Picture: Hubble Deep Field-North. (CFHT WIRCam Ks; Spitzer IRAC 3.6+4.5 micron; Spitzer IRAC 5.8+8.0 micron.)
Picture: Hubble Deep Field-North. (CFHT WIRCam Ks; Spitzer IRAC 3.6+4.5 micron; Spitzer IRAC 5.8+8.0 micron.)
Paper: 2010, ApJS, 187, 251
Data Release:
Ultradeep Ks Imaging in the GOODS-N and a Combined Ks and IRAC Catalog
Data Product v2 |
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| File | Size (KB) | Description |
| HDF_K_uJy.fits.gz | 406884 | WIRCam Ks-band image |
| HDF_K_time.fits.gz | 231976 | Exposure time map for the Ks-band image |
| table3_ver2.txt.gz | 1908 | Ks-Selected Multi-Band Catalog (Table 3) |
| table5_ver2.txt.gz | 12 | IRAC Sources without Ks Counterparts (Table 5) |
| table6_ver2.txt.gz | 420 | Ks-to-IRAC Colors Derived with Cross-Convolution (Table 6) |
Data Product v1 |
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| File | Size (KB) | Description |
| HDF_K_uJy.fits.gz | 406908 | WIRCam Ks-band image |
| HDF_K_time.fits.gz | 232032 | Exposure time map for the Ks-band image |
| Ks_WIRCAM.ASC.gz | 10836 | Raw SExtractor (2.5.0) Ks catalog |
| default.param | 4 | SExtractor output parameter file |
| default.sex | 4 | SExtractor configuration file |
| table3.txt.gz | 1904 | Ks-Selected Multi-Band Catalog (Table 3) |
| table5.txt.gz | 12 | IRAC Sources without Ks Counterparts (Table 5) |
| table6.txt.gz | 420 | Ks-to-IRAC Colors Derived with Cross-Convolution (Table 6) |
Important!
Typos in the paper |
1. The conversion between AB magnitude and flux should be AB = 23.9 - 2.5log(uJy) |
2. In Section 7.4, Ks and IRAC Color-Color Diagrams, the third equation should be log(F4.5/FKs) > 3.0 log(F4.5/F3.6) + 0.26 |
Data Pipeline |
| SIMPLE Imaging and Mosaicking PipeLinE |
Contact: Wei-Hao Wang