juliensimon commited on
Commit
abde817
·
verified ·
1 Parent(s): 54af31a

Upload APOGEE DR17: 733,901 stars, 20 elements

Browse files
Files changed (2) hide show
  1. README.md +333 -0
  2. data/apogee_dr17.parquet +3 -0
README.md ADDED
@@ -0,0 +1,333 @@
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
1
+ ---
2
+ license: cc-by-4.0
3
+ pretty_name: "APOGEE DR17 Stellar Parameters & Abundances"
4
+ language:
5
+ - en
6
+ description: >-
7
+ APOGEE DR17 AllStar catalog: high-resolution infrared spectroscopic stellar
8
+ parameters and 20+ individual chemical element abundances for ~657K stars.
9
+ The final SDSS-IV APOGEE release and the premier stellar chemical abundance catalog.
10
+ task_categories:
11
+ - tabular-classification
12
+ - tabular-regression
13
+ tags:
14
+ - space
15
+ - stars
16
+ - stellar
17
+ - spectroscopy
18
+ - chemical-abundances
19
+ - apogee
20
+ - sdss
21
+ - astronomy
22
+ - open-data
23
+ - tabular-data
24
+ - parquet
25
+ size_categories:
26
+ - 100K<n<1M
27
+ configs:
28
+ - config_name: default
29
+ data_files:
30
+ - split: train
31
+ path: data/apogee_dr17.parquet
32
+ default: true
33
+ ---
34
+
35
+ # APOGEE DR17 Stellar Parameters & Abundances
36
+
37
+ *Part of the [Astronomy Datasets](https://huggingface.co/collections/juliensimon/astronomy-datasets-69c24caf2f17e36128946743) collection on Hugging Face.*
38
+
39
+ The APOGEE DR17 AllStar catalog provides high-resolution infrared (H-band)
40
+ spectroscopic stellar parameters and **20+ individual chemical element
41
+ abundances** for **733,901** stars across the Milky Way. This is the final
42
+ data release from SDSS-IV APOGEE and represents the premier stellar chemical
43
+ abundance catalog available today.
44
+
45
+ ## Dataset description
46
+
47
+ The Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a
48
+ large-scale, high-resolution (R ~ 22,500), near-infrared (H-band, 1.51-1.70 um)
49
+ spectroscopic survey of Milky Way stellar populations. DR17 is the final release
50
+ of SDSS-IV, containing the complete APOGEE-2 dataset with observations from both
51
+ the Northern (APO 2.5m) and Southern (du Pont 2.5m at LCO) hemispheres.
52
+
53
+ The ASPCAP pipeline (APOGEE Stellar Parameter and Chemical Abundances Pipeline)
54
+ derives effective temperature, surface gravity, metallicity, and individual
55
+ elemental abundances by comparing observed spectra against synthetic spectral
56
+ libraries. The catalog covers a wide range of stellar types including red giants,
57
+ red clump stars, and main-sequence stars across the Galactic disk, bulge, and halo.
58
+
59
+ ## Schema
60
+
61
+ | Column | Type | Description |
62
+ |--------|------|-------------|
63
+ | `file` | object | -- |
64
+ | `apogee_id` | string | APOGEE unique star identifier |
65
+ | `target_id` | object | -- |
66
+ | `ap_star` | object | -- |
67
+ | `ascap` | object | -- |
68
+ | `tel` | object | -- |
69
+ | `loc` | int64 | -- |
70
+ | `field` | object | -- |
71
+ | `alt_id` | object | -- |
72
+ | `ra_deg` | float64 | Right ascension ICRS (degrees) |
73
+ | `dec_deg` | float64 | Declination ICRS (degrees) |
74
+ | `glon_deg` | float64 | Galactic longitude (degrees) |
75
+ | `glat_deg` | float64 | Galactic latitude (degrees) |
76
+ | `j_mag` | float64 | 2MASS J magnitude |
77
+ | `j_mag_error` | float64 | -- |
78
+ | `h_mag` | float64 | 2MASS H magnitude |
79
+ | `h_mag_error` | float64 | -- |
80
+ | `k_mag` | float64 | 2MASS K magnitude |
81
+ | `e_ksmag` | float64 | -- |
82
+ | `r_hmag` | object | -- |
83
+ | `mmag` | float64 | -- |
84
+ | `e_mmag` | float64 | -- |
85
+ | `t2mag` | float64 | -- |
86
+ | `e_t2mag` | float64 | -- |
87
+ | `ddo51` | float64 | -- |
88
+ | `e_ddo51` | float64 | -- |
89
+ | `3_6mag` | float64 | -- |
90
+ | `e_3_6mag` | float64 | -- |
91
+ | `4_5mag` | float64 | -- |
92
+ | `e_4_5mag` | float64 | -- |
93
+ | `5_8mag` | float64 | -- |
94
+ | `e_5_8mag` | float64 | -- |
95
+ | `8_0mag` | float64 | -- |
96
+ | `e_8_0mag` | float64 | -- |
97
+ | `4_5mag_w` | float64 | -- |
98
+ | `e_4_5mag_w` | float64 | -- |
99
+ | `4_5mag_t` | float64 | -- |
100
+ | `e_4_5mag_t` | float64 | -- |
101
+ | `giant` | int64 | -- |
102
+ | `star` | int64 | -- |
103
+ | `pm_rat` | float64 | -- |
104
+ | `pm_det` | float64 | -- |
105
+ | `r_pm_t` | object | -- |
106
+ | `ak_t` | float64 | -- |
107
+ | `n_ak_t` | object | -- |
108
+ | `ak` | float64 | -- |
109
+ | `e(b_v)` | float64 | -- |
110
+ | `ap1_t1` | int64 | -- |
111
+ | `ap1_t2` | int64 | -- |
112
+ | `ap2_t1` | int64 | -- |
113
+ | `ap2_t2` | int64 | -- |
114
+ | `ap2_t3` | int64 | -- |
115
+ | `survey` | object | -- |
116
+ | `prog` | object | -- |
117
+ | `n_visits` | Int64 | Number of visits |
118
+ | `snr` | float64 | Combined signal-to-noise ratio |
119
+ | `snrev` | float64 | -- |
120
+ | `s_flag` | int64 | -- |
121
+ | `sa_flag` | int64 | -- |
122
+ | `radial_velocity_kms` | float64 | Heliocentric radial velocity (km/s) |
123
+ | `rv_scatter_kms` | float64 | RV scatter across visits (km/s) |
124
+ | `radial_velocity_error_kms` | float64 | RV uncertainty (km/s) |
125
+ | `teff_rv` | float64 | -- |
126
+ | `logg_rv` | float64 | -- |
127
+ | `fe_h_rv` | float64 | -- |
128
+ | `chi2_rv` | float64 | -- |
129
+ | `fwhmcc` | float64 | -- |
130
+ | `fwhm` | float64 | -- |
131
+ | `fl_rv` | int64 | -- |
132
+ | `ncomp` | int64 | -- |
133
+ | `nfib` | float64 | -- |
134
+ | `e_nfib` | float64 | -- |
135
+ | `hmin` | float64 | -- |
136
+ | `hmax` | float64 | -- |
137
+ | `j_kmin` | float64 | -- |
138
+ | `j_kmax` | float64 | -- |
139
+ | `gaia_source_id` | string | Gaia DR3 source ID |
140
+ | `parallax_mas` | float64 | Parallax (mas) |
141
+ | `parallax_error_mas` | float64 | Parallax uncertainty (mas) |
142
+ | `pmra_mas_yr` | float64 | Proper motion in RA (mas/yr) |
143
+ | `e_pm_ra` | float64 | -- |
144
+ | `pmdec_mas_yr` | float64 | Proper motion in Dec (mas/yr) |
145
+ | `e_pm_de` | float64 | -- |
146
+ | `gaia_g_mag` | float64 | -- |
147
+ | `gaia_bp_mag` | float64 | -- |
148
+ | `gaia_rp_mag` | float64 | -- |
149
+ | `gaia_radial_velocity_kms` | float64 | -- |
150
+ | `gaia_radial_velocity_error_kms` | float64 | -- |
151
+ | `distance_geo_pc` | float64 | -- |
152
+ | `b_rgeo` | float64 | -- |
153
+ | `distance_photogeo_pc` | float64 | -- |
154
+ | `b_rpgeo` | float64 | -- |
155
+ | `grid` | object | -- |
156
+ | `chi2` | float64 | -- |
157
+ | `a_flag` | int64 | -- |
158
+ | `bad_px` | float64 | -- |
159
+ | `low_snr` | float64 | -- |
160
+ | `sig_sky` | float64 | -- |
161
+ | `e_flag` | int64 | -- |
162
+ | `p_mm` | object | -- |
163
+ | `teff_k` | float64 | Effective temperature (K) |
164
+ | `teff_error_k` | float64 | Teff uncertainty (K) |
165
+ | `logg` | float64 | Surface gravity log g (dex) |
166
+ | `logg_error` | float64 | log g uncertainty (dex) |
167
+ | `m_h` | float64 | [M/H] abundance (dex) |
168
+ | `m_h_error` | float64 | -- |
169
+ | `alpha_m` | float64 | Alpha enhancement [alpha/M] (dex) |
170
+ | `e_[a/m]` | float64 | -- |
171
+ | `vmicro_kms` | float64 | -- |
172
+ | `vmacro_kms` | float64 | -- |
173
+ | `vsini_kms` | float64 | -- |
174
+ | `teff_sp` | float64 | -- |
175
+ | `logg_sp` | float64 | -- |
176
+ | `c_fe` | float64 | [C/Fe] abundance (dex) |
177
+ | `c_fe_sp` | float64 | -- |
178
+ | `c_fe_err` | float64 | -- |
179
+ | `c_fe_flag` | int64 | -- |
180
+ | `ci_fe` | float64 | [CI/Fe] abundance (dex) |
181
+ | `ci_fe_sp` | float64 | -- |
182
+ | `ci_fe_err` | float64 | -- |
183
+ | `ci_fe_flag` | int64 | -- |
184
+ | `n_fe` | float64 | [N/Fe] abundance (dex) |
185
+ | `n_fe_sp` | float64 | -- |
186
+ | `n_fe_err` | float64 | -- |
187
+ | `n_fe_flag` | int64 | -- |
188
+ | `o_fe` | float64 | [O/Fe] abundance (dex) |
189
+ | `o_fe_sp` | float64 | -- |
190
+ | `o_fe_err` | float64 | -- |
191
+ | `o_fe_flag` | int64 | -- |
192
+ | `na_fe` | float64 | [NA/Fe] abundance (dex) |
193
+ | `na_fe_sp` | float64 | -- |
194
+ | `na_fe_err` | float64 | -- |
195
+ | `na_fe_flag` | int64 | -- |
196
+ | `mg_fe` | float64 | [MG/Fe] abundance (dex) |
197
+ | `mg_fe_sp` | float64 | -- |
198
+ | `mg_fe_err` | float64 | -- |
199
+ | `mg_fe_flag` | int64 | -- |
200
+ | `al_fe` | float64 | [AL/Fe] abundance (dex) |
201
+ | `al_fe_sp` | float64 | -- |
202
+ | `al_fe_err` | float64 | -- |
203
+ | `al_fe_flag` | int64 | -- |
204
+ | `si_fe` | float64 | [SI/Fe] abundance (dex) |
205
+ | `si_fe_sp` | float64 | -- |
206
+ | `si_fe_err` | float64 | -- |
207
+ | `si_fe_flag` | int64 | -- |
208
+ | `s_fe` | float64 | [S/Fe] abundance (dex) |
209
+ | `s_fe_sp` | float64 | -- |
210
+ | `s_fe_err` | float64 | -- |
211
+ | `s_fe_flag` | int64 | -- |
212
+ | `k_fe` | float64 | [K/Fe] abundance (dex) |
213
+ | `k_fe_sp` | float64 | -- |
214
+ | `k_fe_err` | float64 | -- |
215
+ | `k_fe_flag` | int64 | -- |
216
+ | `ca_fe` | float64 | [CA/Fe] abundance (dex) |
217
+ | `ca_fe_sp` | float64 | -- |
218
+ | `ca_fe_err` | float64 | -- |
219
+ | `ca_fe_flag` | int64 | -- |
220
+ | `ti_fe` | float64 | [TI/Fe] abundance (dex) |
221
+ | `ti_fe_sp` | float64 | -- |
222
+ | `ti_fe_err` | float64 | -- |
223
+ | `ti_fe_flag` | int64 | -- |
224
+ | `tiii_fe` | float64 | [TIII/Fe] abundance (dex) |
225
+ | `tiii_fe_sp` | float64 | -- |
226
+ | `tiii_fe_err` | float64 | -- |
227
+ | `tiii_fe_flag` | int64 | -- |
228
+ | `v_fe` | float64 | [V/Fe] abundance (dex) |
229
+ | `v_fe_sp` | float64 | -- |
230
+ | `v_fe_err` | float64 | -- |
231
+ | `v_fe_flag` | int64 | -- |
232
+ | `cr_fe` | float64 | [CR/Fe] abundance (dex) |
233
+ | `cr_fe_sp` | float64 | -- |
234
+ | `cr_fe_err` | float64 | -- |
235
+ | `cr_fe_flag` | int64 | -- |
236
+ | `mn_fe` | float64 | [MN/Fe] abundance (dex) |
237
+ | `mn_fe_sp` | float64 | -- |
238
+ | `mn_fe_err` | float64 | -- |
239
+ | `mn_fe_flag` | int64 | -- |
240
+ | `fe_h` | float64 | Metallicity [Fe/H] (dex) |
241
+ | `fe_h_sp` | float64 | -- |
242
+ | `fe_h_err` | float64 | -- |
243
+ | `fe_h_flag` | int64 | -- |
244
+ | `co_fe` | float64 | [CO/Fe] abundance (dex) |
245
+ | `co_fe_sp` | float64 | -- |
246
+ | `co_fe_err` | float64 | -- |
247
+ | `co_fe_flag` | int64 | -- |
248
+ | `ni_fe` | float64 | [NI/Fe] abundance (dex) |
249
+ | `ni_fe_sp` | float64 | -- |
250
+ | `ni_fe_err` | float64 | -- |
251
+ | `ni_fe_flag` | int64 | -- |
252
+ | `ce_fe` | float64 | [CE/Fe] abundance (dex) |
253
+ | `ce_fe_sp` | float64 | -- |
254
+ | `ce_fe_err` | float64 | -- |
255
+ | `ce_fe_flag` | int64 | -- |
256
+ | `dr16` | int64 | -- |
257
+
258
+ ## Quick stats
259
+
260
+ - **733,901** stars total
261
+ - **689,024** with effective temperature
262
+ - **647,042** with [Fe/H] metallicity
263
+ - **20** individual abundance elements
264
+ - Teff range: **3088** -- **19870** K
265
+ - [Fe/H] range: **-2.47** to **0.96** dex
266
+
267
+ ## Usage
268
+
269
+ ```python
270
+ from datasets import load_dataset
271
+
272
+ ds = load_dataset("juliensimon/apogee-dr17", split="train")
273
+ df = ds.to_pandas()
274
+
275
+ # Kiel diagram (Teff vs log g)
276
+ import matplotlib.pyplot as plt
277
+ valid = df.dropna(subset=["teff_k", "logg"])
278
+ plt.scatter(valid["teff_k"], valid["logg"], c=valid["fe_h"],
279
+ s=0.1, alpha=0.3, cmap="coolwarm", vmin=-2, vmax=0.5)
280
+ plt.gca().invert_xaxis()
281
+ plt.gca().invert_yaxis()
282
+ plt.xlabel("Teff (K)")
283
+ plt.ylabel("log g (dex)")
284
+ plt.colorbar(label="[Fe/H]")
285
+ plt.title("APOGEE DR17 Kiel Diagram")
286
+
287
+ # [Mg/Fe] vs [Fe/H] — chemical evolution
288
+ if "mg_fe" in df.columns:
289
+ valid = df.dropna(subset=["fe_h", "mg_fe"])
290
+ plt.figure()
291
+ plt.scatter(valid["fe_h"], valid["mg_fe"], s=0.1, alpha=0.2)
292
+ plt.xlabel("[Fe/H] (dex)")
293
+ plt.ylabel("[Mg/Fe] (dex)")
294
+ plt.title("Chemical Evolution: [Mg/Fe] vs [Fe/H]")
295
+ ```
296
+
297
+ ## Data source
298
+
299
+ Abdurro'uf et al. (2022), "The Seventeenth Data Release of the Sloan Digital
300
+ Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data", ApJS, 259, 35.
301
+ Accessed via [VizieR III/286](https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/286),
302
+ CDS Strasbourg.
303
+
304
+ ## Related datasets
305
+
306
+ - [rave-dr6](https://huggingface.co/datasets/juliensimon/rave-dr6) -- RAVE DR6 stellar parameters and chemical abundances
307
+ - [wolf-rayet-stars](https://huggingface.co/datasets/juliensimon/wolf-rayet-stars) -- Galactic Wolf-Rayet star catalog
308
+ - [brown-dwarf-catalog](https://huggingface.co/datasets/juliensimon/brown-dwarf-catalog) -- Brown dwarf catalog
309
+
310
+ ## Pipeline
311
+
312
+ Source code: [juliensimon/space-datasets](https://github.com/juliensimon/space-datasets)
313
+
314
+ ## Support
315
+
316
+ If you find this dataset useful, please give it a heart on the [dataset page](https://huggingface.co/datasets/juliensimon/apogee-dr17) and share feedback in the Community tab! Also consider giving a star to the [space-datasets](https://github.com/juliensimon/space-datasets) repo.
317
+
318
+ ## Citation
319
+
320
+ ```bibtex
321
+ @dataset{apogee_dr17,
322
+ author = {Simon, Julien},
323
+ title = {APOGEE DR17 Stellar Parameters & Abundances},
324
+ year = {2026},
325
+ publisher = {Hugging Face},
326
+ url = {https://huggingface.co/datasets/juliensimon/apogee-dr17},
327
+ note = {Based on Abdurro'uf et al. (2022, ApJS 259 35) via VizieR CDS Strasbourg}
328
+ }
329
+ ```
330
+
331
+ ## License
332
+
333
+ [CC-BY-4.0](https://creativecommons.org/licenses/by/4.0/)
data/apogee_dr17.parquet ADDED
@@ -0,0 +1,3 @@
 
 
 
 
1
+ version https://git-lfs.github.com/spec/v1
2
+ oid sha256:7d331a2d93e394da6e22ba53268ed3d874f0618c6bace39cf89b6bfeb11e8ee3
3
+ size 247535057