Search

Start Over Resource Type Archive
211. 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.
212. 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.
213. 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.
214. HST Planned and Archived Observations
ID:
ivo://nasa.heasarc/hstpaec
Title:
HST Planned and Archived Observations
Short Name:
HSTPAEC
Date:
18 Apr 2025
Publisher:
NASA/GSFC HEASARC
Description:
This is the HST Planned and Archived Exposures Catalog (PAEC) as obtained from the Space Telescope Science Institute (STScI) Archive which created the original compilation from their Archive and Proposal databases. This database table provides a summary of all approved HST observations, including already completed observations and those which are planned to be executed as part of the current cycle or are reserved for execution by Guaranteed Time Observer (GTO) programs for the upcoming cycles. This database table provides a summary of both planned and completed HST observations. Much more information can be obtained about each exposure, and the data themselves can be retrieved, using STScI's Multimission Archive (URL is <a href="http://archive.stsci.edu/hst/">http://archive.stsci.edu/hst/</a>) or STScI's Archive Web Interface (URL is <a href="http://archive.stsci.edu/hst/search.php">http://archive.stsci.edu/hst/search.php</a>). Note that a number of solar system and other objects have 0 values for their 2000 equinox RA and declination coordinates in the original HST table and hence also in this HEASARC database. This HEASARC version of the HSTPAEC will be updated on a regular basis, usually within one month of the data files on the STScI Web site (URL <a href="http://archive.stsci.edu/hst/paec.html">http://archive.stsci.edu/hst/paec.html</a>) being updated. This database table is recreated by the HEASARC on a routine basis, usually within one month of the PAEC data files at the STScI Hubble Data Archive (HDA) being modified. This is a service provided by NASA HEASARC .
215. HST Space Telescope Imaging Spectrograph
ID:
ivo://mast.stsci/ssap/hst/stis
Title:
HST Space Telescope Imaging Spectrograph
Short Name:
HST STIS Spectra
Date:
22 Jul 2020 21:58:09
Publisher:
Space Telescope Science Institute Archive
Description:
MAST-produced spectral container files for STIS spectra. STIS spectra range from 1150 to 10,300 at low to medium spectral resolution, high spatial resolution echelle spectroscopy in the ultraviolet. STIS began operation in 1997. (Note the included echelle spectra are technically not yet supported by the SSAP.)
216. HST trans-Neptunian Objects Search field images
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).
217. HST Ultra Deep Field (UDF) Images
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).
218. HST Ultraviolet Atlas of Nearby Galaxies
ID:
ivo://mast.stsci/siap/hst.maoz_atlas
Title:
HST Ultraviolet Atlas of Nearby Galaxies
Short Name:
HST.maoz_atlas
Date:
23 Jul 2020 19:27:41
Publisher:
Space Telescope Science Institute Archive
Description:
A pictorial atlas of UV (2300 Å) images, obtained with the Hubble Space Telescope (HST) Faint Object Camera, of the central 22''× 22'' of 110 galaxies (Maoz, Filippenko, Ho, Macchetto, Rix, & Schneider 1996). The observed galaxies are an unbiased selection constituting about one half of a complete sample of all large (D>6 arcmin) and nearby (V< 2000 km/s ) galaxies. This is the first extensive UV imaging survey of normal galaxies. The data are useful for studying star formation, low-level nuclear activity, and UV emission by evolved stellar populations in galaxies. At the HST resolution (~ 0.05''), the images display an assortment of morphologies and UV brightnesses. These include bright nuclear point sources, compact young star clusters scattered in the field or arranged in circumnuclear rings, centrally-peaked diffuse light distributions, and galaxies with weak or undetected UV emission. We measure the integrated ~2300 Å flux in each image, and classify the UV morphology.
219. HST WFPC2 Spiral Galaxies
ID:
ivo://mast.stsci/siap/hst.sgal
Title:
HST WFPC2 Spiral Galaxies
Short Name:
HST.SGAL
Date:
23 Jul 2020 19:36:54
Publisher:
Space Telescope Science Institute Archive
Description:
Holwerda et al. examined 32 HST/WFPC2 archival fields of 29 spiral galaxies (Sab and later) for their paper The Opacity of Spiral Galaxy Disks. IV. Radial Extinction Profiles from Counts of Distant Galaxies Seen through Foreground Disks (2005, AJ,129:1396-1411). The majority of the data are from the Cepheid distance scale Key Project. The explicit goal was to provide deep mosaics in both V- and I-band with a better sampling in order to identify background galaxies through the foreground disk.
220. Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES)
ID:
ivo://mast.stsci/hippies
Title:
Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES)
Short Name:
HST.HIPPIES
Date:
22 Jul 2020 22:31:09
Publisher:
Space Telescope Science Institute Archive
Description:
Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) utilizes long-duration pure parallel visits (~> 3 orbits) of HST at high Galactic latitude (|b|>20o) to take deep, multi-band images in WFC3 (since Cycle 17) and in ACS (starting Cycle 18). It is unique in its large number of descrete fields along random sightlines, and thus is complementary to other surveys over contiguous fields but along limited sightlines.

Limit your search

more »

more »

more »

more »

more »

  • 2442