Early Data Release (EDR)¶
Overview¶
The DESI Early Data Release includes spectra for 1.8 million unique targets from Survey Validation observations taken from December 2020 through June 2021, as well as a few commissioning and special tiles observed during the same time period. These data include “Target Selection Validation” (sv1) observations with looser target selection cuts and deeper S/N spectra, and “One-Percent Survey” (sv3) observations with highly complete coverage over 20 different fields overlapping other major surveys.
The EDR data are released under the Creative Commons Attribution 4.0 International License (CC BY 4.0). Use of DESI data requires including the citation and acknowledgment text given on the Data License and Acknowledgments page.
Data URL: https://data.desi.lbl.gov/public/edr
For a full description of the Survey Validation observations and EDR data, see DESI Collaboration et al. (2024) and DESI Collaboration et al. (2024). For an overview of how DESI data are organized see Data Organization, and see Data Access for how to access the data.
Coverage area¶
The figure below shows tile centers of the DESI observations included in EDR. The colored symbols the 20 rosette locations that compose the ~175 square degrees of the DESI One-Percent Survey (sv3). Each location was observed at least 12 times with overlapping tile centers to ensure a fiber assignment completeness of at least 95% for ELG and MWS targets, and over 99% for BGS, LRGs, and quasars targets within the central 6.5 square degrees of each rosette. In addition to these highly complete areas covering datasets from other surveys, EDR includes ~1200 additional square degrees covered by tiles with lower completeness but deeper S/N, centered at black dots in the figure.
Summary statistics¶
Summary of EDR | |
---|---|
Number of HEALPixel coadded spectra(1) | 2,044,588 |
Number of useful(2) spectra | 1,769,157 |
Number of useful spectra of unique targets | 1,712,004 |
Galaxies ( |
1,125,635 |
Quasars ( |
90,241 |
Stars ( |
496,128 |
Spectral coverage(3) | 360–982.4 nm |
Spectral resolution R | 2000 (at 360 nm)–5500 (at 980 nm) |
Wavelength system | vacuum |
Photometric bands (Legacy Surveys DR9) | g, r, z, W1, W2, W3, W4 |
Approximate area | ~1390 square degrees |
Footnotes: (1) Number of spectra for fibers placed on targets (OBJTYPE==TGT
), which excludes sky fibers and known faulty fibers. (2) Useful spectra defined as having ZWARN==0
, which means no errors due to instrument or data and no flags from spectral fitting issues. (3) Spectra are split on three spectrograph arms: blue (B), red (R), infrared (Z).
Table 6 from DESI Collaboration et al. (2024), reproduced below, contains the number of “good” spectra obtained for each DESI target class in each phase of Survey Validation, along with details for dedicated pointings (special) and commissioning (cmx). “Good” refers to science targets that have no Redrock redshift warning bits set (e.g. ZWARN==0
) and whose best-fitting templates are consistent with the tracer (e.g. SPECTYPE==GALAXY
for LRG and ELG targets, and SPECTYPE==QSO
for QSO targets).
Survey Validation Phase | NBGS | NELG | NLRG | NQSO | NSTAR |
---|---|---|---|---|---|
Commissioning (cmx) | 247 | 761 | 1,037 | 275 | 468 |
Target Selection Validation (sv1) | 134,419 | 111,692 | 66,161 | 29,839 | 163,254 |
Operations Testing (sv2) | 46,628 | 12,308 | 22,151 | 11,032 | 10,506 |
One-Percent Survey (sv3) | 253,915 | 312,790 | 137,317 | 34,173 | 295,232 |
Special | 925 | 3,866 | 3,588 | 3,045 | 867 |
Total | 428,758 | 437,664 | 227,318 | 76,079 | 466,447 |
Redshift distributions¶
The following figure (Figure 2 of DESI Collaboration et al. (2024)) shows the number of good, unique target redshifts as a function of redshift for each tracer type: ELG (green), LRG (red), BGS (purple), and QSO (blue). Stars are shown in the top panel. The gray histograms (e.g. STAR*, GALAXY*, QSO*) include all objects of a given SPECTYPE
classification, regardless of their target type. These differ slightly from the colored histograms because of secondary targets and other target types that were classified to a different category (e.g. a QSO target that was classified as a star).
Value-added Catalogs¶
The DESI science collaboration has generated a set of value-added catalogs (VACs) to accompany the Early Data Release. These catalogs provide curated subsets of data with additional analysis beyond the core spectroscopic data processing pipeline outputs.
Available now¶
- AGN Host Galaxies Physical Properties Catalog
- Broad Absorption Line (BAL) Quasar Catalog
- Damped Lyman-alpha (DLA) Quasar Catalog
- FastSpecFit Spectral Synthesis and Emission-Line Catalog
- Large-scale Structure Catalogs
- Legacy Surveys DR9 Photometric Catalog
- Lyman-alpha Catalog
- Mg II Absorber Catalog
- Milky Way Survey Catalog of Stellar Parameters
- PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Catalog
- Quasar (QSO) Redshift Catalog
- Redshift Summary Catalog
- Stellar Mass and Emission Line Catalog
- Uchuu-DESI Catalog
- Visual Inspection Catalogs
- Visualization and Outreach Catalog
Coming soon¶
The following VACs are currently in development:
- Active Galactic Nuclei (AGN) Summary Catalog
- QuasarNET Catalog
Known Issues¶
Known issues with the Early Data Release are documented here.
Software Package Versions¶
The versions of DESI software packages used for the Early Data Release are available here.