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Start Over Content Level Research Capability Type Simple Image Access Protocol
11. Archive of Nearby Galaxies: Reduce, Reuse, Recycle (ANGRRR)
ID:
ivo://mast.stsci/angrrr
Title:
Archive of Nearby Galaxies: Reduce, Reuse, Recycle (ANGRRR)
Short Name:
HST.ANGRRR
Date:
22 Jul 2020 22:28:43
Publisher:
Space Telescope Science Institute Archive
Description:
An archive of stellar photometry for galaxies within 3.5 Mpc, excluding Local Group galaxies, based on primary and parallel wide-filter UV and optical observations taken with HST ACS/WFC or WFPC2.The sample includes all observations taken through Dec. 2008, as well as observations taken as part of Cycle 16 Supplemental GO programs 11986 and 11987. This release includes the ANGST targets within 3.5 Mpc; these observations have been rereduced using updated CTE corrections and zeropoints. Galaxies with 3.5 < D <= 5 Mpc will be included in a later release.
12. ASCA Master Catalog
ID:
ivo://nasa.heasarc/ascamaster
Title:
ASCA Master Catalog
Short Name:
ASCA
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
The ASCAMASTER table contains data on all ASCA observations that were ever in any of the following states: &#39;Accepted&#39;, &#39;Scheduled Long-Term&#39;, &#39;Scheduled Short-Term&#39;, &#39;Processed&#39;, and &#39;Archived&#39;. 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 .
13. ASCA SIS Source Catalog
ID:
ivo://nasa.heasarc/ascasis
Title:
ASCA SIS Source Catalog
Short Name:
ASCASIS
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
This preliminary ASCA SIS Source Catalog contains a list of point sources detected by the Solid-state Imaging Spectrometers (SIS) on-board the ASCA Observatory. This catalog was generated by searching for point-like sources in all data available from the HEASARC&#39;s ASCA public archive (ASCAPUBLIC) as of 24 Oct 1996; and is populated by both target and serendipitous sources in the SIS field-of-view. For each catalogued source various information is available, which includes the celestial coordinates of the source, the count rate, the significance of detection, and the hardness ratio, total aperture counts, exposure time, and start time of the observation. In addition, a set of three GIF &quot;thumbnail&quot; images is available in the broad (0.5 - 12 keV), soft (2 &lt; keV), and hard (&gt; 2 keV) spectral bands centered on the apparent detection. These images are convenient for accessing the quality of the source detection. The current catalog is preliminary, the goal of the catalog authors being to make the SIS source list available as quickly as possible. To accomplish this, they took an incremental approach and placed their &quot;work in progress&quot; on-line, warts and all. They urge caution in using and citing these preliminary results, as they point out that the information is not, as yet, 100% reliable. This catalog was generated in January 1997 by Drs. Eric Gotthelf and Nicholas White and resulted from their search for point-like sources in all of the then-available SIS data files in the HEASARC&#39;s Public ASCA Data Archive as of 24 Oct 1996. The catalog is populated with both targeted and serendipitous sources that were present in the SIS field-of-view. This is a service provided by NASA HEASARC .
14. ATLAS DR1 SIAP Service
ID:
ivo://wfau.roe.ac.uk/atlasdr1-siap
Title:
ATLAS DR1 SIAP Service
Short Name:
ATLAS DR1 SIAP
Date:
09 Jul 2019 14:38:11
Publisher:
WFAU, Institute for Astronomy, University of Edinburgh
Description:
Simple image access to OmegaCAM ATLAS Survey data release 1 images
15. Auriga-California Molecular Cloud
ID:
ivo://irsa.ipac/Herschel/Images/ACMC
Title:
Auriga-California Molecular Cloud
Short Name:
ACMC
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Auriga-California molecular cloud is a large region of relatively modest star formation that is part of the Gould Belt. The Herschel Space Observatory program OT1_pharvey01_3 ("The Auriga-California Molecular Cloud: A Massive Nearby Cloud With Powerful Diagnostics For Early Stages of Star Formation", PI Paul Harvey) observed a 14.5 square degree area of the cloud in five far-infrared bands.
16. Balloon-borne Large Aperture Submillimeter Telescope
ID:
ivo://irsa.ipac/BLAST/Images
Title:
Balloon-borne Large Aperture Submillimeter Telescope
Short Name:
BLAST
Date:
31 Aug 2023 01:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Balloon-borne Large-Aperture Sub-millimeter Telescope (BLAST) is a 2-m telescope that conducted the first wide-area (> many square degrees) sub-mm surveys at wavelengths 250--500 um. Built and flown by an international collaboration headed by the University of Pennsylvania (P.I. Mark Devlin), the telescope uses a prototype of the SPIRE camera for the Herschel satellite. Despite parts of this band being available to ground-based telescopes from high-altitude sites such as Mauna Kea (e.g. JCMT) and Chile (e.g. future ALMA site), BLAST surveys are currently un-matched in sensitivity and area given the comparatively negligible atmospheric water vapour at 38 km altitude.
17. Bisei Space Guard Center images
ID:
ivo://jvo/isas/darts/bsgc
Title:
Bisei Space Guard Center images
Short Name:
BSGC_IMAGE
Date:
05 Feb 2025 04:12:46
Publisher:
JVO
Description:
Bisei Space Guard Center (BSGC) is an optical telescope facility in Japan, operated by JAXA. It tracks near-Earth asteroids and space debris. DARTS provides data observed by a 25 cm telescope from 2000 to 2002 and data observed by a 1 m telescope from 2007 to 2017.
18. Bochum Galactic Disk Survey (BGDS) images
ID:
ivo://org.gavo.dc/bgds/q/sia
Title:
Bochum Galactic Disk Survey (BGDS) images
Short Name:
bgds sia
Date:
27 Dec 2024 08:31:07
Publisher:
The GAVO DC team
Description:
The Bochum Galactic Disk Survey is a project to monitor the stellar content of the Galactic disk in a 6 degree wide stripe centered on the Galactic plane. The data has been recorded from September 2010 to September 2019 with the RoBoTT Telecsope at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It contains measurements of more than 2x10^7 stars. The second and final data release contains follow-up observations from January 2017 to September 2019 in Sloan r and i and intermittent measurements in Johnson UVB, Sloan z and the narrowbands OIII, NB, Halpha and SII.
19. Bolocam Galactic Plane Survey
ID:
ivo://irsa.ipac/Bolocam_GPS/Images
Title:
Bolocam Galactic Plane Survey
Short Name:
BOLOCAM_GPS
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Bolocam Galactic Plane Survey (BGPS) is a 1.1 mm continuum survey of the Galactic Plane made using Bolocam on the Caltech Submillimeter Observatory. Millimeter-wavelength thermal dust emission reveals the repositories of the densest molecular gas, ranging in scale from cores to whole clouds. By pinpointing these regions, the connection of this gas to nascent and ongoing star formation may be explored. The BGPS coverage totals 170 square degrees (with 33" FWHM effective resolution). The survey is contiguous over the range -10.5 ≤ l ≤ 90.5, |b| ≤ 0.5. Towards the Cygnus X spiral arm, the coverage was flared to |b| ≤ 1.5 for 75.5 ≤ l ≤ 87.5. In addition, cross-cuts to |b| ≤ 1.5 were made at l = 3, 15, 30 and 31. The total area of this section is 133 square degrees. With the exception of the increase in latitude, no pre-selection criteria were applied to the coverage in this region. In addition to the contiguous region, four targeted regions in the outer Galaxy were observed: IC1396 (9 square degrees, 97.5 ≤ l ≤ 100.5, 2.25 ≤ l ≤ 5.25), a region towards the Perseus Arm (4 square degrees centered on l = 111, b=0 near NGC7538), W3/4/5 (18 square degrees, 132.5 ≤ l ≤ 138.5) and Gem OB1 (6 square degrees, 187.5 ≤ l ≤ 193.5). The survey has detected approximately 8,400 sources, to an rms noise level in the maps ranging from 30 to 60 mJy beam-1. The BGPS survey and catalog provide an important database for sub/millimeter observations with the Herschel Space Observatory, ALMA, SCUBA-2, APEX, and others.
20. Bolocam Lockman Hole Map
ID:
ivo://irsa.ipac/Bolocam/Images/Bolocam_LH
Title:
Bolocam Lockman Hole Map
Short Name:
Bolocam_LH
Date:
23 May 2023 20:55:52
Publisher:
NASA/IPAC Infrared Science Archive
Description:
A deep 1.1 mm survey using Bolocam of the Lockman Hole, producing a map and galaxy candidate list. This survey encompasses 324 square arcmin to an rms noise level (filtered for point sources) of 1.4 mJy/beam. This project is described by Laurent et al., ApJ, 2005.

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