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Start Over Resource Type Archive Capability Type Table Access Protocol
1. AKARI Far-infrared All-Sky Survey Maps
ID:
ivo://jvo/isas/akari/fis_v1
Title:
AKARI Far-infrared All-Sky Survey Maps
Short Name:
AKARI_FIS_V1
Date:
18 Dec 2022 01:11:53
Publisher:
JVO
Description:
The AKARI Far-infrared All-Sky Survey Maps is produced with the participation of people from the following institutes: University of Tokyo, ISAS/JAXA, Tohoku University, and University of Tsukuba. The image data in this release are produced based on the AKARI All-Sky Survey with 4 far-infrared bands at N60 (65 um), WIDE-S (90 um), WIDE-L (140 um), and N160 (160 um).
2. Archive of AGN spectral observations
ID:
ivo://fai.kz/spectra_agn_archive/q/ssa
Title:
Archive of AGN spectral observations
Short Name:
spectra_agn_archive SSAP
Date:
04 May 2024 09:44:08
Publisher:
Fesenkov Astrophysical Institute
Description:
The archive of AGN spectral observations is obtained on AZT-8 telescope at the Fesenkov Astrophysical Institute (FAI), Almaty, Kazakhstan. It represents the result of observations for abot 25 years - from 1970 to 1995. All observations were carried out at AZT-8 (D = 700 mm, F[main] = 2800 mm, F[Cassegrain] = 11000 mm) with a high-power spectrograph. In 1967-68, on the basis of the image intensifier (https://doi.org/10.1080/1055679031000084795a) developed and assembled the spectrograph of the original design in the workshops of the FAI. To use the spectra, please, download raw .fit file of required object, date and exposure. The open 'Calibration frames' in Related links and then use them to calibrate object spectra frames. For more information about calibration process please visit https://github.com/ill-i/Spectra-Reduction.
3. Ariel V All-Sky Monitor
ID:
ivo://nasa.heasarc/ariel5
Title:
Ariel V All-Sky Monitor
Short Name:
ARIEL5
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The All Sky Monitor was one of six X-ray instruments on the Ariel 5 satellite. The satellite was launched into a low inclination (2.8 degrees), nearly circular orbit (altitude ~520 km) on 15 October 1974. Ariel 5 was actively pointed so that objects of interest could be observed by the four instruments aligned along its spin axis. The ASM was mounted 90 degrees from the spin axis; the satellite had a spin period of 6 seconds. The ASM operated from October 18, 1974 to March 10, 1980. The ASM instrument, built by the Lab for High Energy Astrophysics at NASA- Goddard Space Flight Center, provided continuous coverage of the entire sky, except for a 20 degree band straddling the satellite's equator. The ASM was intended to act as an early detection system for transients, and to monitor the variability of bright ( > 0.2 Crab) galactic sources. The instrument consisted of a pair of X-ray pinhole cameras, each covering opposite halves of the sky, with gas-filled imaging proportional counters. Position determination of sources was accomplished through position-sensitive anode wires and satellite rotation. Each camera had a 1-cm<sup>2</sup> aperture. Overall telemetry constraints limited the duty cycle for any given source to 1 percent. With the low telemetry rate provided for this instrument (1 bit/s), temporal and spectral information were sacrificed for the sake of all-sky coverage. Hence, spectral information was limited to a single 3 - 6 keV bandpass, and temporal resolution was limited to the satellite orbital period, ~100 minutes. This is a service provided by NASA HEASARC .
4. ASCA Master Catalog
ID:
ivo://nasa.heasarc/ascamaster
Title:
ASCA Master Catalog
Short Name:
ASCA
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The ASCAMASTER table contains data on all ASCA observations that were ever in any of the following states: 'Accepted', 'Scheduled Long-Term', 'Scheduled Short-Term', 'Processed', and 'Archived'. The final status of an observation is given by the parameter Status. Specific dates that affect the status of an observation are listed as the parameters scheduled_date, observed_date, processed_date, archived_date, and cycle. Notice that, if one or more of the date parameters are empty for a given observation, this means that that those particular processes have not occurred: e.g., if observed_date is empty, this means that the planned observation was not observed. This is a service provided by NASA HEASARC .
5. ASCAProposalInfo&Abstracts
ID:
ivo://nasa.heasarc/ascaprspec
Title:
ASCAProposalInfo&Abstracts
Short Name:
ASCAPRSPEC
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The ASCAPRSPEC table was created for the purpose of providing a complete, accurate, and easily accessible tracking of ASCA proposal information. This is a service provided by NASA HEASARC .
6. ASCA Proposals
ID:
ivo://nasa.heasarc/ascao
Title:
ASCA Proposals
Short Name:
ASCAO
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The ASCAO database contains the listing of accepted targets from all proposals submitted in repsonse to the ASCA Guest Observer (GO) Announcements of Opportunities (AOs), as well as the targets that were selected for the Performance Verification (PV) phase. The current version of ASCAO includes all accepted targets from AOs 1 through 8.5 inclusive. Notice that, since the accepted targets include Priority 3 ones of which only a fraction have or will actually be observed, some of the listed targets in this database will never have been observed. To obtain more detailed information about the status of particular targets, please consult either the Master ASCA database table (ASCAMASTER) or the ASCA Observing Log database table (ASCALOG). This database was last updated in August 2000 based on information provided by the ASCA Project. This is a service provided by NASA HEASARC .
7. BBXRT Archive
ID:
ivo://nasa.heasarc/bbxrt
Title:
BBXRT Archive
Short Name:
BBXRT
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The BBXRT database table contains information about each observation made by the Broad Band X-Ray Telescope. It includes a catalog of observations and spectral and lightcurve products for each of the 10 pixels per observation. This is a service provided by NASA HEASARC .
8. BeppoSAX Approved Pointings
ID:
ivo://nasa.heasarc/saxao
Title:
BeppoSAX Approved Pointings
Short Name:
SAXAO
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The SAXAO database contains the list of the all accepted AO1/AO2/AO3/A04/AO5 SAX CORE and GO program proposals, approved for the first year of operations. The database also includes targets scheduled for the Science Verification Phase (SVP) (from launch, 30 April 1996, till August 1996). The CORE program includes proposals led by Principal Investigator belonging to Italian or Dutch institutions, to the Space Science Department of ESA or to the Max Planck Institute for Extraterrestial Physics in Garching. Approximately 80 percent of the first year observing time is allocated to the CORE program. The remaining 20 percent of time for the first year operations is reserved for the GO program. For the AO2 60 percent is allocated to the CORE program and 40 percent to the GO. For the AO3 and AO4 50 percent is allocated to the CORE program and 50 percent to the GO. More information on the SAX mission is available at the following address <a href="http://www.asdc.asi.it">http://www.asdc.asi.it</a> and also <a href="https://heasarc.gsfc.nasa.gov/docs/sax/saxgof.html">https://heasarc.gsfc.nasa.gov/docs/sax/saxgof.html</a>. This is a service provided by NASA HEASARC .
9. BeppoSAX NFI Archive and Observation Log
ID:
ivo://nasa.heasarc/saxnfilog
Title:
BeppoSAX NFI Archive and Observation Log
Short Name:
SAXNFI
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The SAXNFILOG database contains the SAX Narrow Field Instruments (NFI) approved pointings, but it also served as an observations log. It includes data taken during AO1, AO2, AO3, A04 and AO5 cycles and the Science Verification Phase (SVP). This is a service provided by NASA HEASARC .
10. BeppoSAX WFC Observation Log
ID:
ivo://nasa.heasarc/saxwfclog
Title:
BeppoSAX WFC Observation Log
Short Name:
SAXWFC
Date:
03 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The SAXWFCLOG database contains the SAX WFCs observations log for the AO cycles and the Science Verification Phase (SVP). The two WFCs are located at 90 degrees from the NFI and set 180 degrees apart. The field of view is 40 deg X 40 deg and the coordinates given in this databases are the pointing positions. The database is updated regularly to include the most recent timeline, and updates are provided by the SAX-Science Data Center in Rome. This is a service provided by NASA HEASARC .

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