- ID:
- ivo://spectrum.iaa/abs_cs/q/collection
- Title:
- Data for numerical modeling of planetary atmospheres
- Date:
- 12 Jun 2017 10:19:38
- Publisher:
- Instituto de Astrofisica de Andalucia-CSIC; INTA-CAB
- Description:
- Numerical modeling of composition and thermal balance of planetary atmospheres requires a considerable amount of laboratory data. Among them, the absorption cross sections in the UV range are needed both for computing the heating in the atmosphere and the photodissociation coefficients to initiate a rich disequilibrium chemistry. Prompted by these needs in the community and by the sparse collection of data in several other web pages (http://www.science-softcon.de/ or http://satellite.mpic.de/spectral_atlas/index.html whose data depend on some pre-processing before being ingested in these models), this web page aims at providing the community with absorption cross sections in the range 20 nm to 400 nm equally spaced every 0.2, 0.5 and 1.0 nm. Also, original data as appearing in the refereed journal and the reference itself are downloadable.
Number of results to display per page
Search Results
- ID:
- ivo://vopdc.obspm/dfbs
- Title:
- Digitized First Byurakan Survey
- Short Name:
- DFBS
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.
- ID:
- ivo://padc.obspm.planeto/dynastvo/q/epn_core
- Title:
- DynastVO ephemeris service
- Short Name:
- DynAstVO
- Date:
- 07 May 2024 02:02:48
- Publisher:
- Paris Astronomical Data Centre
- Description:
- This database displays calculated orbital parameters for small bodies
64. 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).
65. 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:
- 07 May 2024 01:00:12
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Encyclopedia of extrasolar planet
67. EXOTOPO
- ID:
- ivo://geops.ipsl/exotopo/q/epn_core
- Title:
- EXOTOPO
- Short Name:
- exotopo.epn_core
- Date:
- 01 May 2024 01:20:13
- 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://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.
- 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.
- 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.
- 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.
- ID:
- ivo://pds-ppi/galileo_hic_prejup_derived/ppi/epn_core
- Title:
- Galileo HIC Derived Ion Fluxes October 89 Solar Event Data Collection
- Short Name:
- GO-HIC-PJ-DER
- Date:
- 15 Dec 2022 19:30:31
- Publisher:
- Planetary Data System
- Description:
- This collection contains values for the fluxes of heavy ions associated with an energetic particle event of solar origin. The values are derived from HIC data taken during the Interplanetary Cruise to Jupiter.
- ID:
- ivo://pds-ppi/galileo_hic_jup_derived/ppi/epn_core
- Title:
- Galileo Jupiter HIC Derived Energetic Ion Competition Data Collection
- Short Name:
- GO-HIC-J-DER
- Date:
- 15 Dec 2022 19:25:36
- Publisher:
- Planetary Data System
- Description:
- This collection contains energetic (MeV) ion fluxes for a variety of different Z values (carbon, oxygen, sulfur) derived from the Heavy Ion Counter (HIC) instrument on the Galileo spacecraft. The data set includes all recorded intervals at Jupiter.
- ID:
- ivo://pds-ppi/galileo_hic_jup_raw/ppi/epn_core
- Title:
- Galileo Jupiter HIC High Resolution Raw Data Collection
- Short Name:
- GO-HIC-J-RAW
- Date:
- 15 Dec 2022 19:24:14
- Publisher:
- Planetary Data System
- Description:
- This collection contains raw energetic (MeV) particle data measured by the Heavy Ion Counter (HIC) instrument on the Galileo spacecraft. This data set contains both real-time and recorded data for all Jupiter orbits.
- ID:
- ivo://pds-ppi/galileo_hic_jup_calibrated_survey_countrate/ppi/epn_core
- Title:
- Galileo Jupiter HIC Survey Energetic Ion Count Rate Calibrated Collection Data Collection
- Short Name:
- HIG-J-SRVY-CNT
- Date:
- 15 Dec 2022 19:30:33
- Publisher:
- Planetary Data System
- Description:
- This collection contains energetic (MeV) ion count rates and events measured by the Heavy Ion Counter (HIC) instrument on the Galileo spacecraft. The data are derived from the raw real-time science (RTS) data. There are two basic types of data files associated with the full-rate reduced data: Detector Count Rates and Events (Pulse Heights).
- ID:
- ivo://pds-ppi/galileo_mag_jup_calibrated_highres_callisto/ppi/epn_core
- Title:
- Galileo Jupiter Magnetometer Highres Callisto Data Collection
- Short Name:
- GO-MAG-JUP-CAL
- Date:
- 15 Dec 2022 19:29:16
- Publisher:
- Planetary Data System
- Description:
- This data collection contains high time resolution magnetic field vectors acquired by the Galileo magnetometer (MAG). It includes satellite flyby Callisto data. These data were acquired in order to characterize various portions of the Jovian magnetosphere at high time resolution.