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Start Over Resource Type Archive Facility HST
11. Great Observatories Origins Deep Survey (GOODS)
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.
12. High Speed Photometer
ID:
ivo://archive.stsci.edu/hst/hsp
Title:
High Speed Photometer
Short Name:
HST.HSP
Date:
23 Jul 2020 19:49:53
Publisher:
Space Telescope Science Institute Archive
Description:
The High Speed Photometer (HSP) was one of the four original axial instruments on the Hubble Space Telescope (HST). The HSP was designed to make very rapid photometric observations of astrophysical sources in a variety of filters and passbands from the near ultraviolet to the visible. The HSP was removed from HST during the First Servicing Mission in December, 1993.
13. HST ACS Coma cluster (Abell 1656) Treasury Survey (COMA)
ID:
ivo://mast.stsci/siap/coma
Title:
HST ACS Coma cluster (Abell 1656) Treasury Survey (COMA)
Short Name:
HST.COMA
Date:
23 Jul 2020 19:33:05
Publisher:
Space Telescope Science Institute Archive
Description:
The HST ACS Coma cluster Treasury survey is a deep two-passband imaging survey of one of the nearest rich clusters of galaxies, the Coma cluster (Abell 1656).
14. HST ACS mosaic images of M51
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.
15. HST Archival Pure Parallels Project
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.
16. HST Cosmic Evolution Survey
ID:
ivo://mast.stsci/siap/hst.cosmos
Title:
HST Cosmic Evolution Survey
Short Name:
HST.COSMOS
Date:
23 Jul 2020 19:35:16
Publisher:
Space Telescope Science Institute Archive
Description:
COSMOS (P.I. Nicholas Scoville, California Institute of Technology, USA/CA) is an HST Treasury Program to survey a 2 square degree equatorial field, centered on RA=10:00:28.6 and DEC=+02:12:21.0 with the ACS in the I band of the VIMOS equatorial field. Parallel observations with WFPC2 and NICMOS were also obtained.
17. HST Galaxy Evolution from Morphology and SEDs
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.
18. HST Hubble Deep Field
ID:
ivo://mast.stsci/siap/hst.hdf
Title:
HST Hubble Deep Field
Short Name:
HST.HDF
Date:
23 Jul 2020 19:35:54
Publisher:
Space Telescope Science Institute Archive
Description:
The Hubble Deep Field (HDF) is a Director's Discretionary program on HST in Cycle 5 to image a typical field at high galactic latitude in four wavelength passbands as deeply as reasonably possible. In order to optimize observing in the time available, a field in the northern continuous viewing zone (CVZ) was selected and images were taken for 10 consecutive days, or approximately 150 orbits. Shorter 1-orbit images were also obtained of the fields immediately adjacent to the primary HDF in order to facilitate spectroscopic follow-up by ground-based telescopes. The observations were carried out from 18-30 December 1995, and the data are available to the community for study.
19. HST Hubble Deep Field South
ID:
ivo://mast.stsci/siap/hst.hdf_south
Title:
HST Hubble Deep Field South
Short Name:
HST.HDF_SOUTH
Date:
23 Jul 2020 19:36:18
Publisher:
Space Telescope Science Institute Archive
Description:
A second Hubble Deep Field campaign was carried out between late September and October of 1998. The raw, pipeline calibrated and reprocessed data were released to the community on November 23, 1998. The rationale for undertaking a second deep field campaign followed from the wealth of information that has come out of HDF-N, and from the desire to provide a point of focus for similar studies of the distant universe from southern-hemisphere facilities. Simultaneous, parallel observations were made with the three HST instruments STIS, WFPC2 and NICMOS of separate, neighboring fields. As was the case for HDF-N, approximately 150 consecutive orbits were devoted to a single telescope pointing.
20. HST Hubble HELIX Observations
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.