NvasClass¶
- class astroquery.nvas.NvasClass[source]¶
Bases:
BaseQuery
Attributes Summary
Methods Summary
extract_image_urls
(html_in[, get_uvfits])Helper function that uses regexps to extract the image urls from the given HTML.
get_image_list
(coordinates[, radius, ...])Function that returns a list of urls from which to download the FITS images.
get_images
(coordinates[, radius, max_rms, ...])Get an image around a target/ coordinates from the NVAS image archive.
get_images_async
(coordinates[, radius, ...])Serves the same purpose as
get_images
but returns a list of file handlers to remote files.Attributes Documentation
- TIMEOUT = 60¶
- URL = 'https://webtest.aoc.nrao.edu/cgi-bin/lsjouwer/archive-pos.pl'¶
- band_freqs = {'C': (4, 8), 'D': (110, 170), 'E': (60, 90), 'F': (90, 140), 'K': (18, 26.5), 'Ka': (26.5, 40), 'L': (1, 2), 'Q': (30, 50), 'S': (2, 4), 'U': (12, 18), 'V': (50, 75), 'W': (75, 110), 'X': (8, 12)}¶
- valid_bands = ['all', 'L', 'C', 'X', 'U', 'K', 'Q']¶
Methods Documentation
- extract_image_urls(html_in, get_uvfits=False)[source]¶
Helper function that uses regexps to extract the image urls from the given HTML.
- get_image_list(coordinates, radius=<Quantity 0.25 arcmin>, max_rms=10000, band='all', get_uvfits=False, get_query_payload=False)[source]¶
Function that returns a list of urls from which to download the FITS images.
- Parameters:
- coordinatesstr or
astropy.coordinates
object The target around which to search. It may be specified as a string in which case it is resolved using online services or as the appropriate
astropy.coordinates
object. ICRS coordinates may also be entered as strings as specified in theastropy.coordinates
module.- radiusstr or
Quantity
object, optional The string must be parsable by
Angle
. The appropriateQuantity
object fromastropy.units
may also be used. Defaults to 0.25 arcmin.- max_rmsfloat, optional
Maximum allowable noise level in the image (mJy). Defaults to 10000 mJy.
- bandstr, optional
The band of the image to fetch. Valid bands must be from [“all”,”L”,”C”,”X”,”U”,”K”,”Q”]. Defaults to ‘all’
- get_uvfitsbool, optional
Gets the UVfits files instead of the IMfits files when set to
True
. Defaults toFalse
.- get_query_payloadbool, optional
if set to
True
then returns the dictionary sent as the HTTP request. Defaults toFalse
.
- coordinatesstr or
- Returns:
- list of image urls
- get_images(coordinates, radius=<Quantity 0.25 arcmin>, max_rms=10000, band='all', get_uvfits=False, verbose=True, get_query_payload=False, show_progress=True)[source]¶
Get an image around a target/ coordinates from the NVAS image archive.
- Parameters:
- coordinatesstr or
astropy.coordinates
object The target around which to search. It may be specified as a string in which case it is resolved using online services or as the appropriate
astropy.coordinates
object. ICRS coordinates may also be entered as strings as specified in theastropy.coordinates
module.- radiusstr or
Quantity
object, optional The string must be parsable by
Angle
. The appropriateQuantity
object fromastropy.units
may also be used. Defaults to 0.25 arcmin.- max_rmsfloat, optional
Maximum allowable noise level in the image (mJy). Defaults to 10000 mJy.
- bandstr, optional
The band of the image to fetch. Valid bands must be from [“all”,”L”,”C”,”X”,”U”,”K”,”Q”]. Defaults to ‘all’
- get_uvfitsbool, optional
Gets the UVfits files instead of the IMfits files when set to
True
. Defaults toFalse
.- verbosebool, optional
- get_query_payloadbool, optional
if set to
True
then returns the dictionary sent as the HTTP request. Defaults toFalse
.
- coordinatesstr or
- Returns:
- A list of
HDUList
objects
- A list of
- get_images_async(coordinates, radius=<Quantity 0.25 arcmin>, max_rms=10000, band='all', get_uvfits=False, verbose=True, get_query_payload=False, show_progress=True)[source]¶
Serves the same purpose as
get_images
but returns a list of file handlers to remote files.- Parameters:
- coordinatesstr or
astropy.coordinates
object The target around which to search. It may be specified as a string in which case it is resolved using online services or as the appropriate
astropy.coordinates
object. ICRS coordinates may also be entered as strings as specified in theastropy.coordinates
module.- radiusstr or
Quantity
object, optional The string must be parsable by
Angle
. The appropriateQuantity
object fromastropy.units
may also be used. Defaults to 0.25 arcmin.- max_rmsfloat, optional
Maximum allowable noise level in the image (mJy). Defaults to 10000 mJy.
- bandstr, optional
The band of the image to fetch. Valid bands must be from [“all”,”L”,”C”,”X”,”U”,”K”,”Q”]. Defaults to ‘all’
- get_uvfitsbool, optional
Gets the UVfits files instead of the IMfits files when set to
True
. Defaults toFalse
.- verbosebool, optional
- get_query_payloadbool, optional
if set to
True
then returns the dictionary sent as the HTTP request. Defaults toFalse
.
- coordinatesstr or
- Returns:
- A list of context-managers that yield readable file-like objects