PS1 3pi DVO Database Snapshop 2011.04.21
The latest 3pi DVO database release can be found at the following location:
rsync://ipp0032.ifa.hawaii.edu/ps1-3pi-catdirs-20110421
This rsync location is protected with a password, see your DRAVG representative for information
The following plots show the coverage in g,r,i,z,y. These plots are centered on 0,0 (ra increasing to the right). The black line is the Galactic Plane; the purple line is the Ecliptic.
| filter | 3pi database coverage |
| g |
|
| r |
|
| i |
|
| z |
|
| y |
|
This database is similar in contents to the previous (2011/2/1) database.
Some notes on what this database contains:
- all1 3pi data taken since the start of demo month (2010/2/12) through the start of April (2011/4/1)
- 2MASS detections matched to all objects
- average fields for grizy and JHK (eg, avextract g i J K would work)
- zero point calibrations for the PS1 data come from the synthetic photometry database.
- astrometric calibration is the default in-line calibration relative to the 2MASS frame
- average magnitudes use a weighted mean, and skip detections that have PSF_QF < 0.85 (excessively masked objects). there is no iterative clipping, however.
1 a caveat regarding coverage: there seem to be some gaps that do not correspond to known gaps in the data taken.
In addition, there are 4 bit flags available in the average table for each object to give a hint at quality and extendedness:
- for all PS1 detections, the detection is considered 'extended' if (mag_psf - mag_ap > 0.5)
- if the number of 'extended detections' exceeds the number of 'psf-like' detections, the object is flagged as "PS1 extended" (objflag & 0x01000000)
- if any of the detections have PSF_QF > 0.85, then the object is considered "PS1 good" (objflag & 0x04000000)
- similarly, if the 2MASS J-band flags indicate the source is extended, the object is considered "2MASS extended" (objflag & 0x02000000)
- if the 2MASS J-band detection is significant (), the source is considered "2MASS good" (objflag & 0x08000000)
- A significant 2MASS source means their field ph_qual is one of the 3 classes A, B, or C, which means the source is > 5 sigma and has some quality limits.
For more information about 2MASS representation in DVO, see 2MASS_info_in_DVO.
Source Counts
| region | N(objects) | N(detections) | 2MASS(objects) | 2MASS(detections) |
| n0000 | 238340242 | 859053094 | 22669788 | 68009364 |
| n0730 | 229407741 | 859900656 | 22234449 | 66703347 |
| n1500 | 215053632 | 892046096 | 21574758 | 64724274 |
| n2230 | 212432167 | 904611990 | 20261912 | 60785736 |
| n3000 | 204921061 | 842451839 | 19573278 | 58719834 |
| n3730 | 170950354 | 711912493 | 17779643 | 53338929 |
| n4500 | 154037392 | 698112737 | 17544366 | 52633098 |
| n5230 | 130632639 | 652426073 | 16378632 | 49135896 |
| n6000 | 92593658 | 461075070 | 11718975 | 35156925 |
| n6730 | 57788695 | 234148770 | 5173377 | 15520131 |
| n7500 | 34429854 | 113871350 | 2214222 | 6642666 |
| n8230 | 9348197 | 27724078 | 633355 | 1900065 |
| s0000 | 249150791 | 902157224 | 24458147 | 73374441 |
| s0730 | 265693154 | 1074361638 | 26321350 | 78964050 |
| s1500 | 301040727 | 1353823003 | 29795032 | 89385096 |
| s2230 | 325386490 | 1559497237 | 33108907 | 99326721 |
| s3000 | 50808007 | 162899768 | 32856544 | 98569632 |
| s3730 | 31141331 | 93423993 | 31141331 | 93423993 |
| s4500 | 33001272 | 99003816 | 33001272 | 99003816 |
| s5230 | 36304694 | 108914082 | 36304694 | 108914082 |
| s6000 | 29756694 | 89270082 | 29756694 | 89270082 |
| s6730 | 11730797 | 35192391 | 11730797 | 35192391 |
| s7500 | 3734364 | 11203092 | 3734364 | 11203092 |
| s8230 | 1026468 | 3079404 | 1026468 | 3079404 |
| total | 3088710421 | 12750159976 | 470992355 | 1412977065 |
| PS1-only | 2617718066 | 11337182911 |
Attachments (5)
- coverage.g.png (42.2 KB ) - added by 15 years ago.
- coverage.r.png (38.0 KB ) - added by 15 years ago.
- coverage.i.png (43.1 KB ) - added by 15 years ago.
- coverage.z.png (42.8 KB ) - added by 15 years ago.
- coverage.y.png (42.6 KB ) - added by 15 years ago.
Download all attachments as: .zip





