MMT Observing Schedule
January-April 1998

Date*    Day  Moon    Observer           Instrument    Operator  Program

 1 (12.0) Th   3.4     Falco            Blue Channel    Milone     SAO2 
 2 ( "  ) F    4.3       "                   "            "          " 
 3 ( "  ) S    5.3  Luhman/UAO TBS      Red Channel       "         S26 
 4 (11.9) S    6.2    McNamara          Blue Channel      "        SAO7 
 5 ( "  ) M    7.2       "                   "            "          " 
 6 ( "  ) T    8.1     Torres             Echelle       Heller     SAO11 
 7 ( "  ) W    9.1       "                   "            "          " 
 8 ( "  ) Th  10.0       "                   "            "          " 
 9 ( "  ) F   11.0       "                   "            "          " 
10 ( "  ) S   11.9       "                   "            "          " 
11 ( "  ) S   12.9       "                   "            "          " 
12 (11.8) M   13.8     Latham                "            "        SAO10 
13 ( "  ) T  -13.2       "                   "          Milone       " 
14 ( "  ) W  -12.3       "                   "            "          " 
15 ( "  ) Th -11.3    Stefanik               "            "        SAO9 
16 ( "  ) F  -10.4  Hinz et al.           Mirac II        "         S11 
17 ( "  ) S   -9.4       "                   "            "          " 
18 (11.7) S   -8.5    Director               "            "     Director
19 ( "  ) M   -7.5       "                   "            "          " 
20 ( "  ) T   -6.6  Green et al.        Blue Channel    McAfee      S10 
21 ( "  ) W   -5.7       "                   "            "          " 
22 ( "  ) Th  -4.7  Green et al.             "            "         S17 
23 (11.6) F   -3.8  Impey et al.             "            "         S34 
24 ( "  ) S   -2.8       "                   "            "          " 
25 ( "  ) S   -1.9    Kirshner               "            "        SAO5 
26 ( "  ) M   -0.9       "                   "            "          " 
27 ( "  ) T    0.0       "                   "          Heller       " 
28 (11.5) W    1.0   Burstein et al.    Red Channel       "         S2 
29 ( "  ) Th   1.9   Impey et al.       Blue Channel      "         S34 
30 ( "  ) F    2.9       "                   "            "          " 
31 ( "  ) S    3.8   Kulkarni et al.         "            "         S3 

 * Numbers in parentheses are the number of hours for which the sun is greater
   than 12 degrees below the horizon.

Date*    Day  Moon    Observer           Instrument    Operator  Program

 1 (11.5) S    4.8  Kulkarni et al.     Blue Channel    Heller      S3 
 2 (11.4) M    5.7    Caldwell               "            "        SAO4 
 3 ( "  ) T    6.7       "                   "          McAfee       " 
 4 ( "  ) W    7.6     Barmby                "            "        SAO8 
 5 ( "  ) Th   8.6    Briceno                "            "        SAO6 
 6 (11.3) F    9.5  Rieke,Biscaya          F-Spec         "         S4 
 7 ( "  ) S   10.5  Luhman/Riekes            "            "      S26/S12
 8 ( "  ) S   11.4      "/"                  "            "          " 
 9 ( "  ) M   12.4      "/"                  "            "          " 
10 ( "  ) T   13.3  Ivanov et al.            "          Milone      S21 
11 (11.2) W  -13.7       "                   "            "          " 
12 ( "  ) Th -12.8   Meyer,Chen              "            "         S6 
13 ( "  ) F  -11.8   Meyer,Chen         Red Channel       "          " 
14 ( "  ) S  -10.9    Director               "            "     Director
15 (11.1) S   -9.9       "                   "            "          " 
16 ( "  ) M   -9.0  Nominal Shutdown                  
                    Hinz (Conditional)    Mirac II        "         S11
17 ( "  ) T   -8.0   "       "                          Heller       " 
18 (11.0) W   -7.1   "       "               "            "          "
19 ( "  ) Th  -6.2   "       "               "            "          "
20 ( "  ) F   -5.2  Kim      "          Blue Channel      "        SAO3 
21 (10.9) S   -4.3   "       "               "            "          "
22 ( "  ) S   -3.3   "       "               "            "          "
23 ( "  ) M   -2.4 Barmby    "               "            "        SAO8
24 ( "  ) T   -1.4 
25 (10.8) W   -0.5 
26 ( "  ) Th   0.5 
27 ( "  ) F    1.4 
28 (10.7) S    2.4 

 * Numbers in parentheses are the number of hours for which the sun is greater
   than 12 degrees below the horizon.

   1  Garcia        GRB OIR Counterparts      SpecB+R  1G    +++    1.05
   2  Falco         Flat Spectrum Sources     SpecB    2D     2D    1.00
   3  Kim           X-ray Selected Red Qsrs   SpecB    3D     +?   -0.88
   4  Caldwell      PN in Dwarf Spheroidals   SpecB    2D     2D   -0.13  
   5  Kirshner      SN Spectroscopy           SpecB    3D     3D    1.18
   6  Briceno       Very Low mass PMS Stars   SpecB    1G     1G    0.57
   7  McNamara      ROSAT Clusters            SpecB    2D     2D   -0.15 
   8  Barmby        NGC 2403 Globs            SpecB    2D    1G+?  -0.82
   9  Stefanik      Hyades Binary Survey      Ech      1G     1L   -0.24
  10  Latham        Thick Disk Origins        Ech      3L     3L   -1.13
  11  Torres        Rosat PMS Candidates      Ech      3L     3L   -0.11
  11  Torres        ROSAT PMS - moved from 60" Ech            3L

   Nights Requested:    14D  +  3G   + 6L

   +++ Ask Scheduled Observers
   +? time scheduled after nominal shutdown


MMT Observing Programs
January - February 1998


S2     Burstein, Li, Chen            Is BATC 329-287 the Most 
                                     Metal-Weak Galaxy Known?

S3     Kulkarni, Bechtold, Ge        Abundances and Ionization of 
                                     Elements in Damped Lyman Alpha 
                                     Galaxies

S4     G. Rieke, Biscaya             Infrared Spectroscopy of Young 
                                     Stellar Objects: Study of Vari-
                                     -ability in the First Overtone CO 
                                     Bands in Emission

S6     Meyer, Chen                   The Origins of Stellar Masses: 
                                     Constraining the Low Mass IMF in
                                     the Mon R2 Stellar Cluster

S10    Green, Liebert, Peterson      Blue Giants, Blue Stragglers, and
                                     Blue Horizontal Branch Stars in 
                                     Old, Metal-Rich Open Clusters

S11    Hinz, Angel, Hoffmann,        Nulling Interferometry
       McCarthy, Woolf

S12    G. Rieke, M. Rieke, Vanzi     Coronal Line Diagnostics for 
                                     Intermediate Line Regions

S17    Green, Liebert, Saffer        Two Different Kinds of Binary 
                                     SdB Stars?

S21    Ivanov, Engelbracht,          High Spatial Resolution Spectros-
       G. Rieke, M. Rieke, -          copy of Starburst Galaxies
       Alonso, Kulesa

S26    Luhman, G. Rieke, Meyer       The Low-Mass IMF in Young Clusters: 
                                     NGC 1333 and NGC 2024
 
S34    Impey, Petry, Liu             Quasar Absorption Probes of the 
                                     Hubble Deep Field

SAO2   Falco, Kochanek, Muqoz        A Redshift Survey of Flat-Spectrum 
                                     Radio Sources

SAO3   Kim, Elvis                    X-Ray Selected Red Quasars

SAO4   Caldwell, Armandroff,         Jacoby Planetary Nebulae in Dwarf 
                                     Spheroidal Galaxies
 
SAO5   Kirshner, Jha, Garnavich,     Supernova Spectroscopy
       Challis

SAO6   Briceqo, Hartmann             Search for Very Low Mass Pre-Main 
                                     Sequence Stars

SAO7   McNamara, Vikhlinin,          Redshifts for Distant ROSAT
       Forman, Jones                 Clusters
 
SAO8   Barmby, Huchra                Globular Cluster Candidates in
                                     NGC2403 

SAO9   Stefanik, Latham, Torres      Hyades Binary Survey

SAO10  Latham, Carney, Naoumov,      Thick Disk Origins
       Stefanik, Laird, Rose

SAO11  Torres, Neuhduser             ROSAT Pre-Main-Sequence Candidates