The Sloan Digital Sky Survey monitor telescope pipeline
- Tucker, D.L.
- Kent, S.
- Richmond, M.W.
- Annis, J.
- Smith, J.A.
- Allam, S.S.
- Rodgers, C.T.
- Stute, J.L.
- Adelman-McCarthy, J.K.
- Brinkmann, J.
- Doi, M.
- Finkbeiner, Douglas
- Fukugita, M.
- Goldston, J.
- Greenway, B.
- Gunn, J.E.
- Hendry, J.S.
- Hogg, D.W.
- Ichikawa, S.-I.
- Ivezić, Ž.
- Knapp, G.R.
- Lampeitl, H.
- Lee, B.C.
- Lin, H.
- McKay, T.A.
- Merrelli, A.
- Munn, J.A.
- Neilsen, E.H.
- Newberg, H.J.
- Richards, G.T.
- Schlegel, D.J.
- Stoughton, C.
- Uomoto, A.
- Yanny, B.
DOIAbstract
The photometric calibration of the Sloan Digital Sky Survey (SDSS) is a multi-step process which involves data from three different telescopes: the 1.0-m telescope at the US Naval Observatory (USNO), Flagstaff Station, Arizona (which was used to establish the SDSS standard star network); the SDSS 0.5-m Photometric Telescope (PT) at the Apache Point Observatory (APO), New Mexico (which calculates nightly extinctions and calibrates secondary patch transfer fields); and the SDSS 2.5-m telescope at APO (which obtains the imaging data for the SDSS proper). In this paper, we describe the Monitor Telescope Pipeline, MTPIPE, the software pipeline used in processing the data from the single-CCD telescopes used in the photometric calibration of the ...
Add to ORKG