Merge pull request #34 from hash889900/Application/f174mz57hgfirq7vgd…

…hu4piwnvrpfg7a7j7qrnfka

Datacap for National Astronomical Observatories, Chinese Academy of Sciences

applications/f174mz57hgfirq7vgdhu4piwnvrpfg7a7j7qrnfka.json

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+{
+  "Version": "1.3",
+  "ID": "f174mz57hgfirq7vgdhu4piwnvrpfg7a7j7qrnfka",
+  "Issue Number": "33",
+  "Client": {
+    "Name": "National Astronomical Observatories, Chinese Academy of Sciences",
+    "Region": "China",
+    "Industry": "Environment",
+    "Website": "http://dr5.lamost.org/",
+    "Social Media": "http://dr5.lamost.org/",
+    "Social Media Type": "Other",
+    "Role": "Data Preparer"
+  },
+  "Project": {
+    "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\r\n 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]\r\n. Now, the fifth data release (DR5) has published online (http://dr5.lamost.org/), and released data products include：\r\n\r\nSpectra. - 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]\r\n at the 5500 angstrom.\r\nSpectroscopic 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.\r\n\r\nhttp://dr5.lamost.org/v3/doc/data-production-description\r\n\r\nGuoshoujing 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",
+    "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\r\n 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]\r\n. Now, the fifth data release (DR5) has published online (http://dr5.lamost.org/), and released data products include：\r\n\r\nSpectra. - 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]\r\n at the 5500 angstrom.\r\nSpectroscopic 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.\r\n\r\nhttp://dr5.lamost.org/v3/doc/data-production-description\r\n\r\nGuoshoujing 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",
+    "How do you plan to prepare the dataset": "No response",
+    "Please share a sample of the data (a link to a file, an image, a table, etc., are good ways to do this.)": "http://dr5.lamost.org/v3/sas/catalog/\r\nhttp://dr5.lamost.org/v3/sas/fits/20111024/F5902/\r\nhttp://dr5.lamost.org/v3/sas/fits/20111024/F5907/\r\nhttp://dr5.lamost.org/v3/sas/fits/20111024/F5909/\r\nhttp://dr5.lamost.org/v3/sas/png/20111024/F5902/\r\nhttp://dr5.lamost.org/v3/sas/png/20111024/F5907/\r\nhttp://dr5.lamost.org/v3/sas/png/20111024/F5909/\r\nhttp://dr5.lamost.org/v3/sas/sky/20111024/",
+    "Confirm that this is a public dataset that can be retrieved by anyone on the network (i.e., no specific permissions or access rights are required to view the data)": "[X] I confirm",
+    "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",
+    "Please list the provider IDs and location of the storage providers you will be working with. Note that it is a requirement to list a minimum of 5 unique provider IDs, and that your client address will be verified against this list in the future": "f01106668   HK\r\nf03055029   HK\r\nf01518369   US\r\nf01889668   US\r\nf03239692  Frankfurt\r\nf03055005   HK\r\nf03055018   HK\r\nf03254235 London\r\nf01315096   HK\r\nf0870558     HK",
+    "Can you confirm that you will follow the Fil+ guideline (Data owner should engage at least 4 SPs and no single SP ID should receive >30% of a client's allocated DataCap)": "Yes"
+  },
+  "Datacap": {
+    "Type": "ldn-v3",
+    "Data Type": "Slingshot",
+    "Total Requested Amount": "5PiB",
+    "Single Size Dataset": "500TiB",
+    "Replicas": 10,
+    "Weekly Allocation": "1000TiB"
+  },
+  "Lifecycle": {
+    "State": "Granted",
+    "Validated At": "2024-12-11 16:34:41.399342503 UTC",
+    "Validated By": "hash889900",
+    "Active": true,
+    "Updated At": "2024-12-11 16:34:41.399339326 UTC",
+    "Active Request ID": "1cc6cba7-2164-4d04-bdcc-129352ca0aa1",
+    "On Chain Address": "f174mz57hgfirq7vgdhu4piwnvrpfg7a7j7qrnfka",
+    "Multisig Address": "false",
+    "edited": false
+  },
+  "Allocation Requests": [
+    {
+      "ID": "1cc6cba7-2164-4d04-bdcc-129352ca0aa1",
+      "Request Type": "First",
+      "Created At": "2024-12-11 15:50:34.988787722 UTC",
+      "Updated At": "2024-12-11 15:50:34.988789273 UTC",
+      "Active": false,
+      "Allocation Amount": "256TiB",
+      "Signers": [
+        {
+          "Github Username": "hash889900",
+          "Signing Address": "f14oq4jctudvidvyhfmrp7qt6ndng7pr7ampp3miq",
+          "Created At": "2024-12-11 16:34:38.427000000 UTC",
+          "Message CID": "bafy2bzacec3amzzrsr4a2fpjcdemkpeyfhhyaso2nae5mhrhnuawydpohihtc"
+        }
+      ]
+    }
+  ]
+}