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    • [ В начало ] Пред. | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | След.

    81. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_01_05_99
    ... STIS/CCD/MA1 7481 (The Wind-momentum Luminosity Relationship for M31 and M33 B-supergiants) The Space Telescope Imaging Spectrograph (CCD and MA1) was used to make observations of the B class supergiant star M-31-OB78-1 which is locate in the M-31 galaxy ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_01_05_99 -- 9.7 Кб -- 05.01.1999
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    82. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_09_08_98
    ... from Accurate Multi-Color WF/PC-2 Photometry of A & B Supergiants in M-31 and M-33) The WF/PC-2 was used to make multi-color ... This is to study A and B supergiant stars in M-31 and M-33 with a precision far exceeding that of existing ground-based ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_09_08_98 -- 22.0 Кб -- 08.09.1998
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    83. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_06_21_99
    ... 1.17 Completed WF/PC-2 6671 (Deep V, I Photometry for 20 M31 Globular Clusters) The WF/PC-2 was used to make deep photometry observations (V=27.5) of the globular cluster M-31-G327 which is located in the Andromeda Galaxy (a.k.a., M-31). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_06_21_99 -- 12.9 Кб -- 21.06.1999
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    84. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_12_07_98
    ... from Accurate Multi-Color WF/PC-2 Photometry of A & B Supergiants in M-31 and M-33) The WF/PC-2 was used to make multi-color ... This is to study A and B supergiant stars in M-31 and M-33 with a precision far exceeding that of existing ground-based ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_12_07_98 -- 16.3 Кб -- 07.12.1998
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    85. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_10_16_95
    ... 1.18 Completed WF/PC-2 5911 (Massive Star Formation in M-31) The WF/PC-2 was used to make observations in the northeast spiral = arm of NGC-224 (aka, M-31, The Andromeda Galaxy) looking for indications = of massive star formation. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_10_16_95 -- 11.1 Кб -- 16.10.1995
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    86. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_01_25_99
    ... from Accurate Multi-Color WF/PC-2 Photometry of A & B Supergiants in M-31 and M-33) The WF/PC-2 was used to make multi-color ... This is to study A and B supergiant stars in M-31 and M-33 with a precision far exceeding that of existing ground-based ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_01_25_99 -- 14.6 Кб -- 25.01.1999
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    87. http://www.stsci.edu/spss/082992b2-spb.cal
    ... D=00:00:08:43 SAA 05 (ENTRY) 299:14:02:34 D=00:10:24:07 SAA 05 (EXIT) 299:14:03:50 NODE Crossing 101129 299:14:20:37 D=00:00:14:31 * M Slew (AN= 47,RA=114,DE=-34,PA=104,O= 0,SN= 88) 299:14:35:08 D=00:00:01:36 FHST Rate (E = 14400 1,2,3) 299:14:36:44 D=00 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/spss/082992b2-spb.cal -- 20.9 Кб -- 23.10.2008
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    88. http://www.stsci.edu/spss/082992b1-spb.cal
    ... D=00:00:08:43 SAA 05 (ENTRY) 299:14:02:34 D=00:10:24:07 SAA 05 (EXIT) 299:14:03:50 NODE Crossing 101129 299:14:20:37 D=00:00:14:31 * M Slew (AN= 47,RA=114,DE=-34,PA=104,O= 0,SN= 88) 299:14:35:08 D=00:00:01:36 FHST Rate (E = 14400 1,2,3) 299:14:36:44 D=00 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/spss/082992b1-spb.cal -- 21.8 Кб -- 22.10.2008
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    89. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_10_04_99
    ... STIS/CCD/MA1 7481 (The Wind-momentum Luminosity Relationship for M31 and M33 B-supergiants) The Space Telescope Imaging Spectrograph (CCD and MA1) was used to make observations of the B class supergiant star M-31-OB10 which is located in the M-31 galaxy ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_10_04_99 -- 19.4 Кб -- 04.10.1999
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    90. http://www.stsci.edu/institute/conference/hsl/Kilston.PDF
    ... SUVO paper) Wavelength Coverage Angular Resolution 0.6 - 28 µm 30 mas (/14 , 0.75 µm) MAB = 31 5x6 0.3 - 1.0 µm 10 x 25 mas (/140) V = 34 >2x2 0.11 - 1.0 µm 15 mas (/14 , 0.5 µm) MAB = 32 12 x 12 System Sensitivity Usable FOV, arcmin S. KILSTON -- LARGE ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/hsl/Kilston.PDF -- 2480.6 Кб -- 10.04.2006
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