Date: Sat, 1 May 1999 05:43:19 -0600 From: long@apo.nmsu.edu (Dan Long) Subject: 2.5m obslog 990430 ( MJD 51299 ) FRIDAY APRIL 30, 1999 APACHE POINT OBSERVATORY SDSS 2.5m OBSERVING LOG The fiber cartridge and corrector are on the telescope, as well as the guider electronics box. Tonight's goal was to get light down the fibers and work on the instrument block. We got starlight, and collected some data which hopefully can be used to generate the instrument block. The first thing we found was that the instrument block for the engineering camera had a rotation 180 degrees off from what the cartridge needed. So I created an instrument block called SPECTRO which had rot_inst_ang 180 degrees from that for the engineering camera. We tried slewing to field containing guide stars, and could not see anything. We then decided to go to Vega and place it on two of the fiber positions. We found the star after a little offsetting. We also found the focus was around +3400, which explains in part why we could never see the 14th and 15th magnitude guide stars with the focus anywhere between +/- 2000. We collected data which I hope will allow the generation of an instrument block for the guider. I started by slewing to Vega, which should put it at the boresight. Coordinates are 279.1883, 38.7783 fk5=1993.5. All data were collected with rotator at 0 object using the SPECTRO instrument block. The first fiber position is offset from the boresight by -0.27713, -0.10787 degrees on the sky. I slewed the telescope to 279.4845, 38.8862 fk5=1993.5 in order to put Vega down that fiber. It took object offsets of .0525, -.009 to center it on the fiber. The resulting position is 279.5370, 38.8772 fk5=1993.5. The second fiber position is offset from the boresight by 0.18376, .40000 degrees on the sky. I slewed the telescope to 279.0045, 38.3783 fk5=1993.5, and had to offset by -.0820, .0055 object to center Vega. The resulting position is 278.9225, 38.3838 fk5=1993.5. Russell, do you think it is possible to take this data and back out the translation, rotation, and scale for the instrument block? It seems that with two points one should be able to at least determine the boresight offset and rotation. Note that once tonight the MCP hung while moving the rotator. I could not get ctrl-x to reboot, so the reset button was pushed. The rotator fiducial is still wrong, so we set the rotator zero by aligning the pointer and mark on the back of the telescope. The wider azimuth stow angle sure is nice. It made putting the telescope away much easier. Thanks Glenn et al. One final note is that we tracked Vega for nearly an hour at one of the fiber positions, and noticed only a slight drift. This should easily be taken out by guiding once a proper instrument block is generated. Dan