Gaseous galaxy halos
Galactic halo gas traces inflowing star-formation fuel and feedback from a galaxy's disk and
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …
The Hi Distribution of the Milky Way
PMW Kalberla, J Kerp - Annual review of astronomy and …, 2009 - annualreviews.org
Neutral atomic hydrogen (Hi) traces the interstellar medium (ISM) over a broad range of
physical conditions. Its 21-cm emission line is a key probe of the structure and dynamics of …
physical conditions. Its 21-cm emission line is a key probe of the structure and dynamics of …
HI4PI: a full-sky H i survey based on EBHIS and GASS
Context. Measurement of the Galactic neutral atomic hydrogen (H i) column density, NH i,
and brightness temperatures, TB, is of high scientific value for a broad range of astrophysical …
and brightness temperatures, TB, is of high scientific value for a broad range of astrophysical …
[PDF][PDF] HI4PI: A full-sky HI survey based on EBHIS and GASS
N Ben Bekhti, L Flöer, R Keller, DJ Pisano - 2016 - researchrepository.wvu.edu
ABSTRACT Context. Measurement of the Galactic neutral atomic hydrogen (H i) column
density, NH i, and brightness temperatures, TB, is of high scientific value for a broad range of …
density, NH i, and brightness temperatures, TB, is of high scientific value for a broad range of …
WALLABY – an SKA Pathfinder H i survey
Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
Eight ultra-faint galaxy candidates discovered in year two of the dark energy survey
A Drlica-Wagner, K Bechtol, ES Rykoff… - The Astrophysical …, 2015 - iopscience.iop.org
We report the discovery of eight new ultra-faint dwarf galaxy candidates in the second year
of optical imaging data from the Dark Energy Survey (DES). Six of these candidates are …
of optical imaging data from the Dark Energy Survey (DES). Six of these candidates are …
Planck 2015 results-X. Diffuse component separation: Foreground maps
R Adam, PAR Ade, N Aghanim, MIR Alves… - Astronomy & …, 2016 - aanda.org
Planck has mapped the microwave sky in temperature over nine frequency bands between
30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz …
30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz …
Planck 2013 results. XI. All-sky model of thermal dust emission
A Abergel, PAR Ade, N Aghanim, MIR Alves… - Astronomy & …, 2014 - aanda.org
This paper presents an all-sky model of dust emission from the Planck 353, 545, and 857
GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky …
GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky …
[PDF][PDF] Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
PAR Ade, N Aghanim - A&A, 2014 - research.aalto.fi
We present new measurements of cosmic infrared background (CIB) anisotropies using
Planck. Combining HFI data with IRAS, the angular auto-and cross-frequency power …
Planck. Combining HFI data with IRAS, the angular auto-and cross-frequency power …
The VMC survey-I. Strategy and first data
MRL Cioni, G Clementini, L Girardi… - Astronomy & …, 2011 - aanda.org
Context. The new VISual and Infrared Telescope for Astronomy (VISTA) has started
operations. Over its first five years it will be collecting data for six public surveys, one of …
operations. Over its first five years it will be collecting data for six public surveys, one of …