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    11. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_09_27_99
    ... Two Sets of 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 clusters M-31-G11 and M-31-G287 which are 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_09_27_99 -- 15.4 Кб -- 27.09.1999
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    12. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_09_14_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_14_98 -- 19.2 Кб -- 14.09.1998
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    13. http://www.stsci.edu/sms-deliv/1998049-220118-SMSSA05.text
    ... 32K,N,-)04974-1E3:E1:01 01 055:17:43:22 055:18:03:22 * M Com (SSAF,C,B:TW,H1, 1K,N,-)04974-1E3:E1:01 01 055:18:11:22 055:18:31:22 * M Com (MAR ,E,B:TE,H2,32K,N,-)04974-1E3:E1:02 01 055:18:11:22 055:18:31:22 * M Com (SSAF,C,B:TE,H2, 1K,N,-)04974-1E3:E1:02 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/sms-deliv/1998049-220118-SMSSA05.text -- 19.5 Кб -- 26.04.1999
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    14. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_06_14_99
    ... WF/PC-2 Photometry of A & B Supergiants in M-31 and M-33) The WF/PC-2 was used to ... is to study A and B supergiant stars in M-31 and M-33 with a precision far exceeding ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_06_14_99 -- 13.5 Кб -- 14.06.1999
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    15. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_11_15_95
    ... Completed WF/PC-2 6125 (Imaging and Spectroscopy of SN 1885 in M-31) The WF/PC-2 was used to make observations of Super Nova SN ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_11_15_95 -- 6.5 Кб -- 15.11.1995
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    16. http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2008-41.pdf
    ... Figure 1 . Montages of measured PSF images at 16 field points and at wavelengths 1.06µ (top) and 1.31µ (botto m). ... unfortunately occur near the core of the PSF at 1.31 m, rendering accurate evaluation of EE, etc., impossible for that image ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2008-41.pdf -- 2362.6 Кб -- 16.09.2008
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    17. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_03_01_99
    ... Two Sets of 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 clusters M-31-G33 and M-31-G319 which are 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_03_01_99 -- 13.4 Кб -- 01.03.1999
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    18. Modifying a USC
    ... N:FGS23GS Comment: Visit was unschedulable or had no FGS23 GSs when USC was cre ated -WMK 1997.122:10:18:52 1997.139:03:31:07 M:o C:25-Feb-1997 N:LRP_0nnnn01_CWV Comment: Override USC created to allow SOGS scheduling - LRP 1997.134:00:00:00 1999.004:00:00 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/spst/lrpg/aux_docs/modusc_proc.html -- 6.4 Кб -- 26.04.1999
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    19. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_09_24_98
    ... 2/3 7876 (The Giant Branch Luminosity Function of M-31's Bulge) The Near Infrared Camera (Cameras One, Two and Three) was used ... in the luminous M giant population of the bulge of M-31 is of considerable interest for stellar synthesis work and for ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_09_24_98 -- 8.7 Кб -- 24.09.1998
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    20. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_25_95
    ... 1.6 Completed FOS/BL 5349 (The UV Interstellar Extinction in M-31 and M-33) The Faint Object Spectrograph (Blue Side) was used to make observations of star M-31-OB8-17 which is located in galaxy M-31 (aka, The Andromeda Galaxy) to study interstellar ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_25_95 -- 6.3 Кб -- 25.01.1995
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