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Start Over Resource Type Archive Capability Type Table Access Protocol
121. OSO8 A Detector Lightcurves
ID:
ivo://nasa.heasarc/oso8alc
Title:
OSO8 A Detector Lightcurves
Short Name:
OSO8ALC
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
This database accesses the FITS lightcurves obtained from the A detector part of the GSFC Cosmic X-ray Spectroscopy experiment (GCXSE) on board OSO8. The Orbiting Solar Observatory-I (OSO-8) was launched on 21 June 1975 into a 550 km circular orbit at 33 degrees inclination. While the primary objectives of the mission were solar in nature, there were 3 detectors (the GCXSE detectors A, B and C) which had exclusively non-solar objectives. The energy band was 2-60 keV for the A and C detector and 2-20 keV for the B detector. The spacecraft structure consisted of a rotating cylindrical base section called the "wheel" and a non-spinning upper section called the "sail". The GCXSE detectors were mounted in the rotating wheel and their fields-of-view were either aligned to the spin axis (B and C) or at small angles to it (A), hence they always viewed the portion of the sky at right angles to the earth-sun line. The GCXSE detectors obtained data until late September 1978. This is a service provided by NASA HEASARC .
122. OSO8B&CDetectorLightcurves
ID:
ivo://nasa.heasarc/oso8bclc
Title:
OSO8B&CDetectorLightcurves
Short Name:
OSO8BCLC
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
OSO8 B&C Detector Lightcurves This is a service provided by NASA HEASARC .
123. OSO8 GCXSE Raw PHA
ID:
ivo://nasa.heasarc/oso8pharaw
Title:
OSO8 GCXSE Raw PHA
Short Name:
OSO8PHARAW
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
The Orbiting Solar Observatory-I (OSO-8) was launched on 21 June 1975 into a 550 km circular orbit at 33 degrees inclination. Data were obtained from the mission until late September 1978. The spacecraft structure consisted of a rotating cylindrical base section called the "wheel" and a non-spinning upper section called the "sail". While the primary objectives of the mission were solar in nature, there were 3 detectors, the GSFC Cosmic X-ray Spectroscopy experiments (GCXSE detectors A, B, and C), mounted in the rotating wheel which had exclusively non-solar objectives. Their fields-of-view were either aligned to the spin axis or at small angles to it, hence they always view the portion of the sky at right angles to the earth-sun line. This database accesses the pha FITS datafiles for the A, B, and C GCXSE detectors. Data was accumulated every quarter of a rotation period (~2.56 s) for the A detector and every 40.96 s for the B and C detectors in the 2-60 keV energy band. This is a service provided by NASA HEASARC .
124. OSO8 GCXSE Raw Rates
ID:
ivo://nasa.heasarc/oso8rtraw
Title:
OSO8 GCXSE Raw Rates
Short Name:
OSO8RTRAW
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
The Orbiting Solar Observatory-I (OSO-8) was launched on 21 June 1975 into a 550 km circular orbit at 33 degrees inclination. Data were obtained from the mission until late September 1978. The spacecraft structure consisted of a rotating cylindrical base section called the "wheel" and a non-spinning upper section called the "sail". While the primary objectives of the mission were solar in nature, there were 3 detectors, the GSFC Cosmic X-ray Spectroscopy experiments (GCXSE detectors A, B and C), mounted in the rotating wheel which had exclusively non-solar objectives. Their fields-of-view were either aligned to the spin axis or at small angles to it, hence they always view the portion of the sky at right angles to the earth-sun line. This database accesses the raw rates FITS datafile for the A, B and C GCXSE detectors, accumulated every 160 ms in the 2-60 keV energy band. This is a service provided by NASA HEASARC .
125. Palomar survey digitized by MAMA
ID:
ivo://padc.obspm.astro/posse/q/siap
Title:
Palomar survey digitized by MAMA
Short Name:
posse_siap
Date:
16 Jul 2024 00:01:13
Publisher:
Paris Astronomical Data Centre
Description:
Survey from Palomar Image plates Digitized using MAMA at Observatoire de Paris .All the image have been resampled and reprojected TAN
126. posse image cutouts
ID:
ivo://padc.obspm.astro/posse/q/cutout
Title:
posse image cutouts
Short Name:
posse
Date:
16 Jul 2024 00:01:13
Publisher:
Paris Astronomical Data Centre
Description:
Survey from Palomar Image plates Digitized using MAMA at Observatoire de Paris .All the image have been resampled and reprojected TAN
127. PPAKM31 – Optical Integral Field Spectroscopy of Star-Forming Regions in M31
ID:
ivo://org.gavo.dc/ppakm31/q/pub
Title:
PPAKM31 – Optical Integral Field Spectroscopy of Star-Forming Regions in M31
Date:
12 Jun 2024 13:04:11
Publisher:
The GAVO DC team
Description:
These observations cover five star-forming regions in the Andromeda galaxy (M31) with optical integral field spectroscopy. Each has a field of view of roughly 1 kpc across, at 10pc physical resolution. In addition to the calibrated data cubes, we provide flux maps of the Hβ, [OIII]5007, Hα, [NII]6583, [SII]6716 and [SII]6730 line emission. Line fluxes have not been corrected for dust extinction. All data products have associated error maps.
128. 3rd Ariel-V SSI Catalog
ID:
ivo://nasa.heasarc/ariel3a
Title:
3rd Ariel-V SSI Catalog
Short Name:
ARIEL3A
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
The 3rd Ariel-V SSI Catalog contains a list of X-ray sources detected by the University of Leicester's Sky Survey Instrument (SSI) on the Ariel-V satellite, and published (in 2 papers) as the Ariel-V (3A) Catalog: Warwick et al. 1981, MNRAS, 197, 865 (the low galactic latitude sources) and McHardy et al. 1981, MNRAS, 197, 893 (the high galactic latitude sources). The catalog is based on observations extending over a 5.5 year period from 1974 October until 1980 March. The SSI had a field of view of 0.75 by 10.6 degrees (FWHM) and had an energy range from 2 to 18 keV. A detailed description of the SSI is given by Villa et al. 1976, MNRAS, 176, 609. For a more detailed discussion of how the 3A Catalog was created, please refer to the Warwick et al. (1981) and McHardy et al. (1981) papers. This online catalog was created by the HEASARC in March 2003 based on the merger of two original tables originally obtained from the ADC website (<a href="https://heasarc.gsfc.nasa.gov/FTP/heasarc/dbase/misc_files/ariel3a/hilat.dat">https://heasarc.gsfc.nasa.gov/FTP/heasarc/dbase/misc_files/ariel3a/hilat.dat</a> and <a href="https://heasarc.gsfc.nasa.gov/FTP/heasarc/dbase/misc_files/ariel3a/lowlat.dat">https://heasarc.gsfc.nasa.gov/FTP/heasarc/dbase/misc_files/ariel3a/lowlat.dat</a>). This is a service provided by NASA HEASARC .
129. ROSAT All-Sky Survey Archival Data
ID:
ivo://nasa.heasarc/rassmaster
Title:
ROSAT All-Sky Survey Archival Data
Short Name:
RASSMASTER
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
This database table contains the list German ROSAT All-Sky Survey observations which were obtained during the ROSAT All-Sky Survey phase (1990 July 30 to 1991 Jan 25) and which have become available to the public. These data were obtained in scanning mode and therefore an individual dataset covers a much larger area of the sky than do pointed moded observations. In addition all these data were obtained with PSPC-C, while all pointed mode observations after the end of the All-Sky Survey were obtained with PSPC-B. For each observation listed in this database table, the instrument used, processing site, and coordinates of the field center are given, as well as the ROSAT observation request number (ROR), actual exposure time, date the observation took place, and more. For details about the ROSAT instruments, consult the ROSAT Mission Description (NASA Research Announcement for ROSAT, Appendix F and its addendum) and the ROSAT GSFC GOF website at <a href="http://heasarc.gsfc.nasa.gov/docs/rosat/rosgof.html">http://heasarc.gsfc.nasa.gov/docs/rosat/rosgof.html</a> for more information. For more information about the ROSAT All Sky Survey, see the ROSAT All Sky Survey page at <a href="http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey">http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey</a>. This database table was created at the HEASARC in March 2002, based on information provided by Max-Planck-Institut fuer extraterrestrische Physik at <a href="http://wave.xray.mpe.mpg.de/">http://wave.xray.mpe.mpg.de/</a>. This is a service provided by NASA HEASARC .
130. ROSAT Archival Data
ID:
ivo://nasa.heasarc/rosmaster
Title:
ROSAT Archival Data
Short Name:
ROSAT
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
This database table contains the list of all Röntgen Satellite (ROSAT) X-Ray Telescope (XRT) pointing-mode observations for which data sets are available, i.e., it excludes the ROSAT All-Sky Survey observations. Users should consult the RASSMASTER database table for those XRT observations which were made in scanning mode during the ROSAT All-Sky Survey (RASS) phase (30 July 1990 to 25 January 1991, and 3 August 1991 to 13 August 1991). For each observation listed in this table, parameters such as the focal-plane instrument used, the data processing site, and the target name and coordinates are given, as well as the ROSAT Observation Request (ROR) number, the actual and requested exposure times, the date(s) on which the observation took place, etc. For details about the ROSAT instruments, consult the ROSAT Guest Observer Facility (GOF) website at <a href="https://heasarc.gsfc.nasa.gov/docs/rosat/">https://heasarc.gsfc.nasa.gov/docs/rosat/</a>. A list of the available online ROSAT documentation can be found at <a href="https://heasarc.gsfc.nasa.gov/docs/rosat/rosdocs.html">https://heasarc.gsfc.nasa.gov/docs/rosat/rosdocs.html</a>. This table was created by the HEASARC in July 2004 by combining the data from two long-standing HEASARC Browse tables into one master table. It was updated by the HEASARC in March 2022 to add start and end times for the 157 sequence IDs which did not already have start and end times. This is a service provided by NASA HEASARC .

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