GSU OBSERVING REQUESTS FOR SMARTS TIME IN 2011A



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FEB 2011 THROUGH JUL 2011 (6 months)
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                              assumes 9.5 hours = 1.0 night during A semesters
                              1.5X --- for all service programs
                              1.2X --- if you need N hours of observations, including makeups

                              1.5m --- can only request time in 2011A for continuing programs
                              1.5m --- possible commissioning targets 11-31 JAN (4000-7000A)

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GSU PRIORITY 1 --- SCHEDULED 12.0 nights
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TELESCOPE + INSTRUMENT        1.3m + ANDICAM
TITLE                         Optical/IR Monitoring of Blazars
ID #                          GSTU51
PI                            Joe Eggen (GSU), Dick Miller (GSU)
CONTACT                       eggen@chara.gsu.edu, 573-301-6769
MODE (service or user)        service
TIME                          1.25 hour every 3 nights = 76 hours X 1.5 service = 114 hours = 12.0 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     N/A
PREFERRED DATES               any
ACCEPTABLE DATES              any
ACCEPTABLE MOON               any

CADENCE                       one observation set every 3 days
FILTERS                       always: first R/K, then B/J, then V/H
# OBJECTS                     4
STANDARDS                     none, differential photometry only

SCIENTIFIC DESCRIPTION        Continuing monitoring effort of variable blazars.  Cadence of one set of
                              observations every 3 days works well.

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GSU PRIORITY 2 --- SCHEDULED 7.0 nights
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TELESCOPE + INSTRUMENT        0.9m + 2K CCD
TITLE                         CTIOPI
ID #                          GSTU01
PI                            Todd Henry (GSU)
CONTACT                       thenry@chara.gsu.edu, 404-413-6054
MODE (service or user)        user
TIME                          7.0 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               FEB
ACCEPTABLE DATES              any
ACCEPTABLE MOON               ***** GRAY TIME IF POSSIBLE, PLEASE *****

CADENCE                       one run of 7 nights
PHOTOMETRIC?                  no
FILTERS                       VRI
                              
SCIENTIFIC DESCRIPTION        Continuing parallax/perturbation search effort.  Requires roughly one
                              week/month to catch appropriate parallax factors for all targets.

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GSU PRIORITY 3 --- SCHEDULED 3.0 nights
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TELESCOPE + INSTRUMENT        1.5m + RCSpec
TITLE                         RECONS Spectroscopy
ID #                          GSTU03
PI                            Adric Riedel (GSU), Todd Henry (GSU)
CONTACT                       riedel@chara.gsu.edu 404-413-6024, thenry@chara.gsu.edu
MODE (service or user)        service
TIME                          24 hours X 1.5 service = 36.0 hours = 3.8 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               any
ACCEPTABLE DATES              any
ACCEPTABLE MOON               any

CADENCE                       two spectra per star, one right after the other
PREFERRED SETUP               32/I with filter OG570 to cover 6000-9500 A
                              prefer 4" slit
EXPOSURE TIMES                varies by target

SCIENTIFIC DESCRIPTION        Spectroscopy of red dwarfs, young stars, and subdwarfs to identify nearby 
                              candidates for parallax program.  Example targets include:
                              
                              Star         V      R      I     SpType   IntTime

                              GJ0784      7.95   7.04   6.12   M0.0V    2 x  60 sec
                              GJ1125     11.72  10.58   9.13   M3.0V    2 x 300 sec
                              GJ1111     14.90  12.90  10.64   M6.0V    2 x 600 sec 
                              LHS2065    18.87  16.04  15.21   M9.0V    2 x 900 sec

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GSU PRIORITY 4 --- SCHEDULED 7.0 nights
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TELESCOPE + INSTRUMENT        0.9m + 2K CCD
TITLE                         CTIOPI
ID #                          GSTU01
PI                            Todd Henry (GSU)
CONTACT                       thenry@chara.gsu.edu, 404-413-6054
MODE (service or user)        user
TIME                          7.0 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               MAR
ACCEPTABLE DATES              any
ACCEPTABLE MOON               ***** GRAY TIME IF POSSIBLE PLEASE *****

CADENCE                       one run of 7 nights
PHOTOMETRIC?                  no
FILTERS                       VRI
                              
SCIENTIFIC DESCRIPTION        Continuing parallax/perturbation search effort.  Requires roughly one
                              week/month to catch appropriate parallax factors for all targets.

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GSU PRIORITY 5 --- SCHEDULED 1.3 nights
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TELESCOPE + INSTRUMENT        1.3m + ANDICAM
TITLE                         Light Curves of O-type Binaries
ID #                          GSTU77
PI                            Philip Massey (Lowell), Doug Gies (GSU)
CONTACT                       phil.massey@lowell.edu, 928-233-3264 
MODE (service or user)        service
TIME                          7.5 hours X 1.5 service = 11.3 hours = 1.2 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               DEC/JAN
ACCEPTABLE DATES              DEC/JAN/FEB/MAR
ACCEPTABLE MOON               any

CADENCE                       specific dates and times for eclipsing binaries
FILTERS                       V
# OBJECTS                     4
STANDARDS                     none, differential photometry only

SCIENTIFIC DESCRIPTION        Filling in light curves of 13 eclipsing variables in five LMC fields 
                              using 3 observations each at critical phases.  Each observation will 
                              consist of 2x10sec exposures in the V band.  Allowing for two readouts
                              (2x3 mins) and 5 minutes for pointing plus 0.5 min for exposure, each 
                              pointing will require 11.5 minutes.  So, 3 observations x 13 x 11.5 
                              minutes = 7.5 hours total.  The "windows" for the critical phases are 
                              a few hours long.

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GSU PRIORITY 6 --- SCHEDULED 7.0 nights
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TELESCOPE + INSTRUMENT        0.9m + 2K CCD
TITLE                         CTIOPI
ID #                          GSTU01
PI                            Todd Henry (GSU)
CONTACT                       thenry@chara.gsu.edu, 404-413-6054
MODE (service or user)        user
TIME                          7.0 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               MAY
ACCEPTABLE DATES              ***** GRAY TIME IF POSSIBLE, PLEASE *****
ACCEPTABLE MOON               any

CADENCE                       one run of 7 nights
PHOTOMETRIC?                  no
FILTERS                       VRI
                              
SCIENTIFIC DESCRIPTION        Continuing parallax/perturbation search effort.  Requires roughly one
                              week/month to catch appropriate parallax factors for all targets.

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GSU PRIORITY 7 --- SCHEDULED 3.0 nights
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TELESCOPE + INSTRUMENT        1.5m + RCSpec
TITLE                         Spectroscopy of AGN from the SWIFT/BAT Survey
ID #                          GSTU62
PI                            Mike Crenshaw, Travis Fischer (GSU)
CONTACT                       crenshaw@chara.gsu.edu, 404-413-6020
MODE (service or user)        service
TIME                          16 hours X 1.5 service X 1.2 tax = 28.8 hours = 3.0 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               any
ACCEPTABLE DATES              any
ACCEPTABLE MOON               dark/gray time preferred for the fainter targets

CADENCE                       only one visit per object
PREFERRED SETUP               26/Ia
EXPOSURE TIMES                single observations of 3600 sec
                              one grating per target = 16 total spectra

SCIENTIFIC DESCRIPTION        We will obtain blue spectra of AGN observed with BAT to get
                              optical data that coincide with the X-ray observations.  We will
                              determine accurate redshifts and emission-line fluxes for the
                              observed x-ray targets.

                              Object         RA  (2000.0)  DEC        Band   Mag    Type

                              ESO 434-40     09 47 40.17  -30 56 55.9   V    13.6    AGN
                              ESO 263-13     10 09 48.22  -42 48 40.4   V    14.9    AGN
                              ESO 374-44     10 13 19.92  -35 58 58.0   V    15.0    AGN
                              2MASXJ10402231-4625264                    V    16.8    AGN
                              ESO439-G009    11 27 23.42  -29 15 27.18  V    15.5    AGN
                              2MASX J12024767-5350082                   V    17.3    AGN
                              ESO 506-27     12 38 54.59  -27 18 28.4   V    14.6    AGN
                              ESO 511-30     14 19 22.43  -26 38 40.8   V    14.9    AGN
                              2MASX J14551742-5134150                   V    16.0    AGN
                              2MASX J16115141-6037549                   V    16.0    AGN
                              2MASX J16183642-5927175                   V    16.0    AGN
                              ESO 137-34     16 35 13.70  -58 04 48.0   V    12.2    AGN
                              2MASXJ16481523-3035037                    V    15.8    AGN
                              ESO103-035     18 38 20.36  -65 25 39.1   V    14.8    AGN
                              ESO 140-43     18 44 54.01  -62 21 53.2   V    14.1    AGN
                              NGC 6860       20 08 46.80  -61 05 59.6   V    13.7    AGN

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GSU PRIORITY 8 --- SCHEDULED 7.0 nights
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TELESCOPE + INSTRUMENT        0.9m + 2K CCD
TITLE                         CTIOPI
ID #                          GSTU01
PI                            Todd Henry (GSU)
CONTACT                       thenry@chara.gsu.edu, 404-413-6054
MODE (service or user)        user
TIME                          7.0 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               JUN
ACCEPTABLE DATES              any
ACCEPTABLE MOON               any

CADENCE                       one run of 7 nights
PHOTOMETRIC?                  no
FILTERS                       VRI
                              
SCIENTIFIC DESCRIPTION        Continuing parallax/perturbation search effort.  Requires roughly one
                              week/month to catch appropriate parallax factors for all targets.

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GSU PRIORITY 9 --- SCHEDULED 0.6 nights
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TELESCOPE + INSTRUMENT        1.5m + echelle
TITLE                         Echelle Monitoring of eta Car
ID #                          Continuation of GSTU75 and NOAO09b-0153 (long term program)
PI                            Noel Richardson, Doug Gies (GSU)
CONTACT                       richardson@chara.gsu.edu
MODE (service or user)        service
TIME                          4.0 hours X 1.5 service = 6.0 hours = 0.6 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     N/A
PREFERRED DATES               FEB-MAY
ACCEPTABLE DATES              FEB-early JUN
ACCEPTABLE MOON               any

CADENCE                       1 spectrum/week while eta Car is observable
PREFERRED SETUP               echelle (presumably the new one)
EXPOSURE TIMES                each visit 15 min with overhead

SCIENTIFIC DESCRIPTION        We wish to continue our spectroscopic monitoring of eta Car, which is 
                              changing in unusual ways, including a possible change in mass-loss rate 
                              by a factor of two. The large brightness makes this the only telescope/
                              instrument combination capable of monitoring H-alpha in high resolution, 
                              and only combination for a detailed monitoring program. This is a 
                              continuation of NOAO-09B-0153, an NOAO approved long term monitoring 
                              program that ends in 2010B, and SMARTS program GSTU75 (2008B, 2009A).

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GSU PRIORITY 10 --- SCHEDULED 7.0 nights
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TELESCOPE + INSTRUMENT        0.9m + 2K CCD
TITLE                         CTIOPI
ID #                          GSTU01
PI                            Todd Henry (GSU)
CONTACT                       thenry@chara.gsu.edu, 404-413-6054
MODE (service or user)        user
TIME                          7.0 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     yes
PREFERRED DATES               JUL
ACCEPTABLE DATES              any
ACCEPTABLE MOON               any

CADENCE                       one run of 7 nights
PHOTOMETRIC?                  no
FILTERS                       VRI
                              
SCIENTIFIC DESCRIPTION        Continuing parallax/perturbation search effort.  Requires roughly one
                              week/month to catch appropriate parallax factors for all targets.

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GSU PRIORITY 11 --- SCHEDULED VIA DIRECTOR'S DISCRETIONARY TIME
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TELESCOPE + INSTRUMENT        1.5m + RCSpec
TITLE                         Activity Cycles of Southern Asteroseismic Targets
ID #                          GSTU09
PI                            Travis Metcalfe (UCAR), Todd Henry (GSU)
CONTACT                       travis@ucar.edu, 303-497-8326
MODE (service or user)        service
TIME                          9.5 hours X 1.5 service = 14.3 hours = 1.5 nights
TRAINING RUN                  N/A
OBSERVER/TRAINER              N/A
INTERPOLATED PROGRAMS OK?     N/A
PREFERRED DATES               any
ACCEPTABLE DATES              any
ACCEPTABLE MOON               any

CADENCE                       8 spectra/star/semester folded in with requests from STScI and Yale
PREFERRED SETUP               47/II
EXPOSURE TIMES                average ~3 min/star = 12 min/star with overhead

SCIENTIFIC DESCRIPTION        Synoptic Ca II H & K monitoring of 58 bright solar-type stars (~35 stars 
                              observable on a given night) to document their magnetic activity cycles,
                              and rotation periods when possible.  This request is a continuation of
                              UCAR01 from 2010B.  This program has also been submitted as a Director's
                              Discretionary request, and if that is approved, this particular request
                              from GSU can be dropped.

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