Number of results to display per page
Search Results
42. ESO-R Survey
- ID:
- ivo://vopdc.obspm/gepi/vopsat/esor
- Title:
- ESO-R Survey
- Short Name:
- ESO-R
- Date:
- 10 Nov 2022
- Publisher:
- Paris Astronomical Data Centre - GEPI
- Description:
- VO-compliant publication of Schmidt survey ESO-R of the southern sky digitized with the MAMA microdensitometer at the Observatoire de Paris Image Analysis Centre (CAI).
43. 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.
- 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
45. EXOTOPO
- ID:
- ivo://geops.ipsl/exotopo/q/epn_core
- Title:
- EXOTOPO
- Short Name:
- exotopo.epn_core
- Date:
- 17 Jul 2024 15:24:58
- Publisher:
- IPSL/GEOPS
- Description:
- "The data consists in topographic maps of synthetic 3D bodies generated by a 3 parameters statistical model : the fractionally integrated flux (FiF) (Lavallee, D., Lovejoy, S., Schertzer, D., Ladoy, P. (1993). Nonlinear variability and landscape topography: analysis and simulation) adapted for spherical coordinates and topography (Landais, F., Schmidt, F., and Lovejoy, S, (2018) Topography of exoplanets, MNRAS). The 3 parameters are the following : H: degree of smoothness; C1: degree of intermittency; alpha: degree of multifractality; The service contains topographic maps (in Fits format) and texture maps (in png format)."
- 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:
- EPD-DELTA-EVE
- Date:
- 15 Dec 2022 19:26:15
- 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.
- ID:
- ivo://pds-ppi/galileo_epd_cal_corrected_high_res/ppi/epn_core
- Title:
- Galileo EPD Calibrated Corrected High Res Data Collection
- Short Name:
- EPD-HIGH-RES
- Date:
- 15 Dec 2022 19:27:32
- 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.
- ID:
- ivo://pds-ppi/galileo_epd_cal_corrected_low_res/ppi/epn_core
- Title:
- Galileo EPD Calibrated Corrected Low Res Data Collection
- Short Name:
- EPD-LOW-RES
- Date:
- 15 Dec 2022 19:28:50
- 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.
- ID:
- ivo://pds-ppi/galileo_epd_cal_corrected_med_res/ppi/epn_core
- Title:
- Galileo EPD Calibrated Corrected Medium Res Data Collection
- Short Name:
- EPD-MED-RES
- Date:
- 15 Dec 2022 19:27:13
- 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.
- 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.
