Lightcurve Project

Hello, and welcome to the lightcurve documentation. So far it’s pretty useless, but hopefully it makes you feel better that it at least exists.

variable source

Contents:

Installation instructions

Install via Anaconda

Note

If you do not have Anaconda, please follow the instructions here to install it, or scroll down for manual installation of lightcurve.

After you have anaconda setup, then you can install lightcurve by specifying the channel in your install command:

$ conda install --channel justincely lightcurve

Install vi pip

If you have pip installed:

$ pip install lightcurve

Install from source

Refstis can also be installed manually using the source code:

$ git clone https://github.com/spacetelescope/lightcurve.git
$ cd lightcurve
$ python setup.py install

Simple extraction

Performing a basic lightcurve extraction from either COS or STIS individual datasets is achieved by a simple call to read() as shown below.

>>> import lightcurve
>>> table = lightcurve.read('lbova4b2q_corrtag_a.fits')

This returns the extracted data as an Astropy Table, which can be used for further analysis and plotting.

>>> type(lc)
astropy.table.table.Table

>>> lc
<Table length=750>
dataset background      mjd       error    bins  ...      flux      signal_to_noise  counts  gross       net
float64  float32      float64    float32 float64 ...    float64         float32     float32 float32    float64
------- ---------- ------------- ------- ------- ... -------------- --------------- ------- ------- -------------
    1.0    12.7314 55899.6041542 46.6337     1.0 ... 0.154727564001         46.3607 2149.24 2161.97 2149.23583984
    1.0    15.3585 55899.6041658 45.9691     1.0 ... 0.149929073704          45.635 2082.44  2097.8 2082.44238281
    1.0     11.119 55899.6041774  45.537     1.0 ... 0.147685074003         45.2928 2051.38  2062.5  2051.3815918
    1.0    16.2978 55899.6041889 45.5294     1.0 ... 0.146895813966         45.1715 2040.33 2056.63 2040.33349609
...

Instrument-specific extraction

More specific tailored extractions for each instrument can be seen on their respective pages below. These detail specific options for extracion, as well as how to setup parameters and reference files.

Extracting COS data

logo for the COS instrument
Reference API

Utility functions for extracting COS spectral data into lightcurves

Functions
extract(filename, \*\*kwargs) Extract lightcurve from COS dataset
collect_inputs(filename) Populate HDU dictionary from available corrtag files
get_both_filenames(filename) Get a list of both filenames for FUV data
get_extraction_region(hdu, segment[, mode]) Get y_start,y_end for given extraction

Extracting STIS data

logo for the STIS instrument
Reference API

Utility functions for extracting STIS spectral data into lightcurves

Functions
extract(filename, \*\*kwargs) Extract lightcurve from STIS dataset
stis_corrtag(tagfile[, clean]) Create a COS-like corrtag file for STIS data
map_image
epsilon(tagfile) Compute the total epsilon factor for each event
dqinit(tagfile) Compute the data quality information for each pixel from the BPIXTAB.

Complete API

lightcurve.io

Library of I/O routines to get data into a LightCurve object.

Functions

check_filetype(filename) Determine the type of data being input.
read([source])
composite(filelist, output[, trim]) Creates a composite lightcurve from files in filelist and saves it to the save_loc.
prepare_header(filename, filelist) Prepare headers with MAST requirements

lightcurve.analysis

Functions

lomb(time, counts, frequencies) Compute the lombscargle periodigram

lightcurve.cos

Utility functions for extracting COS spectral data into lightcurves

Functions

extract(filename, \*\*kwargs) Extract lightcurve from COS dataset
collect_inputs(filename) Populate HDU dictionary from available corrtag files
get_both_filenames(filename) Get a list of both filenames for FUV data
get_extraction_region(hdu, segment[, mode]) Get y_start,y_end for given extraction

lightcurve.stis

Utility functions for extracting STIS spectral data into lightcurves

Functions

extract(filename, \*\*kwargs) Extract lightcurve from STIS dataset
stis_corrtag(tagfile[, clean]) Create a COS-like corrtag file for STIS data
map_image
epsilon(tagfile) Compute the total epsilon factor for each event
dqinit(tagfile) Compute the data quality information for each pixel from the BPIXTAB.

lightcurve.utils

General purpose utility functions

Functions

expand_refname(refname) Expand header reference file name to full path if $ is present.
enlarge(a[, x, y]) Enlarges 2D image array a using simple pixel repetition in both dimensions.
is_uniq(values) Check if input items are unique

Issue Reporting

If you find bugs, problems, or even new features that you’d like to see, please report it on the github issue tracker.

Citing

TODO