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April 15, 2020 03:35
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## When True, use Unicode characters when outputting values, and displaying | |
## widgets at the console. | |
# unicode_output = False | |
## When True, use ANSI color escape sequences when writing to the console. | |
# use_color = True | |
## Maximum number of lines in the display of pretty-printed objects. If not | |
## provided, try to determine automatically from the terminal size. Negative | |
## numbers mean no limit. | |
# max_lines = None | |
## Maximum number of characters per line in the display of pretty-printed | |
## objects. If not provided, try to determine automatically from the terminal | |
## size. Negative numbers mean no limit. | |
# max_width = None | |
[io.fits] | |
## If True, enable support for record-valued keywords as described by FITS WCS | |
## distortion paper. Otherwise they are treated as normal keywords. | |
# enable_record_valued_keyword_cards = True | |
## If True, extension names (i.e. the ``EXTNAME`` keyword) should be treated | |
## as case-sensitive. | |
# extension_name_case_sensitive = False | |
## If True, automatically remove trailing whitespace for string values in | |
## headers. Otherwise the values are returned verbatim, with all whitespace | |
## intact. | |
# strip_header_whitespace = True | |
## If True, use memory-mapped file access to read/write the data in FITS | |
## files. This generally provides better performance, especially for large | |
## files, but may affect performance in I/O-heavy applications. | |
# use_memmap = True | |
## If True, use lazy loading of HDUs when opening FITS files by default; that | |
## is fits.open() will only seek for and read HDUs on demand rather than | |
## reading all HDUs at once. See the documentation for fits.open() for more | |
## datails. | |
# lazy_load_hdus = True | |
## If True, default to recognizing the convention for representing unsigned | |
## integers in FITS--if an array has BITPIX > 0, BSCALE = 1, and BZERO = | |
## 2**BITPIX, represent the data as unsigned integers per this convention. | |
# enable_uint = True | |
[io.votable] | |
## Can be 'exception' (treat fixable violations of the VOTable spec as | |
## exceptions), 'warn' (show warnings for VOTable spec violations), or | |
## 'ignore' (silently ignore VOTable spec violations) | |
# verify = ignore | |
[logger] | |
## Threshold for the logging messages. Logging messages that are less severe | |
## than this level will be ignored. The levels are ``'DEBUG'``, ``'INFO'``, | |
## ``'WARNING'``, ``'ERROR'``. | |
# log_level = INFO | |
## Whether to log `warnings.warn` calls. | |
# log_warnings = True | |
## Whether to log exceptions before raising them. | |
# log_exceptions = False | |
## Whether to always log messages to a log file. | |
# log_to_file = False | |
## The file to log messages to. If empty string is given, it defaults to a | |
## file ``'astropy.log'`` in the astropy config directory. | |
# log_file_path = | |
## Threshold for logging messages to `log_file_path`. | |
# log_file_level = INFO | |
## Format for log file entries. | |
# log_file_format = %(asctime)r, %(origin)r, %(levelname)r, %(message)r | |
## The encoding (e.g., UTF-8) to use for the log file. If empty string is | |
## given, it defaults to the platform-preferred encoding. | |
# log_file_encoding = | |
[nddata] | |
## Whether to issue a warning if `~astropy.nddata.NDData` arithmetic is | |
## performed with uncertainties and the uncertainties do not support the | |
## propagation of correlated uncertainties. | |
# warn_unsupported_correlated = True | |
## Whether to issue a warning when the `~astropy.nddata.NDData` unit attribute | |
## is changed from a non-``None`` value to another value that data | |
## values/uncertainties are not scaled with the unit change. | |
# warn_setting_unit_directly = True | |
[samp] | |
## Whether to allow `astropy.samp` to use the internet, if available. | |
# use_internet = True | |
## How many times to retry communications when they fail | |
# n_retries = 10 | |
[table] | |
## The template that determines the name of a column if it cannot be | |
## determined. Uses new-style (format method) string formatting. | |
# auto_colname = col{0} | |
## The table class to be used in Jupyter notebooks when displaying tables (and | |
## not overridden). See <https://getbootstrap.com/css/#tables for a list of | |
## useful bootstrap classes. | |
# default_notebook_table_class = table-striped table-bordered table-condensed | |
## List of conditions for issuing a warning when replacing a table column | |
## using setitem, e.g. t['a'] = value. Allowed options are 'always', 'slice', | |
## 'refcount', 'attributes'. | |
# replace_warnings = [] | |
## Always use in-place update of a table column when using setitem, e.g. | |
## t['a'] = value. This overrides the default behavior of replacing the | |
## column entirely with the new value when possible. This configuration option | |
## will be deprecated and then removed in subsequent major releases. | |
# replace_inplace = False | |
[table.jsviewer] | |
## The URL to the jquery library. | |
# jquery_url = https://code.jquery.com/jquery-3.1.1.min.js | |
## The URL to the jquery datatables library. | |
# datatables_url = https://cdn.datatables.net/1.10.12/js/jquery.dataTables.min.js | |
## The URLs to the css file(s) to include. | |
# css_urls = ['https://cdn.datatables.net/1.10.12/css/jquery.dataTables.css'] | |
[units.quantity] | |
## The maximum size an array Quantity can be before its LaTeX representation | |
## for IPython gets "summarized" (meaning only the first and last few elements | |
## are shown with "..." between). Setting this to a negative number means that | |
## the value will instead be whatever numpy gets from get_printoptions. | |
# latex_array_threshold = 100 | |
[utils.data] | |
## Primary URL for astropy remote data site. | |
# dataurl = http://data.astropy.org/ | |
## Mirror URL for astropy remote data site. | |
# dataurl_mirror = http://www.astropy.org/astropy-data/ | |
## Default User-Agent for HTTP request headers. This can be overwrittenfor a | |
## particular call via http_headers option, where available.This only provides | |
## the default value when not set by https_headers. | |
# default_http_user_agent = astropy | |
## Time to wait for remote data queries (in seconds). | |
# remote_timeout = 10.0 | |
## Block size for computing file hashes. | |
# compute_hash_block_size = 65536 | |
## Number of bytes of remote data to download per step. | |
# download_block_size = 65536 | |
## Number of seconds to wait for the cache lock to be free. It should normally | |
## only ever be held long enough to copy an already-downloaded file into the | |
## cache, so this will normally only run over if something goes wrong and the | |
## lock is left held by a dead process; the exception raised should indicate | |
## this and what to do to fix it. | |
# download_cache_lock_attempts = 5 | |
## If True, temporary download files created when the cache is inaccessible | |
## will be deleted at the end of the python session. | |
# delete_temporary_downloads_at_exit = True | |
[utils.iers.iers] | |
## Enable auto-downloading of the latest IERS data. If set to False then the | |
## local IERS-B and leap-second files will be used by default. Default is | |
## True. | |
# auto_download = True | |
## Maximum age (days) of predictive data before auto-downloading. Default is | |
## 30. | |
# auto_max_age = 30.0 | |
## URL for auto-downloading IERS file data. | |
# iers_auto_url = ftp://cddis.gsfc.nasa.gov/pub/products/iers/finals2000A.all | |
## Mirror URL for auto-downloading IERS file data. | |
# iers_auto_url_mirror = https://datacenter.iers.org/data/9/finals2000A.all | |
## Remote timeout downloading IERS file data (seconds). | |
# remote_timeout = 10.0 | |
## System file with leap seconds. | |
# system_leap_second_file = | |
## URL for auto-downloading leap seconds. | |
# iers_leap_second_auto_url = https://hpiers.obspm.fr/iers/bul/bulc/Leap_Second.dat | |
## Alternate URL for auto-downloading leap seconds. | |
# ietf_leap_second_auto_url = https://www.ietf.org/timezones/data/leap-seconds.list | |
[visualization.wcsaxes] | |
## The number of samples along each image axis when determining the range of | |
## coordinates in a plot. | |
# coordinate_range_samples = 50 | |
## How many points to sample along the axes when determining tick locations. | |
# frame_boundary_samples = 1000 | |
## How many points to sample along grid lines. | |
# grid_samples = 1000 | |
## The grid size to use when drawing a grid using contours | |
# contour_grid_samples = 200 | |
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