Downloading and Formatting Data

Guide To Downloading and Formatting Pierre Auger Observatory Data


NOTE: This set of instructions was created using a PC running Microsoft Excel 2007. Some of these instructions will likely be different for Mac users

  1. Go to Event Display
  2. In this page there are several ways to view event data. The way you choose to display this data depends largely on what you wish to accomplish with it. This guide is focused on the use of data for ALL EVENTS
  1. To download data on all events you must click on the ascii file link on the second paragraph. This will download a .txt file containing data for every public event since January 1st 2004. The file should look something like this:

The data may be analyzed using any software of your choosing. Microsoft Excel is a reasonably good choice. The following steps describe how to copy all the data to an Excel File.

  1. Open Microsoft Excel click on the office icon , click and choose the .txt file from the location in which you saved it.
  2. Choose Delimited, since the data fields are separated by spaces in the text file.

  1. Click
  2. In the next screen deselect “Tab” and select “Space”. This will tell Excel to interpret information separated by spaces as separate columns.

In this same window Excel will show a small preview of what the data will look like. Scroll down in this preview window to make sure your data are organized correctly. If your data look as shown in this picture it should be ok

  1. Click and select “General” in the following screen then click

  1. Your data should be neatly organized in a spreadsheet. You’ll notice that the data columns are not directly labeled. What you have is a legend at the top identifying each “field”. Each “field” is essentially a column. If you wish to simplify reading the data you may label the columns directly.

What the data labels mean

  1. Event ID – Every time an event is recorded it is assigned it’s own identification number to help distinguish it from the rest
  2. Number of stations in event – when a cosmic ray produces a shower it “hits” a number of stations in the Auger array of stations.
  3. Theta of incoming cosmic ray– zenith angle
  4. Phi of incoming cosmic ray– azimuth angle
  5. Reconstructed Energy – energy of the original particle that caused the shower in EeV.
  6. Unix time – time elapsed in seconds from January 1st 1970 at 12:00 am to the moment the event was recorded.
  7. Galactic Longitude and Latitude – direction of the original cosmic ray with respect to the Milky Way Plane

Observatorio Pierre Auger
Av. San Martín Norte 304
Malargüe, Mendoza, Argentina

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