Optically selected rest-frame UV-bright galaxies are a key component of the zvirgul1.5-3 high redshift galaxy population. No understanding of the evolution of cosmic star formation or mass assembly can be obtained without them. Initial Herschel results find a discrepancy between their total infrared luminosity as estimated by extrapolation from the mid-IR and the directly measured rest-frame far-infrared, suggesting changed SEDs compared to local objects of similar luminosity. Because high fidelity individual Herschel SEDs cannot be obtained for the typical UV-bright galaxy from blank field surveys, we here describe a project to obtain full PACS/SPIRE SEDs for a sample of 16 strongly lensed UV-bright objects, found behind massive lensing clusters as well as behind individual lensing SDSS galaxies.
Publication
The spectral energy distribution of galaxies at z > 2.5: Implications from the Herschel/SPIRE color-color diagram | Yuan Fangting et al. | Astronomy & Astrophysics Volume 582 id.A90 16 pp. | 582 | 10.1051\\/0004-6361\\/201425497 | 2015A&A...582A..90Y | http://adsabs.harvard.edu/abs/2015A%26A...582A..90Y
Validation of the Equilibrium Model for Galaxy Evolution to z virgul 3 through Molecular Gas and Dust Observations of Lensed Star-forming Galaxies | Saintonge Amelie et al. | The Astrophysical Journal Volume 778 Issue 1 article id. 2 25 pp. (2013). | 778 | 10.1088\\/0004-637X\\/778\\/1\\/2 | 2013ApJ...778....2S | http://adsabs.harvard.edu/abs/2013ApJ...778....2S
Herschel Extreme Lensing Line Observations: CII Variations in Galaxies at Redshifts z=1-3 | Malhotra Sangeeta et al. | The Astrophysical Journal Volume 835 Issue 1 article id. 110 9 pp. (2017). | 835 | 10.3847\\/1538-4357\\/835\\/1\\/110 | 2017ApJ...835..110M | http://adsabs.harvard.edu/abs/2017ApJ...835..110M
Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0 < z < 4 | Schreiber C. et al. | Astronomy & Astrophysics Volume 609 id.A30 25 pp. | 609 | 10.1051\\/0004-6361\\/201731506 | 2018A&A...609A..30S | http://adsabs.harvard.edu/abs/2018A%26A...609A..30S
The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue | Bongiovanni Angel et al. | Astronomy and Astrophysics | null | null | 2019A&A...631A...9B |
Instrument
PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage
2010-07-11T15:12:15Z/2011-10-10T21:45:25Z
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.
European Space Agency, lutz et al., 2012, 'SEDs and energetics of lensed UV-bright high redshift galaxies', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-jdodr3j
