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Good tutorial 😁

Hello, I am currently pursuing MSc in Physics and Astronomy at NIT Rourkela. I have taken my research project on Solar physics and currently in 3rd semester. I can explain in details on what Im working on but I really want to pursue my PhD in ARIES. If you could possibly help me by telling me the GATE and NET cutoff to sit for the interview for ARIES, it will be a lot of help Sir.

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Great tutorial 😊

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Thanks you Sir

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Learn how to get SDSS spectra for this tutorial :kzbin.info/www/bejne/h6Knn4d5edGjsNk

Hello Sir.. I'm reaching out for your guidance..Is there any platform where I can text you directly? Your help would be appreciated.

What if I want to use string on x axis

Madam I am very much interested to do phd in Astronomy & Astrophysics & my gate score is 85 percentile madam can u tell me what is external registration & fee structure of that

Nice

Greatest astronomer ever met

Sir, I would like to contact you regarding some research-related queries. If possible, could you kindly provide me with your email address? I have a bachelor's degree in physics with a minor in astronomy, and I am interested in working with you.

Double sharing room milta hai??

Thank you very much for creating this course

my ears are not working after the intro sound of this video

Thanks a lot sir. Hope this will encourage homegrown geniuses also who can't make it to good institutions for PhD and research project. You very kind generous 🧡🧡🙏

Kl to pakka fail ho jaon ga😢

What is the difference between astropy and PyRAF and why do researchers prefer PyRAF over astropy?

please make a video about baseline correction of spectrum.

I am actually learning python from scratch and I came across this KZbin shorts. I was blown away at what python can do. Can you share a video of how you are able to use python to solve for the arbitrary constants C1, C2 and C3 given the boundary conditions y(0), y'(0), y"(0). I just subscribed

Is there any othery way to find the continuum and how to get the equivalent width from it ?

For desi, we can also use sparcel

How do you save the masked image in the fits file format?

on following the steps the output is WARNING: Model is linear in parameters; consider using linear fitting methods. [astropy.modeling.fitting] WARNING:astropy:Model is linear in parameters; consider using linear fitting methods. [0. 0. 0. ... 0. 0. 0.] erg / (Angstrom cm2 s2)... please help

Hello, i have a doubt. If i have 3-4 contours for a certain level, and i have to choose pixels from only one of them. how can i do that?

Pls share 2nd round video❤

Thanks for the great tutorial!

Sir, I'm using VSC to write the code. After running In[32] (7:49), it's showing error in the line plt.imshow(image) and sometimes it shows that the image is not defined. How do I rectify this error?

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Sir I have a problem & Question. I wrote the code properly and got the image properly but When i ran the code below i got the problem like this Cell In[23], line 2 1 from astropy.stats import sigma_clipped_stats ----> 2 mean,median,std=sigma_clipped_stats(data,sigma=3.0) 3 print(mean,median,std) NameError: name 'data' is not defined I could not solve this, Please can you tell me what is the solution. Thanks you sir

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there shows me that the variable file is not define

Can I use pip to install it?

Very Helpful. Thank you so much 👍

*Promo sm*

Gajab Marde

Love your content!

What i simply did is using iraf , i removed median bkg from same image using imarith

I really appreciate ur efforts to make astronomy easier. ...

After creating final_data=data-bkg, what to do to save this image as a fits file with expected header as original image??

Sir, kaha se liye. Kitne ka pada

Verynice

Very helpful video. How can I position the zoomed plot to where I want? For example I want mine to be in the middle left. Thanks