A dataset provided by the European Space Agency

Name OT2_aleroy_2
Title Imaging a Complete Sample of Equatorial, Star-Forming Galaxies: the Foundation for the Next Generation of Star Formation and ISM Studies


DOI https://doi.org/10.5270/esa-7elvp94
Author leroy, a.
Description We propose imaging with PACS (70+160 mciron) and SPIRE to ensure full resolved far-infrared (FIR) spectral energy distribution (SED) coverage of a complete equatorial sample of star-forming galaxies. This sample consists of every equatorial, face-on, star-forming galaxy of large angular extent and luminosity larger than M33. Because of their accessibility to all major facilities, particularly ALMA and the EVLA, these are the natural targets of the next generation of local galaxy studies. Herschel data are critical to estimate star formation rates, dust masses, and energetics in these galaxies and no comparable coverage of the IR SED will be possible in the foreseeable future. Without our proposed program only 13 of the 67 galaxies in this key sample will have high resolution data that span the IR peak, hindering studies of the life cycle of dust, dependence of star formation on host galaxy and local conditions, and development of robust calibrations of star formation rate tracers and the CO-to-H _2 conversion factor. Observations of this sample therefore would represent a key part of Herschel.s legacy and significantly enhance the nearby galaxy science from the next generations of northern and southern telescopes. In order to ensure maximal yield from both Herschel and ALMA-EVLA, we commit to waive our proprietary period and rapidly release our reduced data products.
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 ,
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 ,
Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample . Trčka Ana et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2020MNRAS.494.2823T ,
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 . Davies J. I. et al. . Astronomy and Astrophysics . null . null . 2019A&A...626A..63D ,
Old and young stellar populations in DustPedia galaxies and their role in dust heating . Nersesian A. et al. . Astronomy and Astrophysics . null . null . 2019A&A...624A..80N ,
UV to submillimetre luminosity functions of TNG50 galaxies . Trčka Ana et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2022MNRAS.516.3728T ,
Local Swift-BAT active galactic nuclei prefer circumnuclear star formation . Lutz D. et al. ...
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2013-02-21T08:39:00Z/2013-02-21T09:08:00Z
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 2013-02-21T08:54:03Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, OT2_aleroy_2, SPG v14.2.0. https://doi.org/10.5270/esa-7elvp94