search

samvanleeuwen / Veil_project

0 stars 0 forks source link

Communication channel log #1

Open samvanleeuwen opened 5 months ago

MilanBom commented 5 months ago

Hallo

EldodeGraaf commented 5 months ago

Test

EldodeGraaf commented 5 months ago

Communications week 1:

Monday: Start of the project, all 3 at the introduction from 9 till 15. Worked in the team setting for the first time and sorted things out and looked at possible useful things + planning and organization.

Tuesday: Introduction to astronomy 9-13, planned a meeting with the TA for Wednesday at 14 to discuss the progress that we had made. Planned a Meeting with the prof at Thursday 10. Due to the resit of calculus II for 2 team members later that afternoon, there wasn't much done outside of work/lecture apart from distributing tasks for the next day.

Wednesday: Chose to meet at 10, where we would work on the compressing of the data gathered at the observation nights. (Because the program is only for windows) Milan and Eldo started analysing the data and Sam looked at possible subjects and articles about the particular supernova that we observed. Later that day we had the meeting with Omar (TA) about the progress made so far and about a possible subject. The result of the meeting was that we were on the right track and just needed to finish compressing the data before the end of the day. However the subject was still a bit unclear. Finished the data stacking/compressing and prepared the meeting with the prof for the next day.

Thursday: Had the meeting with the prof at 10 which gave us some good insights in the next steps of the project. One of the possible subjects was ruled out and we picked some data of existing databases to compare with. After the meeting was finished we knew what was expected and made a plan of subjects to do till the next meeting. This includes: Research question, further data analysis, programming, to apply feedback and finally prepare the next meeting. After this discussion once again there were resits for 2 team members later that afternoon, so the work done later in the day was minimal.

Friday: Working from home and finishing some things, applying feedback.

samvanleeuwen commented 5 months ago

Communications week 2:

Monday: Sam and Milan worked at the project from 11 till 16. We corrected our feedback from the last meeting and tried to make the code work to sync the data from Skyview with our own data. We didn't complete this because we had some difficulties with the code. At 16 Eldo arrived and we prepared everything for the next meeting and tried to make the program work.

Tuesday: Everyone worked from home.

EldodeGraaf commented 5 months ago

Taken:

Sam: meeting 3 minutes en overleaf invullen Milan: plaatje voor poster gereed maken en referenties--> waarom dit resultaat goed? --richting (deel van: inleiding, resultaten conclusie) en meer in overleg Eldo: Resultaten en deel conclusie en meer =overleaf invullen Sam: layout, inleiding en meer in overleg

samvanleeuwen commented 5 months ago

Punten voor poster:

samvanleeuwen commented 5 months ago

script animation: If a star is at the end of its life span and has a mass of more than eight times the sun it's can go supernova. This explosion can create shockwaves. These waves have a great amount of energy that can collide with the remnants of the star. These high energy waves ionize the elements and create O(III). If the elements slow and cool down there doesn't take place anymore ionizing. These elements give off H-alfa radiation. With these knowns you can determine the direction of the shockwaves.

samvanleeuwen commented 5 months ago

If a star is at the end of its life span and has a mass of more than eight times the sun it can go supernova. This explosion can create shockwaves. These waves have a great amount of energy that can collide with the remnants of the star. These high energy waves ionize the elements and create O(III). If the elements lose their energy and slowdown there doesn't take anymore ionizing place. Therefore the elements will give off H-alfa radiation instead of O(III). The radiation of the O(III) shows where the wave has high speed witch is where the front of the wave will be. With these knowns you can determine the direction of the shockwaves by localizing the front and back of the shockwave. To know the direction of the shock waves is important for the evolution of the super nova. Knowing the direction can help determine the origin of the star.