i. Sky Coverage and Observation Parameters
|Target||Hydra Cluster||Type||galaxy cluster||Central Position1||RA (J2000 deg)||Dec (J2000 deg)|
|Scan Length (deg)||No. of Tiles2||No. of Scans3||Approximate
|Tile Numbers5||335512-335527, 33529, 335611-335629, 335711-335728|
|Approximate Boundaries (J2000 deg)6|
Notes to Table 1
1 - Geometric center of area covered by 6x scans. Because of gaps in the scan coverage of some fields, there may not be a scan covering this location. See Figure 1.
2 - Number of unique pre-defined observation areas (tiles) that cover this field.
3 - Number of 6x scans that cover the tiles in this field. The number of scans may exceed the number of tiles because some tiles were observed more than once.
4 - Approximate area is computed from the number of tiles covering this field, accounting for RA and Dec overlap between tiles. It is not the area defined by the approximate field boundaries.
5 - 6° long 6x tiles have the same number and cover the same region as the corresponding tile from the main survey. 1° long 6x tiles are assigned numbers in the range 30000-39999 for northern observatory scans and 333000-349999 for southern observatory scans. 1° long 6x tile numbers do not match tile numbers from the main survey.
6 - Approximate field boundaries define the smallest rectangular region on the sky that encloses all scans of this field. This region may not be completely covered by 6x observations because of gaps in the 6x coverage. See Figure 1.
|Figure 1 - Sky map showing outlines of 6x Hydra scans in blue and distribution of 6x point source WDB extractions (red dots). Some tiles may have been observed more than once and have a corresponding higher density of extractions in the WDB.||Figure 2 - Sky map showing outlines of 6x Hydra scans in blue and distribution of 6x extended source WDB extractions (green dots).|
ii. Field-Specific Notes
The Hydra 6x field was targeted on the Hydra galaxy cluster as part of a program to probe 2MASS galaxy completeness as a function of galactic latitude.
The scan coverage of this field is split into two 3° long declination bands separated by 2° as a result of the telescope commanding error that affected the 1° long 6x scans. The north and south sections of the Hydra field coverage are comprised of three partially filled declination rows of scans. There are a number of gaps throughout each of the sections. See Figure 1.
The nominal cluster center is located approximately in the center of the northern section of the field. While the core of the cluster was covered by a 6x scan, the overall coverage of the cluster is fragemnted.
Seventeen of the scans in the southern part of the Hydra field were
incorrectly assigned tile numbers that duplicate those of tiles in the
northern section: 335513, 335515, 335517, 335519,
335521, 335524, 335526, 335711, 335713, 335714, 335716, 335718,
335720, 335722, 335724, 335725, 335727.
Caution should be used when selecting or searching for observations in this
region according to tile number.
iii. Working Database and Catalog Source Properties
|Full 6x Working DB1||6x "Catalog" subset2|
Notes to Table 2
1 - "Full 6x Working DB" refers to the total number of Scans and Atlas Images available from all 6x observations of this field. The "Point Source" and "Extended Source" entries refer to the total number of sources extracted from all observations of this field in the respective 6x Point and Extended Source Working Databases.
2 - "6x Catalog Subset" refers to the subset of all scans covering this field that were selected to constitute a single, unique coverage of the field (A3.6.b), the images from those scans, and the subset of all source extractions from the selected scans that satisfy the "6x-PSC" and "6x-XSC" quality selection criteria described in A3.6.c. The "6x Catalog subset" can be identified in the 6x Scan and Image Metadata tables, and Point and Extended Source WDB tables by selecting entries with "cat=1".
|Extracted Source Counts and Statistics|
|Figure 3 - Full 6x point and extended source Working Database source counts as a function of magnitude. Point source counts are shown by the red line and extended source counts are the blue shaded region. The default magnitudes are used for point sources, and the Ks=20 mag arcsec-2 elliptical isophotal magnitudes are used for extended sources.||Figure 4 - Differential source densities as a function of magnitude for the 6x Point and Extended Catalogs compared with those for the All-Sky PSC and XSC. 6x PSC and XSC counts are shown by the red and blue lines, respectively. All-Sky PSC and XSC counts are shown in the grey and cyan shaded regions.|
|Figure 5 - Color-magnitude diagram for extractions in the point and extended source 6x WDBs in the Hydra field. Point sources are shown as small red dots and extended sources as larger green dots. The black contours trace the density of point sources. The horizontal discontinuity in the point source distribution near Ks~10.5 mag in the color-magnitude diagram is caused by the sensitivity gap between the 51 ms R1 and 7.8 s R2-R1 exposures in the 6x data.||Figure 6 - Color-color diagram for extractions in the point and extended source 6x WDBs in the Hydra field. Point sources are shown as small red dots and extended sources as larger green dots. The black contours trace the density of point sources.|
|Figure 7 - Differences between 6x and main survey point source photometry plotted as a function of 6x source default magnitude. Black contours trace the density of individual sources that are shown as light grey points. The large blue points and error bars show the trimmed average and RMS of the 6x-survey magnitude differences for all sources in 0.25 magnitude wide bins.||Figure 8 - Differences between 6x and main survey extended source photometry in 7" circular apertures ([jhk]_m_7) plotted as a function of 6x extended source magnitude. Black contours trace the density of individual sources that are shown as light grey points. The large blue points and error bars show the trimmed average and RMS of the 6x-survey magnitude differences for all sources in 0.25 magnitude wide bins.|
[Last updated: 2006 June 13; by R. Cutri]