Highly oxygenated organic molecule cluster decomposition in atmospheric pressure interface time-of-flight mass spectrometers

Zanca, Tommaso; Kubečka, Jakub; Zapadinsky, Evgeni; Passananti, Monica; Kurtén, Theo; Vehkamäki, Hanna

doi:https://doi.org/10.5194/amt-13-3581-2020

Articles | Volume 13, issue 7

https://doi.org/10.5194/amt-13-3581-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/amt-13-3581-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 13, issue 7

Research article

|

03 Jul 2020

Research article |

| 03 Jul 2020

Highly oxygenated organic molecule cluster decomposition in atmospheric pressure interface time-of-flight mass spectrometers

Tommaso Zanca, Jakub Kubečka, Evgeni Zapadinsky, Monica Passananti, Theo Kurtén, and Hanna Vehkamäki

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Final revised paper (published on 03 Jul 2020)
Preprint (discussion started on 04 Feb 2020)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

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- Supplement

RC1: 'referee comments', Anonymous Referee #1, 13 Mar 2020
- AC1: 'Reply to Referee #1', Tommaso Zanca, 03 May 2020
RC2: 'Review of "HOM Cluster decpmposition in APi-ToF mass spectrometers"', Anonymous Referee #2, 21 Apr 2020
- AC2: 'Reply to Referee #2', Tommaso Zanca, 03 May 2020

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision

AR by Tommaso Zanca on behalf of the Authors (03 May 2020) Author's response Manuscript

ED: Publish as is (23 May 2020) by Hartmut Herrmann

Short summary

In this paper we quantify (using a statistical model) the probability of decomposition of a representative class of HOM clusters in an APi-TOF mass spectrometer. This is important because it quantifies the systematic error of measurements in a APi-TOF MS due to cluster decomposition. The results (specific for our selected clusters) show that decomposition is negligible, provided their bonding energy is large enough to allow formation in the atmosphere in the first place.