GSC
2.3 Release Notes
(NOT COMPLETE YET)
These notes contain
basic information about the GSC2.3 catalog content, format and data
access methods. Several new fields are provided with this release including
proper motions, additional magnitude columns, and identifiers. The file
structure is identical to GSC2.2.
General Description
Source Counts
Catalog Fields
Data Access Software
Export Catalog File Format
FITS HDU 2, ASCII Table: HTM Level 10 lookup
FITS HDU 3, Export Binary Table Fields and Types
Future Release Enhancements
Classification and Source Status Codes
Known catalog limitations
General
Description
GSC2.3
is an all-sky export of calibrated photographic
survey
plate source
parameters from the COMPASS database. All
sources exported are from the second-generation plate-processing
pipeline
with the exception of Tycho-2 and Skymap sources in the case of very
bright objects. The Skymap sources are exported when there is no matching
GSC or Tycho sources.
Source
Counts
The number
of unique objects exported is approximately 945,592,683. The catalog
properties for this release represent a magnitude-selected subset
of the full COMPASS database. The storage capacity required for
GSC 2.3 is approximately 200 Gigabytes.
Catalog
Fields
Each
GSC 2.3 entry contains only one position and one magnitude per
bandpass for each unique sky object. In addition this
version also contains proper motions for sources which satisfy specific
constraints since the COMPASS database contains multiple epochs
and
observations for a given source. To maximize the quality of the exported
data the catalog parameter selection was performed as follows:
- Positions and magnitudes from plate observations
were selected by choosing the observation which
occurs closest to the plate center. Position selection was then prioritized
by
- If an observation occurred at different
plate scanning resolutions, the highest resolution (15 um pixels)
was selected over the lower resolution (25 um pixels) for each bandpass
regardless of plate location.
- Star/nonstar classifications were assigned
by voting all available classifications from 15um scans, before
applying the magnitude cutoff. Classifications from 25um scans were
used only if no 15um data were available for the object. Ties were
broken in favor of nonstar, and defect classifications were considered
to be nonstellar for matched objects. Unmatched plate defects were
excluded from the catalog.
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Data
Access Software
For this
release, the main public access supported is through the GSC-2.3
Web form interface. The underlying software is currently only
for specialized distribution to the GSC-II consortium until the
final 2.3
catalog calibrations are completed. A C++ cgi script has been
developed for integration into telescope observation tools consistent
with the standard interfaces used with SkyCat. There
is a Beta version of ShowSky
visualization tool , a JAVA application available to the public
which query access to GSC-2.2, DSS, and various other catalogs .
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Export
Catalog File Format
The export catalog is a distributed FITS file system
based on the linear quad-tree Hierarchical Triangular Mesh (HTM) sky
partitioning scheme (see HTM Reference
). GSC-2 catalog uses a level 6 HTM triangulation which results in each
file containing roughly 1 square degree of sky data. The source numbers
per file are not balanced at this time, but future options are available
to extend this capability into the HTM access methods.
Each FITS file contains all calibrated celestial
sources for a single triangular section of sky (HTM level 6 leafnode).
The file names are the quad-tree representation of each triangular section,
with the 1st character being either an 'N' or 'S' representing
North or South.
A FITS file contains 1 primary HDU, a second HDU
(1st extension) ACSII table, and a third HDU (2nd
extension) binary table. HDU 2 is a fixed length 256 entry lookup table
into a variable sized HDU 3. The HDU 3 is sorted into HTM level 10 cells,
and thus the lookup points to the first record of each level 10 cell
with the number of entries in that cell also included in the ASCII table.
The level 10 provides an indexing resolution of approximately 18 square
arc minutes.
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HDU 2, ASCII Table
Variable Type |
Variable Name |
Description |
Integer
|
tfields=2 |
"Table fields" The
table will contains 2 columns. |
Long
|
nrows=256 |
"Number of Rows" Table
will have 256 rows. |
Char
|
extname[]="HTMLevel10Idx" |
"Extension name" Name
of the extention. |
Char
|
*ttype[]={"Freq", "L10Pointer"}; |
"Table Type" |
Char
|
*tform[]={"I10","I10"}; |
"Table
Form" |
Char
|
*tunit[]={" "," "}; |
"Table
Unit" |
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HDU
3, Export Binary Table Fields and Types
Field |
Type |
Form |
Unit |
Description |
1 |
gscID2 |
J |
id |
internal id# |
2 |
gsc1ID |
11A |
id |
GSC1 name |
3 |
hstID |
11A |
id |
GSC2 name for HST ops |
4 |
RightAsc |
D |
rad |
RA (J2000) |
5 |
Declination |
D |
rad |
Dec (J2000) |
6 |
PositionEpoch |
E |
year |
Epoch of position |
7 |
RaEpsilon |
E |
arcsec |
RA error |
8 |
DecEpsilon |
E |
arcsec |
Dec error |
9 |
RaProperMotion |
E |
mas/yr |
Proper motion |
10 |
DecProperMotion |
E |
mas/yr |
Proper motion |
11 |
RaProperMotionErr |
E |
mas/yr |
PM error |
12 |
DecProperMotionErr |
E |
mas/yr |
PM error |
13 |
deltaEpoch |
E |
year |
time baseline used for pm calculation |
14 |
FpgMag |
E |
mag |
IIIaF magnitude |
15 |
FpgMagErr |
E |
mag |
mag err |
16 |
FpgMagCode |
I |
|
bandpass code |
17 |
JpgMag |
E |
mag |
IIIaJ magnitude |
18 |
JpgMagErr |
E |
mag |
mag err |
19 |
JpgMagCode |
I |
|
bandpass code |
20 |
Vmag |
E |
mag |
'V' band magnitude |
21 |
VmagErr |
E |
mag |
mag error |
22 |
VmagCode |
I |
|
bandpass code |
23 |
Nmag |
E |
mag |
IV-N magnitude |
24 |
NpgMagErr |
E |
mag |
mag error |
25 |
NpgMagCode |
I |
|
bandpass code |
26 |
UMag |
E |
mag |
'U' magnitude |
27 |
UMagErr |
E |
mag |
mag error |
28 |
UMagCode |
I |
|
bandpass code |
29 |
BMag |
E |
mag |
'B' magnitude |
30 |
BMagErr |
E |
mag |
mag error |
31 |
BMageCode |
I |
|
bandpass code |
32 |
RMag |
E |
mag |
'R' magnitude |
33 |
RMagErr |
E |
mag |
mag error |
34 |
RMagCode |
I |
|
bandpass code |
35 |
IMag |
E |
mag |
'I' magnitude |
36 |
IMagErr |
E |
mag |
mag error |
37 |
IMagCode |
I |
|
bandpass code |
38** |
JMag |
E |
mag |
2MASS J magnitude |
39** |
JMagErr |
E |
mag |
mag error |
40** |
JMagCode |
I |
|
bandpass code |
41** |
HMag |
E |
mag |
2MASS H magnitude |
42** |
HMagErr |
E |
mag |
mag error |
43** |
HMagCode |
I |
|
bandpass code |
44** |
KMag |
E |
mag |
2MASS K magnitude |
45** |
KMagErr |
E |
mag |
mag error |
46** |
KMagCode |
I |
|
bandpass code |
47 |
Classification |
J |
|
classification code |
48 |
SemiMajorAxis |
E |
pixels |
Object size |
49 |
Eccentricity |
E |
|
Object eccentricity |
50 |
Positionangle |
E |
deg |
Object Position Angle |
51 |
Source
Status Flag |
J |
|
Object Flags |
52 |
Variable Flag |
J |
|
Flag for known variable |
53 |
MultipleFlag |
J |
|
Flag for known multiple |
** 2MASS magnitudes not yet filled in - will be needed for JWST so
placeholder fields were allocated.
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Future
Release Enhancements
Return to top.
Classification
Codes
0 |
Star |
1 |
Galaxy |
2 |
Blend |
3 |
Non-Star |
4 |
Unclassified |
5 |
Defect |
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Source
Status Flag Codes
The source status flag is a 10 digit field used
to encode more detailed information about the properties of the catalog
object and its calibrated values. Since no GSC-II processed data is
included for Tycho or SkyMap objects, the value of the Source Status
Flag for a Tycho object is 99999900, Skymap is 88888800.
Digit
(counting from the right)
|
Flag
|
0
|
1
|
2
|
3
|
1
|
Number of plates on which
this object appeared.
|
This may include plate observations
that were excluded from the GSC2.3.
|
These two digits are read
together as an ordinary base ten number, eg, 04 or 12.
|
-
|
-
|
2
|
3
|
Centroider
type associated with the exported position
|
0 |
Barycenter |
4 |
multicircular |
1 |
Circular Gaussian |
5 |
multielliptical |
2 |
Elliptical Gaussian |
6 |
FPA + circular |
3 |
FPA-applied
barycenter |
7 |
FPA
+ elliptical |
|
4
|
Quality of exported J magnitude
|
not present
|
fit
|
extrapolated
|
-
|
5
|
Quality of exported F magnitude
|
not present
|
fit
|
extrapolated
|
-
|
6
|
Quality of exported V magnitude
|
not present
|
fit
|
extrapolated
|
-
|
7
|
|
mixed vote
|
unanimous vote
|
unanimous defect
|
-
|
8
|
Classification voters
|
More than one 15um scan
|
One 15um scan
|
More than one 25um scan
|
One 25um scan
|
9
|
Incomplete processing
|
Completed processing on
all plates
|
Object
was too big to be cut out (> 256x256 pixels) on at least
one plate
|
-
|
-
|
10
|
Deblended object
|
Single object on all plates
|
Child (deblended) object
on at least one plate
|
-
|
-
|