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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END
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