Share a brief history of your project and organization
Experienced Personal Data Provider.The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) is a Chinese national scientific research facility operated by the National Astronomical Observatories, Chinese Academy of Sciences. It is a special reflecting Schmidt telescope with 4000 fibers in a field of view of 20 deg2
in the sky. Until July 2017, LAMOST has completed its pilot survey which was launched in October 2011 and ended in June 2012, and the first five years of regular survey which was initiated on September 2012. After this six-year-survey, we totally obtain 9,026,365 spectra, which consist of stars, galaxies, quasars and other unknown objects[1−7]
. Now, the fifth data release (DR5) has published online (http://dr5.lamost.org/), and released data products include:
Spectra. - IIn general, there are 9,026,365 flux- and wavelength-calibrated, sky-subtracted spectra in DR5, including 8,183,160 stars, 152,863 galaxies, 52,453 quasars, and 637,889 unknown objects, and these spectra cover the wavelength range of 3690-9100 angstrom with a resolution of 1800[2−3]
at the 5500 angstrom.
Spectroscopic Parameters Catalogs. - In this data release, six spectroscopic parameters catalogs are also published,and they are the LAMOST general catalog, the A, F, G and K type star catalog, the A type star catalog, the M dwarf catalog, the observed plate information catalog, and the input catalog respectively. In the LAMOST general catalog, it includes 36 columns of basic spectroscopic information, for example, right ascension, declination, signal to noise ratio, magnitude, classification and redshift, which are also provided by the A, F, G and K type star catalog, the A type star catalog, and the M dwarf catalog. These three catalogs also provide other parameters, for example, atmospheric parameters (effective temperature, surface gravity, and metallicity), spectral line indices, line widths, the metallicity sensitive parameter, and the magnetic activity flag. In addition, the observed plate information catalog mainly contains nine basic plate information for all published plates, and the input catalog includes 24 basic fields mentioned above and three new fields which are not included in above catalogs.
http://dr5.lamost.org/v3/doc/data-production-description
Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences.
Is this project associated with other projects/ecosystem stakeholders?
No
If answered yes, what are the other projects/ecosystem stakeholders
No response
Describe the data being stored onto Filecoin
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) is a Chinese national scientific research facility operated by the National Astronomical Observatories, Chinese Academy of Sciences. It is a special reflecting Schmidt telescope with 4000 fibers in a field of view of 20 deg2
in the sky. Until July 2017, LAMOST has completed its pilot survey which was launched in October 2011 and ended in June 2012, and the first five years of regular survey which was initiated on September 2012. After this six-year-survey, we totally obtain 9,026,365 spectra, which consist of stars, galaxies, quasars and other unknown objects[1−7]
. Now, the fifth data release (DR5) has published online (http://dr5.lamost.org/), and released data products include:
Spectra. - IIn general, there are 9,026,365 flux- and wavelength-calibrated, sky-subtracted spectra in DR5, including 8,183,160 stars, 152,863 galaxies, 52,453 quasars, and 637,889 unknown objects, and these spectra cover the wavelength range of 3690-9100 angstrom with a resolution of 1800[2−3]
at the 5500 angstrom.
Spectroscopic Parameters Catalogs. - In this data release, six spectroscopic parameters catalogs are also published,and they are the LAMOST general catalog, the A, F, G and K type star catalog, the A type star catalog, the M dwarf catalog, the observed plate information catalog, and the input catalog respectively. In the LAMOST general catalog, it includes 36 columns of basic spectroscopic information, for example, right ascension, declination, signal to noise ratio, magnitude, classification and redshift, which are also provided by the A, F, G and K type star catalog, the A type star catalog, and the M dwarf catalog. These three catalogs also provide other parameters, for example, atmospheric parameters (effective temperature, surface gravity, and metallicity), spectral line indices, line widths, the metallicity sensitive parameter, and the magnetic activity flag. In addition, the observed plate information catalog mainly contains nine basic plate information for all published plates, and the input catalog includes 24 basic fields mentioned above and three new fields which are not included in above catalogs.
http://dr5.lamost.org/v3/doc/data-production-description
Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences.
Where was the data currently stored in this dataset sourced from
Other
If you answered "Other" in the previous question, enter the details here
http://dr5.lamost.org/
If you are a data preparer. What is your location (Country/Region)
None
If you are a data preparer, how will the data be prepared? Please include tooling used and technical details?
No response
If you are not preparing the data, who will prepare the data? (Provide name and business)
No response
Has this dataset been stored on the Filecoin network before? If so, please explain and make the case why you would like to store this dataset again to the network. Provide details on preparation and/or SP distribution.
Data Owner Name
National Astronomical Observatories, Chinese Academy of Sciences
Data Owner Country/Region
China
Data Owner Industry
Environment
Website
http://dr5.lamost.org/
Social Media Handle
http://dr5.lamost.org/
Social Media Type
Other
What is your role related to the dataset
Data Preparer
Total amount of DataCap being requested
15PiB
Expected size of single dataset (one copy)
3000TiB
Number of replicas to store
5
Weekly allocation of DataCap requested
1000TiB
On-chain address for first allocation
f1kpgxzqwotybdmbo5zpqbisxytuj4n55ktnzl3ki
Data Type of Application
Public, Open Dataset (Research/Non-Profit)
Custom multisig
Identifier
No response
Share a brief history of your project and organization
Is this project associated with other projects/ecosystem stakeholders?
No
If answered yes, what are the other projects/ecosystem stakeholders
No response
Describe the data being stored onto Filecoin
Where was the data currently stored in this dataset sourced from
Other
If you answered "Other" in the previous question, enter the details here
If you are a data preparer. What is your location (Country/Region)
None
If you are a data preparer, how will the data be prepared? Please include tooling used and technical details?
No response
If you are not preparing the data, who will prepare the data? (Provide name and business)
No response
Has this dataset been stored on the Filecoin network before? If so, please explain and make the case why you would like to store this dataset again to the network. Provide details on preparation and/or SP distribution.
No response
Please share a sample of the data
Confirm that this is a public dataset that can be retrieved by anyone on the Network
If you chose not to confirm, what was the reason
No response
What is the expected retrieval frequency for this data
Sporadic
For how long do you plan to keep this dataset stored on Filecoin
1.5 to 2 years
In which geographies do you plan on making storage deals
Greater China, Asia other than Greater China, Africa, North America, South America, Europe, Australia (continent), Antarctica
How will you be distributing your data to storage providers
HTTP or FTP server, Shipping hard drives
How did you find your storage providers
Slack, Big Data Exchange, Partners
If you answered "Others" in the previous question, what is the tool or platform you used
No response
Please list the provider IDs and location of the storage providers you will be working with.
How do you plan to make deals to your storage providers
Boost client, Lotus client, Singularity
If you answered "Others/custom tool" in the previous question, enter the details here
No response
Can you confirm that you will follow the Fil+ guideline
Yes