diff --git a/src/test/resources/github238/valid/bundle_kaguya_derived.xml b/src/test/resources/github238/valid/bundle_kaguya_derived.xml index 2f5023ebc..030308f08 100644 --- a/src/test/resources/github238/valid/bundle_kaguya_derived.xml +++ b/src/test/resources/github238/valid/bundle_kaguya_derived.xml @@ -123,7 +123,7 @@ Archive - urn:nasa:pds:kaguya_grs_spectra:data_spectra + urn:nasa:pds:kaguya_grs_spectra:data_spectra::1.0 Primary bundle_has_data_collection diff --git a/src/test/resources/github238/valid/bundle_kaguya_derived_2.xml b/src/test/resources/github238/valid/bundle_kaguya_derived_2.xml index 6c388954d..176ad513d 100644 --- a/src/test/resources/github238/valid/bundle_kaguya_derived_2.xml +++ b/src/test/resources/github238/valid/bundle_kaguya_derived_2.xml @@ -123,7 +123,7 @@ Archive - urn:nasa:pds:kaguya_grs_spectra:data_spectra + urn:nasa:pds:kaguya_grs_spectra:data_spectra::2.0 Primary bundle_has_data_collection diff --git a/src/test/resources/github238/valid/bundle_kaguya_derived_3.xml b/src/test/resources/github238/valid/bundle_kaguya_derived_3.xml index af5c2d11e..d14335da8 100644 --- a/src/test/resources/github238/valid/bundle_kaguya_derived_3.xml +++ b/src/test/resources/github238/valid/bundle_kaguya_derived_3.xml @@ -123,7 +123,7 @@ Archive - urn:nasa:pds:kaguya_grs_spectra:data_spectra + urn:nasa:pds:kaguya_grs_spectra:data_spectra::3.0 Primary bundle_has_data_collection diff --git a/src/test/resources/github238/valid/bundle_kaguya_derived_4.xml b/src/test/resources/github238/valid/bundle_kaguya_derived_4.xml index 8bbb3da9f..6f88dc037 100644 --- a/src/test/resources/github238/valid/bundle_kaguya_derived_4.xml +++ b/src/test/resources/github238/valid/bundle_kaguya_derived_4.xml @@ -123,7 +123,7 @@ Archive - urn:nasa:pds:kaguya_grs_spectra:data_spectra + urn:nasa:pds:kaguya_grs_spectra:data_spectra::4.0 Primary bundle_has_data_collection diff --git a/src/test/resources/github238/valid/bundle_kaguya_derived_5.xml b/src/test/resources/github238/valid/bundle_kaguya_derived_5.xml index 6c61c5493..b1015772f 100644 --- a/src/test/resources/github238/valid/bundle_kaguya_derived_5.xml +++ b/src/test/resources/github238/valid/bundle_kaguya_derived_5.xml @@ -123,7 +123,7 @@ Archive - urn:nasa:pds:kaguya_grs_spectra:data_spectra + urn:nasa:pds:kaguya_grs_spectra:data_spectra::5.0 Primary bundle_has_data_collection diff --git a/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per4.csv b/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per4.csv new file mode 100644 index 000000000..e69de29bb diff --git a/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per4.xml b/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per4.xml new file mode 100644 index 000000000..d7162057b --- /dev/null +++ b/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per4.xml @@ -0,0 +1,238 @@ + + + + + + urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per4 + 1.0 + Kaguya Gamma-Ray Spectrometer Corrected Spectra + 1.11.0.0 + Product_Observational + + + 2019-09-30 + 1.0 + First release + + + + + + 2009-02-10T18:26:40Z + 2009-05-28T07:43:22Z + + + Science + Derived + + This collection contains Kaguya Gamma-Ray Spectrometer (KGRS) corrected and calibrated time-series + spectra acquired during the nominal and extended observation periods of JAXA's SELENE (Kaguya) mission. + + The SELENE mission was the Japanese mission to the Moon with a main orbiter “Kaguya” and + two daughter relay satellites launched on Sep. 14, 2007. KGRS was mounted on the deck of the + main orbiter. It employed a high-purity Ge (HPGe) crystal as a main detector, and surrounding + BGO and plastic scintillators as anti-coincidence detectors to reduce backgrounds. The + Ge crystal was cooled by a Sterling refrigerator. It made close-proximity observations of the + Moon from Dec. 14, 2007 to Dec. 11, 2008 at the high circular orbital altitude of 100 km, and + from Feb. 10 to May 28 in 2009 at the low elliptical orbital altitude of ~30 x 50 km. + + KGRS recorded energy spectra of gamma rays in two gain modes simultaneously; high gain (0.1 + to 3 MeV) and low gain (0.1 to 13 MeV), each of which was analyzed by the 13-bit (8192 ch) + analog-to-digital converter (ADC). While the former has a higher spectral resolution over the + energy range of radioactive elements, the latter has better statistics and covers the whole energy + range of major rock-forming elements, including the Fe neutron capture line at 7.6 MeV. The + accumulation time of each spectrum was 17 s. Both modes of spectra are included in this archive. + + The observation epochs of KGRS consists of three regular measurement periods (Period 1 to 3), + background measurements, and the annealing of the Ge crystal. The HPGe detector was annealed + from 16 to 25, December 2008, which improved energy resolution by a factor of two. + Period 1 and 2 lasted two and five months, respectively, with limited spatial or spectral + resolutions. Period 3 lasted ~3.5 months (including dead time) with the best spatial and spectral + resolutions. In addition, spectra from the background measurement when the satellite was flipped + and the detector faced deep space can be analyzed to estimate the background gamma-ray intensity + from the satellite due to the exposure to galactic cosmic rays. + + The following data reduction processes, based on those successfully used for Lunar Prospector and + Dawn missions, were applied to the raw time-series spectra of KGRS: 1) Filtering of invalid events, + 2) ADC Differential Non-Linearity, and 3) Gain correction and energy calibration. Correction factors + for satellite altitude and galactic cosmic ray intensities are provided as part of the KGRS ephemeris + data. + + + + Kaguya + Mission + + urn:nasa:pds:context:investigation:mission.kaguya + data_to_investigation + + + + Kaguya + + Kaguya + Spacecraft + + urn:nasa:pds:context:instrument_host:spacecraft.kaguya + is_instrument_host + + + + GRS + Instrument + + urn:nasa:pds:context:instrument:kaguya.grs + is_instrument + + + + + Moon + Satellite + + urn:nasa:pds:context:target:satellite.earth.moon + collection_to_target + + + + + + urn:nasa:pds:kaguya_grs_spectra:document:kgrs_calibrated_spectra + data_to_document + + + + + kgrs_calibrated_spectra_per4.csv + 2019-08-22T22:26:09Z + + + 0 + PDS DSV 1 + + This archive consists of three spectrum files (each corresponding to one KGRS epoch) and one unified + EPG file. The spectrum files contain a time series of corrected and calibrated pulse height spectra + acquired by KGRS's HPGe detector in the lunar orbit. In the spectrum files, each row contains the + spacecraft clock (sclk) ticks and UTC time corresponding to the end of the accumulation interval + (17 s), with the two sets of the 8192-channel HPGe spectra accumulated. In the EPG file, each row + starts with sclk recorded at the end of the accumulation interval to match spacecraft positions, + pointing, and correction factors with the corrected spectra. Note that the UTC time and ephemeris time + included in the EPG file correspond to the midpoint of the accumulation interval. + + 527736 + Carriage-Return Line-Feed + Comma + + 10 + 2 + + sclk + 1 + ASCII_Integer + seconds + + Spacecraft clock (sclk) ticks at the end of the accumulation interval in seconds. The origin + of the sclk is Jan 6, 1980, 0:0:0. Each spectrum, scaler value, and ephemeris have a unique + sclk value, which can be used as an identifier. Kaguya's sclk is also known as a time index + (TI). + + + + utc + 2 + ASCII_String + UTC time corresponding to the sclk at the end of the accumulation interval + + + Period + 3 + ASCII_Integer + Epoch of the Kaguya GRS mission, 1-3. + + + background_observation + 4 + ASCII_Integer + + A flag to indicate the special operations of the Kaguya spacecraft where it was flipped and the GRS + was pointed to the deep space to measure background gamma rays from spacecraft. 0 indicates nominal + measurements suitable for geochemical study of the Moon. 1 indicates spectra were obtained during + the background-measuring operations. + + + + live_time + 5 + ASCII_Real + seconds + Live time of the spectrometer + + + ge_over + 6 + ASCII_Integer + + Overload scaler value for the HPGe detector. A good proxy for variations in intensities of galactic + cosmic rays. + + + + offset_HG + 7 + ASCII_Real + 0th order coefficient for calibration of ADC channels to energies for high-gain spectra + + + gain_HG + 8 + ASCII_Real + 1st order coefficient for calibration of ADC channels to energies for high-gain spectra + + + offset_LG + 9 + ASCII_Real + 0th order coefficient for calibration of ADC channels to energies for low-gain spectra + + + gain_LG + 10 + ASCII_Real + 1st order coefficient for calibration of ADC channels to energies for low-gain spectra + + + 1 + 8192 + 1 + 0 + + high_gain_histogram + 1 + ASCII_Integer + + 8192-channel, high-gain calibrated HPGe spectrum covering up to ~3.3 MeV. + The pulse height of each channel (0-8191), E, is given by E (keV) = gain_HG x ch + offset_HG. + + + + + 2 + 8192 + 1 + 0 + + low_gain_histogram + 1 + ASCII_Integer + + 8192-channel, low-gain calibrated HPGe spectrum covering up to ~13 MeV. + The pulse height of each channel (0-8191), E, is given by E (keV) = gain_LG x ch + offset_LG. + + + + + + + diff --git a/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per5.csv b/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per5.csv new file mode 100644 index 000000000..e69de29bb diff --git a/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per5.xml b/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per5.xml new file mode 100644 index 000000000..00abca577 --- /dev/null +++ b/src/test/resources/github238/valid/data_spectra/kgrs_calibrated_spectra_per5.xml @@ -0,0 +1,238 @@ + + + + + + urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per5 + 1.0 + Kaguya Gamma-Ray Spectrometer Corrected Spectra + 1.11.0.0 + Product_Observational + + + 2019-09-30 + 1.0 + First release + + + + + + 2009-02-10T18:26:40Z + 2009-05-28T07:43:22Z + + + Science + Derived + + This collection contains Kaguya Gamma-Ray Spectrometer (KGRS) corrected and calibrated time-series + spectra acquired during the nominal and extended observation periods of JAXA's SELENE (Kaguya) mission. + + The SELENE mission was the Japanese mission to the Moon with a main orbiter “Kaguya” and + two daughter relay satellites launched on Sep. 14, 2007. KGRS was mounted on the deck of the + main orbiter. It employed a high-purity Ge (HPGe) crystal as a main detector, and surrounding + BGO and plastic scintillators as anti-coincidence detectors to reduce backgrounds. The + Ge crystal was cooled by a Sterling refrigerator. It made close-proximity observations of the + Moon from Dec. 14, 2007 to Dec. 11, 2008 at the high circular orbital altitude of 100 km, and + from Feb. 10 to May 28 in 2009 at the low elliptical orbital altitude of ~30 x 50 km. + + KGRS recorded energy spectra of gamma rays in two gain modes simultaneously; high gain (0.1 + to 3 MeV) and low gain (0.1 to 13 MeV), each of which was analyzed by the 13-bit (8192 ch) + analog-to-digital converter (ADC). While the former has a higher spectral resolution over the + energy range of radioactive elements, the latter has better statistics and covers the whole energy + range of major rock-forming elements, including the Fe neutron capture line at 7.6 MeV. The + accumulation time of each spectrum was 17 s. Both modes of spectra are included in this archive. + + The observation epochs of KGRS consists of three regular measurement periods (Period 1 to 3), + background measurements, and the annealing of the Ge crystal. The HPGe detector was annealed + from 16 to 25, December 2008, which improved energy resolution by a factor of two. + Period 1 and 2 lasted two and five months, respectively, with limited spatial or spectral + resolutions. Period 3 lasted ~3.5 months (including dead time) with the best spatial and spectral + resolutions. In addition, spectra from the background measurement when the satellite was flipped + and the detector faced deep space can be analyzed to estimate the background gamma-ray intensity + from the satellite due to the exposure to galactic cosmic rays. + + The following data reduction processes, based on those successfully used for Lunar Prospector and + Dawn missions, were applied to the raw time-series spectra of KGRS: 1) Filtering of invalid events, + 2) ADC Differential Non-Linearity, and 3) Gain correction and energy calibration. Correction factors + for satellite altitude and galactic cosmic ray intensities are provided as part of the KGRS ephemeris + data. + + + + Kaguya + Mission + + urn:nasa:pds:context:investigation:mission.kaguya + data_to_investigation + + + + Kaguya + + Kaguya + Spacecraft + + urn:nasa:pds:context:instrument_host:spacecraft.kaguya + is_instrument_host + + + + GRS + Instrument + + urn:nasa:pds:context:instrument:kaguya.grs + is_instrument + + + + + Moon + Satellite + + urn:nasa:pds:context:target:satellite.earth.moon + collection_to_target + + + + + + urn:nasa:pds:kaguya_grs_spectra:document:kgrs_calibrated_spectra + data_to_document + + + + + kgrs_calibrated_spectra_per5.csv + 2019-08-22T22:26:09Z + + + 0 + PDS DSV 1 + + This archive consists of three spectrum files (each corresponding to one KGRS epoch) and one unified + EPG file. The spectrum files contain a time series of corrected and calibrated pulse height spectra + acquired by KGRS's HPGe detector in the lunar orbit. In the spectrum files, each row contains the + spacecraft clock (sclk) ticks and UTC time corresponding to the end of the accumulation interval + (17 s), with the two sets of the 8192-channel HPGe spectra accumulated. In the EPG file, each row + starts with sclk recorded at the end of the accumulation interval to match spacecraft positions, + pointing, and correction factors with the corrected spectra. Note that the UTC time and ephemeris time + included in the EPG file correspond to the midpoint of the accumulation interval. + + 527736 + Carriage-Return Line-Feed + Comma + + 10 + 2 + + sclk + 1 + ASCII_Integer + seconds + + Spacecraft clock (sclk) ticks at the end of the accumulation interval in seconds. The origin + of the sclk is Jan 6, 1980, 0:0:0. Each spectrum, scaler value, and ephemeris have a unique + sclk value, which can be used as an identifier. Kaguya's sclk is also known as a time index + (TI). + + + + utc + 2 + ASCII_String + UTC time corresponding to the sclk at the end of the accumulation interval + + + Period + 3 + ASCII_Integer + Epoch of the Kaguya GRS mission, 1-3. + + + background_observation + 4 + ASCII_Integer + + A flag to indicate the special operations of the Kaguya spacecraft where it was flipped and the GRS + was pointed to the deep space to measure background gamma rays from spacecraft. 0 indicates nominal + measurements suitable for geochemical study of the Moon. 1 indicates spectra were obtained during + the background-measuring operations. + + + + live_time + 5 + ASCII_Real + seconds + Live time of the spectrometer + + + ge_over + 6 + ASCII_Integer + + Overload scaler value for the HPGe detector. A good proxy for variations in intensities of galactic + cosmic rays. + + + + offset_HG + 7 + ASCII_Real + 0th order coefficient for calibration of ADC channels to energies for high-gain spectra + + + gain_HG + 8 + ASCII_Real + 1st order coefficient for calibration of ADC channels to energies for high-gain spectra + + + offset_LG + 9 + ASCII_Real + 0th order coefficient for calibration of ADC channels to energies for low-gain spectra + + + gain_LG + 10 + ASCII_Real + 1st order coefficient for calibration of ADC channels to energies for low-gain spectra + + + 1 + 8192 + 1 + 0 + + high_gain_histogram + 1 + ASCII_Integer + + 8192-channel, high-gain calibrated HPGe spectrum covering up to ~3.3 MeV. + The pulse height of each channel (0-8191), E, is given by E (keV) = gain_HG x ch + offset_HG. + + + + + 2 + 8192 + 1 + 0 + + low_gain_histogram + 1 + ASCII_Integer + + 8192-channel, low-gain calibrated HPGe spectrum covering up to ~13 MeV. + The pulse height of each channel (0-8191), E, is given by E (keV) = gain_LG x ch + offset_LG. + + + + + + + diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.csv b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.csv index 1f4646883..53331b083 100644 --- a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.csv +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.csv @@ -1,3 +1 @@ -P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per1::1.0 -P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per2::1.0 -P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per3::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per1::1.0 \ No newline at end of file diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.xml b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.xml index b2a27d030..8589d47b9 100644 --- a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.xml +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory.xml @@ -85,7 +85,7 @@ 0 PDS DSV 1 - 3 + 1 Carriage-Return Line-Feed Comma diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_2.csv b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_2.csv new file mode 100644 index 000000000..36b9d4f5a --- /dev/null +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_2.csv @@ -0,0 +1,2 @@ +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per1::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per2::1.0 \ No newline at end of file diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_2.xml b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_2.xml index c14fff2f0..fa9e8d68b 100644 --- a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_2.xml +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_2.xml @@ -79,13 +79,13 @@ - spectra_data_collection_inventory.csv + spectra_data_collection_inventory_2.csv 2019-09-27 0 PDS DSV 1 - 3 + 2 Carriage-Return Line-Feed Comma diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_3.csv b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_3.csv new file mode 100644 index 000000000..1f4646883 --- /dev/null +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_3.csv @@ -0,0 +1,3 @@ +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per1::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per2::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per3::1.0 diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_3.xml b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_3.xml index e22cb206b..778f2dbfa 100644 --- a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_3.xml +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_3.xml @@ -79,7 +79,7 @@ - spectra_data_collection_inventory.csv + spectra_data_collection_inventory_3.csv 2019-09-27 diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_4.csv b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_4.csv new file mode 100644 index 000000000..6f939f487 --- /dev/null +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_4.csv @@ -0,0 +1,4 @@ +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per1::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per2::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per3::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per4::1.0 \ No newline at end of file diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_4.xml b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_4.xml index 9174259a8..559888088 100644 --- a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_4.xml +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_4.xml @@ -8,7 +8,7 @@ xsi:schemaLocation="http://pds.nasa.gov/pds4/pds/v1 https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1B00.xsd"> urn:nasa:pds:kaguya_grs_spectra:data_spectra - 2.1 + 1.4 Kaguya Gamma-Ray Spectrometer Corrected Spectra Collection 1.11.0.0 Product_Collection @@ -79,13 +79,13 @@ - spectra_data_collection_inventory.csv + spectra_data_collection_inventory_4.csv 2019-09-27 0 PDS DSV 1 - 3 + 4 Carriage-Return Line-Feed Comma diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_5.csv b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_5.csv new file mode 100644 index 000000000..35915f300 --- /dev/null +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_5.csv @@ -0,0 +1,5 @@ +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per1::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per2::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per3::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per4::1.0 +P,urn:nasa:pds:kaguya_grs_spectra:data_spectra:kgrs_calibrated_spectra_per5::1.0 \ No newline at end of file diff --git a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_5.xml b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_5.xml index 1f987a540..508581cc2 100644 --- a/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_5.xml +++ b/src/test/resources/github238/valid/data_spectra/spectra_data_collection_inventory_5.xml @@ -8,7 +8,7 @@ xsi:schemaLocation="http://pds.nasa.gov/pds4/pds/v1 https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1B00.xsd"> urn:nasa:pds:kaguya_grs_spectra:data_spectra - 2.03 + 1.5 Kaguya Gamma-Ray Spectrometer Corrected Spectra Collection 1.11.0.0 Product_Collection @@ -79,13 +79,13 @@ - spectra_data_collection_inventory.csv + spectra_data_collection_inventory_5.csv 2019-09-27 0 PDS DSV 1 - 3 + 5 Carriage-Return Line-Feed Comma