A dataset provided by the European Space Agency

Name OT1_schapman_1
Title Measuring the PAH emission in a z=6.1 star forming Submillimetre Galaxy
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342262049&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342262050&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-4dzuu1s
Author chapman, s.
Description We have discovered a z=6.1 Submillimetre Galaxy from a detailedsurvey of 0.5 sq deg in GOODS-N, FLS, and LockmanEast. HDF259 was originally detected by SCUBA and the VLA, but recentlyconstrained through Herschel-SPIRE detections.The redshift is confirmed through a Keck spectroscopic redshift,an optical-near/mid-IR photo-z (as an I-band dropout with a rising stellar bump at 1.6um),and through template fitting with a most likely T_dustin the SPIRE through 1.2mm wavelengths.Even if the optical data incorrect redshift, an extreme rangeof T_dust secures the redshift as lying from z=4-8.This SMG represents the first opportunity yet to study the rest-frame7.7um region PAH features in a z>6 star forming galaxy,using the PACS spectrometer (where the 7.7um strong PAH featurecomes into the PACS 51-70um and 70-105um bands only at z>5.9).The strength of the PAH, estimated both from extrapolated flux measurements from Spitzer-MIPS, and from the z~2 L_IR-L_PAHrelation (Pope et al. 2008) ensures that a typical PAH in this SMGwill be well detected in 4.8hrs total programme duration.
Publication
    Instrument PACS_PacsRangeSpec_point
    Temporal Coverage 2013-01-26T12:18:40Z/2013-01-26T17:01:25Z
    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 2013-07-26T14:41:07Z
    Last Update 2026-03-02
    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, chapman et al., 2013, 'Measuring the PAH emission in a z=6.1 star forming Submillimetre Galaxy', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-4dzuu1s