Results 71 to 80 of about 405,217 (280)
FIGS -- Faint Infrared Grism Survey: Description and Data Reduction [PDF]
The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR (Wide Field Camera 3 Infrared) slitless spectroscopic survey of four deep fields.
Christensen, Lise +28 more
core +4 more sources
WSRT Observations of the Hubble Deep Field Region
We present deep WSRT 1.4 GHz observations of the Hubble Deep Field region. At the 5 sigma level, the WSRT clearly detects 85 regions of radio emission in a 10' x 10' field centred on the HDF. Eight of these regions fall within the HDF itself, four of these are sources that have not previously been detected at 1.4 GHz, although two of these are VLA ...
Garrett, MA +4 more
openaire +3 more sources
CLEAR: Survey Overview, Data Analysis, and Products
We present an overview of the CANDELS Ly α Emission At Reionization (CLEAR) survey. CLEAR is a 130 orbit program of the Hubble Space Telescope using the Wide Field Camera 3 (WFC3) IR G102 grism.
Raymond C. Simons +21 more
doaj +1 more source
Detectability of High Redshift Ellipticals in the Hubble Deep Field [PDF]
Relatively few intensively star-forming galaxies at redshifts z>2.5 have been found in the Hubble Deep Field (HDF). This has been interpreted to imply a low space density of elliptical galaxies at high z, possibly due to a late (z4.5, and were fading ...
Dan Maoz +3 more
core +3 more sources
Radio Observations of the Hubble Deep Field-South Region. II. The 1.4 GHz Catalog and Source Counts [PDF]
This paper is part of a series describing the results from the Australia Telescope Hubble Deep Field–South (ATHDFS) survey obtained with the Australia Telescope Compact Array.
M. Huynh +3 more
semanticscholar +1 more source
ABSTRACT On‐orbit rendezvous and docking constitute one of the most technically challenging activities in the history of space activities. As space endeavours mature to crewed missions, space rendezous and docking technologies (RDT) emerge as an area of technological innovation critical to advances in future crewed space exploration.
Nikita Chiu, Markus Kornprobst
wiley +1 more source
The MUSE Hubble Ultra Deep Field Survey
Star-forming galaxies have been found to follow a relatively tight relation between stellar mass ( M * ) and star formation rate (SFR), dubbed the “star formation sequence”. A turnover in the sequence has been observed, where galaxies with M * < 10 10 M ⊙ follow a steeper relation than their higher mass counterparts, suggesting that the low-mass
Boogaard, Leindert A +18 more
openaire +3 more sources
The Visibility of Galactic Bars and Spiral Structure At High Redshifts [PDF]
We investigate the visibility of galactic bars and spiral structure in the distant Universe by artificially redshifting 101 B-band CCD images of local spiral galaxies from the Ohio State University Bright Spiral Galaxy Survey. Our artificially redshifted
Abraham R. G. +9 more
core +2 more sources
Sampling the volcanic plumes at Io: Impact speeds and shock conditions
Abstract The desire to sample material from the interior of Io, by flying through its volcanic plumes, requires consideration of the flyby speed and the types of sample collection techniques that can be utilized. Low speed collection (1–2.5 km s−1) would require an orbit around Io itself, which is unlikely due to the accumulated radiation dose that ...
M. J. Burchell +2 more
wiley +1 more source
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey
The Hubble Ultra Deep Field Survey has not only provided the deepest optical and near infrared views of universe, but has enabled a search for the most distant supernovae to z~2.2.
Abdul-Aziz H. +5 more
core +2 more sources

