Leonardo dos Santos ladsantos
ladsantos
/ ref_solar_irradiance_whi-2008_ver2.dat
Created
December 21, 2023 15:49
Reference solar irradiance from the LASP Interactive Solar Irradiance Datacenter
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| ; | |
| ; Solar Spectral Irradiance Reference Spectra for | |
| ; Whole Heliosphere Interval (WHI) 2008: | |
| ; Carrington Rotation 2068 | |
| ; 20 March 2008 to 16 April 2008 | |
| ; | |
| ; Three periods within WHI are of particular interest: | |
| ; -------------------------------------------------- | |
| ; March 25 - March 29 had 3 small active regions on the solar disk, but TSI is lower. | |
| ; This is considered moderately low solar activity and has sunspot blocking (darkening). |
ladsantos
/ HAT-P-11_spec.dat
Created
May 6, 2021 11:32
Stellar flux from 5 to 2600 Angstrom arriving at the planet HAT-P-11 b (from the MUSCLES database)
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| # Wavelength (A) Flux density at planet (erg/s/cm^2/A) | |
| 4.809181690216064453e+00 1.481037364097737097e+01 | |
| 9.661773681640625000e+00 4.090424111402812812e-01 | |
| 1.538304710388183594e+01 6.987623281623321247e+00 | |
| 1.977779579162597656e+01 8.841277458904285069e+00 | |
| 2.345973968505859375e+01 8.969739574618197153e+00 | |
| 2.906380081176757812e+01 5.054996994071267125e+00 | |
| 3.409113693237304688e+01 5.435642157408120845e+00 | |
| 3.957408714294433594e+01 2.511019224362939006e+00 | |
| 4.713372802734375000e+01 2.708297311014336906e+00 |
ladsantos
/ WASP-107_b_He.dat
Last active
May 4, 2021 12:12
He transmission spectrum of WASP-107b measured with CARMENES (Source: DACE database at https://dace.unige.ch/openData/)
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| # Wavelength (A) Spectrum (%) Uncertainty (%) | |
| 10828.9872 0.314256480616 0.949015359519 | |
| 10829.0448 -0.025338358943 0.941966797162 | |
| 10829.1024 -0.031281248915 0.944411071456 | |
| 10829.16 0.784594190059 0.941737150927 | |
| 10829.2176 0.049979064183 0.950244132561 | |
| 10829.2752 0.287439894142 0.952406033855 | |
| 10829.3327 0.031721629378 0.957437455371 | |
| 10829.3903 -0.37997013748 0.965386897659 | |
| 10829.4479 -0.104825249096 0.969886614003 |
ladsantos
/ HAT-P-11_b_He.dat
Last active
May 4, 2021 12:12
He transmission spectrum of HAT-P-11b measured with CARMENES (Source: DACE database at https://dace.unige.ch/openData/)
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| # Wavelength (A) Spectrum (%) Uncertainty (%) | |
| 10829.0277 -0.006339032842 0.209804955372 | |
| 10829.0855 -0.008565300696 0.209826803783 | |
| 10829.1434 -0.168555670491 0.210010233094 | |
| 10829.2012 -0.070905015076 0.210003399084 | |
| 10829.259 -0.013467100496 0.210058883742 | |
| 10829.3168 -0.024191369498 0.210226748916 | |
| 10829.3746 -0.058682056888 0.210397418468 | |
| 10829.4324 -0.3108329101 0.210806401951 | |
| 10829.4902 -0.233068506802 0.210937116893 |
ladsantos
/ exoplanet_transmission_list.txt
Last active
February 17, 2021 09:30
List of exoplanets that have had their atmospheres probed in transmission
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| CoRoT-1 b | |
| GJ 436 b | |
| GJ 1214 b | |
| GJ 3470 b | |
| GJ 9827 b | |
| GJ 9827 c | |
| GJ 9827 d | |
| HAT-P-1 b | |
| HAT-P-11 b | |
| HAT-P-12 b |
ladsantos
/ telesc_diffr.py
Last active
August 29, 2015 14:14
This code plots the diffraction pattern produced by a point-like source of light in a telescope
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| import numpy as np | |
| import scipy.special as sp | |
| from pylab import imshow,show,gray,hot | |
| import matplotlib.pyplot as plt | |
| from timeit import default_timer as timer | |
| def func(x,m,theta): | |
| return np.cos(m*theta-x*np.sin(theta)) | |
| wl = 500E-9 # wavelength, in meters |
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| { | |
| "metadata": { | |
| "name": "", | |
| "signature": "sha256:98fcea68ba105712b72f7e888ccceecb26f7e7b0f814f9f6a58c21f28de2453b" | |
| }, | |
| "nbformat": 3, | |
| "nbformat_minor": 0, | |
| "worksheets": [ | |
| { | |
| "cells": [ |