Public Data¶
classy sources the databases listed
alphabetically below to allow for quick comparisons between literature data and
your observations.[1]
You can download and visualize a spectrum using the command line via the $
classy spectra command. To download all spectra from public repositories, use the $ classy status
command.
Available Public Data
Number of Spectra: 68,280
Number of Individual Asteroids: 62,045
24CAS¶
24 Color Asteroid Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
276 |
0.33µm |
1.1µm |
|
10 |
0.33µm |
1.1µm |
These spectra do not have any additional attributes.
52CAS¶
52 Color Asteroid Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
144 |
0.83µm |
2.57µm |
|
2 |
0.83µm |
2.57µm |
These spectra do not have any additional attributes.
AKARI AcuA¶
AKARI Asteroid-catalog-using-AKARI
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
64 |
2.5µm |
5.0µm |
The following attributes are copied from the AKARI AcuA archive and added to each spectrum. See the AKARI AcuA-spec catalogue description for details.
Attribute |
Description |
|
Saturation flag. |
|
Thermal-emission contamination flag. |
|
Stellar contamination flag. |
These attributes are added by classy.
Attribute |
Description |
|
Merged flag which is |
ECAS¶
Eight Color Asteroid Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
911 |
0.337µm |
1.041µm |
The available spectra are the single-epoch spectra, not the average spectra as e.g. used in Tholen (1984).
Compared to the original catalogue, cells with value -9.999 are replaced with np.nan values.
Gaia DR3¶
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
60 518 |
0.374µm |
1.034µm |
Important
The Gaia spectra show artifical reddening towards the UV. classy
automatically applies the correction proposed by Tinaut-Ruano+ 2023.
The following attributes are copied from the Gaia archive and added to each spectrum. See Galluccio+ 2022 for details.
Attribute |
Description |
|
Wavelength of observation (same as |
|
Reflectance values (same as |
|
Reflectance error values (same as |
|
Photometric quality flag ( |
|
Gaia source ID. |
|
Number of target asteroid. |
|
Gaia solution ID. |
|
Denomination of target asteroid. |
|
|
|
Number of individual spectra averaged here. |
M4AST¶
Modelling For Asteroids
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
80 |
0.34µm |
2.56µm |
Unpublished |
1 |
0.89µm |
1.29µm |
|
1 |
0.48µm |
2.50µm |
|
30 |
0.44µm |
2.40µm |
|
2 |
0.51µm |
1.32m |
|
2 |
0.37µm |
2.50µm |
|
1 |
0.55µm |
2.45µm |
|
4 |
0.82µm |
2.49µm |
|
1 |
0.33µm |
0.87µm |
No additional attributes are added.
MANOS¶
Mission Accessible Near-Earth Object Spectroscopy
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
197[2] |
0.4µm |
1.0µm |
These spectra do not have any additional attributes.
MITHNEOS¶
MIT-Hawaii Near-Earth Object Spectroscopic Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
537 |
0.337µm |
2.49µm |
|
88 |
0.65µm |
2.49µm |
|
475 |
0.36µm |
2.49μm |
|
36 |
0.35μm |
2.49μm |
|
769 |
0.35μm |
2.49μm |
Unpublished* |
Important
Binzel+ 2019 published 805 spectra, however, it is not evident which
MITHNEOS spectra this includes. 537 of the 805 can be identified
as they are the only spectrum of the respective asteroid in MITHNEOS.
These spectra are associated to Binzel+ 2019 in classy.
To identify the remaining published spectra, it is necessary to
visually compare the published spectra to the spectra in MITHNEOS.
Feel free to contribute should you have identified a misreferenced spectrum.
The following attributes are copied from the MITHNEOS website and added to each spectrum. The following attributes are copied from the SMASS website and added to each spectrum. See the SMASS website for details.
Attribute |
Description |
|
Column 4 of MITHNEOS data, equal to number of SpeX nights averaged. |
Misc¶
Miscellaneous: A collection of spectra published by different observers, not part of larger surveys.
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
1 |
0.82 |
2.49 |
|
42 |
0.82 |
2.49 |
|
52 |
0.82 |
2.49 |
|
3 |
0.82 |
2.49 |
|
75 |
0.39 |
0.99 |
|
106 |
0.33 |
2.54 |
|
25 |
0.68 |
2.54 |
|
1 |
0.73 |
2.47 |
|
59 |
0.70 |
2.62 |
|
8 |
0.65 |
2.51 |
|
9 |
0.67 |
2.54 |
|
14 |
0.67 |
2.54 |
|
17 |
0.32 |
2.56 |
|
8 |
0.4 |
2.52 |
|
51 |
0.65 |
2.55 |
|
24 |
0.33 |
0.97 |
Moskovitz+ 2020 |
66 |
0.82 |
2.49 |
|
35 |
0.82 |
2.49 |
|
76 |
0.45 |
0.87 |
|
40 |
0.65 |
2.57 |
|
27 |
0.65 |
2.50 |
Reddy and Sanchez 2017 |
90 |
0.64 |
2.50 |
Reddy and Sanchez 2020 |
22 |
0.64 |
2.55 |
|
5 |
0.82 |
2.49 |
|
94 |
0.34 |
1.04 |
|
17 |
0.82 |
2.49 |
|
12 |
0.82 |
2.49 |
|
8 |
0.82 |
2.49 |
|
7 |
0.82 |
2.49 |
|
37 |
0.5 |
0.99 |
|
13 |
0.46 |
1.00 |
|
1 |
0.57 |
1.00 |
|
30 |
0.31 |
0.95 |
|
11 |
0.40 |
0.95 |
These spectra do not have any additional attributes.
PRIMASS¶
PRIMitive Asteroids Spectroscopic Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
67 |
0.34µm |
0.92µm |
|
101 |
0.50µm |
0.90µm |
|
19 |
0.40µm |
0.87µm |
|
97 |
0.50µm |
0.90µm |
|
73 |
0.50µm |
0.90µm |
|
53 |
0.40µm |
0.91µm |
|
28 |
0.40µm |
0.91µm |
The following metadata provided by PRIMASS is added:
Attribute |
Description |
|
Time at the start of the observations |
|
Time at the end of the observations |
|
Number of exposures |
|
Total exposure time |
|
Airmass at the start of the observation |
|
Phase angle at the time of the observation |
|
Geocentric distance at the time of the observation |
|
Heliocentric distance at the time of the observation |
S3OS2¶
Small Solar System Objects Spectroscopic Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
820 |
0.49µm |
0.92µm |
No additional attributes are available for these spectra.
SCAS¶
Seven Color Asteroid Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
126 |
0.91µm |
2.3µm |
These spectra do not have any additional attributes.
SMASS¶
Small Main-Belt Asteroid Spectroscopic Survey
Number of Spectra |
\(\lambda_{min}\) |
\(\lambda_{max}\) |
Reference |
316 |
0.42µm |
1.02µm |
|
63 |
0.36µm |
1.67µm |
|
1 |
0.55µm |
2.5µm |
|
1,341 |
0.44µm |
0.93µm |
|
251 |
0.87µm |
1.66µm |
|
254 |
0.55µm |
1.66µm |
|
4 |
0.45µm |
2.49µm |
|
22 |
0.34µm |
0.93µm |
|
4 |
0.34µm |
2.44µm |
No additional attributes are available for these spectra.
SsODNet¶
The taxonomies by Tholen 1984 and by Mahlke+ 2022 make
use of the visual albedo. classy queries the SsODNet database via rocks
for values from the literature. See Berthier+ 2023 to learn more about SsODNet.