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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
