A dataset provided by the European Space Agency

Name GT1_aconturs_1
Title CII , OI and far infrared continuum emission properties of local Lyman Break Analogs
URL

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DOI https://doi.org/10.5270/esa-p5xizrm
Author contursi, a.
Description CII , OI and far infrared continuum emission properties of local Lyman Break Analogs We propose to observe 9 Ultra Compact UV-luminous galaxies, selected from Overzier et al (2009) with the PACS spectrometer in the CII and OI lines at 158 micron and 63 micron, and with the PACS photometer in the green and red filters.These galaxies are at redshifts ~0.2-0.3, they are rare in the nearby Universe and they were chosen because they are analogs of theLyman Break Galaxies (LBGs), (Heckman et al 2005). For this reason, they have been called: Local Break Analogs (LBAs). LBAs and LBGs share many global properties such as, stellar mass, metallicity, dust extinction, star sormation rate (SFR), physical size and gas velocity dispersion.Despite they have been observed with SPITZER at 24 and 70 micron, no systematic and detailed studies of their infrared properties has been done so far.We want to characterize the far infrared (FIR) properties of these galaxies. The porposed CII and OI observations together with ancillary CO data will allow us to study the physics of the ISM and its interplay with the heating sources. Given the similarity between LBAs and LBGs, these results will shed light also for the LBGs population, helping their further characterization. We will also verify if LBAs, and by analogy also LBGs, are CII deficient or not. In the case LBAs are not CII deficient, we will empirically calibrate the CII emission as a SFR indicator. The SFR will be calculated from the FIR emission measured with PACS, assuming that in such UV bright sources most of the FIR is produced by young stars. Thus, this data set will provide an unique local reference sample for the future infaredobservations of high redshift UV-bright galaxies with ALMA.
Publication
Instrument PACS_PacsPhoto_largeScan, PACS_PacsRangeSpec_point, PACS_PacsLineSpec_point
Temporal Coverage 2010-11-14T23:56:32Z/2011-07-09T19:42:42Z
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 2012-01-09T00:00:00Z
Last Update 2026-07-09
Keywords Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, contursi et al., 2012, '[CII] , [OI] and far infrared continuum emission properties of local Lyman Break Analogs', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-p5xizrm
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.