The MegaPipe image stacking pipeline
The MegaPipe image stacking pipeline The MegaCam ugriz filter set
The MegaCam ugriz filter set
This page describes the MegaCam ugriz filters and contrasts them with the SDSS ugriz filters.
The filter curves presented here are produced using data from the Paris Supernova Cosmology Group.
The figure below shows the MegaCam ugriz filter set from the first (2003) and second (2007) generations. The light-coloured lines show the filters' responses. The labeled black lines show the response of the primary mirror, optics and the QE of the CCD's as obtained from the Paris Supernova Cosmology Group tarball. The grey line shows the astmospheric transmission. The filter responses are multiplied by the telescope (atomsphere+mirror+optics+CCD) response to obtain total transmissions for the whole system. These total transmissions are shown as the heavy coloured lines The labels i1 and i2 refer to the old (before June 2007) and new (after October 2007) i filters.
The figure below shows the MegaCam ugriz filter set from the third (2015) generation. The raw filter curves were retrieved from the CFHT MegaPrime Filter page.
The final response curves are given in text format below:
- uMega.fil Gen1 (u.MP9301)
- gMega.fil Gen1 (g.MP9401)
- rMega.fil Gen1 (r.MP9601)
- iMega.fil Gen1 (i.MP9701)
- zMega.fil Gen1 (z.MP9801)
- i2Mega.fil Gen2 (z.MP9702)
- u2Mega.fil Gen3 (u.MP9302)
- g2Mega.fil Gen3 (g.MP9402)
- r2Mega.fil Gen3 (r.MP9602)
- i3Mega.fil Gen3 (i.MP9703)
- z2Mega.fil Gen3 (z.MP9901)
Comparing the MegaCam and SDSS filter sets
The figure below shows the final MegaCam filter transmission functions. The same data for the SDSS ugriz filter set are shown in heavier lines. Note the MegaCam u and g filters are slightly redder than their SDSS counterparts.
The transformation between the Vega and AB magnitude system is different for the SDSS and MegaCam filters, particularly for the u. This is shown in the following table:
These numbers are computed for zero airmass.
The colour terms between the two filter sets can be described by the following equations:
u_Mega = u_SDSS - 0.241 (u_SDSS - g_SDSS) g_Mega = g_SDSS - 0.153 (g_SDSS - r_SDSS) r_Mega = r_SDSS - 0.024 (g_SDSS - r_SDSS) i_Mega = i_SDSS - 0.085 (r_SDSS - i_SDSS) (old) i_Mega = i_SDSS - 0.003 (r_SDSS - i_SDSS) (new) z_Mega = z_SDSS + 0.074 (i_SDSS - z_SDSS)
The relations for the griz bands (including the old i-filter) come from the analysis of the SNLS group. The relation for the u band comes from the CFHT MegaPipe web pages. The relation for the new i filter was calculated separately.
The reverse transformations (MegaCam to SDSS) have also been calculated.
u_SDSS=u_Mega +0.181 (u_Mega - g_Mega) g_SDSS=g_Mega +0.195 (g_Mega - r_Mega) g_SDSS=g_Mega +0.103 (g_Mega - i_Mega) r_SDSS=r_Mega +0.011 (g_Mega - r_Mega) i_SDSS=i_Mega +0.079 (r_Mega - i_Mega) (old) i_SDSS=i_Mega +0.044 (g_Mega - i_Mega) (old) i_SDSS=i_Mega +0.001 (r_Mega - i_Mega) (new) i_SDSS=i_Mega -0.003 (g_Mega - i_Mega) (new) z_SDSS=z_Mega -0.099 (i_Mega - z_Mega)
- Date modified: