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:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotAIMPOL.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 21,236 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotometryUtils.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 41,523 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/AlignDOT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxx----------------------------IMAGE ALIGNMENT---------------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 26,445 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotTempDOT.py | # xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 30,019 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotTemp_2.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 30,426 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/Align_5.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxx----------------------------IMAGE ALIGNMENT---------------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 26,602 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/Photometry_6.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 42,355 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/PhotGROWTH.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxx-------------------PHOTOMETRY OF OBJECT FRAMES-----------------xxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 30,863 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | photometry/CombineFrames_2.py | # /usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxx----------------------------COMBINE IMAGES----------------------------xxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 9,134 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcRLambda.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxx-------------------CALCULATE EXTINCTION COEFFICIENTS (R_Lambda)---------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 3,630 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcInstrMag.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxx-----------Calculate Instrumental Magnitudes From TXDumped Photometry Files--------------xxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,705 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcTrueSecStdMagBVRI.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxx---------Calculate True Magnitudes Of The Secondary Standards In The SN Field----------xxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 35,964 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcSNMag_6.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxx---------Calculate SN Magnitudes For All The Epochs Using Secondary Standard Magnitudes---------xxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 26,132 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcInstrMag_2.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxx-----------Calculate Instrumental Magnitudes From TXDumped Photometry Files--------------xxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,715 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcInstrMagDOT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxx-----------Calculate Instrumental Magnitudes From TXDumped Photometry Files--------------xxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 12,875 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcTrueSecStdMagUBVRI.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxx---------Calculate True Magnitudes Of The Secondary Standards In The SN Field----------xxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 36,342 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | calibrate/CalcSNMagDOT.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxx---------Calculate SN Magnitudes For All The Epochs Using Secondary Standard Magnitudes---------xxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 26,475 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | spectroscopy/PostProcSpec.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxx-------------------------SPECTROSCOPIC DATA REDUCTION-----------------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 35,404 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | spectroscopy/PostProcSpec_2.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxx-------------------------SPECTROSCOPIC DATA REDUCTION-----------------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 36,060 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | spectroscopy/BBFluxCalibSpec.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxx-----------------OBTAIN SED AND FIT BLACKBODY FROM PHOTOMETRY---------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 24,923 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | spectroscopy/PostProcSpec_3.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxx-------------------------SPECTROSCOPIC DATA REDUCTION-----------------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 34,649 |
[ascl:2106.024] | https://github.com/sPaMFouR/RedPipe | spectroscopy/FluxCalib_5.py | #!/usr/bin/env python
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxx-------------------------FLUX CALIBRATION OF 1-D Spectra----------------------xxxxxxxxxxxxxxxxxxxx #
# xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx... | Python | Unknown | 26,340 |
[ascl:2103.004] | https://github.com/multiwavelength/redshifts | redshiftconfig.yaml | # Search radius
radius: 2 arcmin
# Uncertainty in redshift to classify a measurement as photometric
uncertainty: 0.002
banned_catalogs_redshift:
- glade1
- glade2
- VIII/29A/abelclus
- J/A+A/425/367/reflex50
- J/A+A/425/367/reflex70
- VII/283/catalog
- VII/258/vv10
- J/ApJS/196/11
- J/A+AS/103/349
... | YAML | null | 1,073 |
[ascl:2103.004] | https://github.com/multiwavelength/redshifts | pyproject.toml | [tool.poetry]
name = "redshift"
version = "0.1.0"
description = ""
authors = ["Andra Stroe <andra.stroe@cfa.harvard.edu>"]
[tool.poetry.dependencies]
python = "^3.8"
pyyaml = "^5.3.1"
astroquery = "^0.4"
astropy = "^4.0.1"
colorama = "^0.4.3"
numpy = "^1.18.4"
click = "^7.1.2"
pydantic = "^1.5.1"
[tool.poetry.dev-dep... | TOML | null | 503 |
[ascl:2103.004] | https://github.com/multiwavelength/redshifts | README.md | # **redshifts**
## What is **redshifts**
**redshifts** is a Python package which collects all unique spectroscopic redshifts from online databases such as VizieR and NED.
[](https://zenodo.org/badge/latestdoi/237040021)
## Features
- Flexible search within a radius of ... | Markdown | null | 3,224 |
[ascl:2103.004] | https://github.com/multiwavelength/redshifts | redshifts/query.py | import os
from io import BytesIO, StringIO
import shutil
import subprocess
from collections import defaultdict
import operator
from functools import reduce
from colorama import Fore
import numpy as np
from astroquery.vizier import Vizier
from astroquery.ned import Ned
from astropy.table import Column, QTable, Table, v... | Python | null | 22,427 |
[ascl:2103.004] | https://github.com/multiwavelength/redshifts | redshifts/constants.py | import yaml
from dataclasses import replace, asdict, is_dataclass, field
from typing import List
from pydantic.dataclasses import dataclass
from astropy import units as u
class Quantity(u.SpecificTypeQuantity):
"""
Validation of the types of unit for each parameter, to ensure the right type
is being give... | Python | null | 1,250 |
[ascl:2103.004] | https://github.com/multiwavelength/redshifts | redshifts/main.py | import os
import warnings
warnings.filterwarnings("ignore")
import click
import redshifts.query as q
import redshifts.constants as c
def redshifts(path, name, RA, DEC, config_path):
# Read in configuration
config = c.read_config(config_path)
# Run the query
q.run_query(path, name, RA, DEC, config)
... | Python | null | 956 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | .travis.yml | language: python
python:
- "3.8.3"
before_install:
- sudo apt-get -y install libbz2-dev
install:
- pip install -r requirements.txt
- python setup.py install
script:
- pytest py/redvsblue/test/test_cor.py -s
| YAML | null | 228 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | setup.py | #!/usr/bin/env python
import glob
from setuptools import setup
scripts = glob.glob('bin/*')
description = "Redshift fitter from PCA and redshift priors"
exec(open('py/redvsblue/_version.py').read())
version = __version__
with open('requirements.txt') as f:
REQUIRED = f.read().splitlines()
setup(name="redvsbl... | Python | null | 714 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | requirements.txt | fitsio>=1.1.5
healpy>=1.15.0
matplotlib>=3.4.3
numpy>=1.21.4
scipy>=1.7.2
setuptools>=58.5.3
| Text | null | 93 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | README.md | # redvsblue
"redshift versus blueshift"<br/>
Quasar and emission line precise redshift fitting from prior
## Presentation
This package aims at measuring a precise redshift
given a broad redshift prior.
To do so the package, for each emission line or the full spectrum:
* Runs a coarse chi2 scan as a function of red... | Markdown | null | 4,067 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | CHANGELOG.md | # Release Notes
## Version 0.0.4 - 2021/11/10
* Correct importing lib with . (relative)
* sort requirements with pipreqs
* numba does not seem to be needed
## Version 0.0.3 - 2021/10/21
* Get requirements directly from file
## Version 0.0.2 - 2021/10/06
* Improve the way the version number is defined
| Markdown | null | 306 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/fitz.py | import scipy as sp
from .zwarning import ZWarningMask as ZW
def find_minima(x):
ii = sp.where(sp.r_[True, x[1:]<=x[:-1]] & sp.r_[x[:-1]<=x[1:], True])[0]
jj = sp.argsort(x[ii])
return ii[jj]
def minfit(x, y):
"""
"""
if x.size<3:
return None
try:
#- y = a x^2 + b x + c... | Python | null | 1,360 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/_version.py | __version__ = '0.0.4'
| Python | null | 22 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/read_SDSS_data.py | from __future__ import print_function
import os
import sys
import fitsio
from functools import partial
import numpy as np
import scipy as sp
import scipy.special
import glob
from .utils import print, get_dz, unred, transmission_Lyman, weighted_var
from ._zscan import _zchi2_one
from .fitline import fit_spec_redshift
... | Python | null | 21,377 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/zwarning.py |
class ZWarningMask(object):
SKY = 2**0 #- sky fiber
LITTLE_COVERAGE = 2**1 #- too little wavelength coverage
SMALL_DELTA_CHI2 = 2**2 #- chi-squared of best fit is too close to that of second best
NEGATIVE_MODEL = 2**3 #- synthetic spectrum is negative
MANY_OUTLIERS = 2**... | Python | null | 1,494 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/constants.py | # Lyman-alpha from eqn 5 of Calura et al. 2012 (Arxiv: 1201.5121)
# Other from eqn 1.1 of Irsic et al. 2013 , (Arxiv: 1307.3403)
# Lyman-limit from abstract of Worseck et al. 2014 (Arxiv: 1402.4154)
Lyman_series = {
'LYA' : { 'line':1215.67, 'A':0.0023, 'B':3.64, 'var_evol':3.8 },
'LYB' : { 'l... | Python | null | 1,234 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/fitline.py | from functools import partial
import numpy as np
import scipy as sp
import scipy.special
from .utils import get_dz, transmission_Lyman
from .zwarning import ZWarningMask as ZW
from ._zscan import _zchi2_one
from .fitz import minfit, maxLine, find_minima
def fit_spec_redshift(z, lam, flux, weight, wflux, modelpca, leg... | Python | null | 4,330 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/plot.py | import fitsio
import scipy as sp
from scipy.interpolate import interp1d
import matplotlib.pyplot as plt
from . import constants
def plot_flux_calibration(path):
"""
"""
h = fitsio.FITS(path)
ll_st = h[1]['LOGLAM'][:]
st = h[1]['STACK'][:]
w = st!=0.
h.close()
plt.plot(10**ll_st[w],s... | Python | null | 1,824 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/read_DESI_data.py | from __future__ import print_function
import healpy
import sys
import fitsio
from functools import partial
import numpy as np
import scipy as sp
import scipy.special
from .utils import print, get_dz, unred, transmission_Lyman
from .fitline import fit_spec_redshift
def read_cat(pathData,zmin=None,zmax=None,zkey='Z',sp... | Python | null | 8,393 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/utils.py | from __future__ import print_function
import os
import sys
import fitsio
import numpy as np
import scipy as sp
import scipy.ndimage
import scipy.interpolate as interpolate
from scipy.interpolate import interp1d
from .constants import Lyman_series
try:
import __builtin__
except ImportError:
import builtins as... | Python | null | 5,562 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/__init__.py | from ._version import __version__
| Python | null | 34 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/_zscan.py | import scipy as sp
import warnings
warnings.filterwarnings('error')
warnings.filterwarnings('ignore', category=DeprecationWarning)
warnings.filterwarnings('ignore', category=FutureWarning)
warnings.filterwarnings('ignore', category=RuntimeWarning)
def _zchi2_one(Tb, weights, flux, wflux, zcoeff):
"""
"""
... | Python | null | 620 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/test/test_cor.py | import unittest
import os
import tempfile
import shutil
from pkg_resources import resource_filename
import subprocess
import fitsio
import numpy as np
import scipy as sp
class TestCor(unittest.TestCase):
@classmethod
def setUpClass(cls):
cls._branchFiles = tempfile.mkdtemp()+"/"
@classmethod
... | Python | null | 6,038 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/test/__init__.py | import unittest
import os
def test_suite():
"""
Returns unittest.TestSuite of redvsblue tests for use by setup.py
"""
thisdir = os,pathdirname(dirname(__file__))
return unittest.defaultTestLoader.discover(thisdir,top_level_dir=dirname(thisdir))
| Python | null | 271 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/test/data/data/sdss/README.md | ```bash
wget https://dr14.sdss.org/sas/dr14/eboss/spectro/redux/v5_10_0/spectra/lite/5138/spec-5138-55830-0020.fits
wget https://dr14.sdss.org/sas/dr14/eboss/spectro/redux/v5_10_0/spectra/lite/4300/spec-4300-55528-0224.fits
```
| Markdown | null | 228 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | py/redvsblue/test/data/data/desi/README.md | ```bash
quickquasars
-i /project/projectdirs/desi/mocks/lya_forest/london/v6.0/v6.0.0/0/0/transmission-16-0.fits
--outdir test-0-0/spectra-16/
--zbest
--bbflux
--eboss
--seed 123
--sigma_kms_fog 0.
--zmin 1.8
--metals LYB
--nmax 1
```
```bash
desi_zcatalog
-i test-0-0/spectra-16/
-o test-0-0/zcat.fits
--fibermap
```
| Markdown | null | 319 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | bin/redvsblue_VAR_SNR.py | #!/usr/bin/env python
import argparse
import fitsio
import numpy as np
import scipy as sp
import copy
from functools import partial
from multiprocessing import Pool,Lock,cpu_count,Value
from redvsblue import read_SDSS_data, constants, utils
if __name__ == '__main__':
parser = argparse.ArgumentParser(formatter_cl... | Python | null | 5,802 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | bin/redvsblue_compute_PCA.py | #!/usr/bin/env python
import argparse
import fitsio
import empca
from functools import partial
import numpy as np
import scipy as sp
from desispec.interpolation import resample_flux
from redvsblue import read_SDSS_data, utils
from redvsblue.utils import unred, print
if __name__ == '__main__':
parser = argparse.A... | Python | null | 10,828 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | bin/redvsblue_lineFitter.py | #!/usr/bin/env python
import argparse
import fitsio
import numpy as np
import scipy as sp
import copy
from functools import partial
from multiprocessing import Pool,Lock,cpu_count,Value
import redvsblue
from redvsblue import read_SDSS_data, read_DESI_data, constants, utils
from redvsblue.zwarning import ZWarningMask a... | Python | null | 13,625 |
[ascl:2106.017] | https://github.com/londumas/redvsblue | etc/dr16-line-sky-mask.txt | #
# File to veto lines in observed frame.
#
# Mask produced with pipeline version v5_11_0
# via masking large sharp variance feature in
# do_cf1d.py of Lya forest [1040,1200]
# calibration forest [2900,3120]
#
CaII 3930.1 3938.2 OBS
CaII 3965.5 3973.8 OBS
sky 4043.0 4051.3 OBS
sky 4353.1 4365.1 OBS
sky 5456.8 5467.3... | Text | null | 394 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | tf_fit.c | /* The following routines implement all of the fitting formulae in
Eisenstein \& Hu (1997) */
/* There are two sets of routines here. The first set,
TFfit_hmpc(), TFset_parameters(), and TFfit_onek(),
calculate the transfer function for an arbitrary CDM+baryon universe using
the fitting formula in Section 3 of th... | C | null | 13,980 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | nbody.h | /* in allotarrays.c */
float **allocate_float_2d(long N1,int N2);
float ***allocate_fftwf_3d(long N1,long N2,long N3);
float Hf(float aa),Df(float aa),ff(float aa);
void Setting_Up_Memory_For_Ro(float av);
void cic(float** rra);
void Get_Phi(int i);
void Update_v(float aa,float delta_aa,float **rra,float **vva);
void ... | C/C++ Header | null | 2,875 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | allotarrays.c | #include<stdlib.h>
#include<fftw3.h>
float ***allocate_fftwf_3d(long N1,long N2,long N3)
{
long ii,jj;
long asize,index;
float ***phia, *phi;
phia=(float ***) fftwf_malloc (N1 * sizeof(float **));
for(ii=0;ii<N1;++ii)
phia[ii]=(float **) fftwf_malloc (N2 * sizeof(float *));
asize = N1*N2;
as... | C | null | 1,015 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | power1.h | float TFfit_onek(float k, float *tf_baryon, float *tf_cdm);
void TFset_parameters(float omega0hh, float f_baryon, float Tcmb);
float TFzerobaryon(float omega0, float hubble, float Tcmb, float k_hmpc);
/*
int TFmdm_set_cosm(float omega_matter, float omega_baryon, float omega_hdm,int degen_hdm, float omega_lambda, float ... | C/C++ Header | null | 429 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | ionz_funcs.c | #include<stdio.h>
#include<math.h>
#include<stdlib.h>
#include<string.h>
#include<fftw3.h>
#include"nbody.h"
#include<omp.h>
/*---------------------GLOBAL VARIABLES declaration---------------------*/
extern float vhh, // Hubble parameter
vomegam, // Omega_matter; total matter density (baryons+CDM) parameter
vo... | C | null | 21,597 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | ionz_main.c | #include<stdio.h>
#include<math.h>
#include<stdlib.h>
#include<string.h>
#include<fftw3.h>
#include<omp.h>
#include"nbody.h"
/*------------------------------GLOBAL VARIABLES-------------------------------*/
//-----------------------------------------------------------------------------//
// ... | C | null | 14,543 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | nbody_funcs.c | #include<stdio.h>
#include<math.h>
#include<stdlib.h>
#include<string.h>
#include<fftw3.h>
#include"nbody.h"
#include<omp.h>
/*---------------------GLOBAL VARIABLES declaration---------------------*/
// Cosmological parameters read from input file "input.zel"
extern float vhh, // Hubble parameter
vomegam, // Omeg... | C | null | 40,299 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | funcs.c | /* ----------------------------------------------------
This has various functions - needed in cosmology
Df(aa) - calculates normalized D(a) (growing mode) at scale factor
aa=1/(1+z) D(1) = 1
ff(aa) - calculates f(a) (dlnD/dlna) at scale factor aa=1/(1+z)
ONLY works for FRW universe with ordinary matter (vomeg... | C | null | 5,272 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | powerspec.c | #include<math.h>
#include<stdio.h>
#include <stdlib.h>
#include "power1.h"
/*
PK(k) is the power spectrum divided by (2 \pi^2) : Pk = A k^n T(k) /(2 pi^2)
kk is wavenumber (in Mpc^{-1}) and power spectrum is in units (Mpc^3).
Notice there are no 'h's in the definitions.
*/
extern float norm,vhh;
float Pk(flo... | C | null | 1,181 |
[ascl:2107.005] | https://github.com/rajeshmondal18/ReionYuga | README.md | # ReionYuga
This is an open-source code to generate the Epoch of Reionization (EoR) neutral Hydrogen (HI) field (successively the redshifted 21-cm signal) within a cosmological simulation box. It is based on semi-numerical techniques. It is written in C. The code is coupled with our N-body code https://github.com/rajes... | Markdown | null | 1,483 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | compile_to_xspec.sh | echo "initpackage relagn lmod_relagn.dat `pwd`/src/fortran_version/relagn_dir" | xspec
echo "initpackage relqso lmod_relqso.dat `pwd`/src/fortran_version/relqso_dir" | xspec
echo "lmod relagn `pwd`/src/fortran_version/relagn_dir" | xspec
echo "lmod relqso `pwd`/src/fortran_version/relqso_dir" | xspec
| Shell | null | 303 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | init_autoLoad_xspec.sh | echo "lmod relagn `pwd`/src/fortran_version/relagn_dir" >> ~/.xspec/xspec.rc
echo "lmod relqso `pwd`/src/fortran_version/relqso_dir" >> ~/.xspec/xspec.rc
| Shell | null | 154 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | README.md | # RELAGN
Spectral model for the calculation of AGN SEDs, ranging from the Optical/UV (outer accretion disc) to the Hard X-ray (Innermost X-ray Corona), including
a fully relativistic treatment. If this code is useful to your work, then please reference: **Hagen & Done (2023b)** (https://ui.adsabs.harvard.edu/abs/20... | Markdown | null | 9,143 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | tests/blurr_test.py | #!/usr/bin/env python3
# -*- coding: utf-8 -*-
"""
Created on Mon Mar 14 11:46:24 2022
@author: wljw75
"""
"""
Tests the relconv convolution on a simple gaussian with a r^-3 emissivity
law - as this should (hoefully!) give the same as kdblur
"""
import numpy as np
import xspec
import matplotlib.pyplot as plt
xspe... | Python | null | 5,110 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | tests/relqso_spec.py | #!/usr/bin/env python3
# -*- coding: utf-8 -*-
"""
Created on Tue Dec 6 15:55:23 2022
@author: Scott Hagen
"""
import numpy as np
import matplotlib.pyplot as plt
import os
import sys
mdir = os.path.abspath(__file__)
mdir = mdir.replace('/tests/relagn_spec.py', '/src/python_version')
sys.path.append(mdir)
from rela... | Python | null | 940 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | tests/relagn_spec.py | #!/usr/bin/env python3
# -*- coding: utf-8 -*-
"""
Created on Tue Dec 6 15:20:33 2022
@author: Scott Hagen
code to play around with the relagn model - test to see if it gives spectra,
unit handling, etc
"""
import numpy as np
import matplotlib.pyplot as plt
import os
import sys
mdir = os.path.abspath(__file__)
mdi... | Python | null | 1,526 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | docs/relagn_docs.tex | \documentclass[a4paper, 11pt, times, onecolumn]{article}
\usepackage{geometry}
\geometry{left=20mm, right=20mm}
\usepackage{titling}
\usepackage{graphics, graphicx, epsfig, ulem}
\usepackage{amsmath}
\usepackage{xcolor}
\usepackage{hyperref}
\hypersetup{colorlinks=true, linkcolor=blue, urlcolor=blue}
\usepackage{... | LaTeX | null | 25,772 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | examples/relagn_modSpec.ipynb | {
"cells": [
{
"cell_type": "markdown",
"id": "56bbdcd5",
"metadata": {},
"source": [
"# Example on using relagn to create an SED\n",
"We will start by creating and plotting the SED corresponding to the model defualts (i.e defualt input parameters, and output units)\n",
"\n",
"We will the... | Jupyter Notebook | null | 212,036 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | examples/relqso_modSpec.ipynb | {
"cells": [
{
"cell_type": "markdown",
"id": "e309ebfe",
"metadata": {},
"source": [
"# Example using relqso to create an SED\n",
"\n",
"This is a quick introduction on how to use relqso to create a model SED\n",
"This is a simplified version of relagn, only taking a handful of parameter... | Jupyter Notebook | null | 204,498 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | src/fortran_version/relqso_dir/relqso.f | c Updated version of QSOSED
c Ref. Hagen and Done (in prep.)
c
c The model consists of two regions: a warm
c Comptonization region where the disc has not thermalised properly,
c and a spherical inner corona modelled as a hot Comptonization
c region. All the energetics are calculated in the... | Fortran | null | 26,019 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | src/fortran_version/relagn_dir/relagn.f | c Fortran version of RELAGN
c Ref. Hagen and Done (in prep.)
c
c Calculates AGNSED (Kubota & Done 2018) with relativistic
c corrections applied at each annulus using KYCONV
c (Dovciak, Karas & Yaqoob 2004)
c
c The model consists of three regions: a standard outer disc, a warm
c Compto... | Fortran | null | 24,175 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | src/python_version/pyNTHCOMP.py |
"""
This was taken from https://github.com/arnauqb/qsosed/tree/master/qsosed,
which in turn was taken from https://github.com/ADThomas-astro/oxaf/blob/master/oxaf.py .
Credit to A.D. Thomas.
Code was adapted from Xspec for https://arxiv.org/pdf/1611.05165.pdf .
"""
import numpy as np
def donthcomp(ear, param):
... | Python | null | 9,946 |
[ascl:2306.023] | https://github.com/scotthgn/relagn | src/python_version/relagn.py | #!/usr/bin/env python3
# -*- coding: utf-8 -*-
"""
Created on Thu Mar 10 16:50:31 2022
@author: Scott Hagen
Relativistic versions of AGNSED (RELAGN) and QSOSED (RELQSO) (Kubota & Done 2018).
The relativistic corrections are calculated using the convolution code
KYCONV (Dovciak, Karas & Yaqoob 2004)
For the Comptonis... | Python | null | 60,113 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | README.md | Full readme in README.pdf
Details of the code are described in “Efficient Computation of Galaxy Bias with Neutrinos
and Other Relics” J.B. Muñoz and C. Dvorkin (2018) Phys. Rev. D 98, 043503 [arXiv:1805.11623].
| Markdown | null | 219 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | example_input.ini | //This file specifies the parameters that RelicFast takes, and gives some fiducial values.
//Make sure that if you add new stuff the code is consistent, and that the first instance of every variable name is right before the equal sign.
//Halo parameters
N_Mhalo = 1 ;//number of halo masses, logspaced. If 1 it c... | Config | null | 2,114 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | source/RelicFast.cpp | ////////////////////////////////////////////////////////////////////////////////////////
//
// Code to find the bias of DM haloes of different masses, at different redshifts--
// --including scale-dependent effects from relics, such as neutrinos.
// By Julian B Munoz (05/2018 @Harvard)
//
////////////////////////////... | C++ | null | 3,699 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | source/pressure.cpp | ////////////////////////////////////////////////////////////////////////////////////
//
// Code to compute the pressure and energy density of an additional non-CDM component
// given its mass and temperature, assuming it's a thermal relic, you can get rho and p.
// By Julian B Munoz (05/2018 @Harvard)
//
/////////////... | C++ | null | 2,926 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | source/collapse.cpp | ////////////////////////////////////////////////////////////////////////////////////////
//
// Code to find the delta_crit necessary for halo of mass Mhalo
// to collapse by some redshift z_collapse.
// By Julian B Munoz (05/2018 @Harvard)
//
/////////////////////////////////////////////////////////////////////////////... | C++ | null | 90,670 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | source/auxiliar.cpp | ////////////////////////////////////////////////////////////////////////////////////////
//
// Auxiliar functions for RelicFast.
// By Julian B Munoz (05/2018 @Harvard)
//
////////////////////////////////////////////////////////////////////////////////////////
#include "auxiliar.h"
//////////////////////////////////
... | C++ | null | 16,938 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | source/boltzmann_Calls.cpp | ////////////////////////////////////////////////////////////////////////////////////////
//
// Code to call a Boltzmann solve (CLASS or CAMB)
// as well as to read the transfer functions from it.
// By Julian B Munoz (05/2018 @Harvard)
//
/////////////////////////////////////////////////////////////////////////////////... | C++ | null | 34,872 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | source/bias.cpp | ////////////////////////////////////////////////////////////////////////////////////////
//
// Code to find the bias of a halo of mass Mhalo
// Input \delta_initial and \delta_crit
// output b_L and b_E (Lagrangian and Eulerian biases)
// By Julian B Munoz (05/2018 @Harvard)
//
////////////////////////////////////////... | C++ | null | 15,144 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | include/boltzmann_Calls.h | #ifndef __BOLTZ_H_INCLUDED__
#define __BOLTZ_H_INCLUDED__
#include <stdio.h>
#include <math.h>
#include <stdlib.h>
#include <string.h>
#include <iostream>
#include <fstream>
#include "common.h"
#include "auxiliar.h"
//tests
int tests_pre_run(Cosmology *cosmo);
//Read the transfer functions from the chosen Bol... | C/C++ Header | null | 1,860 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | include/auxiliar.h |
#ifndef __AUX_H_INCLUDED__
#define __AUX_H_INCLUDED__
#include <stdio.h>
#include <math.h>
#include <stdlib.h>
#include <string.h>
#include "common.h"
//array functions:
double *allocate_1D_array(int n1);
int *allocate_1D_array_int(int n1);
double **allocate_2D_array(int n1, int n2);
void free_2D_array(dou... | C/C++ Header | null | 2,653 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | include/RelicFast.h |
#ifndef __RELICFAST_H_INCLUDED__
#define __RELICFAST_H_INCLUDED__
#include <stdio.h>
#include <math.h>
#include <stdlib.h>
#include <string.h>
#include <iostream>
#include <fstream>
#include "auxiliar.h"
#include "bias.h"
#include "boltzmann_Calls.h"
#include "collapse.h"
#include "common.h"
#endi... | C/C++ Header | null | 322 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | include/bias.h |
#ifndef __BIAS_H_INCLUDED__
#define __BIAS_H_INCLUDED__
#include <stdio.h>
#include <math.h>
#include <stdlib.h>
#include <string.h>
#include "common.h"
#include "auxiliar.h"
#include "boltzmann_Calls.h"
int get_bias(Cosmology *cosmo, double *zlist_transfer);
#endif
| C/C++ Header | null | 278 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | include/pressure.h | #ifndef __PRESS_H_INCLUDED__
#define __PRESS_H_INCLUDED__
#include <stdio.h>
#include <math.h>
#include "common.h"
double pressure_WDM(double mass, double Temp);
double density_WDM(double mass, double Temp);
double EoS_WDM(double mass, double Temp);
#endif
| C/C++ Header | null | 273 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | include/collapse.h | #ifndef __COLL_H_INCLUDED__
#define __COLL_H_INCLUDED__
#include <stdio.h>
#include <math.h>
#include <stdlib.h>
#include <string.h>
#include "common.h"
#include "auxiliar.h"
#include "boltzmann_Calls.h"
#include "pressure.h"
#ifdef _OPENMP
#include <omp.h> // For nested loops.
#endif
//\delta_crit as a func... | C/C++ Header | null | 2,747 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | include/common.h |
#ifndef __COMMON_H_INCLUDED__
#define __COMMON_H_INCLUDED__
#define _CLASS_ 0
#define _CAMB_ 1
#define _FALSE_ 0
#define _TRUE_ 1
//Boltzmann code options:
#define boltzmann_tag _CLASS_ //0 for CLASS, 1 for CAMB. CLASS needed in most cases.
#define run_boltzmann_option _TRUE_ //0 if no, otherwise Y... | C/C++ Header | null | 8,515 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/camb.f90 | !Interface module for CAMB. Call CAMB_GetResults to do the work.
module CAMB
use Precision
use ModelParams
use ModelData
use Transfer
use GaugeInterface
use InitialPower
use Reionization
use Recombination
use lensing
implicit none
Type CAMBdata
Type (ClTrans... | Fortran | null | 18,500 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/recfast.f90 | !Recombination module for CAMB, using RECFAST
!cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc
!C Integrator for Cosmic Recombination of Hydrogen and Helium,
!C developed by Douglas Scott (dscott@astro.ubc.ca)
!C based on calculations in the paper Seager, Sasselov &... | Fortran | null | 47,141 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/inifile.f90 | !Module to read in name/value pairs from a file, with each line of the form line 'name = value'
!Should correctly interpret FITS headers
!Antony Lewis (http://cosmologist.info/). Released to the public domain.
!Apr 11, added support for INCLUDE(file); check for duplicate keys
!Jun 12, added support ... | Fortran | null | 24,516 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/cmbmain.f90 | ! This this is the main CAMB program module.
!
! Code for Anisotropies in the Microwave Background
! by Antony lewis (http://cosmologist.info) and Anthony Challinor
! See readme.html for documentation.
! Note that though the code is internally parallelised, it is not thread-... | Fortran | null | 88,394 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/tester.f90 | !Simple program to get the scalar and tensor Cls, and print them out (and the sum)
program tester
use CAMB
implicit none
integer l
real(dl) ratio
type(CAMBparams) P !defined in ModelParams in modules.f90
call CAMB_SetDefParams(P)
P%omegab = .04... | Fortran | null | 1,815 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/inidriver.F90 | ! Code for Anisotropies in the Microwave Background
! by Antony Lewis (http://cosmologist.info/) and Anthony Challinor
! See readme.html for documentation. This is a sample driver routine that reads
! in one set of parameters and produdes the corresponding output.
program driver
... | Fortran | null | 14,321 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/hyrec.F90 | !---------------------------------------------------------------------------------------------------
! Recombination module for CAMB, using HyRec
! Author: Antony Lewis
!---------------------------------------------------------------------------------------------------
module Recombination
use ... | Fortran | null | 2,073 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/utils.F90 | !Module of generally useful routines and definitions
!Antony Lewis, http://cosmologist.info/
!April 2006: fix to TList_RealArr_Thin
!March 2008: fix to Ranges
!June 2010: fixed bug in DeleteFile gradually using up file units
module Ranges
!A collection of ranges, consisting of sections of... | Fortran | null | 82,796 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/sigma8.f90 | !Simple test program to print out sigma_8 as a function of the CDM density
program GetSigma8
use CAMB
implicit none
integer i
type(CAMBparams) P !defined in ModelParams in modules.f90
call CAMB_SetDefParams(P)
P%WantTransfer= .true.
P%WantCls = ... | Fortran | null | 1,444 |
[ascl:2307.003] | https://github.com/JulianBMunoz/RelicFast | CAMB_Current/cosmorec.F90 | !---------------------------------------------------------------------------------------------------
! Recombination module for CAMB, using CosmoRec
! Author: Richard Shaw (CITA)
!---------------------------------------------------------------------------------------------------
! 08.06.2012: added... | Fortran | null | 6,303 |
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