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61. EUV-SYN
ID:
ivo://idoc/medoc/eit_syn/q/epn_core
Title:
EUV-SYN
Short Name:
eit_syn.epn_core
Date:
16 Nov 2023 13:44:59
Publisher:
IDOC
Description:
*** EUV-SYN *** Synchronous synoptic maps of the corona in the extreme-UV (EUV), built from series of SoHO/EIT observations, in each of the 4 wavelength bands of the instrument. Synchronous synoptic maps are maps of the EUV radiance in different wavelength bands on the full solar sphere, in heliographic (Carrington) longitude and latitude, where data are taken as close as possible to a reference time. They capture the state of the corona at any given reference time by including data taken as close as possible to this time. EUV-SYN is available as part of the generic MEDOC interface which is currently located at https://idoc-medoc.ias.u-psud.fr/. These interfaces are based on the CNES SiTools2 framework. EUV-SYN is also available from IDL and Python scripts, using a specialization of the generic SiTools2 IDL and Python clients developed by MEDOC.
62. Exoplanet Catalog
ID:
ivo://padc.obspm.planeto/exoplanet/q/epn_core
Title:
Exoplanet Catalog
Short Name:
ExoPlanet
Date:
26 Feb 2025 11:04:07
Publisher:
Paris Astronomical Data Centre
Description:
Encyclopedia of extrasolar planet
63. Extrasolar Planets Encyclopaedia
ID:
ivo://vopdc.obspm/luth/exoplanet
Title:
Extrasolar Planets Encyclopaedia
Short Name:
ExoPlanet
Date:
10 Jan 2017
Publisher:
Paris Astronomical Data Centre - LUTH
Description:
VO-compliant and interactive encyclopaedia of extrasolar planets.
64. Five Supernova Survey Galaxies
ID:
ivo://vopdc.iap/fss
Title:
Five Supernova Survey Galaxies
Short Name:
FSS
Date:
10 Jan 2017
Publisher:
Institut d'Astrophysique de Paris
Description:
VO-compliant publication of the properties of the 3838 galaxies that were monitored for SNe events, including newly determined morphologies and their DENIS and POSS-II/UKST I, 2MASS and DENIS J and Ks and 2MASS H magnitudes.
65. Galaxie – Etoile – Physique – Instrumentation
ID:
ivo://vopdc.obspm/gepi
Title:
Galaxie – Etoile – Physique – Instrumentation
Short Name:
GEPI
Date:
10 Jan 2017
Publisher:
Paris Astronomical Data Centre - GEPI
Description:
The principal research topics of the GEPI (Galaxy - Star - Physics - Instrumentation) Laboratory are the formation and evolution of stars in our Galaxy as well as in numerous other galaxies, which constitute the luminous matter (baryonic matter) component of the Universe. This research calls upon many disciplines, from chemistry to physics, from instrumentation to data-processing engineering, and from project management to financial management within an international framework.
66. Galileo EPD Calibrated Corrected Delta Event Data Collection
ID:
ivo://pds-ppi/galileo_epd_cal_corrected_cms_events_deltaexe/ppi/epn_core
Title:
Galileo EPD Calibrated Corrected Delta Event Data Collection
Short Name:
galileo_epd_cal_
Date:
25 Apr 2025 02:01:31
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle Detector (EPD) instrument onboard the Galileo spacecraft that orbited Jupiter and measured intensities of ion and electron radiation in the keV and MeV energy range. This set is version 31 of reprocessing and version 1.0 of PDS delivery. The TOFxE and DeltaExE files include event data of ion measurements. Event data are different than the channelized data in the high, medium, and low resolution files. Event data record the full information of a measured particle. Every "event" is the measurement of a time of flight (TOF) within the instrument and energy deposited within a detector (TOFxE file), or two energy values deposited within the two detector layers (DeltaExE file). The deposited energy values are generally different from the energy the particle has in the ambient space. Event data provides measured values in the native resolution of the instrument. Because such high resolution increases data volume, event data cannot be taken continuously and downlinked all the time. Only the provided subset of this data was kept. The files are comma separated. Invalid entries will have values of -1.000000E+38. Times are provided in the format Year.DOYHHMMSSM (first column) and fractional year (second column) More information can be found in the User Guide. This file includes measurements by the EPD/CMS/DeltaExE instrument. For each counted event, the energy deposited in the two solid state detector layers (Ej_keV and Ek_keV columns) of the instrument are recorded.
67. Galileo EPD Calibrated Corrected High Res Data Collection
ID:
ivo://pds-ppi/galileo_epd_cal_corrected_high_res/ppi/epn_core
Title:
Galileo EPD Calibrated Corrected High Res Data Collection
Short Name:
galileo_epd_cal_
Date:
25 Apr 2025 02:03:34
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle Detector (EPD) instrument onboard the Galileo spacecraft that orbited Jupiter and measured intensities of ion and electron radiation in the keV and MeV energy range. This set is version 31 of reprocessing and version 1.0 of PDS delivery. Data in the high resolution files include measurements that are binned into channels responding to certain energy and species ranges. The files are comma separated. Invalid entries will have -1.000000E+38 as an entry. The first 4 lines of each data text file provide information on the channels included here: The first line of each file lists the names of the channels included. The second line lists the center energies of these channels in keV. The third line lists the channels again. The forth line lists the mass of the measured particle in AMU. Zero mass refers to electrons. The forth line in the data text file labels the columns that follow in the file. The columns include times, radiation measurements, spacecraft location, instrument look direction, and some supplementary information. Radiation measurements are provided both as best calibrated and cleaned intensities as well as raw, uncorrected count rates. Columns with channel names followed by a "j" include calibrated differential intensities of the given channel. If the value is negative, it should be ignored and particularly not included in averages. For the difference between -1.000000E+38 and all other negative values, see the User Guide. Columns ending with "f" provide differential intensities based on a combination of various channels. Columns ending with "i" include calibrated integral intensities. Columns with plain channel names describe the raw uncorrected count rate. Columns ending with "bg" are raw count rates measured behind the calibration shield. Each following line will provide the same data but for different times. More information can be found in the User Guide. This file provides data with the highest available time and pitch angle resolution. Only a small set of channels is provided, limiting the energy resolution and coverage. If columns with plain channel names have -1.000000E+38 values, you might find valid values in the lower resolution files.
68. Galileo EPD Calibrated Corrected Low Res Data Collection
ID:
ivo://pds-ppi/galileo_epd_cal_corrected_low_res/ppi/epn_core
Title:
Galileo EPD Calibrated Corrected Low Res Data Collection
Short Name:
galileo_epd_cal_
Date:
25 Apr 2025 02:05:24
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle Detector (EPD) instrument onboard the Galileo spacecraft that orbited Jupiter and measured intensities of ion and electron radiation in the keV and MeV energy range. This set is version 31 of reprocessing and version 1.0 of PDS delivery. Data in the low resolution files include measurements that are binned into channels responding to certain energy and species ranges. The files are comma separated. Invalid entries will have -1.000000E+38 as an entry. The first 4 lines of each data text file provide information on the channels included here: The first line of each file lists the names of the channels included. The second line lists the center energies of these channels in keV. The third line lists the channels again. The forth line lists the mass of the measured particle in AMU. Zero mass refers to electrons. The forth line in the data text file labels the columns that follow in the file. The columns include times, radiation measurements, spacecraft location, instrument look direction, and some supplementary information. Radiation measurements are provided both as best calibrated and cleaned intensities as well as raw, uncorrected count rates. Columns with channel names followed by a "j" include calibrated differential intensities of the given channel. If the value is negative, it should be ignored and particularly not included in averages. For the difference between -1.000000E+38 and all other negative values, see the User Guide. Columns ending with "f" provide differential intensities based on a combination of various channels. Columns ending with "i" include calibrated integral intensities. Columns with plain channel names describe the raw uncorrected count rate. Columns ending with "bg" are raw count rates measured behind the calibration shield. Each following line will provide the same data but for different times. More information can be found in the User Guide. This includes the full set of channels covering the full energy and species range of EPD. The time and pitch angle resolution is low. Higher resolution is available for some channels that can be found in the medium and high resolution files.the energy deposited in the one solid state detector (Energy_keV column) and the time of flight (TOF_ns) within the instrument are recorded.
69. Galileo EPD Calibrated Corrected Medium Res Data Collection
ID:
ivo://pds-ppi/galileo_epd_cal_corrected_med_res/ppi/epn_core
Title:
Galileo EPD Calibrated Corrected Medium Res Data Collection
Short Name:
galileo_epd_cal_
Date:
25 Apr 2025 02:02:57
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle Detector (EPD) instrument onboard the Galileo spacecraft that orbited Jupiter and measured intensities of ion and electron radiation in the keV and MeV energy range. This set is version 31 of reprocessing and version 1.0 of PDS delivery. Data in the medium resolution files include measurements that are binned into channels responding to certain energy and species ranges. The files are comma separated. Invalid entries will have -1.000000E+38 as an entry. The first 4 lines of each data text file provide information on the channels included here: The first line of each file lists the names of the channels included. The second line lists the center energies of these channels in keV. The third line lists the channels again. The forth line lists the mass of the measured particle in AMU. Zero mass refers to electrons. The forth line in the data text file labels the columns that follow in the file. The columns include times, radiation measurements, spacecraft location, instrument look direction, and some supplementary information. Radiation measurements are provided both as best calibrated and cleaned intensities as well as raw, uncorrected count rates. Columns with channel names followed by a "j" include calibrated differential intensities of the given channel. If the value is negative, it should be ignored and particularly not included in averages. For the difference between -1.000000E+38 and all other negative values, see the User Guide. Columns ending with "f" provide differential intensities based on a combination of various channels. Columns ending with "i" include calibrated integral intensities. Columns with plain channel names describe the raw uncorrected count rate. Columns ending with "bg" are raw count rates measured behind the calibration shield. Each following line will provide the same data but for different times. More information can be found in the User Guide. This includes a limited set of channels with intermediate time and pitch angle resolution. If columns with plain channel names have -1.000000E+38 values, you might find valid values in the lower resolution files.
70. Galileo EPD Calibrated Corrected Time-of-Flight Event Data Collection
ID:
ivo://pds-ppi/galileo_epd_cal_corrected_cms_events_tof/ppi/epn_core
Title:
Galileo EPD Calibrated Corrected Time-of-Flight Event Data Collection
Short Name:
EPD-TOF-EVE
Date:
15 Dec 2022 19:26:10
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle Detector (EPD) instrument onboard the Galileo spacecraft that orbited Jupiter and measured intensities of ion and electron radiation in the keV and MeV energy range. This set is version 31 of reprocessing and version 1.0 of PDS delivery. The TOFxE and DeltaExE files include event data of ion measurements. Event data are different than the channelized data in the high, medium, and low resolution files. Event data record the full information of a measured particle. Every "event" is the measurement of a time of flight (TOF) within the instrument and energy deposited within a detector (TOFxE file), or two energy values deposited within the two detector layers (DeltaExE file). The deposited energy values are generally different from the energy the particle has in the ambient space. Event data provides measured values in the native resolution of the instrument. Because such high resolution increases data volume, event data cannot be taken continuously and downlinked all the time. Only the provided subset of this data was kept. The files are comma separated. Invalid entries will have values of -1.000000E+38. Times are provided in the format Year.DOYHHMMSSM (first column) and fractional year (second column) More information can be found in the User Guide. This file includes measurements by the EPD/CMS/TOFxE instrument. For each counted event, the energy deposited in the one solid state detector (Energy_keV column) and the time of flight (TOF_ns) within the instrument are recorded.

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