Date: Fri, 4 Jun 1999 07:59:58 -0600 From: long@apo.nmsu.edu (Dan Long) Subject: 2.5m obslog 990603 ( MJD 51333 ) THURSDAY JUNE 3, 1999 APACHE POINT OBSERVATORY SDSS 2.5m OBSERVING LOG Observering team: Dan Long (APO) Jeff Hayes (APO) Ellyne Kinney (APO) After last night's poor model, the scraping sound when moving the primary, and the conical baffle coming loose, we were looking for some good news. We got some! The source of the scraping sound was found and removed, and I took a 70 point model which had a sky rms of 1.4 arcseonds! Jeff and Ellyne mounted the spectrographic cartridge for FASTT field L and got the fiducials set in the evening twilight. Az: 120:45:46.957 Alt: 14:53:09.490 Rot: 0:59:38.003 French came back in around 22:30 and listened while I homed the primary. He tracked the scraping sound to the number 2 astigmatism actuator. When it was removed, it was found that the piston was damaged, and was the source of the scraping sound, rather than the primary. The damaged actuator was left out, but the astigmatism corrector was left on. At this point it was a little after 23:00. Given the time and the removal of the damaged actuator it was best to continue to improve or at least characterize the pointing. With Matt Newcomb's help, I switched to the engineering camera ( including the swapping of kinematic mounts ). Balance was at a counterweight setting of 330. I was on the sky by 00:30. The first thing I did was home and relax the primary. Next, I took a focus sweep consisting of -400, -50, 0, 50, and 400 units out of focus. I then homed the secondary and repeated the sweep. The images are in /data/spectro/guider on sdsshost, and are called 990603_*. The ones called 990603_ah* are the sweep after homing the secondary. There is considerably less coma in these images compared to last night, but it is not entirely absent. I decided not to tweak the coma adjustment until the astigmatism corrector is back to its full compliment of actuators. MIRROR NUMBERS Primary: setmir: 0 3.9 -2.3 -128 -214 galil: 4350 -1750 0 16300 -11550 -11450 The linear gauges after setting to above position and relaxing 1.9325 0.5555 0.5575 0.4220 1.8850 0.3845 Secondary: SecOrient=-1400.0, -219.4, -100.0, -50.0, -44.8 El=58.0 homing secondary yielde the following errors. -000020000, -000010000, -000010000, 000000350, 000000150 position error I then proceeded to repeat last night's 70 point grid collecting pointing model data. I also found a value for the change in piston of the secondary versus elevation, by focusing on the first dozen points of the model. A number for the sin component of SecPistCoef of about -380 was found, and I added that to DEFAULT.DAT. I then observed the focus during the rest of the model, and saw that it remained within about 25 microns of the compensated value. The grid was completed at about 05:20. I closed up at that point, and went to check the data set ( not without some trepidation ). However, the first fit to existing coefficients and removing no points yielded a 2.5 arcsecond rms. By adding some terms and removing two outliers, I got the fit down to 1.4 arcseconds. I output the model listed below coeff change value sigma 1 IE -179.119 -179.12 0.517 2 IA -232.665 -232.66 0.860 3 PZZ1 -129.527 -129.53 0.658 4 AN -6.502 -6.50 0.371 5 AW -54.314 -54.31 0.351 6 CA +13.131 +13.13 0.588 7 ACEC -4.813 -4.81 0.715 8 ACES -0.904 -0.90 0.735 9 HWSA2 +3.956 +3.96 0.780 10 HWCA2 -2.271 -2.27 0.383 11 HXSA2 -3.261 -3.26 0.606 12 HNSA2 +0.628 +0.63 0.430 13 HNCA2 +1.678 +1.68 0.409 14 HZSA2 -1.027 -1.03 0.254 15 HZCA2 +0.574 +0.57 0.241 Sky RMS = 1.43 Popn SD = 1.62 I noticed during tonight's model as well as last night's, that the windscreen azimuth is quite jittery, more so than I remember it being recently, and _much_ more than when motor 3 was removed to power the altitude. Maybe we should run with just 1 and 2 all the time? :) WEATHER Weather tonight was clear or mostly clear all night. Winds were southwesterly at 10 to 20 MPH, temperatures were 11 to 14 C, the dewpoint depression was between 20 and 31 C, dust counts were less than 1000. Dan