2016MNRAS.458.1977F

Query : 2016MNRAS.458.1977F

2016MNRAS.458.1977F - Mon. Not. R. Astron. Soc., 458, 1977-1989 (2016/May-2)

The data processing pipeline for the Herschel SPIRE Fourier Transform Spectrometer.

FULTON T., NAYLOR D.A., POLEHAMPTON E.T., VALTCHANOV I., HOPWOOD R., LU N., BALUTEAU J.-P., MAINETTI G., PEARSON C., PAPAGEORGIOU A., GUEST S., ZHANG L., IMHOF P., SWINYARD B.M., GRIFFIN M.J. and LIM T.L.

Abstract (from CDS):

We present the data processing pipeline to generate calibrated data products from the Spectral and Photometric Imaging Receiver (SPIRE) imaging Fourier Transform Spectrometer on the Herschel Space Observatory. The pipeline processes telemetry from SPIRE observations and produces calibrated spectra for all resolution modes. The spectrometer pipeline shares some elements with the SPIRE photometer pipeline, including the conversion of telemetry packets into data timelines and calculation of bolometer voltages. We present the following fundamental processing steps unique to the spectrometer: temporal and spatial interpolation of the scan mechanism and detector data to create interferograms; Fourier transformation; apodization; and creation of a data cube. We also describe the corrections for various instrumental effects including first- and second-level glitch identification and removal, correction of the effects due to emission from the Herschel telescope and from within the spectrometer instrument, interferogram baseline correction, temporal and spatial phase correction, non-linear response of the bolometers, and variation of instrument performance across the focal plane arrays. Astronomical calibration is based on combinations of observations of standard astronomical sources and regions of space known to contain minimal emission.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: data analysis - space vehicles: instruments - techniques: spectroscopic

CDS comments: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 IRAS 16293-2422 cor 16 32 22.56 -24 28 31.8           ~ 1357 1

Query : 2016MNRAS.458.1977F

Basic data :
IRAS 16293-2422 -- Dense Core
Other object types: otypes_help 		smm (2008ApJ,JCMTLSG,...), IR (2013ApJS,HGBS,...), MIR (SSTc2d,WISEA,...), Y*O (2015MNRAS,[EES2009]), Y*? (2015ApJS,[HL2013]), mm (2009ApJ,[YEE2006]), cor (2020A&A), PoC ([FST86])
ICRS coord. (ep=J2000) : 		16 32 22.56 -24 28 31.8 (Infrared) [ 300 300 90 ] C 2009ApJ...692..973E
FK4 coord. (ep=B1950 eq=1950) : 		16 29 20.71 -24 22 11.7 [ 300 300 90 ]
Gal coord. (ep=J2000) : 		353.93571 +15.84097 [ 300 300 90 ]
Angular size (arcmin): 		0.35 0.13 136 (FIR) C 2020A&A...638A..74L
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
: 2 		: 2355 Display criteria :

Identifiers (18) :
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HGBS J163223.1-242836 NAME IRAS 16293 WISE J163222.62-242833.6 [JJK2008] SMM J163223-24284
IRAS 16293-2422 NAME rho Oph East [EDJ2009] 1008 [NWA2006] SMM 20
JCMTLSG J163222.6-242833 SSTc2d J163222.6-242832 [EES2009] Oph-emb 2 [YEE2006] 37
JCMTSE J163222.8-242837 SSTc2d J163222.6-242831 [FST86] rho Oph E
JCMTSF J163222.8-242837 WISEA J163222.60-242833.6 [HL2013] 248.09427-24.47550

References (1357 between 1850 and 2026) (Total 1357)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Observing logs

Herschel : 27    ISO : 23   

   

External archives :

Data at NED - NASA/IPAC Extragalactic Database : IRAS 16293-2422

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IRAS 16293-2422 WISEA J163222.60-242833.6 WISE J163222.62-242833.6

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