A dataset provided by the European Space Agency

Name OT1_smolinar_5
Title Hi-GAL360: the crucial step toward a global understanding of star formation in the Milky Way
URL

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DOI https://doi.org/10.5270/esa-bitplie
Author European Space Agency
Description Hi-GAL360 will use PACS and SPIRE in parallel mode to obtain a 5-band
photometric survey of the Outer Galactic Plane (OGP, beyond the solar
circle) in the longitude range complementary to the Hi-GAL Open Time
KP, i.e., 68 < l < 288 in a 2-wide strip in latitude following the
mid-plane of emission.

Hi-GAL360 data will enable a complete census of temperature, mass,
density, column density and luminosity of filaments, clumps, and cores
in the less confused outer Galaxy, where the assembly of filamentary
structures and clouds and their fragmentation into clumps
and cores can be uniquely characterised in low-metallicity and
HI-dominated environments that are so different with respect to the
inner Galaxy.

A complete OGP survey is required to obtain a statistically significant
sampling of Galactic diversity - the full range of spiral arm,
inter-arm, dust cloud, and star formation region properties - avoiding
biases introduced by the study of specific or limited regions.

Hi-GAL360, together with Hi-GAL, will chart the Star Formation Rate
and Efficiency from the Galactic Center to the far outer Galaxy, mapping
the location and properties of star formation thresholds, thus providing
the much needed connection between global scaling laws and the
diversity of physical processes at work in the Galaxy. It will lay the
foundations for a predictive, quantitative model of how star formation
is triggered and regulated on all scales in the Milky Way. Such a model
is vital to a full understanding of galaxy formation and evolution.

The merged Hi-GAL360/Hi-GAL .Atlas of the Galaxy. will provide
essential .ground truth. for the interpretation of Herschel data on
other galaxies from the Local Group to the high-redshift Universe
where these objects are blended, and it will be the Herschel leg...acy
that will remain unsurpassed for decades as the definitive
survey of far-IR emission from the Galaxy.

Given our demonstrated community-oriented approach, we again
waive our proprietary period.
Publication Multifractal analysis of the interstellar medium: first application to Hi-GAL observations . Elia Davide et al. . Monthly Notices of the Royal Astronomical Society, Volume 481, Issue 1, p.509-532 . 481 . 10.1093\/mnras\/sty2170 . 2018MNRAS.481..509E ,
The Hi-GAL compact source catalogue - II. The 360° catalogue of clump physical properties . Elia Davide et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2021MNRAS.504.2742E ,
A high dust emissivity index β for a CO-faint galaxy in a filamentary Lyα nebula at z = 3.1 . Kato Yuta et al. . Publications of the Astronomical Society of Japan, Volume 70, Issue 5, id.L6 . 70 . 10.1093\/pasj\/psy087 . 2018PASJ...70L...6K ,
A systematic study of Galactic infrared bubbles along the Galactic plane with AKARI and Herschel . Hanaoka Misaki et al. . Publications of the Astronomical Society of Japan, Volume 71, Issue 1, id.6 . 71 . 10.1093\/pasj\/psy126 . 2019PASJ...71....6H ,
First Extended Catalogue of Galactic bubble infrared fluxes from WISE and Herschel surveys . Bufano F. et al. . Monthly Notices of the Royal Astronomical Society, Volume 473, Issue 3, p.3671-3692 . 473 . 10.1093\/mnras\/stx2560 . 2018MNRAS.473.3671B ,
The First Hi-GAL Observations of the Outer Galaxy: A Look at Star Formation in the Third Galactic Quadrant in the Longitude Range 216.°5 <virgul l <virgul 225.°5 . Elia D. et al. . The Astrophysical Journal, Volume 772, Issue 1, article id. 45, 20 pp. (2013). . 772 . 10.1088\/0004-637X\/772\/1\/45 . 2013ApJ...772...45E ,
The Hi-GAL catalog...
Instrument SPIRE\/PACS parallel_SpirePacsParallel_
Temporal Coverage 2011-05-05T14:33:03Z/2013-03-01T06:53:25Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2013-03-01T04:03:36Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Hi-Gal360: The Crucial Step Toward A Global Understanding Of Star Formation In The Milky Way, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-bitplie