Subject: galaxies / Facility: HST / Capability Type: Simple Cone Search

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

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

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.

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.

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.

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.

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).

ID:: ivo://CDS.VizieR/J/A+A/364/517
Title:: HDF-N spiral and irregular galaxies
Short Name:: J/A+A/364/517
Date:: 21 Oct 2021
Publisher:: CDS
Description:: We analyze a morphologically-selected complete sample of 52 late-type (spiral and irregular) galaxies in the Hubble Deep Field North with total K-magnitudes brighter than K=20.47 and typical redshifts z~0.5 to 1.4. This sample exploits in particular the ultimate imaging quality achieved by HST in this field, allowing us to clearly disentangle the early- from late-type galaxy morphologies, based on accurate profiles of the surface brightness distributions.

ID:: ivo://CDS.VizieR/J/ApJ/513/34
Title:: HDF photometric redshifts catalog
Short Name:: J/ApJ/513/34
Date:: 21 Oct 2021
Publisher:: CDS
Description:: Using the newly available infrared images of the Hubble Deep Field in the J, H, and K bands and an optimal photometric method, we have refined a technique to estimate the redshifts of 1067 galaxies. A detailed comparison of our results with the spectroscopic redshifts in those cases where the latter are available shows that this technique gives very good results for bright enough objects [AB(814nm)<26.0]. From a study of the distribution of residuals [{Delta}z_rms_/(1+z)~0.1 at all redshifts], we conclude that the observed errors are mainly due to cosmic variance. This very important result allows for the assessment of errors in quantities to be directly or indirectly measured from the catalog. We present some of the statistical properties of the ensemble of galaxies in the catalog, and we finish by presenting a list of bright high-redshift (z~5) candidates extracted from our catalog together with recent spectroscopic redshift determinations confirming that two of them are at z=5.34 and z=5.60.

ID:: ivo://CDS.VizieR/J/A+AS/145/111
Title:: HDF-South catalogue of galaxies
Short Name:: J/A+AS/145/111
Date:: 21 Oct 2021
Publisher:: CDS
Description:: We present a catalogue of galaxies in the HDF-S, created using the public version 1 images of the WFPC2 data. We created a catalogue with 4 pass-band (I(814), V(606), B(450), U(300). In V(606), B(450), U(300) and I(814), for each galaxy the catalogue gives photometric parameters. For the I(814), we estimated also the colours and for I(814)<26, the petrosian radius, the mean surface brightness within the petrosian radius, light concentration indexes, that is C_eta_ and C_abr_, and the asymmetry index as computed by Abraham software.

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