Scope

Overview

DR12 imaging and optical spectroscopic coverage in Equatorial coordinates (plot centered at RA = 6h, or 90 deg.)
DR12 imaging and optical spectroscopic coverage in Equatorial coordinates (plot centered at RA = 6h, or 90 deg.)

Data Release 12 represents the culmination of the third phase of the Sloan Digital Sky Survey. It includes all SDSS data taken through 14 July 2014, and encompasses more than one-third of the entire celestial sphere.

With so much sky measured in so many different ways, questions about the size of the SDSS can be answered in many different ways. This page details the SDSS survey area and provides object counts in Data Release 12 in various ways.


Imaging statistics

Total unique area covered
14,555 square degrees
Total area of imaging (including overlaps)
31,637 square degrees (excluding supernova runs)
Individual image field size
1361×2048 pixels (0.0337 square degrees)
Number of individual fields
938,046 (excluding supernova runs)
Number of catalog objects
1,231,051,050
Number of unique detections
932,891,133
Median PSF FWHM, r-band
1.3 arcsec
Pixel scale
0.396 arcsec
Exposure time per band
53.9 sec
Time difference between observations of each band
71.72 sec (in riuzg order)
Global astrometric precision
0.1 arcsec rms (absolute)
Number of unique, primary sources
Total
469,053,874
Stars
260,562,744
Galaxies
208,478,448
Unknown
12,682
Effective wavelengths & magnitude limits
(95% completeness for point sources)
u
3551Å
22.0
g
4686Å
22.2
r
6165Å
22.2
i
7481Å
21.3
z
8931Å
20.5
Relative photometric
calibration accuracy (RMS)

(Padmanabhan et al. 2008)
u
1.3%
g
0.8%
r
0.8%
i
0.7%
z
0.8%

Optical spectroscopy data statistics

All programs combined

Total spectra
4,355,200
Useful spectra
4,266,444
Galaxies
2,401,952
Quasars
477,161
Stars
851,968
Sky
341,140
Unknown
200,490

Stellar (SEGUE)

Effective area (deg2)
1,317
Plates
229
Total spectra
155,520
Unique objects
138,099

Extragalactic (BOSS)

Statistic Total Unique
Spectroscopic effective area (deg2) 9,376
Plates 2,512 2,438
Spectra 2,497,484 2,269,478
All Galaxies 1,480,945 1,372,737
    CMASS 931,517 862,735
    LOWZ 368,335 343,160
All Quasars 350,793 294,512
    Main 241,516 220,377
    Main, 2.15 ≤ z ≤ 3.5 175,244 158,917
Stars 274,811 247,216
    Standard stars 52,328 42,815
Sky 238,094 223,541
Unclassified spectra 163,377 140,533

Infrared (APOGEE) spectroscopic data statistics

DR12 includes data for ~163,000 APOGEE targets. This includes 146,000 science targets, located in distinct types of survey fields:

~15,000 stars
in Bulge fields
~28,000 stars
in Halo fields
~55,000 stars
in Disk fields
~14,000 stars
in Kepler/CoRoT fields
~8,000 objects
in Ancillary Science fields
~1,800 stars
in Halo Stream fields
~1,200 stars
in Sagittarius dSph fields
~8,000 stars
in Star Cluster fields
~900 bright stars
observed with the NMSU 1m telescope + APOGEE, including bright standards

Exact counts are given in the table below.

Statistic Total Unique
Pointings 435
Plates 2,349 817
All stars 618,080 156,593
    with NMSU 1-m 1,196 882
Commissioning stars 27,660 12,140
Survey stars 590,420 149,502
    with S/N > 100 141,320
    with ≥ 3 visits 120,883
    with ≥ 12 visits 6,107
    Stellar parameter standards 8,307 1,169
    Radial velocity standards 269 17
    Telluric line standards 83,127 17,116
    Ancillary science program objects 36,123 12,515
    Kepler target stars 15,242 7,953