=============================================================================== 2003 0301 Contained 10 biases, skyflats B,V, # IMAGE NPIX MEAN STDDEV MIN MAX ccd030301ccdskyflatb.0005 1080428 57064. 10892. 0. 65535. ccd030301ccdskyflatb.0006 1080428 43040. 8235. 0. 65535. ccd030301ccdskyflatb.0007 1080428 30070. 5812. 0. 65535. ccd030301ccdskyflatb.0008 1080428 22716. 4462. 0. 65535. ccd030301ccdskyflatb.0009 1080428 23575. 4621. 0. 65535. ccd030301ccdskyflatb.0010 1080428 14105. 2766. 0. 47570. Did not include ccd030301ccdskyflatb.0005 in IMCOMBINE because mean > 45,000. ccd030301.skyflatb 1080428 26514. 5198. 1. 69650. ccd030301ccdskyflatv.0001 1080428 7879. 1418. 0. 23629. ccd030301ccdskyflatv.0002 1080428 6958. 1250. 0. 20902. ccd030301ccdskyflatv.0003 1080428 7063. 1299. 0. 65535. ccd030301.skyflatv 1080428 7109. 1300. 1. 21737. For R,I used: ccd030228.skyflatr.fits ccd030228.skyflati.fits No U was necessary since there were no U object images. =============================================================================== 2003 0302 Contained 10 biases, no skyflats, no U filter objects For B,V,R,I used: ccd030301.skyflatb ccd030301.skyflatv ccd030228.skyflatr ccd030228.skyflati =============================================================================== 2003 0303 Contained 10 biases, skyflats U,R,I, no U filter objects (for Uflat processing, see 2003 0305). # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatr.0001 1080428 63597. 10814. 0. 65535. ccdskyflatr.0002 1080428 63473. 10897. 0. 65535. ccdskyflatr.0003 1080428 59935. 10846. 0. 65535. ccdskyflatr.0004 1080428 45176. 8180. 0. 65535. ccdskyflatr.0005 1080428 34808. 6328. 0. 65535. ccdskyflatr.0006 1080428 26899. 4939. 0. 65535. ccdskyflatr.0007 1080428 20224. 3707. 0. 58129. ccdskyflatr.0008 1080428 14431. 2639. 0. 47534. Did not include ccdskyflatr.0001,0002,0003,0004 in IMCOMBINE because mean > 45K ccd030303.skyflatr 1080428 24092. 4413. 0. 63747. ccdskyflati.0001 1080428 14425. 2724. 0. 58324. ccdskyflati.0002 1080428 12126. 2318. 0. 49210. ccdskyflati.0003 1080428 18806. 3573. 0. 65535. ccdskyflati.0004 1080428 23283. 4429. 0. 65535. ccdskyflati.0005 1080428 24276. 4649. 0. 65535. ccdskyflati.0006 1080428 18489. 3508. 0. 65535. ccd030303.skyflati 1080428 18566. 3524. 0. 64470 For B,V used: ccd030301.skyflatb ccd030301.skyflatv =============================================================================== 2003 0304 Contained 10 biases, skyflats B,V, U filter images were not those we currently process so ignored; (retroactively, used ccd030303.skyflatu). # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatb.0004 1080428 63743. 10509. 0. 65535. ccdskyflatb.0005 1080428 63600. 10864. 0. 65535. ccdskyflatb.0006 1080428 63484. 10995. 0. 65535. ccdskyflatb.0007 1080428 63095. 11261. 0. 65535. ccdskyflatb.0008 1080428 52811. 10101. 0. 65535. ccdskyflatb.0009 1080428 40906. 7837. 0. 65535. ccdskyflatb.0010 1080428 31347. 6051. 0. 65535. ccdskyflatb.0011 1080428 24263. 4751. 0. 65535. ccdskyflatb.0012 1080428 18345. 3608. 0. 62460. ccdskyflatb.0013 1080428 12797. 2507. 0. 43061. ccdskyflatb.0014 1080428 9853. 1924. 0. 32748. ccdskyflatb.0015 1080428 14127. 2774. 0. 47873. Did not include ccdskyflatb.0004thru0008 sicne mean exceeded 45,000. ccd030304.skyflatb 1080428 21671. 4232. 0. 64466 ccdskyflatv.0001 1080428 7720. 1394. 0. 23199. ccdskyflatv.0002 1080428 8530. 1543. 0. 25665. ccdskyflatv.0003 1080428 10540. 1912. 0. 32202. ccd030304.skyflatv 1080428 8929. 1615. 0. 26860 For R,I used: ccd030303.skyflatr ccd030303.skyflati 03/13/03 V's REDONE because found there was error in making ccd030304.skyflatv. cc> cat flat.v ccdskyflatv.0001.fits ccdskyflatv.0002.fits ccdskyflatv.0003.fits cc> imcombine @flat.v List of output images (ccd030304.bias): ccd030304.skyflatv # IMAGE NPIX MEAN STDDEV MIN MAX ccd030304.skyflatv 1080428 8929. 1615. 0. 26860. Renamed correct030304.skyflatv.fits =============================================================================== 2003 0305 Contained 10 biases, no skyflats For B,V,R,I used: ccd030304.skyflatb ccd030304.skyflatv ccd030303.skyflatr ccd030303.skyflati For U, took the U object images and the bias and skyflatu from 20030303 and ran them all through ccdproc. This had to be done so that the skyflatu would be processed with its bias. Then threw out the processed U object images and reprocessed them with ccd030305.bias and the (processed) ccd030303.skyflatu. # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatu.0001 1080428 42711. 9135. 0. 65535. ccdskyflatu.0002 1080428 37474. 8006. 0. 65535. ccdskyflatu.0003 1080428 31838. 6814. 0. 65535. ccdskyflatu.0004 1080428 26070. 5618. 0. 65535. ccdskyflatu.0005 1080428 21942. 4763. 0. 65535. ccdskyflatu.0006 1080428 20622. 4488. 0. 65535. ccdskyflatu.0007 1080428 16386. 3564. 0. 60866. ccd030303.skyflatu 1080428 28156. 6060. 0. 70318. 3/13/03 V's REDONE because found there was error in making ccd030304.skyflatv. See above under 20030304. =============================================================================== 2003 0306 Contained 10 biases, skyflats U,R,I and objects in UBVRI # IMAGE NPIX MEAN STDDEV MIN MAX ccd030306skyu.0001 1080428 16980. 3937. 0. 65535. ccd030306skyu.0002 1080428 28202. 6430. 0. 65535. ccd030306skyu.0003 1080428 19739. 4594. 0. 65535. ccd030306skyu.0004 1080428 20642. 4790. 0. 65535. ccd030306.skyflatu 1080428 21394. 4965. 0. 69463. ccd030306skyr.0001 1080428 46717. 8469. 0. 65535. ccd030306skyr.0002 1080428 17571. 3222. 0. 50216. ccd030306skyr.0003 1080428 21432. 3928. 0. 62317. ccd030306skyr.0004 1080428 19739. 3635. 0. 56995. ccd030306skyr.0005 1080428 21352. 3912. 0. 61394. Did not include ccd030306skyr.0001 because mean exceeded 45,000. ccd030306.skyflatr 1080428 20024. 3673. 0. 57684. ccd030306skyi.0001 1080428 11108. 2091. 0. 44314. ccd030306skyi.0002 1080428 18902. 3575. 0. 65535. ccd030306skyi.0003 1080428 21632. 4100. 0. 65535. ccd030306skyi.0004 1080428 16963. 3247. 0. 65535. For B,V, used: ccd030304.skyflatb ccd030304.skyflatv 3/13/03 V's REDONE because found there was error in making ccd030304.skyflatv. See above under 20030304. =============================================================================== 2003 0307 Contained 10 biases, skyflats B,V and objects in U,B,V,R,I # IMAGE NPIX MEAN STDDEV MIN MAX ccd030307skyb.0002 1080428 15651. 3158. 0. 52992. ccd030307skyb.0003 1080428 19054. 3855. 0. 64685. ccd030307skyb.0004 1080428 18520. 3746. 0. 63557. ccd030307skyb.0005 1080428 21198. 4294. 0. 65535. ccd030307.skyflatb 1080428 18606. 3762. 0. 63082. ccd030307skyv.0001 1080428 8655. 1573. 0. 47227. ccd030307skyv.0002 1080428 11308. 2053. 0. 53935. ccd030307skyv.0003 1080428 9300. 1690. 0. 57388. ccd030307.skyflatv 1080428 9752. 1760. 0. 29612. For U,R,I used: ccd030306.skyflatu ccd030306.skyflatr ccd030306.skyflati =============================================================================== 2003 0308 Contained 10 biases, no skyflats, objects in B,V,R,I (no U) For U,B,V,R,I used: ccd030306.skyflatu (not needed) ccd030307.skyflatb ccd030307.skyflatv ccd030306.skyflatr ccd030306.skyflati =============================================================================== 2003 0309 Contained 10 biases, skyflats U,R,I and objects in B,V,R,I (no U) # IMAGE NPIX MEAN STDDEV MIN MAX ccd030309skyr.0001 1080428 42280. 7695. 0. 65535. ccd030309skyr.0002 1080428 13707. 2515. 0. 39314. ccd030309skyr.0003 1080428 18880. 3474. 0. 54535. ccd030309skyr.0004 1080428 25608. 4716. 0. 65535. ccd030309skyr.0005 1080428 24781. 4566. 0. 65535. ccd030309.skyflatr 1080428 25059. 4613. 0. 67439. ccd030309skyi.0001.fits 1080428 12253. 2306. 0. 49077. ccd030309skyi.0002.fits 1080428 16431. 3103. 0. 65535. ccd030309skyi.0003.fits 1080428 13020. 2461. 0. 65535. ccd030309.skyflati 1080428 13900. 2618. 0. 55487. For B,V used: ccd030307.skyflatb ccd030307.skyflatv =============================================================================== 2003 0310 Contained 10 biases, skyflats B,V and objects in U,B,V,R,I # IMAGE NPIX MEAN STDDEV MIN MAX ccd030310skyb.0002.fits 1080428 24504. 4807. 0. 65535. ccd030310skyb.0003.fits 1080428 21225. 4192. 0. 65535. ccd030310skyb.0004.fits 1080428 22971. 4525. 0. 65535. ccd030310.skyflatb 1080428 22900. 4509. 0. 65354. ccd030310skyb.0002.fits 1080428 24504. 4807. 0. 65535. ccd030310skyb.0003.fits 1080428 21225. 4192. 0. 65535. ccd030310skyb.0004.fits 1080428 22971. 4525. 0. 65535. ccd030310.skyflatv 1080428 15786. 2866. 0. 48546 For U,R,I used: ccd030306.skyflatu.fits ccd030309.skyflatr.fits ccd030309.skyflati.fits DEFECTIVE CD meant that *some* of these had to be reprocessed. These were OK: rccd030310.0001.fits rccd030310.0012.fits rccd030310.0023.fits rccd030310.0002.fits rccd030310.0013.fits rccd030310.0024.fits rccd030310.0003.fits rccd030310.0014.fits rccd030310.0025.fits rccd030310.0004.fits rccd030310.0015.fits rccd030310.0026.fits rccd030310.0005.fits rccd030310.0016.fits rccd030310.0027.fits rccd030310.0006.fits rccd030310.0017.fits rccd030310.0028.fits rccd030310.0007.fits rccd030310.0018.fits rccd030310.0029.fits rccd030310.0008.fits rccd030310.0019.fits rccd030310.0030.fits rccd030310.0009.fits rccd030310.0020.fits rccd030310.0031.fits rccd030310.0010.fits rccd030310.0021.fits rccd030310.0011.fits rccd030310.0022.fits The rest had to be redone. Used ccd030306.skyflatu taken from CD ccd030309.skyflati ccd030309.skyflatr ccd030310.bias.fit ccd030310.skyflatb ccd030310.skyflatv =============================================================================== 2003 0311 Contained 10 biases, no skyflats, and objects in U,B,V,R,I For U,B,V,R,I used: ccd030306.skyflatu ccd030310.skyflatb ccd030310.skyflatv ccd030309.skyflatr ccd030309.skyflati =============================================================================== 2003 0312 Contained 10 biases, skyflats U,R,I and objects in U,B,V,R,I # IMAGE NPIX MEAN STDDEV MIN MAX ccd030312skyu.0001.fits 1080428 21135. 4790. 0. 65535. ccd030312skyu.0002.fits 1080428 22566. 5095. 0. 65535. ccd030312skyu.0003.fits 1080428 20550. 4665. 0. 65535. ccd030312skyu.0004.fits 1080428 22515. 5088. 0. 65535. cl> cat flat.u ccd030312skyu.0001.fits ccd030312skyu.0002.fits ccd030312skyu.0003.fits ccd030312skyu.0004.fits cl> imcombine @flat.u List of output images (ccd030312.bias): ccd030312.skyflatu ccd030312.skyflatu 1080428 21691. 4907. 0. 65189. ccd030312skyr.0001.fits 1080428 31410. 5730. 0. 65535. ccd030312skyr.0002.fits 1080428 12683. 2317. 0. 47729. ccd030312skyr.0003.fits 1080428 23120. 4246. 0. 65535. ccd030312skyr.0004.fits 1080428 20868. 3829. 0. 60582. ccd030312skyr.0005.fits 1080428 18387. 3369. 0. 52775. cl> cat flat.r ccd030312skyr.0001.fits ccd030312skyr.0002.fits ccd030312skyr.0003.fits ccd030312skyr.0004.fits ccd030312skyr.0005.fits cl> imcombine @flat.r List of output images (ccd030312.skyflatu): ccd030312.skyflatr ccd030312.skyflatr 1080428 21297. 3906. 0. 60725. ccd030312skyi.0001.fits 1080428 10724. 2024. 0. 65535. ccd030312skyi.0002.fits 1080428 10921. 2054. 0. 43692. ccd030312skyi.0003.fits 1080428 14479. 2737. 0. 65535. cl> cat flat.i ccd030312skyi.0001.fits ccd030312skyi.0002.fits ccd030312skyi.0003.fits cl> imcombine @flat.i List of output images (ccd030312.skyflatr): ccd030312.skyflati cl> imstat ccd030312.skyflati ccd030312.skyflati 1080428 12041. 2265. 0. 48183. For U,B,V,R,I used: ccd030310.skyflatb ccd030310.skyflatv hsel ccd030312.0* $I 'ccdfltid?="U"' > in.u hsel ccd030312.0* $I 'ccdfltid?="V"' > in.v hsel ccd030312.0* $I 'ccdfltid?="B"' > in.b hsel ccd030312.0* $I 'ccdfltid?="R"' > in.r hsel ccd030312.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r" $1}' in.u > out.u !awk '{print "r" $1}' in.b > out.b !awk '{print "r" $1}' in.v > out.v !awk '{print "r" $1}' in.r > out.r !awk '{print "r" $1}' in.i > out.i =============================================================================== 2003 0313 Contained NO biases, skyflats B,V and objects in U,B,V,R,I For U,B,V,R,I used: ccd030312.skyflatu ccd030310.skyflatb ccd030310.skyflatv ccd030312.skyflatr ccd030312.skyflati For bias, used ccd030312.bias. hsel ccd030313.0* $I 'ccdfltid?="U"' > in.u hsel ccd030313.0* $I 'ccdfltid?="B"' > in.b hsel ccd030313.0* $I 'ccdfltid?="V"' > in.v hsel ccd030313.0* $I 'ccdfltid?="R"' > in.r hsel ccd030313.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r"$1}' in.u > out.u !awk '{print "r"$1}' in.b > out.b !awk '{print "r"$1}' in.v > out.v !awk '{print "r"$1}' in.r > out.r !awk '{print "r"$1}' in.i > out.i DEFECTIVE CD meant that *some* of these had to be reprocessed. These were OK: rccd030313.0001.fits rccd030313.0009.fits rccd030313.0017.fits rccd030313.0002.fits rccd030313.0010.fits rccd030313.0018.fits rccd030313.0003.fits rccd030313.0011.fits rccd030313.0019.fits rccd030313.0004.fits rccd030313.0012.fits rccd030313.0020.fits rccd030313.0005.fits rccd030313.0013.fits rccd030313.0021.fits rccd030313.0006.fits rccd030313.0014.fits rccd030313.0022.fits rccd030313.0007.fits rccd030313.0015.fits rccd030313.0023.fits rccd030313.0008.fits rccd030313.0016.fits The rest had to be redone. Used ccd030310.skyflatb ccd030310.skyflatv ccd030312.skyflati ccd030312.skyflatr ccd030312.skyflatu =============================================================================== 2003 0314 NO biases again, no skyflats, and objects in U,B,V,R,I For U,B,V,R,I used: ccd030312.skyflatu ccd030310.skyflatb ccd030310.skyflatv ccd030312.skyflatr ccd030312.skyflati For bias, used ccd030312.bias. hsel ccd030314.0* $I 'ccdfltid?="U"' > in.u hsel ccd030314.0* $I 'ccdfltid?="B"' > in.b hsel ccd030314.0* $I 'ccdfltid?="V"' > in.v hsel ccd030314.0* $I 'ccdfltid?="R"' > in.r hsel ccd030314.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r"$1}' in.u > out.u !awk '{print "r"$1}' in.b > out.b !awk '{print "r"$1}' in.v > out.v !awk '{print "r"$1}' in.r > out.r !awk '{print "r"$1}' in.i > out.i =============================================================================== 2003 0315 Contained ten biases, skyflats U,R,I and objects in U,B,V,R,I # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatu.0001.fits 1080428 13420. 3048. 0. 52179. ccdskyflatu.0002.fits 1080428 10922. 2472. 0. 41925. ccdskyflatu.0003.fits 1080428 15534. 3540. 0. 60611. cl> hsel @flat.u $I,title,ccdfltid boolean expression governing selection (yes): ccdskyflatu.0001.fits "Sky flat u" U ccdskyflatu.0002.fits "Sky flat u" U ccdskyflatu.0003.fits "Sky flat u" U cl> imcombine @flat.u List of output images (ccd030315.bias): ccd030315.skyflatu # IMAGE NPIX MEAN STDDEV MIN MAX ccd030315.skyflatu 1080428 13292. 3019. 0. 51698. # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatr.0001.fits 1080428 63723. 10715. 0. 65535. ccdskyflatr.0002.fits 1080428 51682. 9299. 0. 65535. ccdskyflatr.0003.fits 1080428 38071. 6875. 0. 65535. ccdskyflatr.0004.fits 1080428 28146. 5131. 0. 65535. ccdskyflatr.0005.fits 1080428 21475. 3931. 0. 62432. ccdskyflatr.0006.fits 1080428 24788. 4539. 0. 65535. Dropped ccdskyflatr.0001 and .0002 because mean exceeded 45,000 cl> hsel @flat.r $I,title,ccdfltid boolean expression governing selection (yes): ccdskyflatr.0003.fits "Sky flat r" R ccdskyflatr.0004.fits "Sky flat r" R ccdskyflatr.0005.fits "Sky flat r" R ccdskyflatr.0006.fits "Sky flat r" R cl> imcombine @flat.r List of output images (ccd030315.skyflatu): ccd030315.skyflatr # IMAGE NPIX MEAN STDDEV MIN MAX ccd030315.skyflatr 1080428 28124. 5137. 0. 69918. # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflati.0001.fits 1080428 20707. 3916. 0. 65535. ccdskyflati.0002.fits 1080428 14670. 2764. 0. 60054. ccdskyflati.0003.fits 1080428 16431. 3100. 0. 65535. cl> hsel @flat.i $I,title,ccdfltid boolean expression governing selection (yes): ccdskyflati.0001.fits "Sky flat i" I ccdskyflati.0002.fits "Sky flat i" I ccdskyflati.0003.fits "Sky flat i" I cl> imcombine List of images to combine (@flat.r): @flat.i List of output images (ccd030315.skyflatr): ccd030315.skyflati cl> imstat ccd030315.skyflati # IMAGE NPIX MEAN STDDEV MIN MAX ccd030315.skyflati 1080428 17269. 3258. 0. 68892. For B,V used: ccd030310.skyflatb ccd030310.skyflatv cl> cat bias.list ccdbias.0001.fits ccdbias.0002.fits ccdbias.0003.fits ccdbias.0004.fits ccdbias.0005.fits ccdbias.0006.fits ccdbias.0007.fits ccdbias.0008.fits ccdbias.0009.fits ccdbias.0010.fits cl> imcombine @bias.list List of output images (ccd030224.bias): ccd030315.bias Something was wrong with image ccd030315.0001.fits RX513; it was 260megs and couldn't be handled by IRAF ("segmentation violation"); DELETED hsel ccd030315.0* $I 'ccdfltid?="U"' > in.u hsel ccd030315.0* $I 'ccdfltid?="V"' > in.v hsel ccd030315.0* $I 'ccdfltid?="B"' > in.b hsel ccd030315.0* $I 'ccdfltid?="R"' > in.r hsel ccd030315.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r"$1}' in.u > out.u !awk '{print "r"$1}' in.v > out.v !awk '{print "r"$1}' in.b > out.b !awk '{print "r"$1}' in.r > out.r !awk '{print "r"$1}' in.i > out.i =============================================================================== 2003 0316 Contained ten biases, skyflats B,V and objects in U,B,V,R,I # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatb.0001.fits 1080428 53111. 25618. 0. 65535. ccdskyflatb.0002.fits 1080428 56272. 19918. 0. 65535. ccdskyflatb.0003.fits 1080428 59173. 15081. 0. 65535. ccdskyflatb.0004.fits 1080428 62938. 11425. 0. 65535. ccdskyflatb.0005.fits 1080428 63463. 10803. 0. 65535. ccdskyflatb.0006.fits 1080428 63589. 10885. 0. 65535. ccdskyflatb.0007.fits 1080428 63446. 11041. 0. 65535. ccdskyflatb.0008.fits 1080428 63179. 11291. 0. 65535. ccdskyflatb.0009.fits 1080428 61364. 11691. 0. 65535. ccdskyflatb.0010.fits 1080428 49533. 9710. 0. 65535. ccdskyflatb.0011.fits 1080428 39089. 7678. 0. 65535. ccdskyflatb.0012.fits 1080428 29811. 5905. 0. 65535. ccdskyflatb.0013.fits 1080428 23306. 4679. 0. 65535. ccdskyflatb.0014.fits 1080428 16217. 3260. 0. 54956. ccdskyflatb.0015.fits 1080428 11865. 2377. 0. 39980. Did not include ccdskyflatb.0001thru.0010 because means exceeded 45,000. ccdskyflatb.0011.fits "Sky flat b" B ccdskyflatb.0012.fits "Sky flat b" B ccdskyflatb.0013.fits "Sky flat b" B ccdskyflatb.0014.fits "Sky flat b" B ccdskyflatb.0015.fits "Sky flat b" B cc> imcombine List of images to combine (@flat.b): @flat.b List of output images (ccd030220.skyflatb): ccd030316.skyflatb # IMAGE NPIX MEAN STDDEV MIN MAX ccd030316.skyflatb 1080428 24065. 4806. 0. 67229. # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatv.0001.fits 1080428 12404. 2250. 0. 38095. ccdskyflatv.0002.fits 1080428 15621. 2842. 0. 52214. ccdskyflatv.0003.fits 1080428 14922. 2713. 0. 46128. ccdskyflatv.0004.fits 1080428 15613. 2841. 0. 48495. hsel @flat.v $I,title,ccdfltid boolean expression governing selection (yes): ccdskyflatv.0001.fits "Sky flat v" V ccdskyflatv.0002.fits "Sky flat v" V ccdskyflatv.0003.fits "Sky flat v" V ccdskyflatv.0004.fits "Sky flat v" V cc> imcombine List of images to combine (@flat.b): @flat.v List of output images (ccd030316.skyflatb): ccd030316.skyflatv # IMAGE NPIX MEAN STDDEV MIN MAX ccd030316.skyflatv 1080428 14639. 2661. 0. 45352. For U,R,I used: ccd030312.skyflatu.fits ccd030312.skyflatr.fits ccd030312.skyflati.fits cc> cat bias.list ccdbias.0001.fits ccdbias.0002.fits ccdbias.0003.fits ccdbias.0004.fits ccdbias.0005.fits ccdbias.0006.fits ccdbias.0007.fits ccdbias.0008.fits ccdbias.0009.fits ccdbias.0010.fits cc> imcombine @bias.list List of output images (ccd030316.skyflatv): ccd030316.bias hsel ccd030316.0* $I 'ccdfltid?="U"' > in.u hsel ccd030316.0* $I 'ccdfltid?="B"' > in.b hsel ccd030316.0* $I 'ccdfltid?="V"' > in.v hsel ccd030316.0* $I 'ccdfltid?="R"' > in.r hsel ccd030316.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r"$1}' in.u > out.u !awk '{print "r"$1}' in.b > out.b !awk '{print "r"$1}' in.v > out.v !awk '{print "r"$1}' in.r > out.r !awk '{print "r"$1}' in.i > out.i =============================================================================== 2003 0317 Contained ten biases, skyflats U,R,I and objects in B,V,R,I (no U) (there was also a single, therefore unusable skyflatb) # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflatr.0001.fits 1080428 28503. 5230. 0. 65535. ccdskyflatr.0002.fits 1080428 20817. 3833. 0. 60130. ccdskyflatr.0003.fits 1080428 25014. 4608. 0. 65535. cc> hsel @flat.r $I,title,ccdfltid boolean expression governing selection (ccdfltid?="U"): yes ccdskyflatr.0001.fits "Sky flat r" R ccdskyflatr.0002.fits "Sky flat r" R ccdskyflatr.0003.fits "Sky flat r" R List of images to combine (@bias.list): @flat.r List of output images (ccd030316.bias): ccd030317.skyflatr # IMAGE NPIX MEAN STDDEV MIN MAX ccd030317.skyflatr 1080428 24779. 4564. 0. 64917. # IMAGE NPIX MEAN STDDEV MIN MAX ccdskyflati.0001.fits 1080428 26932. 5079. 0. 65535. ccdskyflati.0002.fits 1080428 18569. 3516. 0. 65535. ccdskyflati.0003.fits 1080428 18482. 3498. 0. 65535. cc> hsel @flat.i $I,title,ccdfltid boolean expression governing selection (yes): ccdskyflati.0001.fits "Sky flat i" I ccdskyflati.0002.fits "Sky flat i" I ccdskyflati.0003.fits "Sky flat i" I cc> imcombine List of images to combine (@flat.r): @flat.i List of output images (ccd030317.skyflatr): ccd030317.skyflati For B,V used: ccd030316.skyflatb ccd030316.skyflatv cc> cat bias.list ccdbias.0001.fits ccdbias.0002.fits ccdbias.0003.fits ccdbias.0004.fits ccdbias.0005.fits ccdbias.0006.fits ccdbias.0007.fits ccdbias.0008.fits ccdbias.0009.fits ccdbias.0010.fits cc> imcombine List of images to combine (@flat.i): @bias.list List of output images (ccd030317.skyflati): ccd030317.bias hsel ccd030317.0* $I 'ccdfltid?="B"' > in.b hsel ccd030317.0* $I 'ccdfltid?="V"' > in.v hsel ccd030317.0* $I 'ccdfltid?="R"' > in.r hsel ccd030317.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r"$1}' in.b > out.b !awk '{print "r"$1}' in.v > out.v !awk '{print "r"$1}' in.r > out.r !awk '{print "r"$1}' in.i > out.i =============================================================================== 2003 0318 Contained ten biases, skyflats B only and objects in B,V,R,I (no U) # IMAGE NPIX MEAN STDDEV MIN MAX ccd030318skyflatb.0001.fits 1080428 6570. 1308. 0. 21843. ccd030318skyflatb.0002.fits 1080428 520.3 1515. 0. 65535. ccd030318skyflatb.0003.fits 1080428 472.4 1527. 0. 65535. ccd030318skyflatb.0004.fits 1080428 435.8 1535. 0. 65535. ccd030318skyflatb.0005.fits 1080428 403.2 1541. 0. 65535. ccd030318skyflatb.0006.fits 1080428 336.5 1545. 0. 65535. These were unusable for skyflatb. For B,V,R,I used: ccd030316.skyflatb ccd030316.skyflatv ccd030317.skyflatr ccd030317.skyflati cc> cat bias.list ccdbias.0001.fits ccdbias.0002.fits ccdbias.0003.fits ccdbias.0004.fits ccdbias.0005.fits ccdbias.0006.fits ccdbias.0007.fits ccdbias.0008.fits ccdbias.0009.fits ccdbias.0010.fits cc> imcombine @bias.list List of output images (ccd030218.skyflati): ccd030318.bias hsel ccd030318.0* $I 'ccdfltid?="B"' > in.b hsel ccd030318.0* $I 'ccdfltid?="V"' > in.v hsel ccd030318.0* $I 'ccdfltid?="R"' > in.r hsel ccd030318.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r" $1}' in.b . out.b !awk '{print "r" $1}' in.v > out.v !awk '{print "r" $1}' in.r > out.r !awk '{print "r" $1}' in.i > out.i =============================================================================== 2003 0319 Contained ten biases, NO skyflats and objects in U,B,V,R,I For U,B,V,R,I used: ccd030312.skyflatu ccd030316.skyflatb ccd030316.skyflatv ccd030317.skyflatr ccd030317.skyflati cl> cat bias.list ccd030319bias.0001.fits ccd030319bias.0002.fits ccd030319bias.0003.fits ccd030319bias.0004.fits ccd030319bias.0005.fits ccd030319bias.0006.fits ccd030319bias.0007.fits ccd030319bias.0008.fits ccd030319bias.0009.fits ccd030319bias.0010.fits cl> imcombine List of images to combine (@flat.v): @bias.list List of output images (ccd030217.skyflatv): ccd030319.bias hsel ccd030319.0* $I 'ccdfltid?="U"' > in.u hsel ccd030319.0* $I 'ccdfltid?="B"' > in.b hsel ccd030319.0* $I 'ccdfltid?="V"' > in.v hsel ccd030319.0* $I 'ccdfltid?="R"' > in.r hsel ccd030319.0* $I 'ccdfltid?="I"' > in.i !awk '{print "r"$1}' in.u > out.u !awk '{print "r"$1}' in.b > out.b !awk '{print "r"$1}' in.v > out.v !awk '{print "r"$1}' in.r > out.r !awk '{print "r"$1}' in.i > out.i =============================================================================== 2003 0320 Contained ten biases, skyflats B,V and objects in B,V,R,I (no U). # IMAGE NPIX MEAN STDDEV MIN MAX ccd030320skyflatb.0003.fits 1080428 38543. 7583. 0. 65535. ccd030320skyflatb.0004.fits 1080428 28658. 5696. 0. 65535. ccd030320skyflatb.0005.fits 1080428 21062. 4251. 0. 65535. ccd030320skyflatb.0006.fits 1080428 21754. 4068. 0. 65535. ccd030320skyflatb.0007.fits 1080428 20648. 3861. 0. 65535. cl> hsel @flat.b $I,title,ccdfltid boolean expression governing selection (ccdfltid?="I"): yes ccd030320skyflatb.0003.fits "Sky Flat B" R ccd030320skyflatb.0004.fits "Sky Flat B" R ccd030320skyflatb.0005.fits "Sky Flat B" R ccd030320skyflatb.0006.fits "Sky Flat B" R ccd030320skyflatb.0007.fits "Sky Flat B" R # IMAGE NPIX MEAN STDDEV MIN MAX ccd030320skyflatv.0001.fits 1080428 15960. 2906. 0. 49113. ccd030320skyflatv.0002.fits 1080428 18075. 3294. 0. 54493. ccd030320skyflatv.0003.fits 1080428 19666. 3596. 0. 65535. ccd030320skyflatv.0004.fits 1080428 15958. 2941. 0. 65535 cl> e hsel @flat.v $I,title,ccdfltid boolean expression governing selection (yes): ccd030320skyflatv.0001.fits "Sky Flat V" R ccd030320skyflatv.0002.fits "Sky Flat V" R ccd030320skyflatv.0003.fits "Sky Flat V" R ccd030320skyflatv.0004.fits "Sky Flat V" R OOPS!!!--------------------------both flats were in wrong filter so didn't use. For B,V,R,I used: ccd030316.skyflatb ccd030316.skyflatv ccd030317.skyflatr ccd030317.skyflati cl> cat bias.list ccd030320bias.0001.fits ccd030320bias.0002.fits ccd030320bias.0003.fits ccd030320bias.0004.fits ccd030320bias.0005.fits ccd030320bias.0006.fits ccd030320bias.0007.fits ccd030320bias.0008.fits ccd030320bias.0009.fits ccd030320bias.0010.fits imcombine @bias.list ccd030320.bias Used speedup.cl to make in and out files. =============================================================================== 2003 0321 Contained NO biases, NO skyflats, and objects in U,B,V,R,I For bias, used ccd030320.bias For U,B,V,R,I used: ccd030312.skyflatu ccd030316.skyflatb ccd030316.skyflatv ccd030317.skyflatr ccd030317.skyflati Used speedup.cl to make in and out files. =============================================================================== 2003 0322 Contained ten biases, skyflats B,V and objects in U,B,V,R,I # IMAGE NPIX MEAN STDDEV MIN MAX ccd030322skyflatB.0003.fits 1080428 61004. 10910. 0. 65535. ccd030322skyflatB.0004.fits 1080428 30101. 5538. 0. 65535. ccd030322skyflatB.0005.fits 1080428 21196. 3964. 0. 65535. ccd030322skyflatB.0006.fits 1080428 24160. 4501. 0. 65535. ccd030322skyflatB.0007.fits 1080428 19061. 3564. 0. 64484. Did not include ccd030322skyflatB.0003.fits since mean > 45000. cl> hsel @flat.b $I,title,ccdfltid boolean expression governing selection (yes): ccd030322skyflatB.0004.fits "B Sky Flat" B ccd030322skyflatB.0005.fits "B Sky Flat" B ccd030322skyflatB.0006.fits "B Sky Flat" B ccd030322skyflatB.0007.fits "B Sky Flat" B cl> imcombine @flat.b ccd030322.skyflatb cl> imstat ccd030322.skyflatb # IMAGE NPIX MEAN STDDEV MIN MAX ccd030322.skyflatb 1080428 23632. 4409. 0. 68579. --------------------------- # IMAGE NPIX MEAN STDDEV MIN MAX ccd030322skyflatV.0001.fits 1080428 25543. 4633. 0. 65535. ccd030322skyflatV.0002.fits 1080428 16762. 3040. 0. 51669. ccd030322skyflatV.0003.fits 1080428 17146. 3112. 0. 52983. ccd030322skyflatV.0004.fits 1080428 15478. 2818. 0. 63186. cl> hsel @flat.v $I,title,ccdfltid boolean expression governing selection (yes): ccd030322skyflatV.0001.fits "V Sky Flat" V ccd030322skyflatV.0002.fits "V Sky Flat" V ccd030322skyflatV.0003.fits "V Sky Flat" V ccd030322skyflatV.0004.fits "V Sky Flat" V cl> imstat ccd030322.skyflatv # IMAGE NPIX MEAN STDDEV MIN MAX ccd030322.skyflatv 1080428 18731. 3397. 0. 57672. --------------------- cl> cat bias.list ccd030322bias.0001.fits ccd030322bias.0002.fits ccd030322bias.0003.fits ccd030322bias.0004.fits ccd030322bias.0005.fits ccd030322bias.0006.fits ccd030322bias.0007.fits ccd030322bias.0008.fits ccd030322bias.0009.fits ccd030322bias.0010.fits cl> imcombine @bias.list ccd030322.bias For U,R,I used: ccd030312.skyflatu ccd030317.skyflatr ccd030317.skyflati Used speedup.cl to make in and out files. =============================================================================== 2003 0323 Contained ten biases, skyflats U,R,I and objects in U,B,V,R,I cc> cat bias.list ccd030323bias.0001.fits ccd030323bias.0002.fits ccd030323bias.0003.fits ccd030323bias.0004.fits ccd030323bias.0005.fits ccd030323bias.0006.fits ccd030323bias.0007.fits ccd030323bias.0008.fits ccd030323bias.0009.fits ccd030323bias.0010.fits cc> imcombine @bias.list ccd030323.bias # IMAGE NPIX MEAN STDDEV MIN MAX ccd030323skyflatU.0001.fits 1080428 38536. 8599. 0. 65535. ccd030323skyflatU.0002.fits 1080428 30661. 6861. 0. 65535. ccd030323skyflatU.0003.fits 1080428 22732. 5150. 0. 65535. ccd030323skyflatU.0004.fits 1080428 27970. 6271. 0. 65535. ccd030323skyflatU.0005.fits 1080428 18749. 4286. 0. 65535. ccd030323skyflatU.0006.fits 1080428 20441. 4658. 0. 65535. cc> hsel @flat.u $I,title,ccdfltid boolean expression governing selection (yes): ccd030323skyflatU.0001.fits "Sky Flat U" U ccd030323skyflatU.0002.fits "Sky Flat U" U ccd030323skyflatU.0003.fits "Sky Flat U" U ccd030323skyflatU.0004.fits "Sky Flat U" U ccd030323skyflatU.0005.fits "Sky Flat U" U ccd030323skyflatU.0006.fits "Sky Flat U" U cc> imcombine @flat.u ccd030323.skyflatU cc> imstat ccd030323.skyflatU # IMAGE NPIX MEAN STDDEV MIN MAX ccd030323.skyflatU 1080428 26519. 5978. 0. 70067. --------------------------- # IMAGE NPIX MEAN STDDEV MIN MAX ccd030323skyflatR.0002.fits 1080428 28181. 5173. 0. 65535. ccd030323skyflatR.0003.fits 1080428 20076. 3695. 0. 58069. ccd030323skyflatR.0004.fits 1080428 19456. 3579. 0. 55966. ccd030323skyflatR.0005.fits 1080428 21831. 4019. 0. 63026. cc> hsel @flat.r $I,title,ccdfltid boolean expression governing selection (yes): ccd030323skyflatR.0002.fits "Sky Flat R" R ccd030323skyflatR.0003.fits "Sky Flat R" R ccd030323skyflatR.0004.fits "Sky Flat R" R ccd030323skyflatR.0005.fits "Sky Flat R" R cc> imcombine @flat.r ccd030323.skyflatR cc> imstat ccd030323.skyflatR # IMAGE NPIX MEAN STDDEV MIN MAX ccd030323.skyflatR 1080428 22387. 4121. 0. 64500. -------------------------------- # IMAGE NPIX MEAN STDDEV MIN MAX ccd030323skyflatI.0001.fits 1080428 15468. 2918. 0. 62750. ccd030323skyflatI.0002.fits 1080428 19095. 3610. 0. 65535. ccd030323skyflatI.0003.fits 1080428 22541. 4291. 0. 65535. ccd030323skyflatI.0004.fits 1080428 18698. 3540. 0. 65535. hsel @flat.i $I,title,ccdfltid boolean expression governing selection (yes): ccd030323skyflatI.0001.fits "Sky Flat I" I ccd030323skyflatI.0002.fits "Sky Flat I" I ccd030323skyflatI.0003.fits "Sky Flat I" I ccd030323skyflatI.0004.fits "Sky Flat I" I cc> imcombine @flat.i ccd030323.skyflatI cc> imstat ccd030323.skyflatI # IMAGE NPIX MEAN STDDEV MIN MAX ccd030323.skyflatI 1080428 18946. 3580. 0. 65731. For B,V used: ccd030322.skyflatb ccd030322.skyflatv Used speedup.cl to make in and out files. =============================================================================== 2003 0324 Contained ten biases, NO skyflats and objects in U,B,V,R,I For U,B,V,R,I used: ccd030323.skyflatU ccd030322.skyflatb ccd030322.skyflatv ccd030323.skyflatR ccd030323.skyflatI cc> cat bias.list ccd030324bias.0001.fits ccd030324bias.0002.fits ccd030324bias.0003.fits ccd030324bias.0004.fits ccd030324bias.0005.fits ccd030324bias.0006.fits ccd030324bias.0007.fits ccd030324bias.0008.fits ccd030324bias.0009.fits ccd030324bias.0010.fits cc> imcombine @bias.list ccd030324.bias Used speedup.cl to make in and out files. =============================================================================== 2003 0325 Contained ten biases, skyflats U,R,(one only),I and objects in U,B,V,R,I cc> cat bias.list ccd030325bias.0001.fits ccd030325bias.0002.fits ccd030325bias.0003.fits ccd030325bias.0004.fits ccd030325bias.0005.fits ccd030325bias.0006.fits ccd030325bias.0007.fits ccd030325bias.0008.fits ccd030325bias.0009.fits ccd030325bias.0010.fits cc> imcombine @bias.list ccd030325.bias # IMAGE NPIX MEAN STDDEV MIN MAX ccd030325skyU.0001.fits 1080428 20865. 4877. 0. 65535. ccd030325skyU.0002.fits 1080428 17085. 4007. 0. 65535. ccd030325skyU.0003.fits 1080428 18865. 4423. 0. 65535. ccd030325skyU.0004.fits 1080428 24987. 5775. 0. 65535. ccd030325skyU.0005.fits 1080428 19369. 4533. 0. 65535. boolean expression governing selection (yes): ccd030325skyU.0001.fits "Sky Flat U" U ccd030325skyU.0002.fits "Sky Flat U" U ccd030325skyU.0003.fits "Sky Flat U" U ccd030325skyU.0004.fits "Sky Flat U" U ccd030325skyU.0005.fits "Sky Flat U" U cc> imcombine @flat.U ccd030325.skyflatU cc> imstat ccd030325.skyflatU # IMAGE NPIX MEAN STDDEV MIN MAX ccd030325.skyflatU 1080428 20236. 4736. 0. 67433. --------------------------- # IMAGE NPIX MEAN STDDEV MIN MAX ccd030325skyI.0001.fits 1080428 14187. 2630. 0. 65535. ccd030325skyI.0002.fits 1080428 35698. 6507. 0. 65535. ccd030325skyI.0003.fits 1080428 32152. 5891. 0. 65535. ccd030325skyI.0004.fits 1080428 20720. 3851. 0. 65535. boolean expression governing selection (yes): ccd030325skyI.0001.fits "Sky Flat I" I ccd030325skyI.0002.fits "Sky Flat I" I ccd030325skyI.0003.fits "Sky Flat I" I ccd030325skyI.0004.fits "Sky Flat I" I cc> imcombine @flat.I ccd030325.skyflatI cc> imstat ccd030325.skyflatI # IMAGE NPIX MEAN STDDEV MIN MAX ccd030325.skyflatI 1080428 25692. 4731. 0. 66824. For B,V,R used: ccd030322.skyflatb ccd030322.skyflatv ccd030323.skyflatR Used speedup.cl to make in and out files. ============================================================================== 2003 0326 Contained ten biases, skyflats B,V and objects in B,V,R,I (no U) ccd030326bias.0001.fits ccd030326bias.0002.fits ccd030326bias.0003.fits ccd030326bias.0004.fits ccd030326bias.0005.fits ccd030326bias.0006.fits ccd030326bias.0007.fits ccd030326bias.0008.fits ccd030326bias.0009.fits ccd030326bias.0010.fits cc> imcombine @bias.list ccd030326.bias # IMAGE NPIX MEAN STDDEV MIN MAX ccd030326skyB.0003.fits 1080428 56976. 10342. 0. 65535. ccd030326skyB.0004.fits 1080428 29393. 5415. 0. 65535. ccd030326skyB.0005.fits 1080428 22265. 4161. 0. 65535. ccd030326skyB.0006.fits 1080428 25675. 4768. 0. 65535. ccd030326skyB.0007.fits 1080428 18648. 3485. 0. 62854. ccd030326skyB.0008.fits 1080428 20303. 3799. 0. 65535. Did not include ccd030326skyB.0003.fits because mean > 45000 hsel @flat.B $I,title,ccdfltid boolean expression governing selection (yes): ccd030326skyB.0004.fits "Sky Flat B" B ccd030326skyB.0005.fits "Sky Flat B" B ccd030326skyB.0006.fits "Sky Flat B" B ccd030326skyB.0007.fits "Sky Flat B" B ccd030326skyB.0008.fits "Sky Flat B" B cc> imcombine @flat.B ccd030326.skyflatB ------------------------------ # IMAGE NPIX MEAN STDDEV MIN MAX ccd030326skyV.0001.fits 1080428 17564. 3193. 0. 54420. ccd030326skyV.0002.fits 1080428 21414. 3915. 0. 65535. ccd030326skyV.0003.fits 1080428 18732. 3417. 0. 65535. boolean expression governing selection (yes): ccd030326skyV.0001.fits "Sky Flat V" V ccd030326skyV.0002.fits "Sky Flat V" V ccd030326skyV.0003.fits "Sky Flat V" V cc> imcombine @flat.V ccd030326.skyflatV For R,I used: ccd030323.skyflatR ccd030325.skyflatI Used speedup.cl to make in and out files. ============================================================================== 2003 0327 Contained ten biases, skyflats U,R,I and objects in U,B,V,R,I Frame ccd030327.0084.fits SN2003bt coudl not be processed since it had no filter identification. ccd030327bias.0001.fits ccd030327bias.0002.fits ccd030327bias.0003.fits ccd030327bias.0004.fits ccd030327bias.0005.fits ccd030327bias.0006.fits ccd030327bias.0007.fits ccd030327bias.0008.fits ccd030327bias.0009.fits ccd030327bias.0010.fits cc> imcombine @bias.list ccd030327.bias # IMAGE NPIX MEAN STDDEV MIN MAX ccd030327skyU.0001.fits 1080428 23623. 5324. 0. 65535. ccd030327skyU.0002.fits 1080428 22267. 5033. 0. 65535. ccd030327skyU.0003.fits 1080428 25494. 5722. 0. 65535. ccd030327skyU.0004.fits 1080428 15839. 3609. 0. 61651. ccd030327skyU.0005.fits 1080428 12437. 2823. 0. 47998. boolean expression governing selection (yes): ccd030327skyU.0001.fits "Sky Flat u" U ccd030327skyU.0002.fits "Sky Flat u" U ccd030327skyU.0003.fits "Sky Flat u" U ccd030327skyU.0004.fits "Sky Flat u" U ccd030327skyU.0005.fits "Sky Flat u" U cc> imcombine @flat.U ccd030327.skyflatU cc> imstat ccd030327.skyflatU # IMAGE NPIX MEAN STDDEV MIN MAX ccd030327.skyflatU 1080428 19933. 4509. 0. 63634. ------------------------------ # IMAGE NPIX MEAN STDDEV MIN MAX ccd030327skyR.0003.fits 1080428 30110. 5516. 0. 65535. ccd030327skyR.0004.fits 1080428 21626. 3983. 0. 62431. ccd030327skyR.0005.fits 1080428 24368. 4491. 0. 65535. ccd030327skyR.0006.fits 1080428 17140. 3151. 0. 49325. boolean expression governing selection (yes): ccd030327skyR.0003.fits "Sky flat r" R ccd030327skyR.0004.fits "Sky flat r" R ccd030327skyR.0005.fits "Sky flat r" R ccd030327skyR.0006.fits "Sky flat r" R cc> imcombine @flat.R ccd030327.skyflatR cc> imstat ccd030327.skyflatR # IMAGE NPIX MEAN STDDEV MIN MAX ccd030327.skyflatR 1080428 23312. 4293. 0. 64888. ------------------------------ # IMAGE NPIX MEAN STDDEV MIN MAX ccd030327skyI.0001.fits 1080428 14171. 2687. 0. 57719. ccd030327skyI.0002.fits 1080428 15738. 2986. 0. 65535. ccd030327skyI.0003.fits 1080428 15004. 2843. 0. 61668. boolean expression governing selection (yes): ccd030327skyI.0001.fits "Sky flat i" I ccd030327skyI.0002.fits "Sky flat i" I ccd030327skyI.0003.fits "Sky flat i" I cc> imcombine @flat.I ccd030327.skyflatI cc> imstat ccd030327.skyflatI # IMAGE NPIX MEAN STDDEV MIN MAX ccd030327.skyflatI 1080428 14971. 2837. 0. 61528. ------------------------------ For B,V used: ccd030326.skyflatB ccd030326.skyflatV Used speedup.cl to make in and out files. ============================================================================== 2003 0328 Contained twenty biases, no skyflats and objects in U,B,V,R,I ccd030328bias.0001.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0002.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0003.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0004.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0005.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0006.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0007.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0008.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0009.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0010.fits BIASES "B STROMGREN" 0.0 ccd030328bias.0011.fits BIASES V 0.0 ccd030328bias.0012.fits BIASES V 0.0 ccd030328bias.0013.fits BIASES V 0.0 ccd030328bias.0014.fits BIASES V 0.0 ccd030328bias.0015.fits BIASES V 0.0 ccd030328bias.0016.fits BIASES V 0.0 ccd030328bias.0017.fits BIASES V 0.0 ccd030328bias.0018.fits BIASES V 0.0 ccd030328bias.0019.fits BIASES V 0.0 ccd030328bias.0020.fits BIASES V 0.0 Decided to use only biases 0011 thru 0020 in absence of further info. Note that a random check previous night's biases show they were R. Note also that the log presents numbers 0001 thru 0010 differerently from other frames. cl> cat bias.list ccd030328bias.0011.fits ccd030328bias.0012.fits ccd030328bias.0013.fits ccd030328bias.0014.fits ccd030328bias.0015.fits ccd030328bias.0016.fits ccd030328bias.0017.fits ccd030328bias.0018.fits ccd030328bias.0019.fits ccd030328bias.0020.fits cl> imcombine @bias.list ccd030328.bias For U,B,V,R,I used: ccd030327.skyflatU ccd030326.skyflatB ccd030326.skyflatV ccd030327.skyflatR ccd030327.skyflatI ============================================================================== 2003 0329 Contained twenty biases, NO skyflats and objects in U,B,V,R,I Decided to use only the last ten biases (although they were all the same ccdfltid) since the first ten did not show up on the log with a JD listing and the last ten did. hsel @bias.list $I,title,ccdfltid,exptime boolean expression governing selection (yes): ccd030329bias.0011.fits BIASES I 0.0 ccd030329bias.0012.fits BIASES I 0.0 ccd030329bias.0013.fits BIASES I 0.0 ccd030329bias.0014.fits BIASES I 0.0 ccd030329bias.0015.fits BIASES I 0.0 ccd030329bias.0016.fits BIASES I 0.0 ccd030329bias.0017.fits BIASES I 0.0 ccd030329bias.0018.fits BIASES I 0.0 ccd030329bias.0019.fits BIASES I 0.0 ccd030329bias.0020.fits BIASES I 0.0 cc> imcombine @bias.list ccd030329.bias For U,B,V,R,I used: ccd030327.skyflatU ccd030326.skyflatB ccd030326.skyflatV ccd030327.skyflatR ccd030327.skyflatI ============================================================================== 2003 0330 Contained ten biases, NO skyflats and objects in U,B,V,R,I cc> hsel @bias.list $I,title,ccdfltid boolean expression governing selection (yes): ccd030330bias.0001.fits BIASES R ccd030330bias.0002.fits BIASES R ccd030330bias.0003.fits BIASES R ccd030330bias.0004.fits BIASES R ccd030330bias.0005.fits BIASES R ccd030330bias.0006.fits BIASES R ccd030330bias.0007.fits BIASES R ccd030330bias.0008.fits BIASES R ccd030330bias.0009.fits BIASES R ccd030330bias.0010.fits BIASES R cc> imcombine @bias.list ccd030330.bias For U,B,V,R,I used: ccd030327.skyflatU ccd030326.skyflatB ccd030326.skyflatV ccd030327.skyflatR ccd030327.skyflatI ============================================================================== 2003 0331 Contained ten biases, skyflats B,V and objects in U,B,V,R,I cat bias.list ccd030331bias.0001.fits ccd030331bias.0002.fits ccd030331bias.0003.fits ccd030331bias.0004.fits ccd030331bias.0005.fits ccd030331bias.0006.fits ccd030331bias.0007.fits ccd030331bias.0008.fits ccd030331bias.0009.fits ccd030331bias.0010.fits imcombine @bias.list ccd030331.bias # IMAGE NPIX MEAN STDDEV MIN MAX # IMAGE NPIX MEAN STDDEV MIN MAX ccd030331skyB.0001.fits 1080428 60159. 13344. 0. 65535. ccd030331skyB.0002.fits 1080428 63285. 10966. 0. 65535. ccd030331skyB.0003.fits 1080428 63642. 10809. 0. 65535. ccd030331skyB.0004.fits 1080428 63488. 10989. 0. 65535. ccd030331skyB.0005.fits 1080428 62917. 11318. 0. 65535. ccd030331skyB.0006.fits 1080428 53258. 10175. 0. 65535. ccd030331skyB.0007.fits 1080428 41238. 7890. 0. 65535. ccd030331skyB.0008.fits 1080428 31911. 6147. 0. 65535. ccd030331skyB.0009.fits 1080428 24734. 4831. 0. 65535. ccd030331skyB.0010.fits 1080428 18613. 3658. 0. 63322. ccd030331skyB.0011.fits 1080428 14395. 2821. 0. 48762. ccd030331skyB.0012.fits 1080428 17059. 3352. 0. 58268. Did not include ccd030331skyB.0001 thru 0006 since mean > 45,000. cc> hsel @flat.B $I,title,ccdfltid boolean expression governing selection (yes): ccd030331skyB.0007.fits "Sky flat b" B ccd030331skyB.0008.fits "Sky flat b" B ccd030331skyB.0009.fits "Sky flat b" B ccd030331skyB.0010.fits "Sky flat b" B ccd030331skyB.0011.fits "Sky flat b" B ccd030331skyB.0012.fits "Sky flat b" B cc> imcombine @flat.B ccd030331.skyflatB cc> imstat ccd030331.skyflatB # IMAGE NPIX MEAN STDDEV MIN MAX ccd030331.skyflatB 1080428 24666. 4809. 0. 70867. ------------------------------ # IMAGE NPIX MEAN STDDEV MIN MAX ccd030331skyV.0001.fits 1080428 10297. 1866. 0. 31406. ccd030331skyV.0002.fits 1080428 9114. 1649. 0. 27597. ccd030331skyV.0003.fits 1080428 9966. 1806. 0. 30631. boolean expression governing selection (yes): ccd030331skyV.0001.fits "Sky flat v" V ccd030331skyV.0002.fits "Sky flat v" V ccd030331skyV.0003.fits "Sky flat v" V cc> imstat ccd030331.skyflatV # IMAGE NPIX MEAN STDDEV MIN MAX ccd030331.skyflatV 1080428 9792. 1773. 0. 29857. ------------------------------ For U,R,I used: ccd030327.skyflatU ccd030327.skyflatR ccd030327.skyflatI ==============================================================================