ggl | Google from command line | Command Line Interface library

For the login action use the below xpaths. This way your code will look neat.

I think you're close. IMHO, this scatter plot is easier than plotting with both skyplot coordinates (projection="aitoff"). The process is similar to the answers I posted on your earlier question: Plot mean and standard dev values on skyplot using astropy from hdf5 file. You just need some minor teaks to the function parameters.

I modified your code to create a 2D scatter plot. Here's a quick summary of the differences:

• Changed from astropy.coordinates import SkyCoord (instead of HEALPix)
• Changed matplot type (removeprojection=)
• Changes y-variable from b_rad to faraday_sky_mean on scatter plot.
• Deleted c=faraday_sky_mean from plt.scatter() so data points are not color coded.

See code below.

The second approach is not faster and is harder to implement, as each container is loaded separately and starts to reload after the first load is done. It looks like a nightmare to automate.

I tried Selenium's explicit waits and time.sleep() neither of the approached worked. The code below clicks the button, switches to a new iframe and tries to get containers content. But the content is almost always empty for the reasons described above.

With Selenium I'd use css selector:

driver.find_elements_by_css_selector(".svg--1nrnH")

Update for Selenium: wait for iframe. This is the reason why element could not be found.

I see why you are having problems plotting this data. The data in the linked file (faraday2020.hdf5) is only the mean and standard deviation of the reconstructed Faraday sky. See this note on the linked page: "All maps are presented in Galactic at a HEALPix resolution of Nside=512 and are stored in RING ordering scheme. The units are rad/m2." In other words, you need to get the skyplot coordinates from another source.

A little Googling found the coordinates on the NASA Goddard LAMBDA-Tools site: HEALPix Pixel Coordinates. Specifically, you want this file for NSide=512 / Galactic / Ring Pixel Ordering: pixel_coords_map_ring_galactic_res9.fits

So, first problem solved. Next you need to read the FITS formatted file to get the coordinates. Astropy has the 'fits' module to do that. See code below.

There is no difference, current_branch is a compatibility alias for git_current_branch. See the code.

in the query's response function, you can get the data from the response argument.

I believe a series argument is treated like a dicitonary with index being keys. The dictionary option is now available for just DataFrame. For Series, a dict to_replace means something else (k:v means replace value k with value v).

Quick fix: turn your df['strip_me'] into a dataframe with:

There are multiple ways to scroll down on web page. Currently ifrane is present on your web page you need to swwitch control to iframe before scrolling try below code section for your ref:

1. you can also use this to scroll down to the bottom of the page.