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added remote data directive
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‎docs/imcce/imcce.rst

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@@ -1,5 +1,3 @@
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.. doctest-skip-all
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.. _astroquery.imcce:
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******************************************************************************************************************************************
@@ -17,7 +15,7 @@ IMCCE provides a number of Solar System-related services, two of which are curre
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* `Miriade <http://vo.imcce.fr/webservices/miriade/>`_: ephemerides service
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Use cases for both services are detailed below.
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SkyBot - Solar System Body Identification Service
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=================================================
@@ -32,14 +30,15 @@ A simple cone search for Solar System objects in a circular field
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looks like this:
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.. code-block:: python
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.. doctest-remote-data::
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>>> from astroquery.imcce import Skybot
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>>> from astropy.coordinates import SkyCoord
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>>> from astropy.time import Time
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>>> import astropy.units as u
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>>> field = SkyCoord(0*u.deg, 0*u.deg)
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>>> epoch = Time('2019-05-29 21:42', format='iso')
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>>> Skybot.cone_search(field, 5*u.arcmin, epoch) # doctest: +SKIP
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>>> Skybot.cone_search(field, 5*u.arcmin, epoch) # doctest: +IGNORE_OUTPUT
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<QTable length=2>
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Number Name RA ... vy vz epoch
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deg ... AU / d AU / d d
@@ -50,8 +49,8 @@ looks like this:
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`~astroquery.imcce.SkybotClass.cone_search` produces a
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`~astropy.table.QTable` object with the properties of all Solar System
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bodies that are present in the cone at the given epoch.
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bodies that are present in the cone at the given epoch.
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The required input arguments for
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`~astroquery.imcce.SkybotClass.cone_search` are the center coordinates
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of the cone, its radius, as well as the epoch of the
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query looks like this:
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.. code-block:: python
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.. doctest-remote-data::
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>>> from astroquery.imcce import Miriade
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>>> Miriade.get_ephemerides('Ceres') # doctest: +IGNORE_OUTPUT
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<Table length=1>
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target epoch RA ... DEC_rate delta_rate
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d deg ... arcsec / min km / s
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str20 float64 float64 ... float64 float64
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------ -------------------- ------------ ... ------------ ------------
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Ceres 2459243.5488214926 355.21360625 ... 0.42203 15.7644188
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>>> from astroquery.miriade import Miriade
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>>> Miriade.get_ephemerides('Ceres')
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<Table masked=True length=1>
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target epoch RA ... DEC_rate delta_rate
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d deg ... arcs / min km / s
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bytes20 float64 float64 ... float64 float64
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------- -------------------- ----------------- ... ---------- ------------
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Ceres 2458519.315165116 242.1874308333333 ... -0.14926 -20.9668673
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This query will return ephemerides for asteroid Ceres, for the current
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epoch, and for a geocentric location. The query output is formatted as
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a `~astropy.table.Table`.
@@ -181,30 +181,38 @@ Consider the following example, which queries ephemerides for asteroid
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Pallas over an entire year with a time step of 1 day:
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.. code-block:: python
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.. doctest-remote-data::
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>>> from astroquery.miriade import Miriade
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>>> from astroquery.imcce import Miriade
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>>> Miriade.get_ephemerides('Pallas', epoch='2019-01-01',
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>>> epoch_step='1d', epoch_nsteps=365) # doctest: +SKIP
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<Table masked=True length=365>
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target epoch RA ... DEC_rate delta_rate
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d deg ... arcs / min km / s
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bytes20 float64 float64 ... float64 float64
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------- -------------------- ------------------ ... ---------- ------------
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Pallas 2458484.5 200.5865645833333 ... 0.15854 -19.3678422
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Pallas 2458485.5 200.92699458333328 ... 0.16727 -19.4137907
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Pallas 2458486.5 201.26416541666663 ... 0.17613 -19.4552649
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Pallas 2458487.5 201.59800958333332 ... 0.18511 -19.4921113
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Pallas 2458488.5 201.9284608333333 ... 0.19421 -19.5241972
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Pallas 2458489.5 202.25545124999996 ... 0.20344 -19.5514101
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... ... ... ... ... ...
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Pallas 2458843.5 261.1308308333333 ... 0.025007 -2.2916737
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Pallas 2458844.5 261.5084158333333 ... 0.029542 -2.5107013
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Pallas 2458845.5 261.88534958333327 ... 0.034077 -2.7290895
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Pallas 2458846.5 262.2616025 ... 0.038612 -2.9467393
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Pallas 2458847.5 262.6371470833333 ... 0.043144 -3.1635784
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Pallas 2458848.5 263.011955 ... 0.047672 -3.3795565
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... epoch_step='1d', epoch_nsteps=365)
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<Table length=365>
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target epoch RA ... DEC_rate delta_rate
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d deg ... arcsec / min km / s
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str20 float64 float64 ... float64 float64
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------ -------------------- ------------------ ... ------------ ------------
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Pallas 2458484.5 200.58657499999998 ... 0.15854 -19.3678409
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Pallas 2458485.5 200.92700499999998 ... 0.16727 -19.4137895
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Pallas 2458486.5 201.26417583333333 ... 0.17613 -19.4552637
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Pallas 2458487.5 201.59802 ... 0.18511 -19.4921101
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Pallas 2458488.5 201.92847124999997 ... 0.19421 -19.524196
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Pallas 2458489.5 202.25546166666663 ... 0.20344 -19.551409
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Pallas 2458490.5 202.57892541666664 ... 0.21278 -19.573655
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Pallas 2458491.5 202.89879624999998 ... 0.22224 -19.5908573
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Pallas 2458492.5 203.2150083333333 ... 0.23182 -19.6029527
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... ... ... ... ... ...
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Pallas 2458839.5 259.61457874999996 ... 0.0069182 -1.4120106
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Pallas 2458840.5 259.9944708333333 ... 0.011429 -1.6321318
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Pallas 2458841.5 260.37383125 ... 0.015948 -1.8522288
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Pallas 2458842.5 260.75262958333326 ... 0.020475 -2.072131
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Pallas 2458843.5 261.13083624999996 ... 0.025007 -2.2916715
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Pallas 2458844.5 261.50842124999997 ... 0.029542 -2.5106991
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Pallas 2458845.5 261.88535499999995 ... 0.034077 -2.7290872
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Pallas 2458846.5 262.26160791666666 ... 0.038612 -2.946737
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Pallas 2458847.5 262.63715249999996 ... 0.043144 -3.1635762
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Pallas 2458848.5 263.0119604166667 ... 0.047672 -3.3795543
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The observer location is defined through the ``location`` keyword,
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expecting a string containing the official IAU observatory code, a
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spacecraft name, or a set of coordinates (see the `Miriade manual
@@ -306,8 +314,8 @@ to be provided to the keyword ``coordtype`` to use these sets) :
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+------------------+-----------------------------------------------+
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| ``vz_h`` | Z heliocentric vel. vector (au/d, float) |
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+------------------+-----------------------------------------------+
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3. Local coordinates:
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+------------------+-----------------------------------------------+
@@ -454,7 +462,7 @@ results:
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ecliptical coordinates
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* ``elements``: switch to MPCORB ephemerides instead of ASTORB
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* ``radial_velocity``: provides additional information on target's radial
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velocity
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velocity
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@@ -483,10 +491,9 @@ Please consider the following notes from IMCCE:
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The development of this submodule is funded through NASA PDART Grant
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No. 80NSSC18K0987 to the `sbpy project <http://sbpy.org>`_.
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Reference/API
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=============
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.. automodapi:: astroquery.imcce
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:no-inheritance-diagram:
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