Search Publications

The Herschel-PACS photometer calibration. Point-source flux calibration for scan maps
DOI: 10.1007/s10686-013-9352-3 Bibcode: 2014ExA....37..129B

Moór, Attila; Sauvage, Marc; Okumura, Koryo +9 more

This paper provides an overview of the PACS photometer flux calibration concept, in particular for the principal observation mode, the scan map. The absolute flux calibration is tied to the photospheric models of five fiducial stellar standards ( α Boo, α Cet, α Tau, β And, γ Dra). The data processing steps to arrive at a consistent and homogeneou…

2014 Experimental Astronomy
Herschel 156
Herschel celestial calibration sources. Four large main-belt asteroids as prime flux calibrators for the far-IR/sub-mm range
DOI: 10.1007/s10686-013-9357-y Bibcode: 2014ExA....37..253M

Pearson, Chris; Lim, Tanya; Linz, Hendrik +9 more

Celestial standards play a major role in observational astrophysics. They are needed to characterise the performance of instruments and are paramount for photometric calibration. During the Herschel Calibration Asteroid Preparatory Programme approximately 50 asteroids have been established as far-IR/sub-mm/mm calibrators for Herschel. The selected…

2014 Experimental Astronomy
Herschel 32
The pointing system of the Herschel space observatory. Description, Calibration, Performance and improvements
DOI: 10.1007/s10686-014-9396-z Bibcode: 2014ExA....37..453S

Marston, Anthony; Linz, Hendrik; Merín, Bruno +13 more

We present the activities carried out to calibrate and characterise the performance of the elements of attitude control and measurement on board the Herschel spacecraft. The main calibration parameters and the evolution of the indicators of the pointing performance are described, from the initial values derived from the observations carried out in…

2014 Experimental Astronomy
Herschel 31
SPIRE point source photometry: within the Herschel interactive processing environment (HIPE)
DOI: 10.1007/s10686-013-9351-4 Bibcode: 2014ExA....37..175P

Griffin, Matt; Pearson, Chris; Lim, Tanya +11 more

The different algorithms appropriate for point source photometry on data from the SPIRE instrument on-board the Herschel Space Observatory, within the Herschel Interactive Processing Environment (HIPE) are compared. Point source photometry of a large ensemble of standard calibration stars and dark sky observations is carried out using the 4 major …

2014 Experimental Astronomy
Herschel 27
Optimized Herschel/PACS photometer observing and data reduction strategies for moving solar system targets
DOI: 10.1007/s10686-013-9350-5 Bibcode: 2014ExA....37..161K

Hartogh, P.; Pál, A.; Lellouch, E. +10 more

The "TNOs are Cool!: A survey of the trans-Neptunian region" is a Herschel Open Time Key Program that aims to characterize planetary bodies at the outskirts of the Solar System using PACS and SPIRE data, mostly taken as scan-maps. In this paper we summarize our PACS data reduction scheme that uses a modified version of the standard pipeline for ba…

2014 Experimental Astronomy
Herschel 21
Herschel SPIRE FTS relative spectral response calibration
DOI: 10.1007/s10686-013-9364-z Bibcode: 2014ExA....37..381F

Valtchanov, Ivan; Hopwood, Rosalind; Lu, Nanyao +9 more

Herschel/SPIRE Fourier transform spectrometer (FTS) observations contain emission from both the Herschel Telescope and the SPIRE Instrument itself, both of which are typically orders of magnitude greater than the emission from the astronomical source, and must be removed in order to recover the source spectrum. The effects of the Herschel Telescop…

2014 Experimental Astronomy
Herschel 9
Herschel SPIRE FTS telescope model correction
DOI: 10.1007/s10686-013-9355-0 Bibcode: 2014ExA....37..195H

Valtchanov, Ivan; Hopwood, Rosalind; Lu, Nanyao +8 more

Emission from the Herschel telescope is the dominant source of radiation for the majority of SPIRE Fourier transform spectrometer (FTS) observations, despite the exceptionally low emissivity of the primary and secondary mirrors. Accurate modelling and removal of the telescope contribution is, therefore, an important and challenging aspect of FTS c…

2014 Experimental Astronomy
Herschel 7
Herschel SPIRE fourier transform spectrometer: calibration of its bright-source mode
DOI: 10.1007/s10686-013-9359-9 Bibcode: 2014ExA....37..239L

Valtchanov, Ivan; Hopwood, Rosalind; Naylor, David A. +10 more

The Fourier Transform Spectrometer (FTS) of the Spectral and Photometric Imaging REceiver (SPIRE) on board the ESA Herschel Space Observatory has two detector setting modes: (a) a nominal mode, which is optimized for observing moderately bright to faint astronomical targets, and (b) a bright-source mode recommended for sources significantly bright…

2014 Experimental Astronomy
Herschel 7
Relative pointing offset analysis of calibration targets with repeated observations with Herschel-SPIRE Fourier-transform spectrometer
DOI: 10.1007/s10686-013-9356-z Bibcode: 2014ExA....37..207V

Valtchanov, Ivan; Hopwood, Rosalind; Lu, Nanyao +9 more

We present a method to derive the relative pointing offsets for SPIRE Fourier-Transform Spectrometer (FTS) solar system object (SSO) calibration targets, which were observed regularly throughout the Herschel mission. We construct ratios R obs( ν) of the spectra for all observations of a given source with respect to a reference. The refe…

2014 Experimental Astronomy
Herschel 6
The effect of sideband ratio on line intensity for Herschel/HIFI
DOI: 10.1007/s10686-014-9382-5 Bibcode: 2014ExA....37..433H

Braine, Jonathan; Ossenkopf, Volker; Higgins, Ronan +8 more

The Heterodyne Instrument for the Far Infrared (HIFI) on board the Herschel Space Observatory is composed of a set of fourteen double sideband mixers. We discuss the general problem of the sideband ratio (SBR) determination and the impact of an imbalanced sideband ratio on the line calibration in double sideband heterodyne receivers. The HIFI SBR …

2014 Experimental Astronomy
Herschel 5