Revolution: 1252 . POS_1252_061009_160_00_0001.XMM . ... PSF version: 1252_02 . ... Slew: 3915 secs . ... Obs_dur: 50300 secs . ... 004: 49286 sec . ... 005: 49281 sec . ... 400: 288 sec . ... 003: 49157 sec . ... 002: 49147 sec . ... 23:38:42 ... exp continues . ... 006: 2964 sec . ... 2006-10-10 | ... 001: 47440 sec . ... 007: 4706 sec . ... 008: 4706 sec . ... 009: 4706 sec . ... 010: 4706 sec . ... 011: 4706 sec . ... 012: 4706 sec . ... 013: 4706 sec . ... 014: 6506 sec . ... 015: 4706 sec . ...

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• XMM POS Summary for rev: 1505
• XMM POS Summary for rev: 0981
• XMM POS Summary for rev: 1192

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Total Magnitudes of Virgo Galaxies. ... Spanning 8th to 18th mag. ... Next Section: Bright-end consistency checks . ... Previous Section: Intermediate galaxy sample (14th-12th . ... This latter distance was set as the point at which the surface brightness of the galaxy would fall to б mag.arcsec -2 if the . ...

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• VLBI Wiki | LBAOct2010 / Vc127bCdLog
• lbaops:lbaoct2010:vc127bcdlog [ATNF VLBI Wiki]
• Archive of VLBI Observations Majordomo List

... xs qpspec source qpoe file (xdata$rp110590n00.qp): xdata$rp110590n00.qp[ time =(1606720.00:1607479.00)] source region descriptor ():c 6947 9325 2' background qpoe file ( ): bkgd region descriptor (): a 6947 9325 3' 4' root name for output files [root_obs.tab, etc.] (): arlac_1 ds: 0 file : arlac_1_obs.tab scale: 0.00 mission: 20 seqno: CA110590P.N6 instrument: ROSAT_PSPC sub-instrument: 1 no. pha channels: 34 mean off-axis angle of events (arcmin ...

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• ChaMPlane observed fields

Each receiver has a turret position to place the horn at the focus. ... current . 14may04 (02may04 survey) . ... sbn rcv . ... 14feb04 horn survey . ... 13feb04 (13 feb04 survey) . ... sbn . ... mod14/sbn/mar03 . ... survey feb04. mod15/may04 . ... horn move,survey,model may04 . ... horn move, survey feb04 . ... horn move,survey,model may04 Notes: . ... After the may04 surveys, sbn and lbw were not moved in the x direction (za) because there was no room in the hole in the turret floor. home_~phil ...

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• software measurements
• vertex drive system

Next: The Stellar Population in Up: NICMOS Science Previous: NICMOS Coronagraphic Surveys-Preliminary Results . ... Searching around young stars . ... We are using NICMOS to search for very low-mass stellar and sub-stellar companions around nearby, young, main-sequence stars. ... NICMOS, coronagraph, young stars, brown dwarfs . ... We present images of a possible companion, probably a low-mass M star, to the star HD102982 which demonstrates our ability to detect substellar objects. ...

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... With the FORS1 instrument of the ESO VLT, we have performed during the 2007 apparition of 133P/Elst-Pizarro quasisimultaneous photometry and polarimetry of its nucleus at nine epochs in the phase angle range 0 - 20 . ... Geometric information about the dust tails of 133P/Elst-Pizarro. ... The most logical explanation of the almost absent coma and the narrow dust tails is low nucleus activity and the small terminal expansion velocity of the dust grains after release by the nucleus of 133P/Elst...

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• http://star.arm.ac.uk/~ambn/veritas.ps
• http://star.arm.ac.uk/preprints/2011/585.pdf

... Oke (AJ, 99, 1621, 1990) has provided absolute spectral energy distributions covering the wavelength range 3200 to 9200A in AB magnitudes for 25 stars. ... The reduced magnitudes are tabulated at 1A intervals from 3300 to 4700A and at 2A intervals from 4700 to 9200A. Comparison of the fluxes with those determined elsewhere showed that Oke's absolute magnitudes are systematically brighter by 0.04 mag. The magnitudes and fluxes plotted have been corrected for this effect. ...

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... 4) 06-11/01/2002 Maiolino-Cresci . 5) 01-06/04/2002 Cresci-Stanga . 6) 28/09-3/10/2002 Cresci-Ranfagni . 7) 10-18/12/2002 Cresci-Gatti-Calamai . ... Here you can find a sample of images of the galaxies . ... 0.0055 . ... 0.0052 . ... For comments please contact: gcresci@arcetri.astro.it . ...

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... The telluric features redward of 6700 A have been removed from the accurate spectro photometric standards of Hamuy et al. to permit more reliable relative and absolute spectrophotometry to be obtained from CCD spectra. Smooth яuxes from 3300 to 10500 A are best determined by dividing the raw spectra of all objects taken in a night by the raw spectrum of a "" smooth оо spectrum star before deriving the instrumental response function using the revised standard star яuxes. ...

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... Сообщения без ответов . ... Последнее сообщение . ... k2s Перейти к последнему сообщению . ... Asya_Schtirlitz Перейти к последнему сообщению . ... DeZeRt Перейти к последнему сообщению . ... Последнее сообщение Re: Химия. ... Vasisualiy57 Перейти к последнему сообщению . ... Ане4ка Перейти к последнему сообщению . ... bootal Перейти к последнему сообщению . ... Последнее сообщение Re: Равноденствие 2010 . Capricornus Перейти к последнему сообщению . ... Dmitry Перейти к последнему сообщению . ...

191. http://www.mrao.cam.ac.uk/~dag/sn1994i.txt

192. http://www.astro.louisville.edu/shared_skies/archive/select/planets/neptune/sequence_2012/notes.txt

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