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Start Over Resource Type Archive Content Level University
1. 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.
2. Be Stars Spectra
ID:
ivo://vopdc.obspm/lesia/BeStars/BeSS
Title:
Be Stars Spectra
Short Name:
BeSS
Date:
10 Jan 2017
Publisher:
Paris Astronomical Data Centre - LESIA
Description:
The BeSS database assembles classical Be star spectra obtained by professional and amateur astronomers at any wavelength, epoch, and spectral resolution.
3. Chandra HiPS Service
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.
4. Chandra X-ray Observatory Data Archive
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.
5. Chandra X-ray Observatory Data Archive
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.
6. Digitized First Byurakan Survey
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.
7. Five Supernova Survey Galaxies
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.
8. HI Extragalactic Database
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.
9. High Energy Stereoscopic System
ID:
ivo://vopdc.obspm/luth/hess
Title:
High Energy Stereoscopic System
Short Name:
H.E.S.S.
Date:
10 Jan 2017
Publisher:
Paris Astronomical Data Centre - LUTH
Description:
H.E.S.S. is a system of Imaging Atmospheric Cherenkov Telescopes that investigates cosmic gamma rays in the 100 GeV to 100 TeV energy range. The name H.E.S.S. stands for High Energy Stereoscopic System.
10. ISEE-1 Energetic Ion Mass Spectrometer Data
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).