Page   1
    PROPOSAL FOR HUBBLE SPACE TELESCOPE OBSERVATIONS   ST ScI Use Only
                                                       ID 5419
                                                       Report Date: 18-Jul-95:17:21
                                                       Version: **********
                                                       Check-in Date: **********

1.Proposal Title:
A SEARCH FOR VERY LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI IN NEARBY  GALAXIES: CYCLE4
MEDIUM
------------------------------------------------------------------------------------
2. Scientific Category   3. Proposal For  4. Proposal Type        5. Continuation ID
QUASARS & AGN               GO               1 Long Term yrs         <none>
Sub Category
OTHER ACTIVE NUCLEI
------------------------------------------------------------------------------------
6. Principal Investigator   Institution                    Country    Telephone
 Wallace W. Sargent         CALTECH                        USA        818-356-4055

------------------------------------------------------------------------------------
7. Abstract
Using UV (F160BW) and visual (F547M) continuum images obtained with WFPC2, we will
search for spatially unresolved, UV-bright nuclei in nearby galaxies. The goals are
to discover very low-luminosity AGNs, and to see whether there is a lower limit to
the activity. This is a natural extension of the large spectroscopic survey we have
already conducted at Palomar. Galaxies to be observed are those in which broad H-
alpha emission was either NOT detected or possibly detected in our ground-based
study, but whose morphology (Hubble type) and narrow emission lines appear similar
to those of galaxies in which broad H-alpha WAS detected. Images of 25 nearby
galaxies will be obtained during Cycle 4. In future cycles, we will propose
spectroscopic observations of the most probable AGNs detected through the imaging
study. In most galaxies, low-luminosity active nuclei are very difficult to discern
at optical wavelengths due to the dominance of the stellar continuum. At UV
wavelengths, on the other hand, contamination from the old stellar population is
low, making it possible to detect a nonstellar continuum. As by-products of this
study, we will publish high-resolution UV and visual surface photometry of the
observed galaxies, and we will identify interesting morphological features (e.g.,
dust lanes, blue stars, HII regions). Moreover, we will be able to recognize compact
cores that may be produced by massive central black holes.
------------------------------------------------------------------------------------
------------------------------------------------------------------------------------
9. Est obs time (hours) pri: 11.58    par: 0       10. Num targs pri: 21     par: 0
------------------------------------------------------------------------------------
11. Instruments requested:  WF/PC
------------------------------------------------------------------------------------
------------------------------------------------------------------------------------
                                                                  Page   2
I. GENERAL FORM    Proposal 5419
PI:  Wallace W. Sargent
Proposal Title:
A SEARCH FOR VERY LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI IN NEARBY  GALAXIES: CYCLE4
MEDIUM
------------------------------------------------------------------------------------

1. Proposers:
Proposers                        Institution                       Country       ESA
------------------------------------------------------------------------------------
 Wallace W. Sargent              1590                              USA
 Alexei V. Filippenko            1500                              USA
 Luis C. Ho                      1500                              USA
------------------------------------------------------------------------------------
  3. Description of proposed observations.
  We plan to obtain two WFPC2 (PC) images of each of 21 bright, nearby galaxies.
 The first exposure will utilize the F160BW (Woods) filter to measure the
 distribution of UV light, while the second will be done through the F547M
 (visual) filter for comparison. In each case the red exposure is short, but quite
 important. At the typical distances and absolute magnitudes of our program
 galaxies, expected core radii based on observed core parameter relations are
 typically 0.2", and many are expected to be < 0.1". Therefore, since the profiles
 are likely to be cuspy anyway, we need to have a method for determining which
 cores are probably AGNs (bright in the UV relative to the visual) --- the V-band
 cusps could just be star clusters. Measurements of color gradients in the nuclear
 regions will also help us eliminate cases in which dust rings or stellar
 population gradients produce unresolved (or nearly unresolved) nuclei. These data
 will allow us to discover galaxies having unresolved UV-bright nuclei. Photometry
 of the nuclei will be done, and the results will be used to determine
 spectroscopic exposure times in future proposals. (The exposure times strongly
 depend on the surface brightness of the inner few tenths of an arc second; prior
 to HST, this was not known for any galaxies.) We will also perform surface
 photometry of these images, and we will look for features such as dust lanes, HII
 regions, and hot stars in the circumnuclear regions.
                                                                  Page   3
------------------------------------------------------------------------------------
  4. Justification of need for HST observations.
  It is extremely difficult to detect a faint, point-like LLAGN in ground- based
 images --- at visual wavelengths, the surrounding starlight completely dominates
 the image. Even in the U and B bands, observable from the ground, starlight
 contamination within the seeing disk is too severe, and in any case the
 contribution of a nonstellar continuum is small. Indeed, we have obtained such
 images of many galaxies in our sample, but unresolved nuclei are not visible in
 them. Ground-based spectroscopic techniques also fail at such low luminosities;
 we have pushed spectroscopy to its limit in our extensive survey for weak, broad
 H-alpha emission in nearby galactic nuclei. Around 1600 A, on the other hand, the
 contribution of starlight is minimal, yet the WFPC2 on HST is fairly efficient.
 Emission from active nuclei much weaker than currently known can easily be
 discerned from the bulge background, as demonstrated in Figure 3. The PC is
 preferred over the FOC/96 because the latter may saturate with the high count
 rates expected in galactic nuclei; moreover, the PC provides a wider field of
 view (35" X 35" instead of a maximum of 14" X 14"), enabling us to study a larger
 portion of each galaxy. Most of the galaxies already observed with HST were not
 imaged through a filter combination that effectively blocks out the red leak.
 Moreover, visual or red images were generally not obtained, so it is difficult to
 determine whether the cuspy nucleus (if present) is simply a dense concentration
 of stars. Finally, many of the imaged galaxies were not good candidates for
 LLAGNs based on our existing survey, or were already known to be Seyferts.   We
 estimate that the typical central UV surface brightness will be 20 mag per square
 arcsec (using AB magnitudes, defined by Oke and Gunn, 1983, ApJ, 266, 713).
 According to the WFPC2 Handbook, the integral of QT dl/l = 0.001 for the F160BW
 filter. Thus, the count rate per 0.046" X 0.046" pixel will be 0.0046 per second,
 and a 30-minute exposure will yield a S/N ratio of about 3 per pixel. Point-like
 UV nuclei should be even brighter in the central few pixels; they will easily be
 detected, and good photometry will be obtained. The F547M observation will
 require only 5 minutes for S/N = 25 per pixel. To evaluate the feasibility of
 this project, we created simulated UV images of galaxies with parameters typical
 of our sample. The spheroid of the simulated galaxy, which fills all of the field
 of view, was modeled as a de Vaucouleurs law, with a central UV surface
 brightness taken from the recent ASTRO measurements of several galaxies
 (O'Connell, 1991, private communication). The image was then convolved with the
 observed HST PSF, and the expected amount of noise was added. Point sources of
 various magnitudes were added to the nucleus of the galaxy, and at various radii
 from the center. Figure 3 shows an example of such a simulation. The central
 point source, of magnitude 20 in this case, is easily visible above the
 background. The other two point sources, also discernable, have UV magnitudes of
 22-23 and correspond to small clusters of O-type stars at the distance of our
 typical galaxy (10 Mpc).
------------------------------------------------------------------------------------
  5. Description of special scheduling requirements.
  None.
------------------------------------------------------------------------------------
  6. Description of special calibration exposures.
  None.
------------------------------------------------------------------------------------
  8. Additional comments or special requests.
  Note that we had request to use the F218W filter
                                                                  Page   4
------------------------------------------------------------------------------------
  9. Description of previous HST work.
  2078, A Search for Primordial Gas: is I Zw 18 a Young Galaxy? -- D. Kunth, J.
 Lequeux, W. Sargent, F. Viallefond 2424, Quasar Absorption Line Survey. -- J.
 Bahcall, W. Sargent, et al. 2590, Deep Imaging of the Site of SN 1961V. -- A.
 Filippenko, et al. 3507, UV Spectroscopy and High-Resolution Imaging of NGC 4395.
 -- A. Filippenko, W. Sargent, L. Ho 3519, UV Imaging of Nearby Galaxies. -- D.
 Maoz, A. Filippenko, et al. 3810, The Stellar Population of Wolf-Rayet Galaxies.
 -- P. Conti, A. Filippenko, W. Sargent, L. Ho, C. Leitherer, C. Robert, W. Vacca
 4302, Supernovae and their Local Environment. -- A. Filippenko, et al. 4312,
 Circumstellar Material around Supernovae. -- A. Filippenko, et al. 4340, Origin
 of Blue Featureless Continuum in Seyfert 2 Nuclei. -- A. Filippenko, L. Ho 4350,
 FOS Observations of LINER Galaxy Nuclei. -- G. Reichert, A. Filippenko, L. Ho, J.
 Shields, R. Mushotzky, K. Mason, G. Branduardi-Raymont, C. Wu. 4635, Accretion
 Disk Line-Profile Hypothesis in Arp 102B. -- A. Filippenko, J. Halpern, M.
 Eracleous, K. Chen PUBLICATIONS: "A Gravitational Lens Candidate Discovered with
 the Hubble Space Telescope." D. Maoz, J. N. Bahcall, D. P. Schneider, R. Doxsey,
 N. A. Bahcall, A. V. Filippenko, W. M. Goss, O. Lahav, and B. Yanny;
 Astrophysical Journal (Letters), 386, L1 (1992).   "HST Observations of NGC 4395,
 the Least Luminous Seyfert 1 Nucleus: Evidence Against the Starburst Hypothesis
 for Broad-Lined Active Galactic Nuclei." A. V. Filippenko, L. C. Ho, and W. L. W.
 Sargent; Astrophysical Journal (Letters), 410, L75 (1993). "NGC 4395: Evidence
 Against the Starburst Hypothesis for Seyfert 1 Nuclei and QSOs." A. V.
 Filippenko, L. C. Ho, and W. L. W. Sargent; in 16th Texas Symposium/3rd Symposium
 on Particles, Strings, and Cosmology; ed. C. Akerlof and M. Srednicki (New York:
 New York Academy of Sciences), 707 (1993). "Was SN 1961V a Genuine Supernova?" G.
 C. Bower, A. V. Filippenko, et al. BAAS, 25, 819 (1993). "The HST Quasar
 Absorption Line Key Project I. First Observational Results, Including Lyman-alpha
 and Lyman Limit Systems." J. N. Bahcall, et al.; Astrophysical Journal, in press
 (1993). "The HST Quasar Absorption Line Key Project II. Data Calibration and
 Absorption Line Selection." D. P. Schneider et al.; Astrophys. Journal, in press
 (1993). "The HST Quasar Absorption Line Key Project III. First Observational
 Results on the Milky Way Gas." B. Savage et al.; Astrophys. Journal, in press
 (1993). "CCD Imaging of Hubble Space Telescope Quasar Fields." S. Kirhakos, W. L.
 W. Sargent, D. P. Schneider, J. N. Bahcall, B. T. Jannuzi, D. Maoz, and T. A.
 Small; Publ. Astron. Soc. Pacific, in press (1993). "Is There Primordial Gas in I
 Zw 18?" D. Kunth, J. Lequeux, W. Sargent, and F. Viallefond; Astron. Astrophys.,
 in press (1993).
------------------------------------------------------------------------------------
 10. Resources to be supplied by investigator's institution(s).
  Both Caltech and U.C. Berkeley have extensive computing facilities (VMS and
 UNIX) in their Astronomy Departments. Image-processing workstations, graphics
 terminals, laser printers, large disks, and tape drives are all available. Many
 computer programs exist for analysis of data. Both institutions also have many
 extremely capable graduate students and postdoctoral fellows, a few of whom may
 participate in various aspects of this project. Ground-based complementary
 observations may readily be obtained at both Palomar and Lick Observatories. The
 usual secretarial and technical support is available at Caltech and Berkeley.
------------------------------------------------------------------------------------
11. Address Information
                                                                  Page   5
Name:  WALLACE W. SARGENT                                  Category: PI
Institution: 1590
Address:  ASTRONOMY/PALOMAR OBSERVATORY
          MAIL CODE 105-24
          CALTECH
City: PASADENA                                  State: CA
Zip Code: 91125                                 Country: USA
Telephone: 818-356-4055
Telex (or e-mail): WWS@DEIMOS.CALTECH.EDU
------------------------------------------------------------------------------------
Name:  ALEXEI V. FILIPPENKO                                Category: CON
Institution: 1500
Address:  ASTRONOMY DEPARTMENT
          601 CAMPBELL HALL
          UNIV. OF CALIFORNIA
City: BERKELEY                                  State: CA
Zip Code: 94720                                 Country: USA
Telephone: 510-642-1813
Telex (or e-mail): ALEX@BKYAST.BERKELEY.EDU
------------------------------------------------------------------------------------
TARGET LIST    a) Fixed Targets                                                                    ID = 5419             [  6]
------------------------------------------------------------------------------------------------------------------------------------
 1 |     2      |           3           |              4             |  5     |   6    |  7  |              8
------------------------------------------------------------------------------------------------------------------------------------
Tar|   Target   |         Target        |            Target          |Coord   | Radial |Acqui|FLX|     Flux data
No |    Name    |       Description     |           Position         |Eqnx    |  Vel.  |Prblm|REF|
   |            |                       |                            |        |        |     |   |
------------------------------------------------------------------------------------------------------------------------------------
1   NGC1961      E,301,317,910           RA = 05H 42M 04.5S +/- 0.1S, 2000     V =            1   V = 11.8 +/- 0.5
                                         DEC = +69D 22' 43.6" +/-              +3940          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
2   NGC2655      E,301,317,910           RA = 08H 55M 37.5S +/- 0.1S, 2000     V =            1   V = 11.0 +/- 0.5
                                         DEC = +78D 13' 24.9" +/-              +1390          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
3   NGC3166      E,301,317,910           RA = 10H 13M 45.6S +/- 0.1S, 2000     V =            1   V = 11.5 +/- 0.5
                                         DEC = +03D 25' 29.6" +/-              +1340          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
4   NGC3169      E,301,317,910           RA = 10H 14M 14.9S +/- 0.1S, 2000     V =            1   V = 11.3 +/- 0.5
                                         DEC = +03D 28' 00.0" +/-              +1240          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
5   NGC3607      E,302,317,910           RA = 11H 16M 54.7S +/- 0.1S, 2000     V = +930       1   V = 11.1 +/- 0.5
                                         DEC = +18D 03' 06.1" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
6   NGC3642      E,301,317,910           RA = 11H 22M 17.9S +/- 0.1S, 2000     V =            1   V = 11.5 +/- 0.5
                                         DEC = +59D 04' 28.4" +/-              +1620          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
7   NGC3718      E,301,317,910           RA = 11H 32M 34.9S +/- 0.1S, 2000     V =            1   V = 11.3 +/- 0.5
                                         DEC = +53D 04' 05.5" +/-              +1000          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
TARGET LIST    a) Fixed Targets                                                                    ID = 5419             [  7]
------------------------------------------------------------------------------------------------------------------------------------
 1 |     2      |           3           |              4             |  5     |   6    |  7  |              8
------------------------------------------------------------------------------------------------------------------------------------
Tar|   Target   |         Target        |            Target          |Coord   | Radial |Acqui|FLX|     Flux data
No |    Name    |       Description     |           Position         |Eqnx    |  Vel.  |Prblm|REF|
   |            |                       |                            |        |        |     |   |
------------------------------------------------------------------------------------------------------------------------------------
8   NGC3992      E,301,317,910           RA = 11H 57M 36.0S +/- 0.1S, 2000     V =            1   V = 10.6 +/- 0.5
                                         DEC = +53D 22' 29.6" +/-              +1050          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
9   NGC4036      E,301,317,910           RA = 12H 01M 26.7S +/- 0.1S, 2000     V =            1   V = 11.6 +/- 0.5
                                         DEC = +61D 53' 45.3" +/-              +1382          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
10  NGC4111      E,301,317,910           RA = 12H 07M 03.1S +/- 0.1S, 2000     V = +790       1   V = 11.8 +/- 0.5
                                         DEC = +43D 03' 56.8" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
11  NGC4192      E,301,317,910           RA = 12H 13M 48.3S +/- 0.1S, 2000     V = -140       1   V = 10.9 +/- 0.5
                                         DEC = +14D 54' 01.6" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
12  NGC4203      E,302,317,910           RA = 12H 15M 05.0S +/- 0.1S, 2000     V = +934       1   V = 11.6 +/- 0.5
                                         DEC = +33D 11' 50.0" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
13  NGC4438      E,301,317,910           RA = 12H 27M 45.6S +/- 0.1S, 2000     V = +934       1   V = 10.9 +/- 0.5
                                         DEC = +13D 00' 32.6" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
14  NGC4569      E,301,317,910           RA = 12H 36M 49.8S +/- 0.1S, 2000     V = -260       1   V = 10.2 +/- 0.5
                                         DEC = +13D 09' 46.5" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
TARGET LIST    a) Fixed Targets                                                                    ID = 5419             [  8]
------------------------------------------------------------------------------------------------------------------------------------
 1 |     2      |           3           |              4             |  5     |   6    |  7  |              8
------------------------------------------------------------------------------------------------------------------------------------
Tar|   Target   |         Target        |            Target          |Coord   | Radial |Acqui|FLX|     Flux data
No |    Name    |       Description     |           Position         |Eqnx    |  Vel.  |Prblm|REF|
   |            |                       |                            |        |        |     |   |
------------------------------------------------------------------------------------------------------------------------------------
15  NGC4651      E,301,317,910           RA = 12H 43M 41.9S +/- 0.1S, 2000     V = +790       1   V = 11.4 +/- 0.5
                                         DEC = +16D 23' 36.1" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
16  NGC5005      E,301,317,910           RA = 13H 10M 56.1S +/- 0.1S, 2000     V =            1   V = 10.6 +/- 0.5
                                         DEC = +37D 03' 30.6" +/-              +1020          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
17  NGC5195      E,302,317,910           RA = 13H 29M 59.3S +/- 0.1S, 2000     V =            1   V = 10.5 +/- 0.5
                                         DEC = +47D 15' 57.7" +/-              +1020          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
18  NGC6500      E,301,317,910           RA = 17H 55M 59.7S +/- 0.1S, 2000     V =            1   V = 12.9 +/- 0.5
                                         DEC = +18D 20' 18.3" +/-              +2000          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
19  NGC6951      E,301,317,910           RA = 20H 37M 14.0S +/- 0.1S, 2000     V =            1   V = 12.2 +/- 0.5
                                         DEC = +66D 06' 21.2" +/-              +1430          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
20  NGC7217      E,301,317,910           RA = 22H 07M 52.4S +/- 0.1S, 2000     V = +950       1   V = 11.1 +/- 0.5
                                         DEC = +31D 21' 34.0" +/-                             2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
21  NGC7743      E,301,317,910           RA = 23H 44M 21.1S +/- 0.1S, 2000     V =            1   V = 12.1 +/- 0.5
                                         DEC = +09D 56' 03.2" +/-              +1800          2   B-V = 0.8 +/- 0.3
                                         1.0"
     Comments: MAGNITUDES AND COLORS REFER TO ENTIRE
             GALAXY, NOT JUST THE NUCLEUS WHICH WILL BE
             IMAGED.
------------------------------------------------------------------------------------------------------------------------------------
EXPOSURE LOGSHEET                                                                                  ID = 5419             [  9]
------------------------------------------------------------------------------------------------------------------------------------
 1      |   2   |      3    |  4   |   5   |   6   |    7   |   8   |       9       |10 |   11  |   12    |13 |14|        15
------------------------------------------------------------------------------------------------------------------------------------
  Line  |  Seq  |   Target  |Instr | Oper. | Aper  |Spectral|Central|   Optional    |Num|  Time |   S/N   |Flx|Pr|     Special
 Number | Name  |    Name   |Config| Mode  |or FOV |Element |Waveln.|  Parameters   |Exp|       |Rel. Time|Ref|  |   Requirements
------------------------------------------------------------------------------------------------------------------------------------
1                NGC1961     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   31 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 1-2 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
2                NGC1961     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   32 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
3                NGC2655     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1600S   3         1   33 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 3-4 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
4                NGC2655     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   34 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
5                NGC3166     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   35 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 5-6 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
6                NGC3166     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   36 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
7                NGC3169     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1600S   3         1   37 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 7-8 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
EXPOSURE LOGSHEET                                                                                  ID = 5419             [ 10]
------------------------------------------------------------------------------------------------------------------------------------
 1      |   2   |      3    |  4   |   5   |   6   |    7   |   8   |       9       |10 |   11  |   12    |13 |14|        15
------------------------------------------------------------------------------------------------------------------------------------
  Line  |  Seq  |   Target  |Instr | Oper. | Aper  |Spectral|Central|   Optional    |Num|  Time |   S/N   |Flx|Pr|     Special
 Number | Name  |    Name   |Config| Mode  |or FOV |Element |Waveln.|  Parameters   |Exp|       |Rel. Time|Ref|  |   Requirements
------------------------------------------------------------------------------------------------------------------------------------
8                NGC3169     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   260S    25        1   38 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
9                NGC3607     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1600S   3         1   39 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 9-10 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
10               NGC3607     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   260S    25        1   40 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
11               NGC3642     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   1  CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 11-12 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
12               NGC3642     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   2  CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
13               NGC3718     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   3  CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 13-14 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
14               NGC3718     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   4  CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
EXPOSURE LOGSHEET                                                                                  ID = 5419             [ 11]
------------------------------------------------------------------------------------------------------------------------------------
 1      |   2   |      3    |  4   |   5   |   6   |    7   |   8   |       9       |10 |   11  |   12    |13 |14|        15
------------------------------------------------------------------------------------------------------------------------------------
  Line  |  Seq  |   Target  |Instr | Oper. | Aper  |Spectral|Central|   Optional    |Num|  Time |   S/N   |Flx|Pr|     Special
 Number | Name  |    Name   |Config| Mode  |or FOV |Element |Waveln.|  Parameters   |Exp|       |Rel. Time|Ref|  |   Requirements
------------------------------------------------------------------------------------------------------------------------------------
15               NGC3992     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1400S   3         1   29 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 15-16 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
16               NGC3992     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   230S    25        1   30 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
17               NGC4036     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   27 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 17-18 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
18               NGC4036     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   28 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
19               NGC4111     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   25 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 19-20 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
20               NGC4111     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   26 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
21               NGC4192     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1400S   3         1   21 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 21-22 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
EXPOSURE LOGSHEET                                                                                  ID = 5419             [ 12]
------------------------------------------------------------------------------------------------------------------------------------
 1      |   2   |      3    |  4   |   5   |   6   |    7   |   8   |       9       |10 |   11  |   12    |13 |14|        15
------------------------------------------------------------------------------------------------------------------------------------
  Line  |  Seq  |   Target  |Instr | Oper. | Aper  |Spectral|Central|   Optional    |Num|  Time |   S/N   |Flx|Pr|     Special
 Number | Name  |    Name   |Config| Mode  |or FOV |Element |Waveln.|  Parameters   |Exp|       |Rel. Time|Ref|  |   Requirements
------------------------------------------------------------------------------------------------------------------------------------
22               NGC4192     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   230S    25        1   22 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
23               NGC4203     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   41 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 23-24 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
24               NGC4203     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   42 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
25               NGC4438     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1600S   3         1   17 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 25-26 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
26               NGC4438     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   260S    25        1   18 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
27               NGC4569     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1400S   3         1   15 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 27-28 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
28               NGC4569     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   230S    25        1   16 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
EXPOSURE LOGSHEET                                                                                  ID = 5419             [ 13]
------------------------------------------------------------------------------------------------------------------------------------
 1      |   2   |      3    |  4   |   5   |   6   |    7   |   8   |       9       |10 |   11  |   12    |13 |14|        15
------------------------------------------------------------------------------------------------------------------------------------
  Line  |  Seq  |   Target  |Instr | Oper. | Aper  |Spectral|Central|   Optional    |Num|  Time |   S/N   |Flx|Pr|     Special
 Number | Name  |    Name   |Config| Mode  |or FOV |Element |Waveln.|  Parameters   |Exp|       |Rel. Time|Ref|  |   Requirements
------------------------------------------------------------------------------------------------------------------------------------
29               NGC4651     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   13 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 29-30 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
30               NGC4651     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   14 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
31               NGC5005     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1400S   3         1   7  CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 31-32 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
32               NGC5005     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   230S    25        1   8  CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
33               NGC5195     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1400S   3         1   11 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 33-34 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
34               NGC5195     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   230S    25        1   12 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
35               NGC6500     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   2200S   3         1   5  CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 35-36 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
EXPOSURE LOGSHEET                                                                                  ID = 5419             [ 14]
------------------------------------------------------------------------------------------------------------------------------------
 1      |   2   |      3    |  4   |   5   |   6   |    7   |   8   |       9       |10 |   11  |   12    |13 |14|        15
------------------------------------------------------------------------------------------------------------------------------------
  Line  |  Seq  |   Target  |Instr | Oper. | Aper  |Spectral|Central|   Optional    |Num|  Time |   S/N   |Flx|Pr|     Special
 Number | Name  |    Name   |Config| Mode  |or FOV |Element |Waveln.|  Parameters   |Exp|       |Rel. Time|Ref|  |   Requirements
------------------------------------------------------------------------------------------------------------------------------------
36               NGC6500     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   350S    25        1   6  CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
37               NGC6951     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   2000S   3         1   9  CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 37-38 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
38               NGC6951     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   10 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
39               NGC7217     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   1800S   3         1   23 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 39-40 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
40               NGC7217     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   24 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
41               NGC7743     WFPC2  IMAGE   PC1     F218W    1523    CR-             1   2000S   3         1   19 CYCLE 4
                                                                     TOLERANCE=0.0                         2      GROUP 41-42 NO GAP
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
42               NGC7743     WFPC2  IMAGE   PC1     F547M    5479    CR-SPLIT=NO     1   300S    25        1   20 CYCLE 4
                                                                                                           2
     Comments: IF THERE IS EXTRA TIME BEFORE
               EARTH OCCULTATION NEAR END OF
               EXPOSURE, CAN INCREASE EXPOSURE
               TIME TO INCREASE S/N RATIO.
------------------------------------------------------------------------------------------------------------------------------------
            Summary Form for Proposal 5419                                                                               [ 15]

  Item                          Used in this proposal
------------------------------------------------------------------------------------------------------------------------------------
  Configurations                WFPC2
------------------------------------------------------------------------------------------------------------------------------------
  Opmodes                       IMAGE
------------------------------------------------------------------------------------------------------------------------------------
  Optional Parameters           CR-TOLERANCE=0.0 CR-SPLIT=NO
------------------------------------------------------------------------------------------------------------------------------------
  Proposal for                  GO
------------------------------------------------------------------------------------------------------------------------------------
  S/C Hours                     11.58
------------------------------------------------------------------------------------------------------------------------------------
  Scientific Category           QUASARS & AGN
------------------------------------------------------------------------------------------------------------------------------------
  Scientific Sub-category       OTHER ACTIVE NUCLEI
------------------------------------------------------------------------------------------------------------------------------------
  Special Requirements          CYCLE 4; GROUP 1-2 NO GAP GROUP 3-4 NO GAP GROUP 5-6 NO GAP GROUP 7-8 NO GAP GROUP 9-10 NO GAP
                                GROUP 11-12 NO GAP GROUP 13-14 NO GAP GROUP 15-16 NO GAP GROUP 17-18 NO GAP GROUP 19-20 NO GAP
                                GROUP 21-22 NO GAP GROUP 23-24 NO GAP GROUP 25-26 NO GAP GROUP 27-28 NO GAP GROUP 29-30 NO GAP
                                GROUP 31-32 NO GAP GROUP 33-34 NO GAP GROUP 35-36 NO GAP GROUP 37-38 NO GAP GROUP 39-40 NO GAP
                                GROUP 41-42 NO GAP
------------------------------------------------------------------------------------------------------------------------------------
  Spectral Elements             F218W F547M
------------------------------------------------------------------------------------------------------------------------------------
  Target Names                  NGC1961 NGC2655 NGC3166 NGC3169 NGC3607 NGC3642 NGC3718 NGC3992 NGC4036 NGC4111 NGC4192 NGC4203
                                NGC4438 NGC4569 NGC4651 NGC5005 NGC5195 NGC6500 NGC6951 NGC7217 NGC7743
------------------------------------------------------------------------------------------------------------------------------------