Subject: optical astronomy / Resource Type: Archive / Capability Type: Simple Image Access Protocol

ID:: ivo://mast.stsci/siap/goods.hst
Title:: Great Observatories Origins Deep Survey (GOODS)
Short Name:: HST.GOODS
Date:: 23 Jul 2020 19:32:07
Publisher:: Space Telescope Science Institute Archive
Description:: GOODS aims to unite extremely deep observations from NASA's Great Observatories, the Spitzer Space Telescope, Hubble, and Chandra, ESA's XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. GOODS will survey a total of roughly 320 square arcminutes in two fields centered on the Hubble Deep Field North and the Chandra Deep Field South.

ID:: ivo://mast.stsci/siap/hst.m51
Title:: HST ACS mosaic images of M51
Short Name:: HST.M51
Date:: 23 Jul 2020 14:15:40
Publisher:: Space Telescope Science Institute Archive
Description:: In January 2005, the Hubble Heritage Team obtained a large 4-color mosaic image of the Whirlpool Galaxy NGC 5194 (M51), and its companion NGC 5195, with the Advanced Camera for Surveys (ACS) onboard the Hubble Space Telescope (HST observing program 10452, PI: Steven V. W. Beckwith). A six-pointing ACS WFC mosaic of the galaxy pair M51 was obtained in four filters: B, V, I, and H-alpha.

ID:: ivo://mast.stsci/siap/hst.appp
Title:: HST Archival Pure Parallels Project
Short Name:: HST.APPP
Date:: 23 Jul 2020 19:33:56
Publisher:: Space Telescope Science Institute Archive
Description:: The Archival Pure Parallel Project processed and combined about 2,000 WFPC2 images, primarily in the wide UBVI filters, obtained in parallel with other HST instruments. Combined, drizzled, cosmic-ray cleaned images were produced for each pointing. These data can be used to address a wide range of science topics: measuring the cosmic shear on scales from 20" to 2'; discovering ~ 50 starforming galaxies at z ~ 4; finding optical counterparts to AGNs in wide-area radio and X-ray catalogs; improving the determination of the scale length of the Galactic disk; and studying stellar populations down to 1 solar mass for about 25 separate lines of sight in the Magellanic Clouds.

ID:: ivo://mast.stsci/siap/hst.gems
Title:: HST Galaxy Evolution from Morphology and SEDs
Short Name:: HST.GEMS
Date:: 22 Jul 2020 22:30:27
Publisher:: Space Telescope Science Institute Archive
Description:: GEMs is a large-area (800 arcmin 2) two-color (F606W and F850LP) imaging survey with the Advanced Camera for Surveys on the Hubble Space Telescope. Centered on the Chandra Deep Field-South, it covers an area of ~ 28'x28', or about 120 HDF areas, to a depth of MAB(F606W)=28.5(5s) for compact sources. Focusing on the redshift range ~ 0.2<z<1.1, GEMS provides morphologies and structural parameters for nearly 10,000 galaxies where redshift estimates, luminosities, and SEDs exist from COMBO-17.

ID:: ivo://mast.stsci/siap/hst.helix
Title:: HST Hubble HELIX Observations
Short Name:: HST.HELIX
Date:: 22 Jul 2020 22:22:06
Publisher:: Space Telescope Science Institute Archive
Description:: For the 14 hours of peak Leonid meteoroid flux in November 2002, the Hubble Space Telescope was pointed away from the radiant, and the solar arrays were oriented to minimize their cross-section. By coincidence, one of the nearest and largest planetary nebulae, the Helix Nebula (NGC 7293), was nearly opposite the incoming Leonids and could be observed. A "Hubble Helix Team" (below) of volunteers led by Margaret Meixner (STScI) organized a nine-orbit campaign to observe the Helix with the ACS, WFPC2, NICMOS, and STIS.

ID:: ivo://mast.stsci/siap/hst.tno
Title:: HST trans-Neptunian Objects Search field images
Short Name:: HST.TNO
Date:: 22 Jul 2020 22:31:56
Publisher:: Space Telescope Science Institute Archive
Description:: The "TNO Search Field" images are the sidereally summed images of a search for trans-Neptunian objects (TNOs) using the Wide Field Camera of the HST/ACS instrument. The observations were taken under Cycle 11 program GO-9433, "The Size Distribution of Kuiper Belt Bodies," with G. Bernstein as PI. The TNO search consisted of approximately 96x400 s exposures in the F606W filter for each of six contiguous ACS fields of view. The TNO search field is approximately 6'x10', centered near 14h 07M 53.3s -11d 21' 38" (J2000).

ID:: ivo://mast.stsci/siap/hst.udf
Title:: HST Ultra Deep Field (UDF) Images
Short Name:: HST.UDF
Date:: 22 Jul 2020 22:32:35
Publisher:: Space Telescope Science Institute Archive
Description:: The ACS Ultra Deep Field (UDF) is a cycle 12 survey carried out using the Advanced Camera for Surveys (ACS) on HST and taking advantage of the Director's Discretionary time. The UDF consists of a single ultra-deep field (412 orbits in total taken in 4 bands) within the CDF-S GOODS area. It is the deepest image ever obtained with Hubble. This service also includes data from the UDF follow-Up program by PI Massimo Stiavelli and colleagues obtained under HST cycle 14 program 10632 titled Searching for galaxies at z>6.5 in the Hubble Ultra Deep Field (also known as UDF05).

ID:: ivo://mast.stsci/siap/xmm-om
Title:: X-ray Multi-Mirror (XMM) Optical Monitor images
Short Name:: XMM-OM
Date:: 23 Jul 2020 19:42:40
Publisher:: Space Telescope Science Institute Archive
Description:: The Newton X-ray Multi-Mirror Mission (XMM) was launched in December, 1999 with a projected lifetime of 10 years. Although intended primarily as an X-ray observatory, XMM included a small but powerful optical/UV 30 cm telescope co-aligned with the X-ray telescopes for contemporaneous observations. The modified Ritchey-Chretien telescope is capable of detecting 24th magnitude sources in its 17 arcmin field of view. It provides images in the 160-600nm wave band with 1 arcsec resolution. MAST is serving a OM Mosaic product that uses a pipeline described by Kuntz et. al. OMCat: Catalog of Serendipitous Sources Detected with the XMM-Newton Optical Monitor PASP, 120:740-758

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