthetic ALMA Band 7 continuum observations [mJy/beam].<b>image.gallery.zip</b> contains a ready-made visualization of everything in <b>data.zip</b>: an image gallery (and quicklook movies) of disk images [mJy/beam] and residual maps [S/N]Loose<b> *.mp4 files </b>are also present in <b>image.gallery.zip</b>.<br>The following model permutations are available:1. <b>Face-on</b> disks:<b>x2</b> equation of state (isothermal, adiabatic with beta=10)<b>x3</b> planet mass (0.3, 1.0 and 3.0 thermal masses)<b>x4</b> disk optical depth (0.1, 0.3, 1.0, 3.0 initial tau at Rp)<b>x6</b> requested observing sensitivity (10, 15, 20, 25, 30, 35 uJy/beam)<b>x3</b> antenna configuration pairs (C43-4 + C43-7, C43-5 + C43-8, C43-6 + C43-9)<b>= 432</b> synthetic ALMA Band 7 continuum images (+24 model dust continuum emission maps that served as input [Jy/arcsec2])<br>2. <b>Inclined</b> disks:<b>x1</b> equation of state (adiabatic with beta=10)<b>x1</b> planet mass (1.0 thermal masses)<b>x4</b> disk optical depth (0.1, 0.3, 1.0, 3.0 initial tau at Rp)<b>x3</b> disk inclinations (30, 50 and 70 degrees)<b>x2</b> planet position angle (on major axis, on minor axis)<b>x6</b> requested observing sensitivity (10, 15, 20, 25, 30, 35 uJy/beam)<b>x1</b> antenna configuration pairs (C43-5 + C43-8)<b>= 144</b> synthetic ALMA Band 7 continuum images---------------------------------------------------------------------------------When you make use of material from this repository, please acknowledge:Speedie, J., Booth R.A. &amp; Dong, R. (2022). Observing Planet-driven Dust Spirals with ALMA. <i>ApJ</i>, 930:40 (22pp).