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    61. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_12_11_96
    ... 1.3 Completed FOS/RD 6300 (The Nature of the Central UV Source in = M-31) The Faint Object Spectrograph (Red Side) was used to make = ultraviolet spectrographic observations of the central 0.5 arcsecond = region of galaxy M-31 (aka, NGC-224). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_12_11_96 -- 4.7 Кб -- 11.12.1996
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    62. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_19_95
    ... 1.3 Completed FOS/96 5420 (Color-Magnitude Diagrams of globular clusters in M-31: Cycle 4 Medium) The Faint Object Spectrograph (F/96) was used to make spectrographic observations of the globular cluster G351 which is located in galaxy M-31 (aka, the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_19_95 -- 4.6 Кб -- 19.01.1995
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    63. http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_08_17_94
    ... 1.8 Completed WF/PC-2 5325 (The Horizontal Branch of the M-31 Dwarf Spheroidal Companion to Andromeda) The WF/PC-2 was used to make multiple long exposure observations of the dwarf spheroidal companion galaxy to the Andromeda galaxy (aka, M-31). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_08_17_94 -- 5.6 Кб -- 17.08.1994
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    64. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_08_18_99
    ... 1.10 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- G64 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_08_18_99 -- 7.9 Кб -- 18.08.1999
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    65. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_02_05_97
    ... Study of the Gaseous Halo of the = Andromeda Galaxy) The WF/PC-2 was used to make absorption line spectrographic = observations of object QSO 0035+4112 which is located behind the = Andromeda Galaxy (aka, M-31) in order to study the galaxy's gaseous halo ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_02_05_97 -- 3.5 Кб -- 05.02.1997
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    66. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_07_12_96
    ... Blue Side) was used to make = ultraviolet spectrographic observations of the super-metal-rich globular = cluster NGC-224-G17 which is located within the Andromeda Galaxy (aka, = M-31) in order to observe the spectral energy distribution of this = cluster ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_07_12_96 -- 3.1 Кб -- 12.07.1996
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    67. http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_07_23_93
    ... 1.9 Completed FOC/96 3870 (Imaging of M-31 Group Galaxies - Cycle 2) The Faint Object Camera (f/96) was used to make seven images of the object NGC-224 which is located near galaxy M-31 (The Andromeda Galaxy) to determine the population and gradients of ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_07_23_93 -- 10.9 Кб -- 26.07.1993
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    68. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_09_30_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- OB48 which is locate in the M-31 galaxy ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_09_30_99 -- 8.1 Кб -- 30.09.1999
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    69. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_11_24_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_11_24_98 -- 10.7 Кб -- 24.11.1998
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    70. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_08_06_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 B-133 which is locate in the M-31 galaxy ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_08_06_99 -- 8.4 Кб -- 06.08.1999
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