Peer Review of PDS 28 Sgr Volume

Colleen A. McGhee, including input of Richard G. French

February 4, 2005

 

1.    Introduction

 

We organize the review directory-by-directory, in the order in which we think an interested scientist would visit them. Then, at the end, we make some general comments.

2.    Files and Directories

In the following, an annotation of ÔFineÕ means that we found the contents to be clear and unambiguous. We did not check the syntax of every data field.

 

AAREADME.TXT Ð This file gives an excellent overview of the volume contents and organization. There are no recommended changes.

ERRATA.TXT Ð Very brief, which is fine.

VOLDESC.CAT Ð Fine.

BROWSE Directory

BROWINFO.TXT Ð Good, very clear and complete description of files.

ESO1M subdirectory Ð Fine

ESO22M subdirectory Ð Fine

IRTF subdirectory Ð Fine

LICK1M subdirectory Ð Fine

MCD27M subdirectory Ð Fine

PAL200 subdirectory Ð Fine

CALIB Directory

CALINFO.TXT Ð No calibration files.

CATALOG Directory

CATINFO.TXT Ð OK Ð Nice summary of other files in this directory.

ESO1M_DATASET.CAT Ð There seems to be an error in the Processing and Data sections of this catalog. In each, it says that four quantities are provided in the tables, but in fact there are only 3 columns. The quantity Ònormal optical depthÓ is not included, and should be removed from this description. Additionally, the catalog lists four values of quality flag, while BROWINFO.TXT lists five possible values.

Done. All data files have the full seven columns with dummy values when data is not available. This was done to simplify the development by users of software to manipulate the data. Descriptions have been updated accordingly. Inconsistencies in the quality flag descriptions have also been corrected.

 

ESO1M_HOST.CAT Ð Fine

ESO1M_INST.CAT Ð Fine

ESO22M_DATASET.CAT Ð Here there is the same problem with the Processing and Data sections of the catalog as for the 1-m dataset catalog: there are in reality only 3 columns, though it says there are 4. Again, the number of quality flags and their definitions are inconsistent with other definitions, e.g. BROWINFO.TXT, DATAINFO.TXT

ESO22M_HOST.CAT Ð Fine

ESO22M_INST.CAT Ð Fine

IRTF_DATASET.CAT Ð Instead of the 4 columns listed in the data files, there are in fact 7. Also, the quality flag definitions are inconsistent with other files, e.g. BROWINFO.TXT, DATAINFO.TXT

LICK1M_DATASET.CAT Ð See comments for IRTF_DATASET.CAT

MCD27M_DATASET.CAT Ð See comments for IRTF_DATASET.CAT

MISSION.CAT Ð Fine

P200_DATASET.CAT Ð See comments for IRTF_DATASET.CAT

PERSON.CAT Ð Fine

REF.CAT Ð Fine

Done. All of the DATASET.CAT files have been edited to remove Ôcut & pasteÕ errors, provide consistent descriptions of the quality flag values and the BROWSE & DATA file holdings and structures.

 

DATA Directory

DATAINFO.TXT Ð There might be a sentence like ÒFor bad or missing data, values are replaced by a constant as described by the label,Ó when discussing the columns and/or the quality flags.

Done.

ESO1M subdirectory

ESO22M subdirectory

IRTF subdirectory

LICK1M subdirectory

MCD27M subdirectory

PAL200 subdirectory

We plotted stellar intensity vs. radius for every file in the data directory without difficulty. In reviewing the *.LBL files, it appears that the descriptions for the observations was copied from the PAL200 description in large part, since each contains the following text:

 

Ex: ES1_EPD.LBL:

DESCRIPTION É.

A total of 64,000 raw frames were recorded, each with an integration time of 0.15 seconds. Observing conditions became partly cloudy during egress observations of the B and A rings; consequently, the photometric quality of these observations is not as good as for the corresponding ingress observations. Absolute timing was achieved by chopping with the secondary mirror exactly 2 arcsec north for exactly 2 sec (13.3 frames) at intervals of 1 minute, and for exactly 4 sec on the hour, using trigger pulses from a crystal-oscillator continuously synchronized with shortwave radio time signals from WWVB. Absolute occultation timing was reconstructed with an accuracy of 0.05 sec.

 

We would recommend simply deleting this phrase from the non-Palomar DESCRIPTION fields.

 

Done.

 

We spot-checked label entries such as telescope coordinates and ring data set information, and found no errors.

 

As mentioned in the CATALOG directory DATASET.CAT files, there seems to be some inconsistency about the definitions for Quality Flags in the documentation.

 

Corrected.

 

DOCUMENT Directory

DOCINFO.TXT Ð Fine

GEOMETRY.pdf Ð Fine

GEOMETRY.TXT Ð Fine

MODEL.pdf Ð Fine

MODEL.TXT Ð Fine

We did not proofread all the polynomial coefficients in the DOCUMENT files, but we did spot-check them.

GEOMETRY Directory

GEOMINFO.TXT Ð Fine

ESO1M subdirectory Ð Fine

ESO22M subdirectory Ð Fine

      IRTF subdirectory Ð Fine

      LICK1M subdirectory Ð Fine

            MCD27M subdirectory Ð Fine

            PAL200 subdirectory Ð Fine

We did not proofread all the polynomial coefficients in the GEOMETRY files, but we did spot-check them.

 

INDEX Directory

Files look fine, but we did not use PDS software to try to read them in and navigate via the labels.

SORCDATA Directory

DATAINFO.TXT

ESO1M subdirectory

ESO22M subdirectory

IRTF subdirectory

LICK1M subdirectory

MCD27M subdirectory

PAL200 subdirectory

3.    General Comments

Overall, we found this volume to be well-organized, clearly documented, and complete.

The directory structure was fairly simple and straightforward, which made it easy to navigate.

 

We did not try to read the files using PDS-compliant software Ð that is, we did not read the LBL files and then try to read the associated TAB files. We assume this is checked by the PDS software.