Articles | Volume 20, issue 12
https://doi.org/10.5194/bg-20-2221-2023
© Author(s) 2023. This work is distributed under the Creative Commons Attribution 4.0 License.
Hyperspectral imaging sediment core scanning tracks high-resolution Holocene variations in (an)oxygenic phototrophic communities at Lake Cadagno, Swiss Alps
Download
- Final revised paper (published on 19 Jun 2023)
- Supplement to the final revised paper
- Preprint (discussion started on 06 Feb 2023)
- Supplement to the preprint
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
-
RC1: 'Comment on egusphere-2023-151', Anonymous Referee #1, 09 Mar 2023
- AC1: 'Reply on RC1', Paul Zander, 28 Apr 2023
-
RC2: 'Comment on egusphere-2023-151', Anonymous Referee #2, 10 Apr 2023
- AC2: 'Reply on RC2', Paul Zander, 28 Apr 2023
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
ED: Publish subject to minor revisions (review by editor) (07 May 2023) by Sebastian Naeher
AR by Paul Zander on behalf of the Authors (15 May 2023)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (21 May 2023) by Sebastian Naeher
AR by Paul Zander on behalf of the Authors (22 May 2023)
The paper is well-written and the idea is ueful for the community. however, there are some doubts about reliability of the new proposed index which require more debates statistically. Here are my comments:
RABD670: There is a review from Van Exem et al. 2022 which they reviewed all the chl indices and they found out that RABAs work better than RABDs. Have you tried to implement that and compare the results since it seems to be possible with your data.
Line 160: how did you determine the percentage reflectance values to remove cracks and mineral reflections? it seems it is based on practical excercise on your core and your hyperspectral scanner which it should be noted in the text.
Fig 2: since RABD710-730 is located in the right shoulder of chl-a and phaephytin-a absorption bands, how would they effect this index? with bigger amount of chl-a and Phae-a it is expected that GSB-related signal disapear. And based on your data was there any detection limitation on this index?
Fig3: It would be better to remake all the plots in a way that the whole dots and the range are observed.
Fig 3C: There are some RABD710-730 dots which are valued less than one, how do you interpret them? moreover, considering RABD710-730, I am curios to see what correlation you will get if you remove Isorenieratene which have big values ( over 1000) and then recalculate the correaltion. It seems the correlation for the samples with Iso under 1000 are weak. Maybe, it can be discussed in terms of limitations of the index!
Fig4: this figure is a bit unclear. suggest to change the caption and specify y-axes is related to which RABD.
Finally, it is always a question that a model or here an index which is applied on one core can be applied on any other cores? what would be the limitations and maybe a discussion on this in the paper would be useful for reader.