The Evolution of the Global Star Formation History as Measured from the Hubble Deep Field [PDF]
, 1997 The Hubble Deep Field (HDF) is the deepest set of multicolor optical photometric observations ever undertaken, and it offers a valuable data set with which to study galaxy evolution.
A. Connolly +6 more
semanticscholar +1 more source
Submillimetre observations of the Hubble Deep Field and Flanking Fields [PDF]
Monthly Notices of the Royal Astronomical Society, 2003 MNRAS in press; minor revisions. 23 pages, 13 figures. Uses BoxedEPS and mn2e.cls (included).
Serjeant, S +13 more
openaire +3 more sources
On the Reionization-era Globular Cluster in the Low-mass Galaxy Eridanus II
The Astrophysical Journal, 2023 Using color–magnitude diagrams from deep archival Hubble Space Telescope imaging, we self-consistently measure the star formation history of Eridanus II (Eri II ), the lowest-mass galaxy ( M _⋆ ( z = 0) ∼ 10 ^5 M _⊙ ) known to host a globular cluster (GC)
Daniel R. Weisz +2 more
doaj +1 more source
Galaxy morphology to I = 25 mag in the Hubble Deep Field [PDF]
, 1996 The morphological properties of galaxies in the range 21 < I < 25 mag in the Hubble Deep Field are investigated using a quantitative classification system based on measurements of the central concentration and asymmetry of galaxian light.
Roberto G. Abraham +5 more
semanticscholar +1 more source
The Astrophysical Journal Letters, 2023 We present the ultraviolet luminosity function and an estimate of the cosmic star formation rate density at 8 < z < 13 derived from deep NIRCam observations taken in parallel with the MIRI Deep Survey of the Hubble Ultra Deep Field (HUDF), NIRCam ...
Pablo G. Pérez-González +43 more
doaj +1 more source
High-z Lyα Emitters. I. A Blank-Field Search for Objects near Redshift z = 3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA 22 [PDF]
, 1998 We present deep narrowband (λ = 5390 Å, Δλ = 77 Å) and multicolor observations of the Hubble Deep Field and the Hawaii Deep Field SSA 22 obtained with the LRIS instrument at the 10 m Keck II Telescope.
L. Cowie, E. Hu
semanticscholar +1 more source
Observations of the Hubble Deep Field with the Infrared Space Observatory V. Spectral energy distributions starburst models and star formation history [PDF]
, 1997 We have modelled the spectral energy distributions of the 13 Hubble Deep Field (HDF) galaxies reliably detected by the Infrared Space Observatoiy (ISO).
The ISO-HDF Consortium Michael Rowan-Robinson et al
semanticscholar +1 more source
Variable Galaxies in the Hubble Deep Field [PDF]
The Astronomical Journal, 2000 31 pages, 8 figures, accepted to the ...
Sarajedini, V. L. +2 more
openaire +2 more sources
Accelerated Structural Evolution of Galaxies in a Starbursting Cluster at z = 2.51
The Astrophysical Journal Letters, 2023 Structural properties of cluster galaxies during their peak formation epoch, z ∼ 2–4 provide key information on whether and how the environment affects galaxy formation and evolution.
Can Xu +13 more
doaj +1 more source
The Multiwavelength Survey by Yale-Chile (MUSYC): Survey Design and Deep Public UBVRIz' Images and Catalogs of the Extended Hubble Deep Field-South [PDF]
, 2005 We present UBVRIz' optical images taken with MOSAIC on the CTIO 4 m telescope of the 0.32 deg2 Extended Hubble Deep Field-South. This is one of four fields comprising the MUSYC survey, which is optimized for the study of galaxies at z = 3, active ...
E. Gawiser +29 more
semanticscholar +1 more source