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Start Over Facility HST Capability Type Simple Cone Search
1. A103, A118 and A114 morphological studies
ID:
ivo://CDS.VizieR/J/ApJ/497/188
Title:
A103, A118 and A114 morphological studies
Short Name:
J/ApJ/497/188
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present the results of a program to study the detailed morphologies of galaxies in intermediate-redshift clusters and hence understand the physical origin of the enhanced star formation seen in the environments at earlier epochs. Deep, high-resolution imagery has been obtained of three rich clusters, AC 103, AC 118 and AC 114 at z=0.31, through the R (F702W) filter of the Wide Field Planetary Camera (WFPC2) of the Hubble Space Telescope (HST).
2. Advanced Camera for Surveys
ID:
ivo://archive.stsci.edu/hst/acs
Title:
Advanced Camera for Surveys
Short Name:
HST.ACS
Date:
23 Jul 2020 19:47:47
Publisher:
Space Telescope Science Institute Archive
Description:
HST Advanced Camera for Surveys (ACS) - Images: CCD images between 3,700 - 11
3. Deep Imaging of 47 Tuc Catalog ConeSearch
ID:
ivo://archive.stsci.edu/catalogs/HLSP_47TUC
Title:
Deep Imaging of 47 Tuc Catalog ConeSearch
Short Name:
47 TUC CS
Date:
23 Jul 2020 20:41:29
Publisher:
Space Telescope Science Institute Archive
Description:
Kalirai et al. have observed the globular cluster 47 Tucanae for 121 orbits using the Advanced Camera for Surveys. These extremely deep images were taken in two filters: F606W (broad V-band) and F814W (I-band). Using these observations, Kalirai et al. were able to construct one of the deepest and most complete color-magnitude diagrams of a stellar population, probing down to 30th magnitude and extending from the faintest end of the main sequence to the coolest white dwarf members. As an added bonus, members of the Small Magellanic Cloud represent background sources, and these observations are able to resolve SMC targets down to 0.2 solar masses. The team have released their stacked ACS mosaics (FITS files), source catalog (ASCII text table), and artificial source lists (ASCII text table) used for testing photometry, astrometry, and completeness, as High Level Science Products. We summarize the creation of the stacked images and generation of the catalogs below, but refer you to the original publication for complete details. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
4. 30 Doradus Catalog ConeSearch
ID:
ivo://archive.stsci.edu/catalogs/HLSP_30DOR
Title:
30 Doradus Catalog ConeSearch
Short Name:
30 DOR CS
Date:
23 Jul 2020 20:40:48
Publisher:
Space Telescope Science Institute Archive
Description:
30 Doradus (a.k.a. the Tarantula Nebula), with its ionizing cluster R136, is one of the few known starbursts in the Local Group. For size (~200 pc in diameter) and density of OB stars, 30 Doradus parallels the regions of intense star formation observed in the starburst knots found in the interacting galaxies in the Local Universe and the young galaxies at high redshift (z>5). HTTP is a panchromatic imaging survey of stellar populations in the Tarantula Nebula in the Large Magellanic Cloud that reaches into the sub-solar mass regime. HTTP utilizes the capability of the Hubble Space Telescope to operate the Advanced Camera for Surveys and the Wide Field Camera 3 in parallel to study this remarkable region in the near-ultraviolet, optical, and near-infrared spectral regions, including narrow-band Hα images. The high sensitivity, spatial resolution and broadband coverage of HTTP allow us to dissect the stellar populations and infer an accurate description of the anatomy of the Tarantula Nebula, and therefore to reconstruct for the first time the temporal and spatial evolution of a prototypical starburst on a sub-parsec scale. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
5. Faint Object Camera
ID:
ivo://archive.stsci.edu/hst/foc
Title:
Faint Object Camera
Short Name:
HST.FOC
Date:
23 Jul 2020 19:48:27
Publisher:
Space Telescope Science Institute Archive
Description:
The Faint Object Camera (FOC) was one of the 4 original axial instruments on the Hubble Space Telescope (HST). FOC is used to make high-resolution observations of faint sources at UV and visible wavel
6. Faint Object Spectrograph
ID:
ivo://archive.stsci.edu/hst/fos
Title:
Faint Object Spectrograph
Short Name:
HST.FOS
Date:
23 Jul 2020 19:48:53
Publisher:
Space Telescope Science Institute Archive
Description:
The Faint Object Spectrograph (FOS) was one of the 4 original axial instruments aboard the Hubble Space Telescope (HST). The FOS was designed to make spectroscopic observations of astrophysical sources from the near ultraviolet to the near infrared (1150 - 8000 Angstroms). The instrument was removed from HST during the Second Servicing Mission in February 1997.
7. F175W and F275W photometry of M31 and M32
ID:
ivo://CDS.VizieR/J/ApJ/504/113
Title:
F175W and F275W photometry of M31 and M32
Short Name:
J/ApJ/504/113
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present Faint Object Camera (FOC) ultraviolet images of the central 14"x14" of Messier 31 and Messier 32. The hot stellar populations detected in the composite UV spectra of these nearby galaxies are partially resolved into individual stars, and their individual colors and apparent magnitudes are measured. We detect 433 stars in M31 and 138 stars in M32, down to detection limits m_F275W_=25.5mag and m_F175W_=24.5mag.
8. Galaxies in the Hubble Deep Field
ID:
ivo://CDS.VizieR/J/AJ/112/359
Title:
Galaxies in the Hubble Deep Field
Short Name:
J/AJ/112/359
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present a catalog of morphological and color data for galaxies with 21<I_814<25mag in the Hubble Deep Field (Williams et al. 1996, in Science with the Hubble Space Telescope II). Galaxies have been inspected and (when possible) independently visually classified on the MDS and DDO systems. Measurements of central concentration and asymmetry are also included in the catalog. The fraction of interacting and merging objects is seen to be significantly higher in the Hubble Deep Field than it is among nearby galaxies. Barred spirals are essentially absent from the deep sample. The fraction of early-type galaxies in the Hubble Deep Field is similar to the fraction of early-types in the Shapley-Ames Catalog, but the fraction of galaxies resembling archetypal grand-design late-type spiral galaxies is dramatically lower in the distant HDF sample.
9. Goddard High Resolution Spectrograph
ID:
ivo://archive.stsci.edu/hst/ghrs
Title:
Goddard High Resolution Spectrograph
Short Name:
HST.GHRS
Date:
23 Jul 2020 19:49:16
Publisher:
Space Telescope Science Institute Archive
Description:
GHRS was used to make finely detailed spectroscopic observations of ultraviolet sources, but was removed from HST in February 1997.
10. GOODS Morphological Catalog
ID:
ivo://CDS.VizieR/VII/246
Title:
GOODS Morphological Catalog
Short Name:
VII/246
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present below the morphological catalogs of galaxies in the GOODS North and South fields, as determined visually by R. S. Ellis with a magnitude limit from HST/ACS imaging of z<22.5 (AB).