1. July 21, 2010 KIAA, PKU NAOC and Steward Observatory of UA The South Galactic Cap U-band Sky Survey Zhou FAN (NAOC)

2. Scientific Goals 1.Supplying the input catalogue for LAMOST (Guo Shoujing); 2.Classifications of the stars, galaxies, AGN and quasars in the south Galactic cap region with the color-color diagram; 3.Detecting the red shift z<3 quasar candidates combining the photometry in other bands; 4.Improving the accuracy of measuring the red shift of the galaxies with PhotoZ combining the photometry in other bands; 5.Searching for the starburst galaxies candidates; 6.Estimating the metallicity of the stellar populations in the galaxies; 7.Identifying the type of the stars in the color-color diagram combining the photometry in other bands, which can help us the control the completeness of the star type for the LAMOST observations; 8.For the flux calibration of the LAMOST spectra.

3. Color-color Diagram 图 1 ： SDSS 测光中的恒星（ × ），星系（△） 和类星体（其中红移 z< 3.5 的源用 □ 表示，红 移 z≥ 3.5 的源用 ■ 表示）的双色图。 图 2 ：不同类型的恒星在双色图上的位置是 不同的

4. Age Estimation  图 1 ： BC03 模型中太阳金属丰度下星族 的谱能量分布随年龄的变化。

5. Project Members PI: Xu Zhou (NAOC) PI: Michael Lesser (SO/UA) Edward Olszewski(UA) Xiaohui Fan(UA) Yipeng Jing(SHAO) Zhaoji Jiang(NAOC/PKU) Xuebin Wu(PKU) Weipeng Lin(SHAO) Shiyin Shen(SHAO) Zhou Fan(NAOC) Zhenyu Wu(NAOC) …….

6. The 90-inch Bok Telescope Organization: Steward Observatory. Location: Kitt Peak, Arizona, USA Wavelength: optical, infrared Diameter: 2.3m (90 inches)

7. Location―Kitt Peak Altitude: 6,900 ft (2071 m) Latitude: +31° 57' 46.5“ Longitude: 111°36' 01.6"W Time Zone: +7 hours

8. The Bok 90 inch (2.3 meter) Reflector Telescope The Telescope

9. Flat fielding

10. Telescope Control Room

11. New CCD Mosaic: ITL of UA

12. CCD configuration NAOC has spent $365,000 for the new CCD Mosaic according to the contract.

13. The 3×3 Pointing one field of view= 1.028 deg^2 Uncovered squre= 0.001 deg^2 0.141% 1 time cover= 0.116 deg^2 11.288% 2 time cover= 0.911 deg^2 88.571%

14. The Telescope Moving Speed in RA N1= 28 N2= 30 V_RA(+)= 6.50402451 SEC/DEG V_RA(-)= 7.75749779 SEC/DEG

15. The Telescope Moving Speed in DEC N1= 30 N2= 30 V_DEC(+)= 12.63 SEC/DEG V_DEC(-)= 12.56 SEC/DEG

16. The weather statistics of Bok

17. The seeing distributions of Bok

18. We have 55 nights, then Exp Time of Each Field=(55 nights ×10 hours / nights ×65% useful night )/ 3700deg^2=5.80 min/deg^2 Total Observation Time

19. Bok 300 s SDSS 53 s Comparison of Bok 300s exposure and SDSS in u band

20. Bok 300s: 1.5 mag deeper than SDSS Limiting Mag (S/N=10)= 21.91 — Limiting Mag (S/N=10)= 20.48 = 1.43 mag Limiting Mag (S/N= 5)= 22.68 — Limiting Mag (S/N= 5)= 21.09 = 1.59 mag

21. Bok 300s: 1.5 mag deeper than SDSS Limiting Mag (S/N=10)= 21.91 — Limiting Mag (S/N=10)= 20.39 = 1.52 mag Limiting Mag (S/N= 5)= 22.68 — Limiting Mag (S/N= 5)= 21.24 = 1.44 mag

22. The u-band Sky MAP Sep-Dec of 2010-2012

23. Survey Priority 6 dark nights / month from Sep to Dec

24. The Pan-Andromeda Archaeological Survey (PAndAS) PAndAS is an astronomical survey using the Canada-France- Hawaii Telescope, which will obtain g and i imaging of over 300 sq. degrees of the M31/M33 sub-group.Canada-France- Hawaii Telescope PI: Alan McConnachie

25. M31-M33 galactic interaction (gray nights)

26. Galactic Anti-center Survey (gray nights) Xuyi Schmidt telescope PI: Xiaowei Liu Bands: g r i

27. Flux calibration with SDSSIII

28. Color Term Examination

29. Flux Calibration: BATC 60/90 cm Schmidt Telescope >12e <4e RON <5%15 μm/pixel 1.7"/pixel 58’×58’ 2K × 2KOld Thick 92.2%12 μm/pixel 1.3"/pixel 93’×93’ 4K × 4KNew E2V BQE(~400nm)‏Pixel ScaleFOVSize

30. cp edo_a1413.0053.fits edo.fit ! for simple coord8 edo ! turn map, coordination, produce uedo.fit badline uedo ! bad line corrected -------------------------------------------------------------------------------- sex uedo.fit ! produce test.cat 1538 chbercoo uedo ! produce uedo.coo, delete edge 10 line 1271 pip231 uedo 1245 coo2als uedo ! putcoo uedo coo2als.dat, will delete it 4 checkmis uedo ! produce miss.dat, all missed are cosmos 26 getcosmos uedo ! from uedo.als <-10, produce cosmos.dat, 107 ! reorder uedo.coo, count in coo2als.dat 1164 pip231 uedo 1163 coo2als uedo ! 0 checkmis uedo ! 108 getcosmos uedo ! cosmos.dat 109 ! uedo.coo 1162 pip231 uedo ! 1162 -------------------------------------------------------------------------------- putcoo uedo cosmos.dat ! produce uedocosmos.fit putcoo uedo uedo.als ! produce uedoals.fit ds9 uedocosmos.fit ds9 uedoals.fit uedo.fits dispsfber uedo 5 -------------------------------------------------------------------------------- extrcat uedo ! extract..from test.cat & uedo.als, prod uedo.ext lastcat uedo [1.0] ! [1.0] is sharpness Data Reduction Catalogues

31. Photometry Comparisons

32. Thanks! Welcome to visit us: http://batc.bao.ac.cn/Uband/