ESA Science Programme Missions: Contributions and Exploitation -- Herschel Observing Time Proposals

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Main Authors: Pilbratt, Goran L., Garcia-Lario, Pedro, Parmar, Arvind N.
Format: Preprint
Published: 2024
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author Pilbratt, Goran L.
Garcia-Lario, Pedro
Parmar, Arvind N.
author_facet Pilbratt, Goran L.
Garcia-Lario, Pedro
Parmar, Arvind N.
contents After an introduction to the ESA Herschel Space Observatory including a mission overview, science objectives, results and productivity we examine the process and outcomes of the announcements of observing opportunities (AOs). For Herschel, in common with other ESA observatories, there were no rules, quotas, or guidelines for the allocation of observing time based on the geographical location of the lead proposer's institute, gender, or seniority (academic age); scientific excellence was the most important single factor. We investigate whether and how success rates vary with these (other) parameters. Due to the relatively short operational duration of Herschel -- compared to XMM-Newton and INTEGRAL -- in addition to the pre-launch AO in 2007 there was just two further AOs, in 2010 and 2011. In order to extend the time-frame we compare results with those from the ESA Infrared Space Observatory (ISO) whose time allocation took place approximately 15 years earlier.
format Preprint
id arxiv_https___arxiv_org_abs_2402_12841
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle ESA Science Programme Missions: Contributions and Exploitation -- Herschel Observing Time Proposals
Pilbratt, Goran L.
Garcia-Lario, Pedro
Parmar, Arvind N.
Instrumentation and Methods for Astrophysics
After an introduction to the ESA Herschel Space Observatory including a mission overview, science objectives, results and productivity we examine the process and outcomes of the announcements of observing opportunities (AOs). For Herschel, in common with other ESA observatories, there were no rules, quotas, or guidelines for the allocation of observing time based on the geographical location of the lead proposer's institute, gender, or seniority (academic age); scientific excellence was the most important single factor. We investigate whether and how success rates vary with these (other) parameters. Due to the relatively short operational duration of Herschel -- compared to XMM-Newton and INTEGRAL -- in addition to the pre-launch AO in 2007 there was just two further AOs, in 2010 and 2011. In order to extend the time-frame we compare results with those from the ESA Infrared Space Observatory (ISO) whose time allocation took place approximately 15 years earlier.
title ESA Science Programme Missions: Contributions and Exploitation -- Herschel Observing Time Proposals
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2402.12841