ascl_id stringclasses 752
values | repo_url stringclasses 737
values | file_path stringlengths 4 194 | content large_stringlengths 1 1M | language stringclasses 29
values | license_type stringclasses 24
values | size int64 1 1M |
|---|---|---|---|---|---|---|
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/test_wcs.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
#import os
#import pixelsplines as pxs
# Script to test WCS routines in astropy:
# Set the plan:
naxis1 = 3000 # log-wavelength
naxis2 = 5 # irregular
naxis3 = 10 #... | Python | BSD | 3,641 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/__init__.py | # redmonster/sandbox/__init__.py
| Python | BSD | 33 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/run_redmonster.py | # Initial top-level script to run redmonster on a single plate, with
# options to use only a subset of fibers. Each spPlate file is assumed
# to be in $BOSS_SPECTRO_REDUX/$RUN2D/pppp/ where pppp is the 4-digit
# plate-id. Templates are assumed to be in $REDMONSTER_DIR/templates/
#
# Tim Hutchinson, University of Utah... | Python | BSD | 6,823 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/multiplot.py | from os.path import join
from os import environ
import numpy as n
from astropy.io import fits
from matplotlib import pyplot as p
from astropy.convolution import convolve, Box1DKernel
# Open spPlate file
path = '/Users/timhutchinson/work/boss/run2d/7848/spPlate-7848-56959.fits'
spp = fits.open(path)
sigma = 1. / n.sqr... | Python | BSD | 4,112 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/donna_spec.py | from os import environ
from os.path import exists, join
from math import ceil, floor
from astropy.io import fits
import numpy as n
from redmonster.physics.misc import flux_check
from redmonster.datamgr.io import remove_log, write_to_log
class Spec:
def __init__(self, filepath):
hdu = fits.open(filepath)... | Python | BSD | 719 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/run_rm.py | # Run a single instance of redmonster on visually inspected CMASS fibers
import numpy as n
import matplotlib.pyplot as p
p.interactive(True)
from redmonster.sandbox import yanny as y
from astropy.io import fits
from redmonster.datamgr import spec, io
from redmonster.physics import zfinder, zfitter, zpicker
from redmon... | Python | BSD | 4,865 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/yanny_to_arrays.py | import numpy as n
from redmonster.sandbox import yanny as y
# Read yanny file
x = y.yanny(filename='/uufs/astro.utah.edu/common/home/u0814744/boss/\
spInspect_alltest_bolton.par.txt', np=True)
# Get fibers, zpipe, zperson for each plate
args = n.where(x['BOSSOBJECT']['plate'] == 3686)[0]
fibers3686 = []
... | Python | BSD | 2,282 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/verify.py | import numpy as n
from astropy.io import fits
from os.path import join, basename
from os import environ
from glob import iglob
from redmonster.sandbox import yanny as y
import matplotlib
matplotlib.use('Agg')
import matplotlib.pyplot as p
from math import isnan
from astropy.convolution import convolve, Box1DKernel
from... | Python | BSD | 62,660 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/multi_exposure_dev.scr.py | #
# multi_exposure_dev.scr.py
#
# script for developping methods that handle multiple
# exposures of a single fiber.
#
from __future__ import print_function
import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
import os
from redmonster.physics impo... | Python | BSD | 21,463 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/test_ndArch.py | import numpy as n
#import matplotlib as m
#m.interactive(True)
#from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
#import os
#import pixelsplines as pxs
# Script to make test file for "read_ndArch" file-reader routine:
# Set the plan:
#naxis1 = 3000 # log-wavelength
naxis1 = 8 # ... | Python | BSD | 2,881 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/par_rm.py | # Run redmonster on a cluster using multiprocessesing
#
# Tim Hutchinson, University of Utah, August 2014
# t.hutchinson@utah.edu
from time import gmtime, strftime
import numpy as n
import matplotlib.pyplot as p
p.interactive(True)
import multiprocessing as mp
from astropy.io import fits
from redmonster.sandbox impo... | Python | BSD | 4,656 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/chi2_optimize.py | import numpy as n
import matplotlib.pyplot as p
p.interactive(True)
from redmonster.sandbox import yanny as y
from astropy.io import fits
from redmonster.datamgr import spec, io
from redmonster.physics import zfinder, zfitter, zpicker
from redmonster.physics import misc
from time import gmtime, strftime
import multipro... | Python | BSD | 4,528 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/verify_sequels.py | from __future__ import print_function
from os.path import join, basename, exists
from os import environ
from math import isnan
import time
from sys import stderr
import numpy as n
from scipy.integrate import trapz
from astropy.io import fits
import matplotlib
matplotlib.use('Agg')
import matplotlib.pyplot as p
from m... | Python | BSD | 199,638 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/RepeatsPlot.py | import pyfits
import glob
import numpy as N
import pylab as P
import os
import shutil
import sys
class Repeatability:
directory = '/uufs/astro.utah.edu/common/home/u0814744/compute/scratch/repeatability'
@staticmethod
def makeSpAllRepeats():
hdu = pyfits.open('/uufs/chpc.utah.edu/common/home/sds... | Python | BSD | 5,032 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/make_best_fit_plot.py | # Make a plot of the "best fit" spectra to any object, of arbitrary
# template type. Only works for a single fiber.
#
# Tim Hutchinson, University of Utah, Oct 2014
# t.hutchinson@utah.edu
from time import gmtime, strftime
import numpy as n
from astropy.io import fits
import matplotlib.pyplot as p
p.interactive(True... | Python | BSD | 3,088 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/run_plot_fit.py | # Command line execution for plot_fit.py
#
# Tim Hutchinson, University of Utah, April 2014
# t.hutchinson@utah.edu
try:
from tkinter import *
except ImportError:
from Tkinter import *
import numpy as n
import matplotlib
matplotlib.use('TkAgg')
from matplotlib.backends.backend_tkagg import FigureCanvasTkAgg, N... | Python | BSD | 918 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/sandbox/top.py | from redmonster.sandbox import main as M
plate = 3686
mjd = 55268
templates = ['ndArch-ssp_em_galaxy-v000.fits', 'ndArch-all-CAP-grids.fits',
'ndArch-QSO-V003.fits']
fiberid = [100]
zmin = [.01, -.005, .4]
zmax = [1.2, .005, 3.5]
npixstep = [1,1,4]
dest = '/Users/boltonlab3/scratch'
M.main(plate=plate, m... | Python | BSD | 413 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/application/zfind.py | # Top level script to run redmonster as a whole.
#
# Required arguments:
# plate (int): 4-digit plate number
# mjd (int): 4-digit mjd for given plate
# templates (list of strings): List of template names, as strings, to be run, up to a max of 5. Template files must be in $REDMONSTER_DIR/templates/
#
# Optional argumen... | Python | BSD | 12,270 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/application/zfind2.py | # Top level script to run redmonster as a whole.
#
# Required arguments:
# plate (int): 4-digit plate number
# mjd (int): 4-digit mjd for given plate
# templates (list of strings): List of template names, as strings, to be run, up to a max of 5. Template files must be in $REDMONSTER_DIR/templates/
#
# Optional argumen... | Python | BSD | 16,386 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | python/redmonster/application/__init__.py | # redmonster/application/__init__.py
# Expose modules in this package.
| Python | BSD | 71 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | conf/zfind_noz.ini | #
# zfind templates configuration
#
[galaxy]
template = ndArch-ssp_galaxy_noemit-v000.fits
npixstep = 2
npoly = 1
group = [0]
| Config | BSD | 127 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | conf/zfind.ini | #
# zfind templates configuration
#
[star]
template = ndArch-all-CAP-grids.fits
zmin = -.005
zmax = .005
npixstep = 1
npoly = 1
group = [0]
[galaxy]
template = ndArch-ssp_galaxy_glob-v000.fits
#template = ndArch-ssp_galaxy_noemit-v000.fits
zmin = -.01
zmax = 1.2
npixstep = 2
npoly = 1
group = [0]
#[elg]
#template = ... | Config | BSD | 503 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/ssp_ztemplate_hires_v01.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 4,457 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/ssp_ztemplate_v002_emit.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 8,945 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/ssp_ztemplate_v002_cont.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 8,187 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/ssp_ztemplate_quickdesi_v00.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 8,083 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/cap_ztemplate_v01.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 3,641 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/ssp_ztemplate_v00.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 7,949 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/cap_ztemplate_v00.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 3,601 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/ssp_ztemplate_hires_v02.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 4,834 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | templates/cap_ztemplate_v02.py | import numpy as n
import matplotlib as m
m.interactive(True)
from matplotlib import pyplot as p
from astropy.io import fits
#from astropy import wcs
import os
#import pixelsplines as pxs
from redmonster.datamgr import io
from redmonster.physics import pixelsplines as pxs
import copy
from redmonster.physics import misc
... | Python | BSD | 3,800 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | bin/chi2_merge.sh | #!/bin/bash
python $REDMONSTER_DIR/python/redmonster/tools/chi2_merge.py | Shell | BSD | 73 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | bin/fiber_merge.sh | #!/bin/bash
python $REDMONSTER_DIR/python/redmonster/tools/fiber_merge.py | Shell | BSD | 74 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | bin/plate_merge.sh | #!/bin/bash
python $REDMONSTER_DIR/python/redmonster/tools/plate_merge.py | Shell | BSD | 74 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | pro/read_spec.pro | ;+
; NAME:
; READ_SPEC
;
; PURPOSE:
; Function to convert a *.spec file into an IDL structure.
; Input may be an array of filenames.
;
; CALLING SEQUENCE:
; res = read_spec(file)
;
; KEYWORD PARAMETERS:
; miles - set this keyword when reading in spectra based on Miles
; NB: you should not need... | IDL | BSD | 3,167 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | pro/ssp_repackage_3.scr.pro | ;
; ssp_repackage_3.scr.pro
;
; repackage the theoretical SSPs from Charlie Conroy
; into a FITS file.
;
; 3rd iteration, 3 sept 2014
; I THINK you have to say ".com read_spec" before you run this script!
;infile = 'SSP_Padova_RRLIB_Kroupa_Z0.0190.out.spec'
;infiles = file_search('/data/SSP/SSP_*.spec')
infiles = fi... | IDL | BSD | 859 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | doc/template-datamodel.tex | \documentclass[12pt]{article}
\parindent=0pt
\parskip=8pt
\begin{document}
\title{Proposed data model for a general archetype
redshift template file format}
\author{Adam S. Bolton}
\maketitle
\section{Introduction}
This note describes a proposed file format for storing general
``archetype'' redshift template grids... | LaTeX | BSD | 8,489 |
[ascl:2511.008] | https://github.com/timahutchinson/redmonster | doc/redmonster-output-file.tex | \documentclass[12pt]{article}
\parindent=0pt
\parskip=8pt
\begin{document}
\title{Documentation of \texttt{redmonster} Output Files}
\author{Timothy A. Hutchinson}
\maketitle
\section{Introduction}
This document describes the format and content of the files
generated by the \texttt{redmonster} software.
The princ... | LaTeX | BSD | 6,305 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | __init__.py | """
This is RedPipe, a python package to perform Photometry & Spectroscopy on Optical FITS Images.
:Authors: Avinash Singh
:License: GPLv3
"""
__author__ = "Avinash Singh"
__copyright__ = "2018, Avinash Singh"
__version__ = "0.1.0"
import Photometry, PhotStandard, PhotTemp, PhotUVIT, PreProcPhot, PreProcSpec, PostP... | Python | Unknown | 471 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | Setup.py | #!/usr/bin/env python
from setuptools import setup
version = re.findall(r"__version__ = \"(.*?)\"", open(fname).read())[0]
setup(name='RedPipe',
version='0.1.1',
description='Optical Photometric & Spectroscopic Reduction Pipeline',
long_description=open('README.rst').read(),
classifiers=['Deve... | Python | Unknown | 1,029 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | setup.py | #!/usr/bin/env python
from setuptools import setup
version = re.findall(r"__version__ = \"(.*?)\"", open(fname).read())[0]
setup(name='RedPipe',
version='0.1.1',
description='Optical Photometric & Spectroscopic Reduction Pipeline',
long_description=open('README.rst').read(),
classifiers=['Deve... | Python | Unknown | 1,029 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | CHANGES.rst | 0.1.0a0 (2018-10-04)
==================
- Initial Release
0.1.0a1 (2020-02-08)
==================
- Updated Directory Structure
| reStructuredText | Unknown | 129 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | LICENSE.txt | GNU GENERAL PUBLIC LICENSE
Version 3, 29 June 2007
Copyright (C) 2007 Free Software Foundation, Inc. <http://fsf.org/>
Everyone is permitted to copy and distribute verbatim copies
of this license document, but changing it is not allowed.
Preamb... | Text | Unknown | 35,147 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | README.md | # RedPipe: Reduction Pipeline #
[](https://github.com/sPaMFouR/RedPipe)
[](https://ascl.net/2106.024)
[](https://github.c... | Markdown | Unknown | 1,117 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | InstallDependencies.py | #!/usr/bin/env python
"""
Installs Necessary Modules To Get The Reduction Pipeline Going.
"""
# ------------------------------------------------------------------------------------------------------------------- #
# Import Required Libraries
# ---------------------------------------------------------------------------... | Python | Unknown | 5,939 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotSpecTypeII_3.py | # !/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxx-----------------------PLOT SPECTRA OF SUPERNOVA----------------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 55,488 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotColorEvolution_5.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxx---------------TABULTATE THE SN MAGNITUDE AND PLOT COLOR CURVES----------------xxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 34,886 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotSpecTypeI.py | # !/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxx---------------------------PLOT 1-D SPECTRA---------------------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 35,867 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotPhotVelTypeII_3.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxx---------------PLOT PHOTOSPHERIC VELOCITY EVOLUTION IN TYPE II SNe----------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 18,981 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotPhotVelTypeII_2.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxx---------------PLOT PHOTOSPHERIC VELOCITY EVOLUTION IN TYPE II SNe----------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 18,105 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotPhotVel_2.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxx---------------Plot The Supernova Photospheric Velocity Evolution----------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 11,290 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotLightCurve_8.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx--------------PLOT THE SUPERNOVA LIGHT CURVES FROM INPUT MAGNITUDE FILES--------------xxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 69,686 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotSpectra_3.py | # !/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxx---------------------------PLOT 1-D SPECTRA---------------------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 35,788 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotSNParamTypeII_3.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxx------------------------PLOT THE TYPE II SNE PARAMETERS-------------------------xxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 42,682 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotPhotVelTypeI.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxx---------------Plot The Supernova Photospheric Velocity Evolution----------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 11,815 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotSNParamTypeI.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxx--------------------PLOT CORRELATION BETWEEN TYPE I SNe PARAMETERS-------------------xxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 13,390 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | plotting/PlotFitNagy.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxx-------------------Nagy LIGHT CURVE MODEL-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 9,076 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/EditHeaderDFOT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxx---------MODIFIES HEADER IN THE HFOSC2 FITS FILES AND APPENDS AIRMASS DETAILS------------xxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 6,547 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/PreProcPhotHCT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxx-------------------------PHOTOMETRIC DATA PRE-PROCESSING----------------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 26,871 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/AppendHeaderInfo.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxx---------------UPDATES AND APPENDS HEADER INFORMATION----------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 14,031 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/PrintHeaderInfo.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxx-------------------------PRINT HEADER INFORMATION----------------------xxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,843 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/PreProcSpec.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxx-------------------------SPECTROSCOPIC DATA REDUCTION-----------------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 19,132 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/read_fits_class.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxx-----------------Read FITS file----------------xxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 2,729 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/PreProcPhotDOT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxx-------------------------PHOTOMETRIC DATA PRE-PROCESSING----------------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 26,570 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/PreProcess.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxx------------------------PERFORMS PRE-PROCESSING----------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 11,565 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/EditHeader.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxx---------MODIFIES HEADER IN THE HFOSC2 FITS FILES AND APPENDS AIRMASS DETAILS------------xxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 6,629 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/CosmicRayCor.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxx-------------------------COSMIC RAY CORRECTION--------------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 13,472 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | preprocess/Rename.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxx-------------------------RENAME RAW FILES-----------------------xxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 10,989 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitBlackBody.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxx-----------------Fit Planckian Function To A Spectrum---------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 7,392 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitTripleGaussian.py | # !/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxx---------------------------PLOT 1-D SPECTRA---------------------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 8,933 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitLatePhase.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx----------FIT RADIOACTIVE DECAY PHASE TO ACCOUNT FOR THE GAMMA-RAY TRAPPING-----------xxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,783 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitMultipleGaussian.ipynb | {
"cells": [
{
"cell_type": "code",
"execution_count": 16,
"id": "45bb88fa",
"metadata": {},
"outputs": [],
"source": [
"# !/usr/bin/env python\n",
"# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #\n",
"# xxxxxxxxxxx... | Jupyter Notebook | Unknown | 953,496 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/ReadJSON.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxx----------------------READ DATA FOR SN 2018hna----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 6,056 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitVinko_2.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxx----------------FITTING VINKO MODEL FOR A STRIPPED ENVELOPE SUPERNOVA--------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 7,918 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitPieceWise.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx--------------FIT PIECEWISE LINEAR POLYNOMIAL TO TYPE IIP SN LIGHT CURVES-------------xxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,600 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitPejcha.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxx-------------------LIGHT CURVE MODELLING-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,811 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitTaddiaR.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx---------------FITTING TADDIA MODEL FOR A STRIPPED ENVELOPE SUPERNOVAE--------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 10,423 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitDualGaussian.py | # !/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxx---------------------------PLOT 1-D SPECTRA---------------------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 9,725 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitMultiComponent.ipynb | {
"cells": [
{
"cell_type": "code",
"execution_count": 1,
"id": "4ae0bf6d-ab60-4e05-9329-091a9acd1397",
"metadata": {},
"outputs": [],
"source": [
"# !/usr/bin/env python\n",
"# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Jupyter Notebook | Unknown | 665,872 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitInterpLC.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxx--------------------FIT SPLINE TO SUPERNOVA LIGHT CURVE-----------------------xxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,650 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitOlivares.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxx----------------FIT THE OLIVARES MODEL TO TYPE IIP SN LIGHT CURVES---------------xxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 13,875 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitElmhamdi.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx--------------DETERMINE THE STEEPNESS PARAMETER FOR TYPE IIP SUPERNOVA---------------xxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 17,389 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitColorTemplate.py | # ------------------------------------------------------------------------------------------------------------------- #
# Read Other Type II SNe Data From The SN Archive Folder
# Read B-V Color Template (Stritzinger et al. 2018)
# -----------------------------------------------------------------------------------------... | Python | Unknown | 10,606 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/DeReddenSpec.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxx-----------------Fit Planckian Function To A Spectrum---------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 18,596 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitPiroNakar.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx----------------FITTING TADDIA MODEL FOR STRIPPED ENVELOPE SUPERNOVAE---------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 10,031 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitRiseTime.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx------------FIT COWEN MODEL TO THE EARLY PHASE LIGHT CURVE IN TYPE IIP SNe------------xxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 10,220 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/CalcTypeIIParam.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxx----------------------CALCULATE TYPE II SN PARAMS---------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,117 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitNagyLC2.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxx-------------------Nagy LIGHT CURVE MODEL-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 8,401 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitEPM.py | ##########################################
## EPM Distance estimation of SN 2016gfy ##
##########################################
import numpy as np
import matplotlib.pyplot as plt
import subprocess
import scipy.optimize as optimize
from scipy.optimize import curve_fit
##########################################
## Par... | Python | Unknown | 10,221 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitValenti.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxx-------------FITTING ARNETT-VALENTI MODEL FOR A STRIPPED ENVELOPE SUPERNOVA--------------xxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 13,912 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/DeReddenPhot.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxx-----------------Fit Planckian Function To A Spectrum---------------xxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 11,751 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitEmpirical.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx---------------DETERMINE THE EMPIRICAL RELATION FOR TYPE IIP SUPERNOVA---------------xxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 8,598 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | analysis/FitTaddiaUBVRIBol_3.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxx---------------FITTING TADDIA MODEL FOR A STRIPPED ENVELOPE SUPERNOVAE--------------xxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 19,601 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotGal.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF GALAXIES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 14,561 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotUVIT_3.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 25,322 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotDOT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 41,399 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/EditHeader.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxx---------MODIFIES HEADER IN THE HFOSC2 FITS FILES AND APPENDS AIRMASS DETAILS------------xxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 6,629 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotStandard.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 40,270 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/Airmass_3.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxx-------------------------CALCULATION OF AIRMASS----------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 8,291 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/AirmassDOT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxx-------------------------CALCULATION OF AIRMASS----------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 8,313 |
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