Astroquery ========== This is the documentation for the Astroquery affiliated package of astropy. Code and issue tracker are on `GitHub `_. Introduction ------------ Astroquery is a set of tools for querying astronomical web forms and databases. The :doc:`api` is intended to be kept as consistent as possible, such that any web service can be used with a minimal learning curve imposed on the user. There are two other packages with complimentary functionality as Astroquery: `astropy.vo `_ is in the Astropy core and `pyvo `_ is an Astropy affiliated package. They are more oriented to general `virtual observatory `_ discovery and queries, whereas Astroquery has web service specific interfaces. Installation ------------ Astroquery must be installed from source: .. code-block:: bash $ git clone git@github.com:astropy/astroquery.git $ cd astroquery $ python setup.py install pip install also works: .. code-block:: bash $ pip install git+http://github.com/astropy/astroquery.git#egg=astroquery Requirements ```````````` The following packages are required for astroquery installation & use: * `numpy `_ * `astropy `_ (v>=0.3) * `requests `_ Using astroquery ---------------- All astroquery modules are supposed to follow the same API. In its simplest form, the API involves queries based on coordinates or object names. Some simple examples, using SIMBAD: .. code-block:: python >>> from astroquery.simbad import Simbad >>> result_table = Simbad.query_object("m1") >>> result_table.pprint(show_unit=True) MAIN_ID RA DEC RA_PREC ... COO_QUAL COO_WAVELENGTH COO_BIBCODE "h:m:s" "d:m:s" ... ------- ----------- ----------- ------- ... -------- -------------- ------------------- M 1 05 34 31.94 +22 00 52.2 6 ... C R 2011A&A...533A..10L All query tools allow coordinate-based queries: .. code-block:: python >>> import astropy.coordinates as coord >>> import astropy.units as u >>> # works only for ICRS coordinates: >>> c = coord.ICRSCoordinates("05h35m17.3s -05h23m28s") >>> r = 5 * u.arcminute >>> result_table = Simbad.query_region(c, radius=r) >>> result_table.pprint(show_unit=True) MAIN_ID RA DEC ... COO_QUAL COO_WAVELENGTH COO_BIBCODE "h:m:s" "d:m:s" ... -------------- ------------- ------------- ... -------- -------------- ------------------- HD 38875 05 34 59.7297 -80 51 09.082 ... A O 2007A&A...474..653V TYC 9390-799-1 05 33 58.2222 -80 50 18.575 ... B 1998A&A...335L..65H Table of Contents ----------------- The modules and their maintainers are listed on the `Maintainers `_ wiki page. The following modules have been completed using a common API: .. toctree:: :maxdepth: 1 simbad.rst vizier.rst irsa_dust.rst ned.rst splatalogue.rst irsa.rst ukidss.rst magpis.rst nrao.rst besancon.rst nist.rst nvas.rst These others are functional, but do not follow a common & consistent API: .. toctree:: :maxdepth: 1 fermi.rst sdss.rst alfalfa.rst sha.rst lamda.rst ogle.rst