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- ID:
- ivo://cdpp/transplanet
- Title:
- Magnetosphere Ionosphere coupling simulation runs
- Short Name:
- PSWS Transplanet
- Date:
- 02 Nov 2020 14:05:09
- Publisher:
- CDPP
- Description:
- A Transplanet model of magnetosphere-ionosphere coupling at Earth, Mars, and Jupiter
- ID:
- ivo://cdpp/amda
- Title:
- Planetary and heliophysics plasma data at CDPP/AMDA
- Short Name:
- AMDA
- Date:
- 02 Nov 2020 14:03:51
- Publisher:
- CDPP
- Description:
- Planetary and heliophysics plasma data at CDPP/AMDA
- ID:
- ivo://cdpp/illu67p
- Title:
- Illumination maps of 67P
- Short Name:
- ILLU67P
- Date:
- 02 Nov 2020 14:04:37
- Publisher:
- Centre de Données de la Physique des Plasmas(CDPP)
- Description:
- Illumination by the Sun of each face of the comet 67P/Churyumov-Gerasimenko based on the shape model CSHP_DV_130_01_LORES_OBJ.OBJ. The service provides the cosine between the normal of each face (in the same order as the faces defined in the shape model) and the Sun direction; both numerical values and images of the illumination are available. Each map is defined for a given position of the Sun in the frame of 67P (67P/C-G_CK). Longitude 0 is at the center of each map. The code is developed by A. Beth, Imperial College London, UK and the service is provided by CDPP (http://cdpp.eu). Acknowlegment: The illumination models have been developed at the Department of Physics at Imperial College London (UK) under the financial support of STFC grant of UK ST/N000692/1 and ESA contract 4000119035/16/ES/JD (Rosetta RPC-PIU). We would also like to warmly thank Bernhard Geiger (ESA) for his support in validating the 2D-illumination maps.
- 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://arecibo.cornell
- Title:
- Arecibo/Cornell Naming Authority
- Short Name:
- Arecibo
- Date:
- 17 Sep 2007 10:51:00
- Publisher:
- Cornell University
- Description:
- This resource represents the naming authority for the Arecibo data resources at Cornell University.
- 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://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://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
25. PVOL
- ID:
- ivo://pvol/pvol/q/epn_core
- Title:
- PVOL
- Date:
- 12 Feb 2019 14:42:11
- Publisher:
- Euskal Herriko Unibertsitatea / Universidad del Pais Vasco / University of the Basque Country
- Description:
- EPN-TAP access to the PVOL data
26. PVOL
- ID:
- ivo://pvol/pvol/q/collection
- Title:
- PVOL
- Date:
- 12 Feb 2019 14:42:11
- Publisher:
- Euskal Herriko Unibertsitatea / Universidad del Pais Vasco / University of the Basque Country
- Description:
- Images, maps, photometries and other kind of planetary graphic platforms made by amateur astronomers. Data is received by the astronomers themselves and can be subject of change
27. 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://idoc/psup/omega_cubes/q/epn_core
- Title:
- L3 Omega Cubes - Mars Express
- Date:
- 12 Mar 2021 16:07:42
- Publisher:
- IDOC
- Description:
- Mars Express - Omega Cubes
- ID:
- ivo://idoc/psup/omega_maps/q/epn_core
- Title:
- Omega mineral maps - Mars Express
- Date:
- 12 Mar 2021 16:07:35
- Publisher:
- IDOC
- Description:
- Mars Express - Omega Mineral Maps
30. SDO GAIA-DEM
- ID:
- ivo://idoc/medoc/gaia_dem/q/epn_core
- Title:
- SDO GAIA-DEM
- Short Name:
- gaia_dem.epn_cor
- Date:
- 30 Nov 2023 19:23:40
- Publisher:
- IDOC
- Description:
- <b>GAIA-DEM</b><br/> GAIA-DEM is a database of Differential Emission Measure (DEM) maps. The DEM is a measure of the thermal structure of the coronal plasma, representing the quantity of light emitting plasma along the line of sight, at different temperatures. In GAIA-DEM, the DEM is modelled by a specific function of temperature, namely a Gaussian of the logarithm of electron temperature. GAIA-DEM maps are then maps of the DEM maximum temperature, of the DEM integral (total Emission Measure), and DEM width (in temperature). These maps are obtained by inversion from the SDO/AIA EUV images in 6 coronal channels (9.4, 13.1, 17.1, 19.3, 21.1, and 33.5 nm). In addition, maps of the χ² for the inversion are provided.<br/> GAIA-DEM is available from a specific interface at <a href="http://medoc-dem.ias.u-psud.fr/">http://medoc-dem.ias.u-psud.fr</a>, as well as part of the generic MEDOC interface which is currently located at <a href="https://idoc-medoc.ias.u-psud.fr/">https://idoc-medoc.ias.u-psud.fr</a>. These interfaces are based on the CNES SiTools2 framework. GAIA-DEM is also available from IDL and Python scripts, using a specialization of the generic SiTools2 IDL and Python clients developed by MEDOC.
31. SDO GAIA-DEM
- ID:
- ivo://idoc/q/epn_core
- Title:
- SDO GAIA-DEM
- Date:
- 08 Dec 2021 14:22:45
- Publisher:
- IDOC
- Description:
- *** GAIA-DEM *** GAIA-DEM is a database of Differential Emission Measure (DEM) maps. The DEM is a measure of the thermal structure of the coronal plasma, representing the quantity of light emitting plasma along the line of sight, at different temperatures. In GAIA-DEM, the DEM is modelled by a specific function of temperature, namely a Gaussian of the logarithm of electron temperature. GAIA-DEM maps are then maps of the DEM maximum temperature, of the DEM integral (total Emission Measure), and DEM width (in temperature). These maps are obtained by inversion from the SDO/AIA EUV images in 6 coronal channels (9.4, 13.1, 17.1, 19.3, 21.1, and 33.5nm). In addition, maps of the ϲ for the inversion are provided. GAIA-DEM is available from a specific interface at http://medoc-dem.ias.u-psud.fr/, as well as part of the generic MEDOC interface which is currently located at http://idocmedoc- test.ias.u-psud.fr/. These interfaces are based on the CNES SiTools2 framework. GAIA-DEM is also available from IDL and Python scripts, using a specialization of the generic SiTools2 IDL and Python clients developed by MEDOC.
- 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://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://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://idoc.d2s/corot/stars-rotation-period-affer-conesearch
- Title:
- Stars with rotation periods from Affer and al. IDOC D2S ConeSearch
- Short Name:
- CoRoT_N2_RotAff
- Date:
- 13 May 2019 17:27:59
- Publisher:
- IDOC D2S
- Description:
- Stars with rotation periods from Affer and al.
- 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://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.
- 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.iap
- Title:
- Institut d'Astrophysique de Paris Authority
- Short Name:
- IAP
- Date:
- 10 Jan 2017
- Publisher:
- Institut d'Astrophysique de Paris
- Description:
- This Naming Authority is used to identify the resources provided by Paris Astronomical Data Centre at Institut d'Astrophysique de Paris, Paris, FRANCE
- 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.
44. 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)."
45. PRETHARSIS
- ID:
- ivo://geops.ipsl/pretharsis/q/epn_core
- Title:
- PRETHARSIS
- Short Name:
- pretharsis.epn_c
- Date:
- 01 May 2024 01:20:23
- Publisher:
- IPSL/GEOPS
- Description:
- "The growth of the Tharsis volcanic complex on Mars during Noachian/Hesperian era induced a reorientation of the spin axis of the planet (true polar wander). This service gives access to a map of Mars topography before Tharsis formation (Early Noachian) and a map of Mars topography before true polar wander (Late Noachian/Early Esperian), from the model described in Bouley, S., Baratoux, D., Matsuyama, I. et al. Late Tharsis formation and implications for early Mars. Nature 531, 344â347 (2016). https://doi.org/10.1038/nature17171 ."
- ID:
- ivo://koa.ipac/KOA
- Title:
- Keck Observatory Archive
- Short Name:
- KOA
- Date:
- 16 Nov 2021 20:00:00
- Publisher:
- Keck Observatory Archive
- Description:
- The archive node for scientific data sets from the Keck Observatory Archive.
- ID:
- ivo://koa.ipac
- Title:
- Keck Observatory Archive
- Short Name:
- KOA
- Date:
- 26 Oct 2021
- Publisher:
- Keck Observatory Archive
- Description:
- The archive node for scientific data sets from the Keck Observatory Archive (KOA).
- ID:
- ivo://konkoly.hu/sbnaf/q/collection
- Title:
- Small Bodies Near and Far
- Date:
- 06 Sep 2023 06:07:48
- Publisher:
- Konkoly Observatory
- Description:
- SBNAF public database of thermal infrared observations of small bodies in the solar system. Our database collects thermal emission measurements of small Solar Systems targets that are otherwise available in scattered sources and gives a complete description of the data, with all information necessary to perform direct scientific calculations and without the need to access additional, external resources. See the details here: https://ird.konkoly.hu/
49. SPICAM
- ID:
- ivo://latmos.ipsl/spicam/q/epn_core
- Title:
- SPICAM
- Short Name:
- spicam.epn_core
- Date:
- 02 May 2022 14:11:03
- Publisher:
- Laboratoire Atmosphères, Milieux, Observations Spatiales
- Description:
- The database contains profiles of atmospheric CO2 density and temperature derived thereof, and ozone concentration profiles, all derived from the first year(s) of SPICAM UV stellar occultation observations (Forget et al. 2009, Lebonnois et al. 2006). The database also includes the full dataset of four Martian years of aerosol extinction profiles from SPICAM UV solar occultations (Määttänen et al. 2013).
50. mars_dust
- ID:
- ivo://lmd.jussieu/mars_dust/q/epn_core
- Title:
- mars_dust
- Date:
- 19 Apr 2024 00:00:02
- Publisher:
- Laboratoire Méteorologie Dynamique
- Description:
- Mars_dust provides a multiannual climatology of Martian airborne dust as measured by various space missions. The retrieved column dust optical depth is mapped for each Martian year and formatted as cubes with time in the 3rd dimension. Two versions are available: irregularly gridded maps, and regular maps produced by kriging. These latter maps are used as column-integrated dust scenarios in the Mars Climate Database (MCD v5). The detailed description of the methodology and dataset can be found in: Montabone et al (2015) Icarus 251, pp. 65-95https://doi.org/10.1016/j.icarus.2014.12.034 ; Montabone et al (2020) JGR-Planets https://doi.org/10.1029/2019JE006111
51. mcd
- ID:
- ivo://lmd.jussieu/mcd/q/epn_core
- Title:
- mcd
- Date:
- 28 Jan 2022 00:57:05
- Publisher:
- Laboratoire Méteorologie Dynamique
- Description:
- The database contains some outputs of the MCD for all the scenarios available, at different positions of latitude and longitude. These MCD outputs are provided as Votables containing profiles of temperatures, pressures, density and abundances of O2 and O3 for altitudes between 0 and 249.5 km from the surface.
52. MCD
- ID:
- ivo://lmd.jussieu/mcd/q/collection
- Title:
- MCD
- Date:
- 26 Aug 2021 09:44:39
- Publisher:
- Laboratoire Méteorologie Dynamique
- Description:
- MCD is a database of atmospheric statistics compiled from Global Climate Model (GCM) numerical simulation of Martian atmosphere (<a href=http://www-mars.lmd.jussieu.fr>http://www-mars.lmd.jussieu.fr</a>). The GCM computes in 3D the atmospheric circulation and climate taking into account radiative transfer through the gaseous atmospheres and the dust and ice aerosols, includes a representation of the CO2 ice condensation and sublimation on the ground and in the atmosphere, simulates the water cycle (with modelling of cloud microphysics), the dust multisize particle transport, the atmospheric composition controlled by the photochemistry and the local non-condensible gas enrichment and depletion induced by CO2 condensation and sublimation, and has been extended into the thermosphere and to model ionospheric processes (due to chemistry). The database extends up to exobase (the top of the thermosphere, roughly at 300km in altitude); in addition to statistics on temperature, wind, pressure, radiative fluxes, it provides data such as atmospheric composition (including dust water vapor and ice content) and make use of 'dust and Extreme Ultra Violet (EUV) scenarios' to represent the variation of dust in the atmosphere and solar EUV conditions. User Manual of the service : <a href=http://vo.lmd.jussieu.fr:8080/MCD_VESPA_service_user_manual.pdf>User Manual of the service </a> .
53. vcd
- ID:
- ivo://lmd.jussieu/vcd/q/epn_core
- Title:
- vcd
- Date:
- 19 Apr 2024 00:05:16
- Publisher:
- Laboratoire Méteorologie Dynamique
- Description:
- The database contains some outputs of the VCD for the scenarios : {1) Standard cloud albedo Scenario, solar EUV average conditions ; 2) Standard cloud albedo Scenario, solar EUV minimum conditions ; 3) Standard cloud albedo Scenario, solar EUV maximum conditions ; 4) Low cloud albedo Scenario, solar EUV average conditions ; 5) High cloud albedo Scenario, solar EUV average conditions available}, at different positions of latitude and longitude. These VCD outputs are provided as Votables containing profiles of temperatures, pressures, density and abundances of main species for altitudes between 0 and 349.5 km from the surface.
- ID:
- ivo://gov.nasa.gsfc.nssdc/SPMS-00560
- Title:
- ISEE-1 Energetic Ion Mass Spectrometer Data
- Short Name:
- ISEE Ion Data
- Date:
- 27 Apr 2006 17:05:46
- Publisher:
- NASA
- Description:
- Ion data from the Plasma Composition Experiment on ISEE-1 consist of a combination of (a) velocity moments for the four principal magnetospheric ion species H+, He++, He+, and O+, calculated in two different ways (using two different sets of assumptions) and covering the 0.01-0.1 and 0.1-16 keV/e energy ranges, (b) energy-angle spectra for the same four ions plus O++, covering the 0.01-17.9 keV/e range, and (c) mass spectra (<1 amu/e to about 150 amu/e) for four energy ranges, all derived once per each complete energy-mass scan cycle of the instrument, or once each 1- to 20-minute interval, depending on mode of operation, as well as (d) "total ion" moments, derived once per energy scan and assuming total count rate is due to H+ ions (0.1-16 keV).
- ID:
- ivo://nasa.gsfc.nssdc/SPMS-00237
- Title:
- ISEE-1 Ion Composition Data Parameter Plots
- Short Name:
- ISEE-1 Ion Plots
- Date:
- 27 Apr 2006 17:35:49
- Publisher:
- NASA
- Description:
- These hardcopy plots were provided as a supplement to the digital data from the Plasma Composition Experiment (NSSDC data set 77-102A-12I). A subset of the data in the digital data files is plotted in graphical form in a series of booklets, one booklet for each month of data. There are two pages of graphs for each day, and each page has a stack of 7 panels showing the variation of different parameters during the course of a 12-hour Universal Time interval. Panel 1 (top panel) shows densities of He++, He+, and O+ ions, and the "total" ion density (per cubic meter); Panel 2 shows He++/H+ density ratio; Panel 3 shows ion "thermal" energy (eV); Panel 4 shows "thermal" energy density multiplied by 2/3 along with the magnetic pressure (eV/m^3) and field strength (nT); Panel 5 shows ion drift speed (meters/sec) in the GSE X-Y plane; Panel 6 shows magnetic field elevation angle (degrees) relative to the GSE X-Y plane; Panel 7 shows ion drift angle and the magnetic longitude angle.
- ID:
- ivo://nasa.gsfc.nssdc/nssdc
- Title:
- NSSDC National Space Science Data Center
- Short Name:
- NSSDC
- Date:
- 27 Apr 2006 17:11:54
- Publisher:
- NASA
- Description:
- NSSDC is the permanent archive for NASA space science mission data: astronomy and astrophysics, solar and space plasma physics, and planetary and lunar science. As permanent archive, NSSDC teams with NASA's discipline-specific space science "active archives" which provide access to data to researchers and to the general public. NSSDC also serves as NASA's primary active archive for space physics mission data and for selected NASA astrophysics missions. It provides access to several geophysical models and to data from some non-NASA mission data. In addition to supporting active space physics and astrophysics researchers, NSSDC also supports the general public both via several public-interest web-based services (e.g., the Photo Gallery) and via the offline mailing of CD-ROMs, photoprints, and other items. NSSDC provides online information about NASA and non-NASA spacecraft and experiments, and about data management standards and technologies.
- ID:
- ivo://gov.nasa.gsfc.nssdc/oao2
- Title:
- OAO-2 Ultraviolet Spectra: An Atlas of Stellar Spectra
- Short Name:
- OAO-2
- Date:
- 24 Apr 2006 21:24:06
- Publisher:
- NASA
- Description:
- This data set is a subset of ultraviolet stellar spectra comprising the highest quality data obtained with both spectrometers aboard the OAO 2. The first file of the data set contains ultraviolet stellar fluxes for 164 bright stars in the spectral range between 1200 to 1300 A, with resolutions of about 22 A in the region from 3600 to 1850 A and about 12 A in the region from 1850 to 1160 A. Files 2 and 3 contain spectra for 132 stars in the region 1200-1850 A and 34 stars in the region 1800-3600 A, respectively, with resolutions as stated above. The data have been published in graphical and tabular form by A.D. Code and M.R. Meade, Astrophys. J. Suppl., v. 39, p. 195, 1979; M.R. Meade and A.D. Code, Astrophys. J. Suppl., v. 42, p. 283, 1980.
- ID:
- ivo://gov.nasa.gsfc.nssdc/ASUV-00020
- Title:
- Skylab Catalog of Far-Ultraviolet Objective-Prism Spectrophotometry
- Short Name:
- Skylab FUV
- Date:
- 24 Apr 2006 21:32:00
- Publisher:
- NASA
- Description:
- This data set is a machine-readable version of the catalog of Far- Ultraviolet Objective-Prism Spectrophotometry (S-019). The data are on one ASCII tape with two files, created on an IBM 3081 computer. The data set contains arrays of ultraviolet flux measurements at wavelengths of 1300 to 4200 A. The spectra were digitized with a PDS 1010 A microdensitometer, and each spectrum was scanned in a series of strips 30 microns wide. This catalog contains data on 494 stars. The data on each star are quite complex and include a number of parameters in addition to the adopted fluxes. Accompanying this data set is a copy of a document entitled "Documentation for the Machine-Readable Version of the Catalogue of Far-Ultraviolet Objective-Prism Spectrophotometry: Skylab Experiment S-019, Ultraviolet Stellar Astronomy" by R.S. Hill and L.E. Brotzman, 1984 (B35702-000A). For more information on this data set, see the above document or contact Dr. Karl Henize, Code SN3, NASA Johnson Space Center, Houst
- ID:
- ivo://gov.nasa.gsfc.nssdc/viking1
- Title:
- Viking 1 Biology Experiment
- Short Name:
- Viking 1 Biology
- Date:
- 24 Apr 2006 19:57:18
- Publisher:
- NASA
- Description:
- Viking 1 Gas Exchange, Labeled Release, and Pyrolytic Release Data on Microfilm. These data, supplied by the investigation team, are on 16- mm microfilm and consist of descriptions of the commands that were sent to operate the three instruments, and tabulations of raw and reduced data returned. The command data include Mars time for each experiment sequence, the commands sent, predicted data points for each command file that were used to time tag the data when it came back from the instrument, and a summary of the major events of each command sequence.
- ID:
- ivo://gov.nasa.gsfc.nssdc/viking2
- Title:
- Viking 2 Biology Experiment
- Short Name:
- Viking 2 Biology
- Date:
- 24 Apr 2006 19:43:32
- Publisher:
- NASA
- Description:
- Viking 2 Gas Exchange, Labeled Release, and Pyrolytic Release Data on Microfilm. These data, supplied by the investigation team, are on 16- mm microfilm and consist of descriptions of the commands that were sent to operate the three instruments, and tabulations of raw and reduced data returned. The command data include: Mars time for each experiment sequence, the commands sent, predicted data points for each command file that were used to time tag the data when it came back from the instrument, and a summary of the major events of each command sequence.
- ID:
- ivo://nexsci.ipac
- Title:
- NASA Exoplanet Science Institute
- Short Name:
- NEXSCI
- Date:
- 27 Nov 2018 17:20:48
- Publisher:
- NASA Exoplanet Science Institute
- Description:
- NExScI is the science operations and analysis center for NASA's Exoplanet Exploration Program
- ID:
- ivo://ned.ipac/NED
- Title:
- The NASA/IPAC Extragalactic Database
- Short Name:
- NED
- Date:
- 10 Jun 2021 18:18:18
- Publisher:
- NASA/IPAC
- Description:
- The NASA/IPAC Extragalactic Database (NED) provides a comprehensive fusion of multi-wavelength data for hundreds of millions of objects located beyond the Milky Way galaxy. As new observations are published in NASA mission archives, journal articles and sky survey catalogs, they are cross-identified with prior measurements and integrated in a unified database. Numerous derived quantities are also provided to facilitate scientific research. For more information see http://ned.ipac.caltech.edu/
- ID:
- ivo://ned.ipac
- Title:
- NASA/IPAC Extragalactic Database
- Short Name:
- NED
- Date:
- 26 Oct 2021
- Publisher:
- NASA/IPAC Extragalactic Database
- Description:
- The archive node for scientific data from the NASA/IPAC Extragalactic Database (NED).
- ID:
- ivo://irsa.ipac/IRSA
- Title:
- NASA/IPAC Infrared Science Archive
- Short Name:
- IRSA
- Date:
- 16 Mar 2017 01:00:00
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The archive node for scientific data sets from NASA's infrared and sub-millimeter astronomy projects and missions.
- ID:
- ivo://irsa.ipac
- Title:
- NASA/IPAC Infrared Science Archive
- Short Name:
- IRSA
- Date:
- 16 Mar 2017 01:00:00
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The archive node for scientific data sets from NASA's infrared and sub-millimeter astronomy projects and missions.
- ID:
- ivo://irsa.ipac/WISE/Catalog/Prelim
- Title:
- WISE Preliminary Release Catalogs
- Short Name:
- WISE-Prelim
- Date:
- 16 Mar 2017 01:00:00
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The WISE Preliminary Release includes data from the first 105 days of WISE survey observations, 14 January 2010 to 29 April 2010, that were processed with initial calibrations and reduction algorithms. Primary release data products include an Atlas of 10,464 calibrated, coadded Image Sets, a Source Catalog containing positional and photometric information for over 257 million objects detected on the WISE images, and an Explanatory Supplement that provides a user's guide to the WISE mission and format, content, characteristics and cautionary notes for the Release products. Ancillary release products include an archive of over 754,000 Single-exposure Image sets and database of over 2.2 billion source extractions from those images, and moving object tracklets identified as part of the NEOWISE program (Mainzer et al. 2011).
- 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://ov-gso
- Title:
- OV-GSO Virtual Observatory services
- Short Name:
- OVGSO
- Date:
- 24 Mar 2016 10:59:25
- Publisher:
- Ov-gso @ irap
- Description:
- This is the Authority under which all relevant VO services provided by OV-GSO will be registered
- 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:
- 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
71. 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://vopdc.obspm/dfbs
- Title:
- Digitized First Byurakan Survey
- Short Name:
- DFBS
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.
- ID:
- ivo://padc.obspm.planeto/dynastvo/q/epn_core
- Title:
- DynastVO ephemeris service
- Short Name:
- DynAstVO
- Date:
- 07 May 2024 02:02:48
- Publisher:
- Paris Astronomical Data Centre
- Description:
- This database displays calculated orbital parameters for small bodies
- 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
- ID:
- ivo://padc.obspm.helio/hfc1ar/q/epn_core
- Title:
- Heliophysics Feature Catalogue: Active regions
- Short Name:
- HFC1AR
- Date:
- 07 May 2024 04:30:11
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Active regions of the Sun from Heliophysics Feature Catalogue (HFC).
- ID:
- ivo://vopdc.obspm
- Title:
- Paris Astronomical Data Centre Authority
- Short Name:
- PADC
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre
- Description:
- This Naming Authority is used to identify the resources provided by Paris Astronomical Data Centre at Observatoire de Paris, Paris, FRANCE
- ID:
- ivo://padc.obspm.planeto/bdip/q/epn_core
- Title:
- Planetary Images Database
- Short Name:
- BDIP
- Date:
- 23 Nov 2022 15:28:18
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Planetary Images Database
- ID:
- ivo://padc.obspm.planeto/bdip/q/observatories
- Title:
- Planetary Images Database
- Short Name:
- bdip.observatori
- Date:
- 23 Nov 2022 15:28:18
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Observatory names
- ID:
- ivo://padc.obspm.planeto/voccdb/q/epn_core
- Title:
- Predictions of stellar occultations by the main planetary satellites
- Short Name:
- voccdb.epn_core
- Date:
- 19 Apr 2024 14:16:01
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The VOccDB database provides prediction and parameters of stellar occultations by the main planetary satellites. Observations of a stellar occultations help to better determine the size and the shape of the occulting body, as well as its astrometric position at the milli-arcsecond level precision. Only the main moons of giant planets Jupiter, Saturn, Uranus and Neptune are considered in the event prediction database. Predictions are provided over period 2023-2032, up to visual magnitude 12 for the biggest satellites, and magnitude 14 for other satellites. For each stellar occultation event prediction, the database provides circumstances and observational data, date and timing of the occultation, star position and magnitude, excepted duration, etc.
- ID:
- ivo://padc.obspm.planeto/basecom/q/epn_core
- Title:
- The Nançay Cometary Database
- Short Name:
- basecom.epn_core
- Date:
- 02 May 2024 18:54:10
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Since 1973, the 18-cm lines of the OH radical have been systematically observed in a number of comets with the Nançay radio telescope. This allowed an evaluation of the cometary water production rates and their evolution with time, as well as a study of several physical processes: the excitation mechanisms of the OH radio lines, the expansion of the cometary atmospheres, their anisotropy in relation with non-gravitational forces, the Zeeman effect in relation with the cometary magnetic field. The Nançay observations of 53 cometary apparitions between 1982 and 2009 are now organized in this database.
- ID:
- ivo://padc.obspm.helio/hfc1t3/q/epn_core
- Title:
- Type 3 event in Helio
- Short Name:
- HFC1T3
- Date:
- 11 Dec 2023 10:23:50
- Publisher:
- Paris Astronomical Data Centre
- Description:
- type 3 events of the sun from helio database.
- ID:
- ivo://padc.obspm.planeto/meteor_showers/q/epn_core
- Title:
- VOEvent meteor shower service
- Short Name:
- Meteor Showers
- Date:
- 08 Mar 2023 13:09:31
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The ephemeris were produced by simulating the ejection of meteoroids from the sunlit hemisphere of cometary nuclei, typically from 0 to 3 au, followed by the propagation of orbits of meteoroids in the Solar System, taking into account the gravity of the Sun, the 8 planets, Pluto, and the Moon, as well as the radiation pressure and the Poynting-Robertson drag. Note that asteroid parent bodies were considered as active (i.e. comet-like bodies) even if they are not active today. The showers are predicted when a planet enters a large enough set of meteoroids, at a distance less than typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new method to predict meteor showers. I. Description of the model, Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: Vaubaillon J. 2017 A confidence index for forecasting of meteor showers, Planetary and Space Science, Volume 143 p.78-82
- ID:
- ivo://vopdc.obspm/portal
- Title:
- VO-Paris Data Discovery Portal
- Short Name:
- PADC Portal
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The Paris Astronomical Data Centre Portal provides an easy way to access to all VO data available at Paris Observatory.
84. Mars Craters
- ID:
- ivo://padc.obspm.planeto/mars_craters/q/epn_core
- Title:
- Mars Craters
- Short Name:
- mars_craters.epn
- Date:
- 17 Apr 2024 13:17:11
- Publisher:
- Paris Astronomical Data Centre - Constructor University
- Description:
- The Mars Crater Catalog by S.J. Robbins was generated from THEMIS Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were selected using 5 points along the rim. The table is statistically complete to the diameter of ~1.0 km. The table contains morphologic and morphometric data for craters with diameter larger than 3 km. The Prometheus basin has been excluded from the Catalog due to technical issues. Reference: "A New Global Database of Mars Impact Craters ≥1 km: (1) Database Creation, Properties, and Parameters", S.J. Robbins and B.M. Hynek, Journal of Geophysical Research - Planets, v.117. (2012) DOI: 10.1029/2011JE003966
- ID:
- ivo://padc.obspm.planeto/mars_craters_lagain/q/epn_core
- Title:
- Mars Craters Lagain
- Short Name:
- mars_craters_lag
- Date:
- 17 Apr 2024 13:07:37
- Publisher:
- Paris Astronomical Data Centre - Constructor University
- Description:
- A catalogue of Mars craters by Lagain et al. (2020), extending the previous catalogue from Robbins and Hynek (2012, DOI:10.1029/2011JE003966). 185 craters were added by Lagain, the object IDs are compatible with the previous work. Reference: "Impact cratering rate consistency test from ages of layered ejecta on Mars", Lagain et al., Planetary and Space Science, v.180. (2020) DOI: 10.1016/j.pss.2019.104755
86. USGS_WMS
- ID:
- ivo://padc.obspm.planeto/usgs_wms/q/epn_core
- Title:
- USGS_WMS
- Short Name:
- usgs_wms.epn_cor
- Date:
- 17 Apr 2024 13:28:42
- Publisher:
- Paris Astronomical Data Centre - Constructor University
- Description:
- Catalogue of USGS Astrogeology WMS Map Layers
87. 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).
- 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://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.
90. SRC-J Survey
- ID:
- ivo://vopdc.obspm/gepi/vopsat/srcj
- Title:
- SRC-J Survey
- Short Name:
- SRC-J
- Date:
- 10 Nov 2022
- Publisher:
- Paris Astronomical Data Centre - GEPI
- Description:
- VO-compliant publication of Schmidt survey SRC-J of the southern sky digitized with the MAMA microdensitometer at the Observatoire de Paris Image Analysis Centre (CAI).
- ID:
- ivo://vopdc.obspm/gepi/vopsat
- Title:
- VO Paris Southern Atlas
- Short Name:
- VOPSAT
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - GEPI
- Description:
- VOPSAT is a set of southern sky digital surveys based on ESO-R, SRC-J and POSS1-E atlases. The plates have been digitized with the MAMA microdensitometer with a resolution of 0.7 arc-sec. Pixel resampling will allow mosaicing neighbouring Schmidt fields up to hundreds of square degrees.
- ID:
- ivo://vopdc.obspm/imcce
- Title:
- IMCCE VO Solar System Portal
- Short Name:
- VO-IMCCE
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - IMCCE
- Description:
- The IMCCE is a research institute of the Paris Observatory, associated with the CNRS (UMR8028), whose work concerns mainly the dynamic and planetologic studies of the bodies of the solar system and of the terrestrial environment: planets, natural satellites, asteroids, comets, meteoroids and space debris. The IMCCE, through its VO Solar System Portal, places at the disposal of the Virtual observatory its knowledge and its expertise which concern the dynamics and the physics of the bodies of the solar system through databases, ephemeris computation services, tools of simulation, and numerical computation services fully compliant with the interoperability concept of the Virtual Observatory.
93. M4AST
- ID:
- ivo://padc.obspm.planeto/m4ast/q/epn_core
- Title:
- M4AST
- Short Name:
- M4AST
- Date:
- 23 Nov 2022 16:33:33
- Publisher:
- Paris Astronomical Data Centre - IMCCE
- Description:
- compiled database for asteroid spectra in the visible and NIR regions
94. Sky Body Tracker
- ID:
- ivo://vopdc.obspm/imcce/skybot
- Title:
- Sky Body Tracker
- Short Name:
- SkyBoT
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - IMCCE
- Description:
- SkyBoT is a VO service which allows to seek and identify solar system objects (planet, satellites, asteroids, comets) in any field of view at a given epoch (cone-search method). It provides also a solar system object name resolver which convert the name or the designation of solar system objects into their celestial coordinates at a given epoch (resolver method). The SkyBoT service are available through a Web interface and a Web service (SOAP+WSDL+HTTP) which implements the IVOA Simple Cone-Search protocol.
- ID:
- ivo://vopdc.obspm/imcce/skybot/cea
- Title:
- Sky Body Tracker - Remote application
- Short Name:
- SkyBoT
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - IMCCE
- Description:
- SkyBoT is a VO service which allows to seek and identify solar system objects (planet, satellites, asteroids, comets) in any field of view at a given epoch (cone-search method). It provides also a solar system object name resolver which convert the name or the designation of solar system objects into their celestial coordinates at a given epoch (resolver method). The SkyBoT service are available through a Web interface and a Web service (SOAP+WSDL+HTTP) which implements the IVOA Simple Cone-Search protocol.
- ID:
- ivo://vopdc.obspm/imcce/miriade
- Title:
- VO Solar System Object Ephemeris Generator
- Short Name:
- Miriade
- Date:
- 03 Feb 2017
- Publisher:
- Paris Astronomical Data Centre - IMCCE
- Description:
- The Miriade project aims to provide a VO-compliant suite of services to compute positional and physical ephemerides of known solar system bodies as seen from any location on Earth as well as various location in space (HST, SPITZER, Gaia, etc.)
- ID:
- ivo://vopdc.obspm/lerma
- Title:
- Laboratoire d’Études du Rayonnement et de la Matière en Astrophysique et Atmosphères
- Short Name:
- LERMA
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LERMA
- Description:
- Laboratoire d’Études du Rayonnement et de la Matière en Astrophysique et Atmosphères
- ID:
- ivo://vopdc.obspm/lerma/simrepo
- Title:
- SimDAL Repository
- Short Name:
- SimDAL Repo
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LERMA
- Description:
- The SimDAL repository hosts numerical projects descriptions as standard XML documents following the Simulation Data Model serialization xsd. It allows clients to search (fulltext) for simulation projects or associated protocols of interest and get URIs towards other SimDAL components: SimDAL Search and SimDAL Data Access.
99. Be Stars Catalog
- 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.
100. Be Stars Database
- 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.
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