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401. Spitzer Survey of Stellar Structure in Galaxies
ID:
ivo://irsa.ipac/Spitzer/Images/S4G
Title:
Spitzer Survey of Stellar Structure in Galaxies
Short Name:
S4G
Date:
27 Sep 2024 01:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Spitzer Survey of Stellar Structure in Galaxies (S4G) is a volume-, magnitude-, and size-limited survey of over 2300 nearby galaxies at 3.6 and 4.5μm. This is an extremely deep survey reaching an unprecedented 1σ surface brightness limit of μ3.6μm(AB) = 27 mag arcsec-2. This translates to a stellar surface density of << 1 M⊙ pc-2 ! S4G can thus probe the stellar structure in galaxies in a regime where the gas dominates the stars (typical HI surface density ~ a few M⊙ pc-2).
402. SSC Interface for the XMM-Newton Catalogue
ID:
ivo://xcatdb
Title:
SSC Interface for the XMM-Newton Catalogue
Short Name:
XCATDB
Date:
28 Apr 2023 13:47:37
Publisher:
Observatory of Strasbourg, SSC Team
Description:
The XMM catalogue provides an effective dataset for generating large, well-defined samples of various types of astrophysical object, notably active galaxies (AGN), clusters of galaxies, interacting compact binaries and active stellar coronae, using the power of X-ray selection. The large sky area covered by the serendipitous survey also means that XMM is a rich resource for exploring the variety of the X-ray source populations and identifying rare source types. Not all public observations are included in the catalogues. The XCATDB interface is design to process complex queries including multiple constraints on cross-correlated couterparts.
403. Subaru HDS Spectrum data service
ID:
ivo://jvo/subaru/hds
Title:
Subaru HDS Spectrum data service
Short Name:
SubaruHDS
Date:
24 Jul 2024 03:30:55
Publisher:
JVO
Description:
This data service provides various data related to Subaru HDS.
404. Subaru MOIRCS data service
ID:
ivo://jvo/subaru/moircs
Title:
Subaru MOIRCS data service
Short Name:
SUBARU_MOIRCS
Date:
14 Nov 2019 03:50:26
Publisher:
JVO
Description:
MOIRCS (Multi-Object InfraRed Camera and Spectrograph) provides wide-field imaging and long-slit / multi-object (MOS) spectroscopic capabilities in the 0.9 ~ 2.5 &#181;m spectral range under the natural seeing condition. The 4'?~7' field of view is covered by two Hawaii-2 2048?~2048 arrays with the spatial resolution of 0.117 arcsec/pixel.
405. Subaru Prime Focus Camera (Suprime-Cam) Exposures Log
ID:
ivo://nasa.heasarc/subpfclog
Title:
Subaru Prime Focus Camera (Suprime-Cam) Exposures Log
Short Name:
SubaruPFC
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
This table contains the Subaru Prime Focus Camera (Suprime-Cam) log of exposures having observation type = &#39;OBJECT&#39; (those with &#39;BIAS&#39;, &#39;FLAT&#39; and other types are not included) which have been made since April 2001. Note that from the version of Nov. 2005 on, the number of rows has significantly increased because those data with worse position determination (up to 30 arcsec error) are now included. The data currently extend to November 2005 and it is anticipated that they will be regularly updated Suprime-Cam is an 80-mega pixels (10240 x 8192) mosaic CCD camera, for the wide-field prime focus of the 8.2m Subaru telescope. Suprime-Cam covers a field of view 34&#39; x 27&#39;, a unique facility among the 8-10m class telescopes, with a resolution of 0.202 arcseconds per pixel. The focal plane consists of ten high-resistivity 2kx2k CCDs developed by MIT Lincoln Laboratory, which are cooled by a large Stirling-cycle cooler. The CCD readout electronics was designed to be scalable, which allows the multiple read-out of tens of CCDs. It takes 50 seconds to readout entire arrays. A filter-exchange mechanism of the jukebox type is designed that can hold up to ten large filters (205 x 170 x 15 mm&lt;sup&gt;3&lt;/sup&gt;). The wide-field corrector is basically a three-lens Wynne-type, but has a new type of atmospheric dispersion corrector. The corrector provides a flat focal plane and an un-vignetted field of view of 30&#39; in diameter. The achieved co-planarity of the focal array mosaic is smaller than 30 um peak-to-peak, which realizes mostly the seeing limited image over the entire field. The median seeing in the I_c-band, measured over one year and a half, is 0.61 arcseconds. The PSF anisotropy in Suprime-Cam images, estimated by stellar ellipticities, is about 2% under this median seeing condition. At the time of its commissioning, Suprime-Cam had the largest survey speed, which is defined as the field of view multiplied by the primary mirror area of the telescope, among those cameras built for sub-arcsecond imaging. For more details, see: Miyazaki et al., Publ. Astron. Soc. Japan 54, 833-853, 2002 (2002PASJ...54..833M). This table was created by the HEASARC in September 2007 based on CDS table B/subaru/suprimc.dat (the ReadMe file for the latter was tagged with a date of August 25th, 2007). This is a service provided by NASA HEASARC .
406. Subaru Suprime-Cam data service
ID:
ivo://jvo/subaru/spcam
Title:
Subaru Suprime-Cam data service
Short Name:
SUBARU_SUP
Date:
04 Nov 2020 06:00:31
Publisher:
JVO
Description:
The Subaru Prime Focus Camera (Suprime-Cam) is a mosaic of ten 2048 x 4096 CCDs, located at the prime focus of Subaru Telescope, which covers a 34' x 27' field of view with a pixel scale of 0.20''. This service provides access to the JVO Subaru Suprime-Cam mosaic image archive. The purpose of this archive is to provide quick look images taken by Subaru/Suprime-Cam. Those images were processed by a pipeline developed by JVO.
407. Suzaku Master Catalog
ID:
ivo://nasa.heasarc/suzamaster
Title:
Suzaku Master Catalog
Short Name:
SUZAMASTER
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
This database table records high-level information for each Suzaku observation and provides access to the data archive. Each record is associated with a single observation. An observation contains data from all instruments on board Suzaku. The Suzaku satellate operated from July 2005 till September 2015. This database table was generated at the Suzaku proceesing site with the final data reprocessing (September 2016) after the mission stopped operating. During operation, it was updated on daily basis. This is a service provided by NASA HEASARC .
408. Suzaku Wide-Band All-Sky Monitor (WAM) Catalog of Event Lightcurves
ID:
ivo://nasa.heasarc/suzakuwam
Title:
Suzaku Wide-Band All-Sky Monitor (WAM) Catalog of Event Lightcurves
Short Name:
SUZAKUWAM
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
This database table contains information of the events detected by the Wide-band All-sky Monitor (WAM) on Suzaku during its ~10 years of operation. Each event has associated data products. The lightcurves are derived from the on-board operating modes that collected the WAM data from each of the sub-detectors. The lightcurves are rates as a function of time in different energy bands, and they can be used with the general FITS tools within HEAsoft or XRONOS. Version 3 of the lightcurves were generated at HEASARC from the version 2 files, and they are now the final versions hosted at both HEASARC and DARTS. This database table reflects version 3 of the data products. &lt;p&gt; Version 2 of the FITS lightcurves and their plots were generated at Saitama University in Japan and a copy hosted at the DARTS archive, located at ISAS (&lt;a href="http://www.darts.isas.ac.jp/pub/suzaku/wam-2.0/"&gt;http://www.darts.isas.ac.jp/pub/suzaku/wam-2.0/&lt;/a&gt;). This is a service provided by NASA HEASARC .
409. Suzaku XIS Configuration Log
ID:
ivo://nasa.heasarc/suzaxislog
Title:
Suzaku XIS Configuration Log
Short Name:
SUZAXISLOG
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
The Suzaku XIS detector units can be configured differently depending on how the user chooses the observation to be carried out. This database table records for each Suzaku observation the different XIS configurations during an observation for all XIS units. The set of parameters that can be configured are: datamode (see also edit mode), window size, on-board window discriminator, on-board grading and event threshold. Each record lists for a given XIS the values set for these parameters in the time interval where they are valid within the observation. Therefore for a given XIS there will be as many records as many different configurations are present within an observation. This database table is generated at the Suzaku processing site. During operation, it is updated on daily basis. This is a service provided by NASA HEASARC .
410. Swift BAT Instrument Log
ID:
ivo://nasa.heasarc/swiftbalog
Title:
Swift BAT Instrument Log
Short Name:
SwiftBAT
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
The BAT can operate several configuration modes simultaneously. Each of the simultaneous modes is listed in separate records within this table. For a given time interval, there are several records (partially overlapping in time), each describing a single configuration/mode. The BAT modes collect data for the entire FOV but also have the capability to record rates (tag mask rate) for up to a few specific sky positions (typically 3) that correspond to a pre-assigned target ID. It is possible that at least two or more of these positions do not coincide with the BAT or NFI pointing position and therefore the target ID does necessarily coincide with Target_ID of the BAT or NFI pointing position. This table records for the position (RA and Dec) and Target_ID parameters the correct values associated to each of the mask tag data. This database table is generated at the Swift processing site. During operation, it is updated on daily basis. This is a service provided by NASA HEASARC .

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