activity
20142026
most citedHerschel SPIRE FTS Relative Spectral Response Calibration

11 citations · 49 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

VAPOLA - A multiyear, multiband polarization survey of AGNs and Sgr A* at millimeter wavelengths with ALMA II. Spectropolarimetric properties and their evolution from 2017 to 2023

Douglas Carlos, Ciriaco Goddi, Alejandro Mus +5

We present a systematic analysis of the spectropolarimetric properties of a sample of 39 active galactic nuclei and Sagittarius A* observed with the Atacama Large Millimeter/submil…

astro-ph.GA2026

Dynamics and geometry of the inner sub-parsec-scale jet in 3C 279 observed with the Event Horizon Telescope

Hendrik Mueller, Sebastiano D. von Fellenberg, Ai-Ling Zeng +275

The 2021 Event Horizon Telescope observations resolve the innermost jet region of the blazar 3C279 with unprecedented detail. The reconstructed images consistently reveal a compact…

astro-ph.GA2026

VAPOLA -- A multi-year, multi-band polarization survey of AGN and Sgr A* at mm wavelengths with ALMA I. Survey Overview and Science-Ready Archival Products

Alejandro Mus, Ciriaco Goddi, Douglas Carlos +13

The Atacama Large Millimeter/submillimeter Array (ALMA) is the most sensitive interferometric array at millimeter and submillimeter wavelengths. Through the ALMA Phasing System (AP…

astro-ph.IM2020★ 4 cited

The Herschel SPIRE Fourier Transform Spectrometer Spectral Feature Finder I. The Spectral Feature Finder and Catalogue

R. Hopwood, I. Valtchanov, Locke D. Spencer +11

We provide a detailed description of the Herschel-SPIRE Fourier Transform Spectrometer (FTS) Spectral Feature Finder (FF). The FF is an automated process designed to extract signif…

astro-ph.IM2017★ 7 cited

Correcting the extended-source calibration for the Herschel-SPIRE Fourier-Transform Spectrometer

Ivan Valtchanov, R. Hopwood, G. Bendo +20

We describe an update to the Herschel-SPIRE Fourier-Transform Spectrometer (FTS) calibration for extended sources, which incorporates a correction for the frequency-dependent far-f…

astro-ph.IM2016★ 3 cited

Calibration of Herschel SPIRE FTS observations at different spectral resolutions

N. Marchili, R. Hopwood, T. Fulton +11

The SPIRE Fourier Transform Spectrometer on board the Herschel Space Observatory had two standard spectral resolution modes for science observations: high resolution (HR) and low r…

astro-ph.IM2014★ 11 cited

Herschel SPIRE FTS Relative Spectral Response Calibration

Trevor Fulton, Rosalind Hopwood, Jean-Paul Baluteau +9

Herschel/SPIRE Fourier transform spectrometer (FTS) observations contain emission from both the Herschel Telescope and the SPIRE Instrument itself, both of which are typically orde…

astro-ph.IM2014★ 7 cited

Herschel SPIRE FTS telescope model correction

Rosalind Hopwood, Trevor Fulton, Edward T. Polehampton +8

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…

astro-ph.IM2014★ 7 cited

Herschel SPIRE Fourier Transform Spectrometer: Calibration of its Bright-source Mode

Nanyao Lu, Edward T. Polehampton, Bruce M. Swinyard +10

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…

astro-ph.IM2014★ 8 cited

Relative pointing offset analysis of calibration targets with repeated observations with Herschel-SPIRE Fourier-Transform Spectrometer

Ivan Valtchanov, Rosalind Hopwood, Edward Polehampton +9

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 regula…

astro-ph.IM2014★ 2 cited

Herschel SPIRE FTS Spectral Mapping Calibration

Dominique Benielli, Edward Polehampton, Rosalind Hopwood +12

The Herschel SPIRE Fourier transform spectrometer (FTS) performs spectral imaging in the 447-1546 GHz band. It can observe in three spatial sampling modes: sparse mode, with a sing…