OM Catalogue 4.1 - XMM-Newton
XMM-OM Serendipitous Ultraviolet Source Survey catalogue: SUSS4.1
SUSS4.1 is a new 2018 release of the XMM OM Serendipitous Ultraviolet Source Survey catalogue. This new release corrects some inconsistencies between IAUNAME and SRCNUM found in the previous release (OM SUSS4).
The catalogue was compiled for the Optical Monitor instrument on board the ESA XMM Newton observatory. This version, the 4th release of the catalogue, spans the period of observations from 2000 to July 2017.
A detailed description of the Catalogue can be found here. A refereed paper on the first version can be found in Page M.J. et al. (2012).
In addition to covering a larger observation period, the fourth release differs from the previous one in the implementation of a new time dependent sensitivity degradation correction. As in the previous release, sources detected on stacked images are properly flagged.
All data have been fully processed at the European Space Astronomy Centre (ESAC, Madrid, Spain) by using the XMM Science Analysis Software (SAS) system version 17.0.
The number of observations (OBSIDs) included in the catalogue is 9,749.
The total number of entries in this release is 8,176,156. They correspond to 5,503,765 sources, of which 1,035,453 have multiple entries in the source table, corresponding to different observations.
The Catalogue consists of two tables. The first one (SRCLIST) contains the sources, with positional and photometric data (count rate, magnitude and flux) and quality flags for each measurement. The content of the different columns (114) is:
| IAUNAME | Source IAU name |
| N_SUMMARY | Index in the SUMMARY table for the source OBSID |
| OBSID | Source OBSID number |
| SRCNUM | Source number in this catalogue |
| UVW2_SRCDIST | Dist. to the nearest source, UVW2 filter |
| UVM2_SRCDIST | Dist. to the nearest source, UVM2 filter |
| UVW1_SRCDIST | Dist. to the nearest source, UVW1 filter |
| U_SRCDIST | Dist. to the nearest source, U filter |
| B_SRCDIST | Dist. to the nearest source, B filter |
| V_SRCDIST | Dist. to the nearest source, V filter |
| RA | Source Right Ascension coordinate (deg) |
| DEC | Source Declination coordinate (deg) |
| RA_HMS | Source Right Ascension in hour units |
| DEC_DMS | Source Declination coordinate in DMS |
| POSERR | Source positional (coordinate) error |
| LII | Source galactic longtude |
| BII | Source galactic latitude |
| N_OBSID | Number of observation IDs for this source |
| UVW2_SIGNIF | Source significance for the filter UVW2 |
| UVM2_SIGNIF | Source significance for the filter UVM2 |
| UVW1_SIGNIF | Source significance for the filter UVW1 |
| U_SIGNIF | Source significance for the filter U |
| B_SIGNIF | Source significance for the filter B |
| V_SIGNIF | Source significance for the filter V |
| UVW2_RATE | Source count rate for the filter UVW2 |
| UVW2_RATE_ERR | Source count rate error, filter UVW2 |
| UVM2_RATE | Source count rate for the filter UVM2 |
| UVM2_RATE_ERR | Source count rate error, filter UVM2 |
| UVW1_RATE | Source count rate for the filter UVW1 |
| UVW1_RATE_ERR | Source count rate error, filter UVW1 |
| U_RATE | Source count rate for the filter U |
| U_RATE_ERR | Source count rate error, filter U |
| B_RATE | Source count rate for the filter B |
| B_RATE_ERR | Source count rate error, filter B |
| V_RATE | Source count rate for the filter V |
| V_RATE_ERR | Source count rate error, filter V |
| UVW2_AB_FLUX | Source flux for the filter UVW2 |
| UVW2_AB_FLUX_ERR | Source flux error for the filter UVW2 |
| UVM2_AB_FLUX | Source flux for the filter UVM2 |
| UVM2_AB_FLUX_ERR | Source flux error for the filter UVM2 |
| UVW1_AB_FLUX | Source flux for the filter UVW1 |
| UVW1_AB_FLUX_ERR | Source flux error for the filter UVW1 |
| U_AB_FLUX | Source flux for the filter U |
| U_AB_FLUX_ERR | Source flux error for the filter U |
| B_AB_FLUX | Source flux for the filter B |
| B_AB_FLUX_ERR | Source flux error for the filter B |
| V_AB_FLUX | Source flux for the filter V |
| V_AB_FLUX_ERR | Source flux error for the filter V |
| UVW2_AB_MAG | Source AB magnitude for the filter UVW2 |
| UVW2_AB_MAG_ERR | Source AB magnitude error, filter UVW2 |
| UVM2_AB_MAG | Source AB magnitude for the filter UVM2 |
| UVM2_AB_MAG_ERR | Source AB magnitude error, filter UVM2 |
| UVW1_AB_MAG | Source AB magnitude for the filter UVW1 |
| UVW1_AB_MAG_ERR | Source AB magnitude error, filter UVW1 |
| U_AB_MAG | Source AB magnitude for the filter U |
| U_AB_MAG_ERR | Source AB magnitude error, filter U |
| B_AB_MAG | Source AB magnitude for the filter B |
| B_AB_MAG_ERR | Source AB magnitude error, filter B |
| V_AB_MAG | Source AB magnitude for the filter V |
| V_AB_MAG_ERR | Source AB magnitude error, filter V |
| UVW2_VEGA_MAG | Source Vega magnitude for the filter UVW2 |
| UVW2_VEGA_MAG_ERR | Source Vega magnitude error, filter UVW2 |
| UVM2_VEGA_MAG | Source Vega magnitude for the filter UVM2 |
| UVM2_VEGA_MAG_ERR | Source Vega magnitude error, filter UVM2 |
| UVW1_VEGA_MAG | Source Vega magnitude for the filter UVW1 |
| UVW1_VEGA_MAG_ERR | Source Vega magnitude error, filter UVW1 |
| U_VEGA_MAG | Source Vega magnitude for the filter U |
| U_VEGA_MAG_ERR | Source Vega magnitude error, filter U |
| B_VEGA_MAG | Source Vega magnitude for the filter B |
| B_VEGA_MAG_ERR | Source Vega magnitude error, filter B |
| V_VEGA_MAG | Source Vega magnitude for the filter V |
| V_VEGA_MAG_ERR | Source Vega magnitude error, filter V |
| UVW2_MAJOR_AXIS | Source major semi-axis for the filter UVW2 |
| UVM2_MAJOR_AXIS | Source major semi-axis for the filter UVM2 |
| UVW1_MAJOR_AXIS | Source major semi-axis for the filter UVW1 |
| U_MAJOR_AXIS | Source major semi-axis for the filter U |
| B_MAJOR_AXIS | Source major semi-axis for the filter B |
| V_MAJOR_AXIS | Source major semi-axis for the filter V |
| UVW2_MINOR_AXIS | Source minor semi-axis for the filter UVW2 |
| UVM2_MINOR_AXIS | Source minor semi-axis for the filter UVM2 |
| UVW1_MINOR_AXIS | Source minor semi-axis for the filter UVW1 |
| U_MINOR_AXIS | Source minor semi-axis for the filter U |
| B_MINOR_AXIS | Source minor semi-axis for the filter B |
| V_MINOR_AXIS | Source minor semi-axis for the filter V |
| UVW2_POSANG | Source position angle for the filter UVW2 |
| UVM2_POSANG | Source position angle for the filter UVM2 |
| UVW1_POSANG | Source position angle for the filter UVW1 |
| U_POSANG | Source position angle for the filter U |
| B_POSANG | Source position angle for the filter B |
| V_POSANG | Source position angle for the filter V |
| UVW2_QUALITY_FLAG | Source quality flag for the filter UVW2 |
| UVM2_QUALITY_FLAG | Source quality flag for the filter UVM2 |
| UVW1_QUALITY_FLAG | Source quality flag for the filter UVW1 |
| U_QUALITY_FLAG | Source quality flag for the filter U |
| B_QUALITY_FLAG | Source quality flag for the filter B |
| V_QUALITY_FLAG | Source quality flag for the filter V |
| UVW2_QUALITY_FLAG_ST | Source quality flag string, filter UVW2 |
| UVM2_QUALITY_FLAG_ST | Source quality flag string, filter UVM2 |
| UVW1_QUALITY_FLAG_ST | Source quality flag string, filter UVW1 |
| U_QUALITY_FLAG_ST | Source quality flag string, filter U |
| B_QUALITY_FLAG_ST | Source quality flag string, filter B |
| V_QUALITY_FLAG_ST | Source quality flag string, filter V |
| UVW2_EXTENDED_FLAG | Source extended flag for the filter UVW2 |
| UVM2_EXTENDED_FLAG | Source extended flag for the filter UVM2 |
| UVW1_EXTENDED_FLAG | Source extended flag for the filter UVW1 |
| U_EXTENDED_FLAG | Source extended flag for the filter U |
| B_EXTENDED_FLAG | Source extended flag for the filter B |
| V_EXTENDED_FLAG | Source extended flag for the filter V |
| UVW2_SKY_IMAGE | Source detected in stacked images filter UVW2 |
| UVM2_SKY_IMAGE | Source detected in stacked images filter UVM2 |
| UVW1_SKY_IMAGE | Source detected in stacked images filter UVW1 |
| U_SKY_IMAGE | Source detected in stacked images filter U |
| B_SKY_IMAGE | Source detected in stacked images filter B |
| V_SKY_IMAGE | Source detected in stacked images filter V |
In the second table (SUMMARY) we give a summary of the observations from which the sources have been detected and measured. The content of the columns (35) in this table is:
| N_SUMMARY | Reference index for the source OBSID data |
| REVOLUTION | XMM revolution number |
| OBSID | Observation ID number |
| TARGET | Observation target name |
| FILTERS | XMM OM filter names used in this observation |
| MJD_START | Initial observation date/time |
| MJD_END | End of observation date/time |
| RA_PNT | Right Ascension of the telescope pointing direc |
| DEC_PNT | Declination of the telescope pointing direction |
| RA_PNT_HMS | Right Ascension of the telescope pointing in HM |
| DEC_PNT_DMS | Declination of the telescope pointing in DMS |
| EXPOSURE_UVW2 | Total exposure time for the filter UVW2 |
| EXPOSURE_UVM2 | Total exposure time for the filter UVM2 |
| EXPOSURE_UVW1 | Total exposure time for the filter UVW1 |
| EXPOSURE_U | Total exposure time for the filter U |
| EXPOSURE_B | Total exposure time for the filter B |
| EXPOSURE_V | Total exposure time for the filter V |
| N_SOURCES | Total number of sources |
| N_SOURCES_UVW2 | Number of sources for the filter UVW2 |
| N_SOURCES_UVM2 | Number of sources for the filter UVM2 |
| N_SOURCES_UVW1 | Number of sources for the filter UVW1 |
| N_SOURCES_U | Number of sources for the filter U |
| N_SOURCES_B | Number of sources for the filter B |
| N_SOURCES_V | Number of sources for the filter V |
| DETLIM_UVW2 | Vega magnitude limit for the filter UVW2 |
| DETLIM_UVM2 | Vega magnitude limit for the filter UVM2 |
| DETLIM_UVW1 | Vega magnitude limit for the filter UVW1 |
| DETLIM_U | Vega magnitude limit for the filter U |
| DETLIM_B | Vega magnitude limit for the filter B |
| DETLIM_V | Vega magnitude limit for the filter V |
| RAOFFSET | Corrected offset in Right Ascension |
| DECOFFSET | Corrected offset in Declination |
| RAOFFSET_ERR | Standard error of the RA offset |
| DECOFFSET_ERR | Standard error of the DEC offset |
| OFFSET_RMS | Offset RMS |
The meaning of the quality flags (columns filter_QUALITY_FLAG and filter_QUALITY_FLAG_ST) in the SRCLIST table are as follows:
| bit 0 (value 1) | source on a bad pixel |
| bit 1 (value 2) | source on a readout streak |
| bit 2 (value 4) | source on a smoke-ring |
| bit 3 (value 8) | source on a diffraction spike |
| bit 4 (value 16) | source affected by Mod-8 pattern |
| bit 5 (value 32) | source within the central enhancement |
| bit 6 (value 64) | source near a bright source |
| bit 7 (value 128) | source near the edge |
| bit 8 (value 256) | point source within an extended source |
| bit 9 (value 512) | weird source (bright pixel) |
| bit 10 (value 1024) | multiple exposure values within photometry aperture |
| bit 11 (value 2048) | the source is too bright (rate > 0.97 c/frame) |
The columns filter_SKY_IMAGE indicate if a source has been detected in stacked (sky) images obtained with that filter. The catalogue contains 948,277 such detections, with 60,889 sources having multiple detections in different observations.
A cross-match of the whole catalogue with GAIA DR2 data set, using a search radius of 3 arcsec gives 82% matches. Detections in the V filter have 89% matches.
The XSA provides access to the OM Catalogue as a complete download of the file (~1 Gb, compressed fits format) as well as through a search interface whose results can be stored by the user in several formats. It should be noted that this interface allows the user to access only part of the information contained in the catalogue: source coordinates, magnitude and flux and their corresponding errors and quality flags. A reduced version of the complete catalogue (500 Mb, compressed fits format) can be downloaded as well.
The ESA-Sky utility allows the user to display the sources from the catalogue on top of sky images from different instruments at all wavelengths. This includes also images obtained with OM in two color combination, Visible (U, B and V OM filters) and UV (UVW1, UVM2 and UVW2 OM filters). It should be noted that OM images have a low dynamic range.