A dataset provided by the European Space Agency

Name OT2_emurph01_3
Title The Herschel EDGE−on galaxy Survey (HEDGES)
URL

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DOI https://doi.org/10.5270/esa-76jwv9m
Author murphy, e.
Description We propose deep PACS and SPIRE imaging for all (6) normal, edge-on (i >85 deg) galaxies with d<10Mpc as part of the Herschel EDGEon galaxy Survey (HEDGES). These data will allow us, for the first time, to characterize variations in the far-infrared (FIR) spectral energy distribution (SED) among and within halos for an energetically diverse sample of nearby, edge-on galaxies as a function of height above the disk. The proper sampling of the halo dust SEDs (i.e., 6 bands between 70500um), will allow us to take inventory of the dust content of halos and illuminate the signatures of dust processing imprinted in the dust SED and its variations. These observations will provide a way to address a number of outstanding questions related to the processes governing the interchange of disk/halo material such as: (1) How does halo dust content relate to disk star formation activity? (2) What are the physical characteristics of halo dust (i.e., temperature(s), mass, emissivity, PAH mass fraction, and what does their variation with height from the plane tell us about grain modification by the energetic processes responsible for disk-halo cycling? (3) What can dust and radio continuum halos tell us about transport effects that are important for understanding the FIR-Radio correlation? (4) How does the distribution of halo dust compare to that of other gas tracers, and hence what can we learn about how such dust is associated with various gas phases? The HEDGES sample galaxies have a treasury of ancillary data (e.g., radio, Spitzer, optical, gas), and the addition of these deep Herschel data will make HEDGES the definitive sample to study multi-phase disk/halo feedback processes arising from the accretion, expulsion, and/or cycling of material between disks and halos into the foreseeable future.
Publication Investigating the growing population of massive quiescent galaxies at cosmic noon . Sherman Sydney et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2020MNRAS.499.4239S ,
DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands . Clark C. J. R. et al. . Astronomy & Astrophysics, Volume 609, id.A37, 30 pp. . 609 . 10.1051\/0004-6361\/201731419 . 2018A&A...609A..37C ,
Probing the spectral shape of dust emission with the DustPedia galaxy sample . Nersesian Angelos et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2021MNRAS.506.3986N ,
HCN 3-2 survey towards a sample of local galaxies . Li Fei et al. . Publications of the Astronomical Society of Japan . null . null . 2020PASJ...72...41L ,
Dense Gas and Star Formation in Nearby Infrared-bright Galaxies: APEX Survey of HCN and HCO+ J = 2 → 1 . Zhou Jing et al. . The Astrophysical Journal . null . null . 2022ApJ...936...58Z ,
A nearby galaxy perspective on dust evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples . Galliano Frédéric et al. . Astronomy and Astrophysics . null . null . 2021A&A...649A..18G ,
The distribution of dust in edge-on galaxies: I. The global structure . Mosenkov Aleksandr V. et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2022MNRAS.515.5698M ,
Dust emissivity and absorption cross section in DustPedia late-type galaxies . Bianchi S. et al. . Astronomy and Astrophysics . null . null . 2019A&A...631A.102B ,
DustPedia: the relationships between stars, gas, and dust for galaxies residing in different environments . ...
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_large
Temporal Coverage 2012-11-28T00:10:04Z/2013-01-22T15:45:53Z
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 2013-07-22T13:56:43Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, murphy, e., 2013, OT2_emurph01_3, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-76jwv9m