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- ID:
- ivo://padc.obspm.helio/bass2000/q/epn_core
- Title:
- BASS2000 Solar Survey Archive
- Short Name:
- Bass2000
- Date:
- 07 May 2024 04:32:22
- Publisher:
- Paris Astronomical Data Centre
- Description:
- EPNcore table of BASS2000, a Solar survey archive: Images, movies of full Sun from groundbased instruments: Spectroheliographs of Meudon and Coimbra, RadioHeliograph and Decametric Array of Nancay, CLIMSO, USET
- ID:
- ivo://pds-ppi/cassini_caps_fitted_parameters/ppi/epn_core
- Title:
- Cassini CAPS Moments Data Collection
- Short Name:
- CO-CAPS-FIT
- Date:
- 15 Dec 2022 19:30:00
- Publisher:
- Planetary Data System
- Description:
- This data collection contains fits (both good and bad) that were found during R. J. Wilson et al's grant from NASA's Cassini Data Analysis Program (NNX12AG90G).
- ID:
- ivo://pds-ppi/cassini_caps_derived_ion_mom/ppi/epn_core
- Title:
- Cassini-Huygens Cassini Plasma Spectrometer (CAPS) Derived Ion Moments Data Collection
- Short Name:
- CO-CAPS-DDR-ION
- Date:
- 15 Dec 2022 19:25:07
- Publisher:
- Planetary Data System
- Description:
- CASSINI ORBITER SAT/SW CAPS DERIVED ION MOMENTS V1.0
- ID:
- ivo://pds-ppi/cassini_caps_derived_scpot/ppi/epn_core
- Title:
- Cassini-Huygens Cassini Plasma Spectrometer (CAPS) Derived Spacecraft Potential Data Collection
- Short Name:
- CO-CAPS-SCPOT
- Date:
- 15 Dec 2022 19:25:30
- Publisher:
- Planetary Data System
- Description:
- CASSINI ORBITER SAT/SW CAPS DERIVED Spacecraft Potential V1.0
- ID:
- ivo://pds-ppi/cassini_caps_calibrated_els/ppi/epn_core
- Title:
- Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Electron Spectrometer Data Collection
- Short Name:
- CO-CAPS-ELS
- Date:
- 16 Dec 2022 17:19:17
- Publisher:
- Planetary Data System
- Description:
- This collection consists of all of the calibrated electron spectrometer data from the Cassini Plasma Spectrometer (CAPS) on-board the Cassini spacecraft during the entire Cassini mission.
- ID:
- ivo://pds-ppi/cassini_caps_calibrated_ibs/ppi/epn_core
- Title:
- Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Ion Beam Spectrometer Data Collection
- Short Name:
- CO-CAPS-IBS
- Date:
- 15 Dec 2022 19:26:37
- Publisher:
- Planetary Data System
- Description:
- This collection consists of all of the calibrated ion beam spectrometer data from the Cassini Plasma Spectrometer (CAPS) on-board the Cassini spacecraft during the entire Cassini mission.
- ID:
- ivo://pds-ppi/cassini_caps_calibrated_ion/ppi/epn_core
- Title:
- Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Ion Mass Spectrometer Ion Data Collection
- Short Name:
- CO-CAPS-ION
- Date:
- 15 Dec 2022 19:24:19
- Publisher:
- Planetary Data System
- Description:
- This collection consists of all of the calibrated Ion Mass Spectrometer ion data from the Cassini Plasma Spectrometer (CAPS) on-board the Cassini spacecraft during the entire Cassini mission.
9. Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Ion Mass Spectrometer Singles Data Collection
- ID:
- ivo://pds-ppi/cassini_caps_calibrated_sng/ppi/epn_core
- Title:
- Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Ion Mass Spectrometer Singles Data Collection
- Short Name:
- CO-CAPS-SNG
- Date:
- 15 Dec 2022 19:30:05
- Publisher:
- Planetary Data System
- Description:
- This collection consists of all of the calibrated ion mass spectrometer singles data from the Cassini Plasma Spectrometer (CAPS) on-board the Cassini spacecraft during the entire Cassini mission.
- ID:
- ivo://pds-ppi/cassini_caps_calibrated_toflef/ppi/epn_core
- Title:
- Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Ion Mass Spectrometer 'Time Of Flight' Linear Electric Field Data Collection
- Short Name:
- CO-CAPS-TOFLEF
- Date:
- 15 Dec 2022 19:27:24
- Publisher:
- Planetary Data System
- Description:
- This collection consists of all of the calibrated ion mass spectrometer 'time of flight' linear electric field data from the Cassini Plasma Spectrometer (CAPS) on-board the Cassini spacecraft during the entire Cassini mission.
- ID:
- ivo://pds-ppi/cassini_caps_calibrated_tofst/ppi/epn_core
- Title:
- Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Ion Mass Spectrometer 'Time Of Flight' Straight Through Data Collection
- Short Name:
- CO-CAPS-TOFST
- Date:
- 15 Dec 2022 19:30:57
- Publisher:
- Planetary Data System
- Description:
- This collection consists of all of the calibrated ion mass spectrometer 'time of flight' straight through data from the Cassini Plasma Spectrometer (CAPS) on-board the Cassini spacecraft during the entire Cassini mission.
- ID:
- ivo://pds-ppi/cassini_caps_derived_ele_mom/ppi/epn_core
- Title:
- Cassini-Huygens Plasma Spectrometer (CAPS) Derived Electron Moments Data Collection
- Short Name:
- CO-CAPS-DDR-ELE
- Date:
- 15 Dec 2022 19:27:26
- Publisher:
- Planetary Data System
- Description:
- This collection consists of all of the electron moments data generated from the Cassini Plasma Spectrometer (CAPS) electron spectrometer uncalibrated data.
- ID:
- ivo://pds-ppi/cassini_mag_cal_1min_krtp/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Min. Avg. Data in KRTP Coords. Collection
- Short Name:
- CO-MAG-1MKRTP
- Date:
- 01 Mar 2024 22:04:43
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 minute averages in KRTP coordinates, from the Fluxgate Magnetometer (FGM) instrument. KRTP coordinates are the standard right-handed spherical triad: R (Saturn to spacecraft), Phi (parallel to Saturn's equator), and Theta (completes right handed set).
- ID:
- ivo://pds-ppi/cassini_mag_cal_1min_ksm/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Min. Avg. Data in KSM Coords. Collection
- Short Name:
- CO-MAG-1MKSM
- Date:
- 01 Mar 2024 22:05:18
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 minute averages in KSM coordinates, from the Fluxgate Magnetometer (FGM) instrument. KSM coordinates consist of X (Saturn to Sun), Z (X-Z plane contains Saturn's centered magnetic dipole axis, M), and Y (completes right handed set)
- ID:
- ivo://pds-ppi/cassini_mag_cal_1min_kso/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Min. Avg. Data in KSO Coords. Collection
- Short Name:
- CO-MAG-1MKSO
- Date:
- 01 Mar 2024 22:10:29
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 minute averages in KSO coordinates, from the Fluxgate Magnetometer (FGM) instrument. KSO coordinates consist of X (Saturn to Sun), Z (parallel to Saturn's orbital plane upward normal), and Y (completes the right handed set).
- ID:
- ivo://pds-ppi/cassini_mag_cal_1min_rtn/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Min. Avg. Data in RTN Coords. Collection
- Short Name:
- CO-MAG-1MRTN
- Date:
- 01 Mar 2024 22:11:02
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 minute averages, from the Cassini Fluxgate Magnetometer (FGM), in RTN coordinates. RTN coordinates consist of R (radial component, Sun to the spacecraft), T (tangential component, parallel to the Solar Equatorial plane and perpendicular to R), and N (normal component, completes right handed set).
- ID:
- ivo://pds-ppi/cassini_mag_cal_1sec_gse/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Sec. Avg. Data in GSE Coords. Collection
- Short Name:
- CO-MAG-1SGSE
- Date:
- 01 Mar 2024 22:11:37
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 second averages, in GSE coordinates, from the Fluxgate Magnetometer (FGM) instrument.
- ID:
- ivo://pds-ppi/cassini_mag_cal_1sec_j3/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Sec. Avg. Data in J3 Coords. Collection
- Short Name:
- CO-MAG-1SJ3
- Date:
- 01 Mar 2024 22:12:04
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 second averages in J3 coordinates, from the Fluxgate Magnetometer (FGM) instrument.
- ID:
- ivo://pds-ppi/cassini_mag_cal_1sec_jmxyz/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Sec. Avg. Data in JMXYZ Coords. Collection
- Short Name:
- CO-MAG-1SJMXYZ
- Date:
- 01 Mar 2024 22:12:40
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 second averages in JMXYZ coordinates, from the Fluxgate Magnetometer (FGM) instrument.
- ID:
- ivo://pds-ppi/cassini_mag_cal_1sec_krtp/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Sec. Avg. Data in KRTP Coords. Collection
- Short Name:
- CO-MAG-1SKRTP
- Date:
- 01 Mar 2024 22:13:10
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 second averages in KRTP coordinates, from the Fluxgate Magnetometer (FGM) instrument.
- ID:
- ivo://pds-ppi/cassini_mag_cal_1sec_ksm/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Sec. Avg. Data in KSM Coords. Collection
- Short Name:
- CO-MAG-1SKSM
- Date:
- 01 Mar 2024 22:13:39
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 second averages in KSM coordinates, from the Fluxgate Magnetometer (FGM) instrument.
- ID:
- ivo://pds-ppi/cassini_mag_cal_1sec_kso/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Sec. Avg. Data in KSO Coords. Collection
- Short Name:
- CO-MAG-1SKSO
- Date:
- 01 Mar 2024 22:14:02
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 second averages in KSO coordinates, from the Fluxgate Magnetometer (FGM) instrument.
- ID:
- ivo://pds-ppi/cassini_mag_cal_1sec_rtn/ppi/epn_core
- Title:
- Cassini MAG Calibrated 1 Sec. Avg. Data in RTN Coords. Collection
- Short Name:
- CO-MAG-1SRTN
- Date:
- 01 Mar 2024 22:14:22
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini magnetic-field 1 second averages in RTN coordinates, from the Fluxgate Magnetometer (FGM) instrument.
- ID:
- ivo://pds-ppi/cassini_rpws_electron_density/ppi/epn_core
- Title:
- Cassini RPWS Electron Densities from Upper Hybrid and Plasma Wave Frequencies
- Short Name:
- CO-RPWS-ELC-DEN
- Date:
- 16 Dec 2022 17:29:24
- Publisher:
- Planetary Data System
- Description:
- This collection provides electron number density values derived from features observed in plasma wave data obtained by the Cassini Radio and Plasma Wave Science (RPWS) instruments, along with observed or derived characteristic frequencies, and useful positional parameters for the spacecraft and related bodies. When present, frequency values of narrowband emissions at the upper hybrid resonance were digitized and combined with measured or model magnetic field to derive electron number density. At other times, features such as the upper cutoff in auroral hiss or electron plasma oscillations were used to determine the plasma frequency and electron density.
- ID:
- ivo://pds-ppi/cassini_mag_cal_shm_hkrate/ppi/epn_core
- Title:
- Cassini Scalar Helium MAG Calibrated Housekeeping ASCII Data Collection
- Short Name:
- CO-MAG-SHHKA
- Date:
- 01 Mar 2024 22:33:54
- Publisher:
- Planetary Data System
- Description:
- This collections contains Cassini scalar helium magnetometer (SHM) housekeeping ASCII data collected between 1999-08-18T02:56:40.391 and 2005-06-08T15:14:44.057.
- ID:
- ivo://pds-ppi/cassini_mag_cal_shm_hkrate_asc/ppi/epn_core
- Title:
- Cassini Scalar Helium MAG Calibrated Housekeeping Data Collection
- Short Name:
- CO-MAG-SHHK
- Date:
- 01 Mar 2024 22:33:40
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini scalar helium (SHM) magnetometer housekeeping data collected between 1999-08-18 and 2005-06-08.
- ID:
- ivo://pds-ppi/cassini_mag_cal_shm_scirate_asc/ppi/epn_core
- Title:
- Cassini Scalar Helium MAG Calibrated Science ASCII Data Collection
- Short Name:
- CO-MAG-SHSA
- Date:
- 01 Mar 2024 22:27:57
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini scalar helium magnetometer (SHM) science ASCII data collected between 1999-08-18 and 2005-10-11.
- ID:
- ivo://pds-ppi/cassini_mag_cal_shm_scirate/ppi/epn_core
- Title:
- Cassini Scalar Helium MAG Calibrated Science Data Collection
- Short Name:
- CO-MAG-SHS
- Date:
- 01 Mar 2024 22:26:13
- Publisher:
- Planetary Data System
- Description:
- This collection contains Cassini scalar helium magnetometer (SHM) science data collected between 1999-08-18 and 2005-10-11.
29. Cassini VIMS
- ID:
- ivo://padc.obspm.planeto/vims_satellites/q/epn_core
- Title:
- Cassini VIMS
- Short Name:
- VIMS satellites
- Date:
- 04 Feb 2024 04:04:45
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The Visual and Infrared Mapping Spectrometer (VIMS) instrument onboard the Cassini spacecraft observed the system of Saturn, acquiring spectral cubes in the range 0.4-5.2 microns. This service focuses on Saturn satellites, and provides access to calibrated and ancillary data, computed as described here: https://vims.univ-nantes.fr/info/isis-calibration. It also provides direct links to a larger web site with previews.
- ID:
- ivo://cxc.harvard.edu/csc
- Title:
- Chandra Source Catalog
- Short Name:
- CSC
- Date:
- 24 Oct 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory and one of NASA"s Great Observatories. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range. The Chandra Source Catalog (CSC) includes information about X-ray sources detected in observations obtained using the Chandra X-ray Observatory. Release 2.0 of the catalog includes 317,167 point, compact, and extended sources detected in ACIS and HRC-I imaging observations released publicly prior to the end of 2014. Observed source positions and multi-band count rates are reported, as well as numerous derived spatial, photometric, spectral, and temporal calibrated source properties that may be compared with data obtained by other telescopes. Each record includes the best estimates of the properties of a source based on data extracted from all observations in which the source was detected. The Chandra Source Catalog is extracted from the CXC"s Chandra Data Archive (CDA). The CXC should be acknowledged as the source of Chandra data. For detailed information on the Chandra Observatory and datasets see: http://cxc.harvard.edu/ for general Chandra information; http://cxc.harvard.edu/cda/ for the Chandra Data Archive; http://cxc.harvard.edu/csc/ for Chandra Source Catalog information.
- ID:
- ivo://cxc.harvard.edu/cscr1
- Title:
- Chandra Source Catalog Release 1
- Short Name:
- CSCR1
- Date:
- 24 Oct 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory and one of NASA"s Great Observatories. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range. The Chandra Source Catalog (CSC) includes information about X-ray sources detected in observations obtained using the Chandra X-ray Observatory. Release 1.1 of the catalog includes about 138,000 point and compact sources with observed spatial extents less than ~30 arcsec detected in a subset of ACIS and HRC-I imaging observations released publicly prior to the end of 2009. Observed source positions and multi-band count rates are reported, as well as numerous derived spatial, photometric, spectral, and temporal calibrated source properties that may be compared with data obtained by other telescopes. Each record includes the best estimates of the properties of a source based on data extracted from all observations in which the source was detected. The Chandra Source Catalog is extracted from the CXC"s Chandra Data Archive (CDA). The CXC should be acknowledged as the source of Chandra data. For detailed information on the Chandra Observatory and datasets see: http://cxc.harvard.edu/ for general Chandra information; http://cxc.harvard.edu/cda/ for the Chandra Data Archive; http://cxc.harvard.edu/csc/ for Chandra Source Catalog information.
- ID:
- ivo://cxc.harvard.edu/cscr2
- Title:
- Chandra Source Catalog Release 2
- Short Name:
- CSCR2
- Date:
- 24 Oct 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory and one of NASA"s Great Observatories. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range. The Chandra Source Catalog (CSC) includes information about X-ray sources detected in observations obtained using the Chandra X-ray Observatory. Release 2.0 of the catalog includes 317,167 point, compact, and extended sources detected in ACIS and HRC-I imaging observations released publicly prior to the end of 2014. Observed source positions and multi-band count rates are reported, as well as numerous derived spatial, photometric, spectral, and temporal calibrated source properties that may be compared with data obtained by other telescopes. Each record includes the best estimates of the properties of a source based on data extracted from all observations in which the source was detected. The Chandra Source Catalog is extracted from the CXC"s Chandra Data Archive (CDA). The CXC should be acknowledged as the source of Chandra data. For detailed information on the Chandra Observatory and datasets see: http://cxc.harvard.edu/ for general Chandra information; http://cxc.harvard.edu/cda/ for the Chandra Data Archive; http://cxc.harvard.edu/csc/ for Chandra Source Catalog information.
- ID:
- ivo://cxc.harvard.edu/cda
- Title:
- Chandra X-ray Observatory Data Archive
- Short Name:
- CDA
- Date:
- 18 Jul 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range.
- ID:
- ivo://padc.obspm.planeto/planets/q/epn_core
- Title:
- Characteristics of Planets
- Short Name:
- Planets
- Date:
- 16 Oct 2023 16:09:45
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- Main characteristics of Solar System planets. Data are included in the table, which includes non-standard EPN-TAP parameters. Data are retrieved from Archinal et al 2018 (IAU report 2015, 2018CeMDA.130...22A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods].
- ID:
- ivo://ov-gso/climso
- Title:
- CLIMSO coronagraphs at pic du midi de Bigorre
- Short Name:
- CLIMSO
- Date:
- 23 Feb 2024 14:58:31
- Publisher:
- OVGSO
- Description:
- Pic du Midi de Bigorre in the French Pyrenees is the place where coronagraphic images were first realized, by Bernard Lyot in the 1930s. Since then, the solar instruments at Pic du Midi regularly provide images of the solar disc, solar prominences and solar corona.
- ID:
- ivo://au.csiro/casda/TAP
- Title:
- CSIRO ASKAP Science Data Archive TAP Service
- Short Name:
- CSIRO ASKAP TAP
- Date:
- 09 Nov 2018 08:39:00
- Publisher:
- CSIRO
- Description:
- Table Access Protocol service for accessing catalogues from ASKAP radio astronomy observations
- ID:
- ivo://au.csiro/atoavo/TAP
- Title:
- CSIRO Australia Telescope Online Archive TAP Service
- Short Name:
- CSIRO ATOA TAP
- Date:
- 17 Jul 2020 16:23:58
- Publisher:
- CSIRO
- Description:
- Table Access Protocol service for accessing Australia Telescope Online Archive
- ID:
- ivo://au.csiro/psrda/ATNF_Pulsar_Data_Archive
- Title:
- CSIRO Parkes Pulsar Data Archive
- Short Name:
- CSIRO Pulsar TAP
- Date:
- 27 Jun 2018 15:23:26
- Publisher:
- CSIRO
- Description:
- Repository of pulsar observations made at the Parkes, Australia radio telescope
- ID:
- ivo://spectrum.iaa/abs_cs/q/epn_core
- 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:
- EPN-TAP access to IAA-CAB-INTA-CSIC absorption cross sections database.
- 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.
- 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
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:
- 07 May 2024 01:00:12
- 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:
- 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://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.