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#ICTS #may2024 | ||
6 - 5 - 2024 | ||
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This is my first day at ICTS in bangalore | ||
Job shadow program | ||
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**10:15** | ||
Reached and had breakfast | ||
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**10:30 to 11:30** | ||
Downloaded & setup vsc and tested anaconda and linux vm (wget <link>) | ||
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**11:30 to 1** | ||
attending a lecture on bayesian procedure | ||
(notes in notebook) | ||
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SpEC | ||
Spectral Einstein code | ||
https://www.black-holes.org/code/SpEC.html | ||
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**1:15 to 2** - Lunch | ||
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**2 to 2:30** | ||
working on assignment given by vaishak | ||
learn arrays in python | ||
![[WhatsApp Image 2024-05-06 at 16.04.03_5faf9ce0.jpg]] | ||
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plot a graph | ||
![[Pasted image 20240506150028.png]] | ||
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**2:30 to 4** | ||
Lecture on Linear Algebra 1 | ||
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Linear vector space | ||
- closure under addition, associativity of addition | ||
- associativity of scalar multiplicatiojn | ||
- distributivity | ||
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R is a real vector space of real scalars | ||
R^n is real vector space of n vector | ||
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Properties of <. , .> | ||
1) <x, y> > 0 Vx not equal to 0 = positive definite | ||
2) <x, y> = <y, x> - symmetry | ||
Operation on vectors in R^n | ||
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Vector can be measured in different scales | ||
1) Euclidean / 2 - norm | ||
2) Manhattan / 1 - norm | ||
3) Chebyshev / infinity norm | ||
4) Minkowski / p - norm | ||
5) Energy Norm | ||
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![[Pasted image 20240506150418.png]] | ||
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Unit sphere: locus of points at unit distance from origin | ||
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Functionals | ||
Let V be a vector space | ||
Any function that maps V into R: f: V -> R is called a functional | ||
f is called linear functional if | ||
f(x1 + x2) = f(x1) + f(x2) -> additive | ||
f(ax) = af(x) = homogenous | ||
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Example | ||
1) ||x|| is a nonlinear functional | ||
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Cauchy Schwarz inequality (CS) | ||
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Span of a set of vectors | ||
orthogonal vectors | ||
linearly independent vectors in 2 dimensions - infinite number possible | ||
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**4:00** | ||
more messing around with numpy | ||
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make the y scale logarithmic | ||
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Damped sinusoid equations | ||
![[Pasted image 20240507190413.png]] | ||
Made a jupyter notebook which contains all python activities from day 1 | ||
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**Reflection** | ||
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- ICTS is a nice and open place, I could go around and be wherever I wanted, which was good. Gave me a sense of freedom I guess | ||
- I am thinking that the outcomes of this job shadow program could be | ||
- writeup on what other researchers do in the astrophysics and relativity group | ||
- github repository with the python notebooks of each day's python work | ||
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#ICTS #may2024 | ||
8 - 5 - 2024 | ||
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**10:30 to 11:15** | ||
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In the bus learned about normal distributions and probability contours. Probability contours are ellipses that show the distribution of a two-dimensional probability density function. | ||
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A chi-squared test, or Khi2 test, is a statistical hypothesis test that compares the observed distribution of data to an expected distribution. | ||
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**11:30** | ||
Supercomputer at ICTS | ||
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"sonic" | ||
https://it.icts.res.in/ | ||
14 nodes | ||
HPC - high performance computing | ||
has to communicate data through the nodes | ||
HTC - high throughput computing | ||
does not need to communicate data through different nodes | ||
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AMD Epyc 7413 | ||
2 socket per node | ||
24 cores per socket = 48 cores per node, 96 threads in total | ||
256 gb ram on signing nodes | ||
384 gb on the computing nodes | ||
running centos | ||
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Recently acquired 2x | ||
Nvidia A40 gpu with 48gb vram | ||
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data analysis | ||
uses gpu and the HTCs | ||
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**12:00 to 1:00** | ||
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Group meeting/discussion on interesting paper found on Arxiv | ||
[Members of Astrophysics Relativity Group at ICTS](https://www.icts.res.in/research/astrorel/members) | ||
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- [Alorika Kar] talked about "Quick recipes for gravitational-wave selection effects | ||
- https://arxiv.org/abs/2404.16930 | ||
- https://arxiv.org/pdf/2404.16930 | ||
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- [Ankur Barsode] talked about "Lens Stochastic Diffraction: A signature of compact structures in gravitational wave data" | ||
- https://arxiv.org/pdf/2404.17405 | ||
- if you have single lens - 2 images | ||
- you can have multiple lenses but the fainter images are all going to overlap on each other and you are going to get a stochastic signal and it will come from the same location as the main image. | ||
- multiple images from multiple lenses all overlapping with each other | ||
- Questions | ||
- How many lenses | ||
- probably 10 - 15 is what he is using | ||
- There should be a threshold | ||
- didnt go that much into the details | ||
- why is it important | ||
- you can use non detection to constrain blackholes?? | ||
- [Prasad R] talked about "Dynamical ejecta from binary neutron star mergers: Impact of residual eccentricity and equation of state implementation" | ||
- https://arxiv.org/pdf/2404.18674 | ||
- ejected mass is whatever is remaining after neutron stars merge | ||
- ejecta is ejected more if neutron star is spinning more | ||
- Concerned about | ||
- accuracy of simulation | ||
- internal reactions | ||
- keeping everything fixed and see how it reacts | ||
- [Prasad R] also talked about "Black hole-neutron star mergers with massive neutron stars in numerical relativity" | ||
- https://arxiv.org/pdf/2404.18714 | ||
- [Krishnendu N V] talked about "Numerical parameterization of stationary axisymmetric black holes in a theory agnostic framework" | ||
- https://arxiv.org/pdf/2404.17055 | ||
- [Vaishak P] "NOTES ON THE PRACTICAL APPLICATION OF NESTED SAMPLING: MULTINEST, (NON)CONVERGENCE, AND RECTIFICATION" | ||
- https://arxiv.org/pdf/2404.16928 | ||
- [Koustav Narayan Maity] "Neutron stars and the cosmological constant problem" | ||
- https://arxiv.org/pdf/2404.19012 | ||
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Mainly the PHD fellows were the ones discussing and asking questions and answering each other's doubts on each of the research papers. | ||
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After lunch, **2:00** | ||
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worked on python notebook, extracting original parameters from noise of a damped sinusoid wave. | ||
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refer "Day 2_assgt.ipynb for more info" | ||
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**EOS** | ||
- should consider installing and learning docker, so i can use vsc and develop inside a linux environment | ||
- vaishak likes using powerful computer resources to find solutions to problems that need answering, not like google and microsoft who use supercomputers to give users better ads | ||
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#ICTS #may2024 | ||
9 - 5 - 2024 | ||
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mainly python stuff | ||
dynesty | ||
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Enter some stuff about LIGO detectors | ||
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physics of it | ||
gravitational waves | ||
LIGO detectors | ||
they are what observe the time series data | ||
binary black hole mergers | ||
waveform generation | ||
numerical relativity** | ||
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computational challenges in brief and then exapnd on it in more detail | ||
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data analysis and parameter | ||
minimization - maximum likelihood estimation - chisquared | ||
bayesian inference | ||
gravitational wave data analysis | ||
matched filter (understanding of it) | ||
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Research ICTS | ||
operational structure | ||
usual week | ||
group activities | ||
computational resources | ||
people in ASTROPHYSICAL RELATIVITY group | ||
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Covariance matrix | ||
Read up on vector spaces because it is matrices and all | ||
fourier transform | ||
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noise sensitivity curve |
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#ICTS #may2024 | ||
13 - 5 - 2024 | ||
- Setup [WSL](https://learn.microsoft.com/en-us/windows/wsl/) | ||
- Ubuntu is running well | ||
- Installed software | ||
- anaconda | ||
- git | ||
- VScode extensions to ssh from wsl to windows machine | ||
- Gui apps (firefox, x11, nautilus) | ||
- Can access files from both within linux and shows up as a separate location in windows | ||
- ![[Pasted image 20240514121747.png]] | ||
- ![[Pasted image 20240514124825.png]] | ||
- Looked through [Parameter estimation](https://gitlab.com/vaishakp/parameter-estimation) | ||
- Read through some of the links |
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<!DOCTYPE html> | ||
<html lang="en"> | ||
<head> | ||
<meta charset="UTF-8"> | ||
<meta name="viewport" content="width=device-width, initial-scale=1.0"> | ||
<title>ICTS Job Shadow Index</title> | ||
<style> | ||
body { | ||
font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; | ||
color: #b31d0f; | ||
background-color: #fafafa; | ||
margin: 0; | ||
padding: 0; | ||
} | ||
.container { | ||
max-width: 800px; | ||
margin: 0 auto; | ||
padding: 20px; | ||
} | ||
h1, h2 { | ||
color: #b31d0f; | ||
} | ||
p { | ||
margin-bottom: 20px; | ||
} | ||
button { | ||
color: #fafafa; | ||
background-color: #b31d0f; | ||
} | ||
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</style> | ||
</head> | ||
<body> | ||
<div class="container"> | ||
<header> | ||
<h1>Week 1 Activities at ICTS </h1> | ||
<nav> | ||
<button onclick="window.location.href='../index.html'">Index</button> | ||
</nav> | ||
</header> | ||
<main> | ||
<section id="Week 1"> | ||
<h2>Week 1</h2> | ||
<p>Python notebooks and Markdown files of activities of Week 1</p> | ||
</section> | ||
<!-- Add your portfolio items here --> | ||
</section> | ||
</main> | ||
<footer> | ||
<!-- Add footer content if needed --> | ||
</footer> | ||
</div> | ||
</body> | ||
</html> |
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#ICTS #may2024 | ||
15 - 5 - 2024 | ||
**10:40** | ||
- Trying out [Parameter estimation](https://gitlab.com/vaishakp/parameter-estimation) in WSL | ||
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**11:00 to 12:00** | ||
- working on the final document on overleaf | ||
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**12:00 to 1:00** | ||
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Group meeting/discussion on interesting paper found on Arxiv | ||
[Members of Astrophysics Relativity Group at ICTS](https://www.icts.res.in/research/astrorel/members) | ||
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- https://arxiv.org/abs/2405.02197 | ||
- dont seem to address any numerical sources, only physical sources | ||
- nrv sources | ||
- listed possible reasons and does not go into that much of detail | ||
- there are no figures in the document by choice | ||
- not about physics but more about physical sources | ||
- https://arxiv.org/abs/2405.05318 | ||
- it is a convoluted way to write | ||
- whether they really did it from the masses | ||
- only the sky location and time and brightness of the flares and the brightness should also be related to the mass | ||
- brightness related to mass and gas | ||
- if the black hole is more massive then there is more gas | ||
- systematic more flare activity if the black hole is massive | ||
- AGN flares | ||
- https://arxiv.org/abs/2405.05884 | ||
- https://arxiv.org/abs/2405.05094 | ||
- https://arxiv.org/abs/2405.04690 | ||
- publically available data set from LISA | ||
- catalog of possible sources | ||
- dont know parameters | ||
- analysing real LISA data and can be used for simulations | ||
- used for software development | ||
- markov chain monte carlo implemented on gpu | ||
- fold the data which you get from LISA | ||
- have they compared cpu vs gpu | ||
- NERYN | ||
- used nvidia a100 and 12 cpu | ||
- dont think there is any machine learning like training over here | ||
- https://lisa-ldc.lal.in2p3.fr/challenge2a | ||
- https://arxiv.org/abs/2405.03841 | ||
- formation channel of neutron stars (factcheck) | ||
- redefining many events | ||
- surprised that they can claim which one formed first | ||
- how do they decide what came first | ||
- prior and then posterior estimation | ||
- one object is a neutron star and another is black hole do we use information to construct priors using () | ||
- https://arxiv.org/abs/2405.03607 | ||
- when spins are gravitationally oriented, the radiation is not symmetric. | ||
- this is also motivated by fact that equal mass binaries form largest kicks | ||
- however asymmetric mass binaries form largest kicks | ||
- equal mass binaries largest kicks is wrong so it is either a typo or something is not understood fully | ||
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#ICTS #may2024 | ||
16 - 5 - 2024 | ||
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**10:30 to 11:30** | ||
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Learned linux terminal commands and how to append a directory to PYTHONPATH | ||
![[Pasted image 20240516132244.png]] | ||
![[Pasted image 20240516132412.png]] | ||
^appended directories to $PYTHONPATH | ||
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![[Pasted image 20240516132459.png]] | ||
creating new environment for yumcee package testing | ||
"-n" is the tag to name the env | ||
"-c" is the tag to specify the repository of packages, in this case it is [conda-forge](https://conda-forge.org/) | ||
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"env" is a command to display current environment in linux | ||
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**11:30 to 1:00** | ||
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Learned the basics of Linear algebra | ||
![[WhatsApp Image 2024-05-16 at 13.31.20_b56691a7.jpg]] | ||
![[WhatsApp Image 2024-05-16 at 13.31.21_23955639.jpg]] | ||
![[WhatsApp Image 2024-05-16 at 13.31.23_11818b52.jpg|330]] | ||
Identity matrix is a diagonal matrix with all its diagonal elements equal to 1 , and zeroes everywhere else. [Newcastle University](https://www.ncl.ac.uk/webtemplate/ask-assets/external/maths-resources/core-mathematics/pure-maths/matrices/matrix-arithmetic.html#:~:text=An%20identity%20matrix%2C%20sometimes%20called,1%20%2C%20and%20zeroes%20everywhere%20else.) | ||
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a(x) = x; where a (scalar) multiplying x (vector) | ||
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Rotation and Translation of matrix [] | ||
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Look through this book when bored so I can learn more about Linear Algebra. Teaches it in a physics point of view. [Linear Algebra Klaus Janich.pdf](file:///C:%5CUsers%5Cdrpro%5CDownloads%5CLinear%20Algebra%20Klaus%20Janich.pdf) | ||
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- also figured out how to resize picture in obsidian, have to add a " | " and a number after image, eg. !["[sample.jpg|330]"] | ||
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Working on showing Autocorrelation code and understanding covariance matrix | ||
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