SDSS Queries (astroquery.sdss)

Default Data Release

The default data release is set to Data Release 17 (DR17), which is the final data release of the Sloan Digital Sky Survey IV. DR17 contains new optical and infrared spectra from both Apache Point Observatory and Las Campanas Observatory. Previously released integral-field datacubes and maps, stellar library spectra, as well as images, are also included in DR17. Users may select alternate DR’s.

Getting started

This example shows how to perform an individual object cross-ID with SDSS. We’ll start with the position of a source found in another survey, and search within a 5 arcsecond radius (a “cone search”) for optical counterparts in SDSS. Note use of the keyword argument spectro, which requires matches to have spectroscopy, not just photometry:

>>> from astroquery.sdss import SDSS
>>> from astropy import coordinates as coords
>>> pos = coords.SkyCoord('0h8m05.63s +14d50m23.3s', frame='icrs')
>>> xid = SDSS.query_region(pos, radius='5 arcsec', spectro=True)
>>> print(xid)
       ra              dec        ...     specobjid      run2d
---------------- ---------------- ... ------------------ -----
2.02344596573482 14.8398237551311 ... 845594848269461504    26

The result is an astropy.Table.

Searching regions and multiple objects

You can use query_region to search multiple locations; the input coordinates can be a single astropy.coordinates object or a list or Column of coordinates. However, it is important to specify exactly what kind of search is desired. When query_region is invoked with the radius keyword, a circle around each point is searched. This is also called a “cone search”. When invoked in this mode, query_region is equivalent to query_crossid. Because of this equivalence, there is a strict limit of 3 arcmin on the value of radius which is imposed by the SDSS servers.

query_region can also be used to search a rectangular region centered on a coordinate or each coordinate in a list. This mode is invoked with the width keyword, which is the width in right ascension. Optionally, the height keyword can be used to specify a different range of declination. With these parameters, query_region constructs a rectangle in RA, dec that does not correct for the geometry at high declination, also known as the \(\cos \delta\) correction. At high declination, these rectangles would appear much more like trapezoids. However, this is the more intuitive interpretation of “this range of RA, that range of Dec” that many people use. Finally, though, the constructed rectangles do account for RA wrap-around, so an appropriate region of the celestial sphere is searched, even if the central coordinate is very close to RA = 0.

Finally note that either radius or width must be specified. Specifying neither or both will raise an exception.

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.

>>> sp = SDSS.get_spectra(matches=xid)
>>> im = SDSS.get_images(matches=xid, band='g')

The variables “sp” and “im” are lists of HDUList objects, one entry for each corresponding object in xid.

Note that in SDSS, image downloads retrieve the entire plate, so further processing will be required to excise an image centered around the point of interest (i.e., the object(s) returned by query_region).

Spectral templates


These templates are from the SDSS-I/II spectroscopic pipeline (DR7 and earlier). SDSS-III/IV (DR8 and later) spectroscopic processing pipelines use different templates.

It is also possible to download spectral templates from SDSS. To see what is available, do

>>> from astroquery.sdss import SDSS
{'star_O': 0, 'star_OB': 1, 'star_B': 2, 'star_A': [3, 4], 'star_FA': 5,
'star_F': [6, 7], 'star_G': [8, 9], 'star_K': 10, 'star_M1': 11, 'star_M3': 12,
'star_M5': 13, 'star_M8': 14, 'star_L1': 15, 'star_wd': [16, 20, 21], 'star_carbon': [17, 18, 19],
'star_Ksubdwarf': 22, 'galaxy_early': 23, 'galaxy': [24, 25, 26], 'galaxy_late': 27, 'galaxy_lrg': 28,
'qso': 29, 'qso_bal': [30, 31], 'qso_bright': 32}

Then, to download your favorite template, do something like

>>> template = SDSS.get_spectral_template('qso')    

The variable “template” is a list of HDUList objects (same object as “sp” in the above example). In this case there is only one result, but in a few cases there are multiple templates available to choose from (e.g., the “galaxy” spectral template will actually return 3 templates).


astroquery.sdss Package

SDSS Spectra/Image/SpectralTemplate Archive Query Tool




Configuration parameters for astroquery.sdss.