Dear User,

Thanks for contacting us,

indeed this is planned and a new version of the Archive Science Portal, containing also the Planck maps will be soon deployed.

Best regards,

the ESO Archive

Dear User,

The MUSE GEOMETRY and ASTROMETRY calibration frames are taken regularly. They are processed automatically and checked for quality. The quality parameters are monitored in the specially designed Health Check plots:

https://www.eso.org/observing/dfo/quality/MUSE/reports/HEALTH/trend_report_GEOMETRY_HC.html

https://www.eso.org/observing/dfo/quality/MUSE/reports/HEALTH/trend_report_ASTROMETRY_WFM_HC.html

https://www.eso.org/observing/dfo/quality/MUSE/reports/HEALTH/trend_report_ASTROMETRY_NFM_HC.html

The MUSE geometry calibrations are quite high volume (~6 GB, 70 input raw frames) and their processing is hardware demanding. Thus, early in operations the decision was taken to provide the users only with the static (frozen in time) version of the master GEOMETRY_TABLE. The regular monitoring shows if there is a need to produce modified, newer version. Since April 2021 there has not been such a need identified yet. That is why the April 2021 version is still distributed with the 2024 science data. The MUSE astrometry is closely tide with geometry, so it is also provided in the static form. The ASTROMETRY version corresponds to the distributed GEOMETRY version.

There is always a possibility to download the latest calibrations (raw data) from the ESO Archive at: http://archive.eso.org/wdb/wdb/eso/muse/form and process them if the users prefer to repeat the data processing themselves.

Hope this answers your question.

Best regards,

The ESO Archive Team

Please click on 'Continue' on the lower right corner of the popup window.

Could you please be more specific? To which web page are you referring to?

Dear User,

Thank you for reaching out to us.

The heliocentric or barycentric correction provided in the header is suitable for general purposes. However, I cannot confirm its precision. For a more detailed response tailored to your scientific requirements, I recommend opening a ticket at the following URL:  https://support.eso.org/ and click on "Contact us"

Dear Mateus,

Unfortunately these data are not available. Back then data from 3.6m (or 1.54m) was not ingested yet in the ESO Archive.

Sorry we cannot help you.

Dear User,

thanks contacting us.

There are no CCV files for radial velocities measurements.

The closest files names are CCF files.

You can find this type of files for examples inside the Ancillary HarpsTar file (TAR file containing several types of files, both FITS and non-FITS.)

You can get an Ancillary files in this way: assuming that you have the ADP name of the file in which you are interested (example ADP.2014-09-16T11:06:15.853), you can go to the Science Portal, query for it, reach the dataset page information

http://archive.eso.org/dataset/ADP.2014-09-16T11:06:15.853

and from here click on the blue button "Dataset Download" that will open the page of the download, and hence you reach the Download portal, where you can click on

"Include ancillary data", and hence select the method for downloading the data that you prefer. Once you download the file, you can extract the ADP and the ancillary file from the archive you downloaded. The ancillary file will be in a tar file that you need to decompress.