06.09.2014 Views

Documentation [PDF] - Canada France Hawaii Telescope ...

Documentation [PDF] - Canada France Hawaii Telescope ...

Documentation [PDF] - Canada France Hawaii Telescope ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

filter u g r i.MP9701 (i) i.MP9702 (y) z<br />

m ab 10.211 9.592 9.343 9.253 9.256 9.241<br />

m bd17 9.769 9.691 9.218 8.914 8.947 8.774<br />

δ ab 0.442 -0.099 0.125 0.339 0.309 0.467<br />

Table 2: Offsets between AB magnitudes and the SNLS Vega-based MegaCam calibration.<br />

It follows that the AB offsets required to bring SNLS magnitudes to AB system, δ ab = m ab − m |x0 , are :<br />

δ ab = −2.5 log 10<br />

∫<br />

λT(λ)φbd17 (λ)dλ<br />

∫<br />

λT(λ)φab (λ)dλ − m bd17 (10)<br />

The pixels in the images are scaled following this relation:<br />

p AB = p VEGA × 10 0.4×δ AB<br />

(11)<br />

3.8 Final catalogue production<br />

In the Wide and Deep surveys, a .ldac SExtractor source catalogue is produced immediately after the<br />

final rescaling of the stacks (using L99 images for the Wide and the SNLS standard star catalogue for<br />

the Deep). The T0007 Wide and Deep .ldac source catalogues have been produced using a 128 pixels<br />

mesh size to derive the local sky background (BACK_SIZE parameter in SExtractor). These catalogues<br />

are the inputs of the QFITS-out processing. The SExtractor configuration file for the production of<br />

the T0007 .ldac catalogues are presented in Appendix B.2.4 and Appendix A.3.4 for Wide and Deep<br />

respectively.<br />

After the production of the chi2 image, SExtractor is run in dual-image mode on the u ∗ g, r, i, y and z<br />

stacks using the chi2 image as reference. The Wide and Deep chi2 .cat catalogues are produced with a<br />

using a background mesh size in SExtractor of 256 pixels. All catalogues contain parameter values for<br />

all quantities listed in Tables 28, 29 and 30. For each source, aperture magnitudes are computed within<br />

27 (26+SNLS) apertures, following same procedure as for the previous T0006 release. The SExtractor<br />

configuration file used for the production of the T0007 .cat dual-image mode catalogues is listed in the<br />

Appendix B.2.5 and Appendix A.3.5 for Deep and Wide surveys respectively. Based on its measured<br />

MAG_SNLS, each source is corrected for aperture, leading to the MAG_IQ20 magnitude.<br />

Additionally, for each survey pointing, the following data products are produced:<br />

• a (u, g, r , i/y, z) Wide or (u, g, r , i,y, z)-merged Deep catalogues that includes a restricted number<br />

of parameters. These catalogues are produced in two versions with either MAG_AUTO, MAG_SNLS<br />

and MAG_IQ20 magnitudes. They also contain the E(B − V) value at each source position derived<br />

from dust map images (Schlegel et al., 1998) and the dk cell number for the given position on<br />

the image, an estimate of a second order term of the photometric flatness of the image, meant to<br />

account for the slight variation in bandwidth of the MegaCam filters from center to edge. See<br />

Regnault et al. (2009) for a full explanation. Since it did not bring any significant gain, the dk term<br />

is not used within T0007.<br />

• a (u, g, r , i/y, z)-merged Wide, or (u, g, r, i, y, z)-merged Deep multi-aperture (.ape) extended<br />

catalogue that only includes the data concerning the 27 MAG_APER informations in all filters.<br />

25

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!