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- ID:
- ivo://arecibo.cornell/hiarchive/alfalfa
- Title:
- Arecibo Legacy Fast ALFA Survey
- Short Name:
- ALFALFA
- Date:
- 08 Apr 2016 18:59:56
- Publisher:
- Cornell University
- Description:
- The Arecibo Legacy Fast ALFA extragalactic HI survey uses the Arecibo multibeam receiver to survey 7000 square degrees of high galactic latitude sky. Utilizing the high sensitivity of Arecibo, the survey will detect over 20000 HI sources in the local universe. The survey products include catalogs with extracted measurements and HI parameters, as well as integrated HI spectral profiles. The survey is currently served by NED.
- ID:
- ivo://astro-wise
- Title:
- Astro-Wise Authority
- Short Name:
- Astro-Wise
- Date:
- 24 May 2007 05:57:00
- Publisher:
- Astro-Wise local publishing registry
- Description:
- This authority ID will be used to identify resources related to Astro- Wise consortium
- ID:
- ivo://padc.obspm.planeto/apis/q/epn_core
- Title:
- Auroral Planetary Imaging and Spectroscopy
- Short Name:
- APIS
- Date:
- 21 Nov 2022 09:23:56
- Publisher:
- Paris Astronomical Data Centre
- Description:
- EpnCore table for APIS service
- ID:
- ivo://padc.obspm.helio/bass2000/q/epn_core
- Title:
- BASS2000 Solar Survey Archive
- Short Name:
- Bass2000
- Date:
- 27 Feb 2024 04:32:19
- 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://vopdc.obspm/lesia/BeStars/BeSC
- Title:
- Be Stars Catalog
- Short Name:
- BeSC
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- The BeSC database contains the complete catalogue of classical Be stars with some of their fundamental stellar parameters.
- ID:
- ivo://vopdc.obspm/lesia/BeStars
- Title:
- Be Stars Database
- Short Name:
- BeStars
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- The BeStars project contains (1) the complete catalogue of classical Be stars, BeSC, with some of their fundamental stellar parameters, and (2) a database, BeSS, which assembles classical Be star spectra obtained by professional and amateur astronomers at any wavelength, epoch, and spectral resolution.
- ID:
- ivo://vopdc.obspm/lesia/BeStars/BeSS
- Title:
- Be Stars Spectra
- Short Name:
- BeSS
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- The BeSS database assembles classical Be star spectra obtained by professional and amateur astronomers at any wavelength, epoch, and spectral resolution.
- ID:
- ivo://idoc.d2s/corot/brightstars-conesearch
- Title:
- Bright stars IDOC D2S ConeSearch
- Short Name:
- CoRoT_N2_Bright
- Date:
- 13 May 2019 17:14:07
- Publisher:
- IDOC D2S
- Description:
- CoRoT bright stars seismo field
- 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.
16. 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.
36. 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/hips
- Title:
- Chandra HiPS Service
- Short Name:
- CXC hips service
- Date:
- 18 Jul 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory Data Archive provides a reference survey via the HiPS protocol. 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/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/csc.siap
- 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. 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/cscr1.siap
- 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. 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/cscr2.siap
- 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. 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/registry
- Title:
- Chandra X-ray Center Publishing Registry
- Short Name:
- CXC-Reg
- Date:
- 02 Oct 2013
- Publisher:
- Chandra X-ray Observatory
- Description:
- This registry provides a simple interface for data providers who wish to register a handful of resources. It is compliant with VOResource v0.10
- 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://cxc.harvard.edu/cda.siap
- Title:
- Chandra X-ray Observatory Data Archive
- Short Name:
- CDA
- Date:
- 21 Dec 2015
- 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://idoc.d2s/corot/stars-rotation-period-medeiros-conesearch
- Title:
- Confirmed Corot exoplanets IDOC D2S ConeSearch
- Short Name:
- CoRoT_N2_RotMed
- Date:
- 13 May 2019 17:28:13
- Publisher:
- IDOC D2S
- Description:
- Stars with rotation periods from de Medeiros et al
- ID:
- ivo://idoc.d2s/corot/confirmedplanet-conesearch
- Title:
- Confirmed Corot exoplanets IDOC D2S ConeSearch
- Short Name:
- CoRoT_N2_ConfExo
- Date:
- 13 May 2019 17:26:07
- Publisher:
- IDOC D2S
- Description:
- This catalog includes the CoRoT targets around which the presence of an exoplanet was confirmed and published. It does not include the more numerous planet candidates.
- ID:
- ivo://arecibo.cornell/hiarchive
- Title:
- Cornell Digital HI Archive
- Short Name:
- digitalHIarchive
- Date:
- 07 Apr 2016 15:07:07
- Publisher:
- Cornell University
- Description:
- The Cornell Digital HI Archive is a homogeneous compilation of HI spectral parameters extracted from global 21 cm line spectra for some 9000 galaxies in the local universe (heliocentric velocity -200 < V > 28,000 km/s) obtained with a variety of large single dish radio telescopes but reanalyzed using a single set of parameter extraction algorithms. The database contains a catalog of HI parameters (systemic velocities, integrated HI line fluxes and full widths), plots of the HI spectra, and the digital spectra themselves. The Cornell Digital HI Archive data is currently served by NED.
- ID:
- ivo://idoc.d2s/corot/redgiants-conesearch
- Title:
- CoRoT Red Giants D2S ConeSearch
- Short Name:
- CoRoT_N2_RedGia
- Date:
- 13 May 2019 17:26:29
- Publisher:
- IDOC D2S
- Description:
- This catalog includes CoRoT targets from the exoplanet channel which were identified as possible red giants and actually presents acoustic oscillations of solar-like type, as published by Hekker et al. (A&A, 2009, vol. 506, p. 465).
- ID:
- ivo://au.csiro/casda/SCS
- Title:
- CSIRO ASKAP Science Data Archive Cone Search Service
- Short Name:
- CSIRO ASKAP Cone
- Date:
- 01 Dec 2023 14:46:51
- Publisher:
- CSIRO
- Description:
- Cone search service for querying catalogues from ASKAP radio astronomy observations
- ID:
- ivo://au.csiro/casda/SIA2
- Title:
- CSIRO ASKAP Science Data Archive Image Access Service
- Short Name:
- CSIRO ASKAP SIA2
- Date:
- 07 Jul 2017 16:23:19
- Publisher:
- CSIRO
- Description:
- Simple Image Access v2 service for querying multi-dimensional image products from ASKAP radio astronomy observations
- ID:
- ivo://au.csiro/casda/SSA
- Title:
- CSIRO ASKAP Science Data Archive Spectrum Access Service
- Short Name:
- CSIRO ASKAP SSA
- Date:
- 29 Apr 2022 07:59:11
- Publisher:
- CSIRO
- Description:
- Simple Spectral Access service for querying spectra from ASKAP radio astronomy observations
- 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://au.csiro/psrda/ATNF_Pulsar_SCS
- Title:
- CSIRO Parkes Pulsar Data Archive Cone Search Service
- Short Name:
- CSIRO Pulsar SCS
- Date:
- 27 Jun 2018 15:26:24
- 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://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:
- 27 Feb 2024 02:02:54
- 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:
- 27 Feb 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:
- 23 Apr 2024 01:18:58
- 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://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.
- ID:
- ivo://pds-ppi/galileo_mag_jup_calibrated_highres_europa/ppi/epn_core
- Title:
- Galileo Jupiter Magnetometer Highres Europa Data Collection
- Short Name:
- GO-MAG-JUP-EUR
- Date:
- 15 Dec 2022 19:29:32
- 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 Europa data. These data were acquired in order to characterize various portions of the Jovian magnetosphere at high time resolution.
- ID:
- ivo://pds-ppi/galileo_mag_jup_calibrated_highres_ganymede/ppi/epn_core
- Title:
- Galileo Jupiter Magnetometer Highres Ganymede Data Collection
- Short Name:
- GO-MAG-JUP-GAN
- Date:
- 15 Dec 2022 19:25:05
- 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 Ganymede data. These data were acquired in order to characterize various portions of the Jovian magnetosphere at high time resolution.
- ID:
- ivo://pds-ppi/galileo_mag_jup_calibrated_highres_io/ppi/epn_core
- Title:
- Galileo Jupiter Magnetometer Highres Io Data Collection
- Short Name:
- GO-MAG-JUP-IO
- Date:
- 15 Dec 2022 19:28:54
- 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 Io data. These data were acquired in order to characterize various portions of the Jovian magnetosphere at high time resolution.
- ID:
- ivo://pds-ppi/galileo_mag_jup_calibrated_highres_magnetoshpere/ppi/epn_core
- Title:
- Galileo Jupiter Magnetometer Highres Magnetosphere Data Collection
- Short Name:
- GO-MAG-JUP-MAGN
- Date:
- 15 Dec 2022 19:24:33
- Publisher:
- Planetary Data System
- Description:
- TThis data collection contains high time resolution magnetic field vectors acquired by the Galileo magnetometer (MAG). It includes satellite flyby data. These data were acquired in order to characterize various portions of the Jovian magnetosphere at high time resolution.
- ID:
- ivo://pds-ppi/galileo_mag_jup_calibrated_magspheric_survey/ppi/epn_core
- Title:
- Galileo Jupiter Magnetometer Magnetospheric Survey Data Collection
- Short Name:
- GO-MAG-JUP-MS
- Date:
- 15 Dec 2022 19:28:55
- Publisher:
- Planetary Data System
- Description:
- Galileo MAG calibrated optimal averager magnetic field data near Jupiter, and in the solar wind from the Jupiter Approach phase in Despun Spacecraft (IRC) coordinates. The data cover 1995-11-01T00:06 to 1995-12-06T02:09 to 1995-12-06T02:09.
- ID:
- ivo://pds-ppi/galileo_pls_jup_fitted_parameters/ppi/epn_core
- Title:
- Galileo Orbiter Jupiter PLS Fitted Parameters Data Collection
- Short Name:
- GO-PLS-J-FIT
- Date:
- 15 Dec 2022 19:29:09
- Publisher:
- Planetary Data System
- Description:
- This collection contains all of the fitted parameters (both good and bad) for fitting an ion species to the Galileo PLS instrument.
- ID:
- ivo://pds-ppi/galileo_hic_jup_calibrated_highres_callisto/ppi/epn_core
- Title:
- Galilieo Jupiter HIC Highres Energetic Ion Count Rate Callisto Data Collection
- Short Name:
- HIG-J-HI-CAL
- Date:
- 15 Dec 2022 19:30:39
- Publisher:
- Planetary Data System
- Description:
- This collection contains Galileo HIC high resolution (LPW) pulse height data acquired at Jupiter and Callisto.
- ID:
- ivo://pds-ppi/galileo_hic_jup_calibrated_highres/ppi/epn_core
- Title:
- Galilieo Jupiter HIC Highres Energetic Ion Count Rate Data Collection
- Short Name:
- HIG-J=HI
- Date:
- 15 Dec 2022 19:24:21
- Publisher:
- Planetary Data System
- Description:
- This collection contains Galileo HIC high resolution (LPW) pulse height data acquired at Jupiter and in the Io plasma torus.
- ID:
- ivo://pds-ppi/galileo_hic_jup_calibrated_highres_amalthea/ppi/epn_core
- Title:
- Galilieo Jupiter HIC Highres Energetic Ion Count Rate Data Collection
- Short Name:
- HIG-J-HI-AMA
- Date:
- 15 Dec 2022 19:30:11
- Publisher:
- Planetary Data System
- Description:
- This collection contains Galileo HIC high resolution (LPW) pulse height data acquired at Jupiter and Amalthea between 2002-11-05T02:45 and 2002-11-05T06:35.
- ID:
- ivo://pds-ppi/galileo_hic_jup_calibrated_highres_europa/ppi/epn_core
- Title:
- Galilieo Jupiter HIC Highres Energetic Ion Count Rate Europa Data Collection
- Short Name:
- HIG-J-HI-EUR
- Date:
- 15 Dec 2022 19:29:11
- Publisher:
- Planetary Data System
- Description:
- This collection contains Galileo HIC high resolution (LPW) pulse height data acquired at Jupiter and Europa.
- ID:
- ivo://pds-ppi/galileo_hic_jup_calibrated_highres_ganymede/ppi/epn_core
- Title:
- Galilieo Jupiter HIC Highres Energetic Ion Count Rate Ganymede Data Collection
- Short Name:
- HIG-J-HI-GAN
- Date:
- 15 Dec 2022 19:24:13
- Publisher:
- Planetary Data System
- Description:
- This collection contains Galileo HIC high resolution (LPW) pulse height data acquired at Jupiter and Ganymede.
- ID:
- ivo://pds-ppi/galileo_hic_jup_calibrated_highres_io/ppi/epn_core
- Title:
- Galilieo Jupiter HIC Highres Energetic Ion Count Rate IO Data Collection
- Short Name:
- HIG-J-HI-IO
- Date:
- 15 Dec 2022 19:27:01
- Publisher:
- Planetary Data System
- Description:
- This collection contains Galileo HIC high resolution (LPW) pulse height data acquired at Jupiter, Io, and in the Io plasma torus.
- ID:
- ivo://bira-iasb/gem_mars/q/epn_core
- Title:
- GEM-Mars GCM profiles
- Short Name:
- gem_mars.epn_cor
- Date:
- 28 Oct 2023 16:50:48
- Publisher:
- Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
- Description:
- Profiles of pressure, temperature and species of the Martian atmosphere simulated with the GEM-Mars general circulation model. See for the main model descritpion Neary, L., et al. 2018. The GEM-Mars general circulation model for Mars: Description and evaluation. Icarus 300, 458-476. https://doi.org/10.1016/j.icarus.2017.09.028. See for the chemistry description Dearden, F. et al., 2019, Mars atmospheric chemistry simulations with the GEM-Mars general circulation model, Icarus, 326, 197-224, https://doi.org/10.1016/j.icarus.2019.02.030.
- ID:
- ivo://padc.obspm.helio/hfc1ar/q/epn_core
- Title:
- Heliophysics Feature Catalogue: Active regions
- Short Name:
- HFC1AR
- Date:
- 27 Feb 2024 04:30:12
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Active regions of the Sun from Heliophysics Feature Catalogue (HFC).
- ID:
- ivo://idoc.ginco/herschel/spirepacs
- Title:
- Herschel Idoc Database (HESIOD) SPIRE PACS
- Short Name:
- HESIOD
- Date:
- 13 Mar 2019 13:04:15
- Publisher:
- IDOC GINCO
- Description:
- All data for the Herschel SPIRE and PACS guaranted time program on Interstellar Medium (SAG-4) and other public data processed at IDOC. All data have been reprocessed at IDOC using advanded reprocessing pipeline.
- ID:
- ivo://idoc.ginco/herschel/spirepacsCutOut
- Title:
- Herschel Idoc Database (HESIOD) SPIRE PACS CutOut
- Short Name:
- HESIOD
- Date:
- 13 Mar 2019 13:04:26
- Publisher:
- IDOC GINCO
- Description:
- All data for the Herschel SPIRE and PACS guaranted time program on Interstellar Medium (SAG-4) and other public data processed at IDOC. All data have been reprocessed at IDOC using advanded reprocessing pipeline.
- ID:
- ivo://vopdc.obspm/gepi/h1g
- Title:
- HI Extragalactic Database
- Short Name:
- HIG
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - GEPI
- Description:
- HI Extragalactic database is a collection of calibrated 21cm hydrogen line profiles for several thousands galaxies.
- ID:
- ivo://vopdc.obspm/luth/hess
- Title:
- High Energy Stereoscopic System
- Short Name:
- H.E.S.S.
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LUTH
- Description:
- H.E.S.S. is a system of Imaging Atmospheric Cherenkov Telescopes that investigates cosmic gamma rays in the 100 GeV to 100 TeV energy range. The name H.E.S.S. stands for High Energy Stereoscopic System.
- ID:
- ivo://padc.obspm.planeto/hst_planeto/q/epn_core
- Title:
- HST observations of planets and satellites
- Short Name:
- HST Planeto
- Date:
- 27 Feb 2024 03:01:05
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- HST observations of planets, dwarf planets, and satellites, extracted from the CADC database catalogue (with daily updates). Data are linked to the CADC repository, with file names common to all HST archives. Both calibrated and derived products are included. The main target is identified. Physical ephemeris and thumbnails are provided when available. Files and previews are not accessible during the proprietary period.
- ID:
- ivo://idoc.ginco/szcluster-db/szcluster-db-conesearch
- Title:
- IDOC SZ Clusters (szcluster-db) ACT/PLANCK/SPT ConeSearch
- Short Name:
- SZCLUSTER-DB
- Date:
- 13 Mar 2019 13:04:46
- Publisher:
- IDOC GINCO
- Description:
- This database provides access to IDOC catalogues and complementary information on clusters of galaxies observed through the Sunyaev-Zeldovich (SZ) effect.
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