Throughput image quality of a MEMS spectrograph ST-ECF Instrument Science Report JWST 2003-01 Calibration concept for the JWST Near-infrared Spectrograph (NIRSpec) Harald Kuntschner, Robert Fosbury, Wolfram Freudling Stefano Cristiani --1-- ST-ECF ISR JWST 2003-01 V1.2 June 18, 2003 Calibration concept for the JWST Near-infrared Sp ectrograph (NIRSp ec) Harald Kuntschner, Rob ert A.E. Fosbury, Wolfram Freudling ST European ... The line calibration lamp exp osure time is assumed to b e 60 sec. ...

Field centres for 6dF/FLAIR observations of the 6QZ survey. # 6dF fields have radius 2.844 deg. and were defined in the # J2000 system. FLAIR fields are square and are 5x5 deg # centred on UKST survey positions and defined in the B1950 # system. # 6dF : coordinates ( B1950 ) coordinates ( J2000 ) # Field hh mm ss.ss dd mm ss.s hh mm ss.ss dd mm ss.s sgp001 21 51 31.25 -30 11 45.4 21 54 25.40 -29 57 33.0 sgp002 22 10 08.35 -29 50 17.3 22 12 59.50 -29 35 25.0 sgp003 22 30 24.34 ...

R And SiO maser. S And SN (NGC 224). W And SiO maser. Z And Outbursts, average cycle 8400d. Porb = 758.8d, it reveals Z And itself in photometry during the low state. A quasi-period, P1, Z And about 656d is present during the outbursts. The beat period Z And between Porb and P1, about 5500d, is also found in the Z And photometric data. RS And H2O maser. RT And Min II = 9.28. P varies, current elements are given. RU And P varies strongly. RX And Porb = 0.209893d. RY And OH, H2O maser. SS And P2 = 650d, P3 =

No. Name R.A.,Decl., 2000.0 Max Min Type Ref. Epoch Period M-m Spectrum h m s o ' " m m JD200000+ d 780001 V956 Cas 00 05 05.4 +59 39 01. 14.2 17.2 B IS: 001 002 780002 CD Scl 00 06 20.8 -35 17 13. 12.7 14.2 V RRAB 130 004 52068.835 0.57769 20 A0 780003 V439 And 00 06 36.8 +29 01 17. 6.13 ( 0.04 ) V BY 005 DM K0Ve 780004 V957 Cas 00 09 45.7 +50 30 39. 11.6 12.8 * SR: 006 USNO 780005 V958 Cas 00 10 48.5 +57 29 27. 8.8 9.8 * SR: 006 GSC 780006 V959 Cas 00 12 02.7 +55 05 19. 12.0 12.6 * EW 006 GSC 040

... Structural Analysis of Disk Galaxies of the NGC 524 Group M. A. Il'ina and O. K. Sil'chenko * Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russia Received February 24, 2012; in final form, March 2, 2012 Abstract--Members of the NGC 524 group of galaxies are studied using data obtained on the 6m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences, with the SCORPIO reducer in an imaging mode. ... NGC 502. ... NGC 524. ... Rev. Astron. ...

ОСНОВНЫЕ ОРТОГОНАЛЬНЫЕ ФУНКЦИИ И ИХ ПРИЛОЖЕНИЯ ЧАСТЬ I. ОРТОГОНАЛЬНЫЕ ФУНКЦИИ ЭКСПОНЕНЦИАЛЬНОГО ТИПА УДК 517.587:519.216 Прохоров С.А., Куликовских И.М. Основные ортогональные функции и их приложения. Часть I. Ортогональные функции экспоненциального типа. Самара: Издательство Самарского научного центра РАН, 2013. 200 с. ISBN 978-5-93424-652-6 В первой части предлагаемой монографии рассматриваются ортогональные функции экспоненциального типа. Структура монографии разработана с учетом дальнейшего приложения к