Planetary and Space Science

Table S1: Supplementary dataset to "Obliquity dependence of the formation of the martian polar layered deposits". Sensitivity of annual net polar water and dust deposition on Mars to all tested MGCM source and obliquity conditions. Values are reported in mm/Earth year. Values are included for the present-day simulation (labelled “NRC”) and for the 55 paleoclimate simulations (prefixed “1.” - “11.”, corresponding to the water ice source configurations listed in section 4.2.) Version 2 notes: In the above data set description, the title of the associated article was updated to be the title of the accepted, final version of the manuscript. The tables in the data file now sequentially appear in the same order as the corresponding initial water ice source configurations listed in section 4.2: NRC (Present Day) 1. Simultaneous north and south polar caps (surface water ice poleward of 77.5 deg N/S) 2. A north polar cap (surface water ice northward of 77.5 deg N) only 3. A south polar cap (surface water ice southward of 77.5 deg S) only 4. Simultaneous north and south midlatitude sources (37.5 - 42.5 deg N/S) 5. Simultaneous north and south high latitude sources (57.5 - 62.5 deg N/S) 6. A northern midlatitude source (37.5 - 42.5 deg N) only 7. A northern high latitude source (57.5 - 62.5 deg N) only 8. A southern midlatitude source (37.5 - 42.5 deg S) only 9. A southern high latitude source (57.5 - 62.5 deg S) only 10. Simultaneous north and south polar caps and simultaneous north and south midlatitude sources (poleward of 77.5 deg N/S and 37.5 - 42.5 deg N/S) 11. Simultaneous north and south polar caps and simultaneous north and south high latitude sources (poleward of 77.5 deg N/S and 57.5 - 62.5 deg N/S)

Images of the shocked sample texture

These two excel data tables contain the reduced CODEX LARIMS data required to reproduce our Zagami isochron diagrams for February and September 2019 data acquisitions. Each excel file has a header explaining each column. Each spot measurement on Zagami is recorded as a row, with a filename to allow us to identify the original raw data if needed, the date acquired, the measurement position on the sample, the integrated peak areas, the 1-sigma standard error uncertainties, and correlation coefficients.

The excel file is broken into 3 categories: Insertion: The description of what hardware and settings were used for each test run and the processed results of each insertion test run. Extraction: The description of what settings were used for each extraction and the processed results for those runs. Run X-Y The raw data for the mapping of an ice surface (prior to each test run), insertion for each run, and extraction for each run (if performed).

Event_list.txt: List of events used in the statistical analysis section. G_correction_coefficients.txt: Tables of correction factors to the geometric factor of the RPC-IES electron sensor.

The .diam files are the creter diameters to be used with the software craterstats2 The olimpo_nocart.exe is the executable to calculate the water splash; input data are requested when running the code; the txt files should not be modified The runup_water_acheron6_pss is a small fortran code to calculate the run-up and velocity of the water wave with the analytical formula provided in the text

Sample video used when testing the convolutional neural network (CNN) on real data. The video is in a raw binary format (unit16 greyscale). To generate all the necessary training data for the CNN, over 2TB of data was processed to find samples, thus only a small segment is shown here.

This is DTM and Shapefiles for GIS software. CTX_DTM_P22_009658_2505_XI_70N093W.rar - The digital terrain model based on CTX images P22_009658_2505 and B01_009935_2505 with spatial resolution ~14 m/pix. The orthomosaic based on P22_009658_2505 CTX image. Crater_266, Crater_249 and Plain_95 folders consist of shapefiles цшер series of moraines in the crater A (70.3°N 266.45°E), crater B (67.25°N 249.45°E) and on the plain (74°N 95°E).

Geocentric radiants and heliocentric orbit of 2018 Draconid meteors

Comparison of different reported anaerobic growth and metal reduction experiments with Shewanella oneidensis. Used electron donors and acceptors are listed and important aspects of the experimental designs are noted. In some cases, reported parameters are combined to obtain missing values.