From: Natalia Kuznetsova (nvkuznetsova@lbl.gov)
Date: Sat Apr 03 2004 - 20:05:43 PST
Hi Vitaliy,
For sub04mar/mar172004suprimeb28956sum.fts and GOODS field 24, I get the
average ratio of Subaru to GOODS fluxes of 51900.
For sub04mar/mar172004suprimef28956sum.fts and GOODS field 34, I get the
average ratio of Subaru to GOODS fluxes of 40688.
Natalia
Vitaliy Fadeyev wrote:
>Rob,
>
>Natalia, Lifan and I are going to do this now.
>
>vitaliy
>
>
>
>"Robert A. Knop Jr." wrote:
>
>
>
>>At some point (probably not until late late tonight) Subaru I-band
>>subtractions will start showing up.
>>
>>These are the zeropoints that will be used for them:
>>
>> sub04mar/mar172004suprimea28956sum.fts | 38.1048017998
>> sub04mar/mar172004suprimeb28956sum.fts | 38.1206147516
>> sub04mar/mar172004suprimec28956sum.fts | 37.131587848
>> sub04mar/mar172004suprimed28956sum.fts | 36.8684151492
>> sub04mar/mar172004suprimef28956sum.fts | 37.7517776011
>> sub04mar/mar172004suprimee28956sum.fts | 37.5677277862
>> sub04mar/mar172004suprimeg28956sum.fts | 37.3110273633
>> sub04mar/mar172004suprimeh28956sum.fts | 37.2026060372
>> sub04mar/mar172004suprimei28956sum.fts | 37.5857562505
>> sub04mar/mar172004suprimej28956sum.fts | 36.4820993053
>> ^
>> |
>>
>>The indicated letter is the chip of the subtraction.
>>
>>These zeropoints are completely bogus. (They are based on the R
>>magnitudes from the USNO catalog and should not be trusted to better
>>than a magnitude or two.) I need somebody to figure out a reasonable
>>zeropoint for these images. At that point, we will need to adjust any
>>magnitudes that come off of the Subaru subtractions by the *difference*
>>between this zeropoint and the real zeropoint determined for these
>>images.
>>
>>These are I-band images. You can get at them with
>>
>> finddbfile -g <filename>
>>
>>or
>>
>> imview -scp <filename>
>>
>>Note that the night was decidedly not photometric, so just taking a
>>published Suprime-Cam zeropoint won't work. (Plus, I'm not sure about
>>the units of this sum.) We have to do something empirical to get a
>>vega-based zeropoint for these imgaes. Perhaps match and compare to
>>GODOS images (whose zeropoints *should* be good), or perhaps match and
>>compare to pre-existing calibrated data.
>>
>>This will be a painful hand-work task, and I don't have time to do it.
>>
>>The same may eventually need to be done for the subaru z-band images.
>>
>>-Rob
>>
>>--
>>--Prof. Robert Knop
>> Department of Physics & Astronomy, Vanderbilt University
>> robert.a.knop@vanderbilt.edu
>>
>>
>
>
>
-- ______________________ Natalia Kuznetsova Lawrence Berkeley National Laboratory 1 Cyclotron Road, MS 50R5032 Berkeley, CA 94720-8164 Tel: (510) 486-4877 FAX: (510) 486-7115 ______________________
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