removing python blocks
@@ -13,7 +13,6 @@ arcsecond radius for optical counterparts in SDSS. Note use of the keyword
argument spectro, which requires matches to have spectroscopy, not just
photometry:
-.. code-block:: python
.. doctest-remote-data::
>>> from astroquery.sdss import SDSS
@@ -21,9 +20,9 @@ photometry:
>>> pos = coords.SkyCoord('0h8m05.63s +14d50m23.3s', frame='icrs')
>>> xid = SDSS.query_region(pos, spectro=True)
>>> print(xid)
- ra dec objid ... run2d instrument
- ---------------- ---------------- ------------------- ... ----- ----------
- 2.02344596573482 14.8398237551311 1237652943176138868 ... 26 SDSS
+ ra dec ... specobjid run2d
+ ---------------- ---------------- ... ------------------ -----
+ 2.02344596573482 14.8398237551311 ... 845594848269461504 26
The result is an astropy.Table.
@@ -32,7 +31,6 @@ Downloading data
If we'd like to download spectra and/or images for our match, we have all
the information we need in the elements of "xid" from the above example.
-.. code-block:: python
.. doctest-remote-data::
>>> sp = SDSS.get_spectra(matches=xid)
@@ -58,7 +56,6 @@ Spectral templates
It is also possible to download spectral templates from SDSS. To see what is
available, do
-.. code-block:: python
.. doctest-remote-data::
>>> from astroquery.sdss import SDSS
