SMARTS 1.5m Observing Schedule
2013A Semester

Schedule Overview:
The RC will be available ONLY February 1-19, after which it will be replaced by SIMON.
The RC queue has 3.5 hours on every odd-numbered night.
The GSU 12B-01 program will be executed on every even-numbered night.

Instructions for Proposers Awarded Service Time

NOW AVAILABLE: The Stony Brook/SMARTS Spectral Standards Database

Go back to:
2003A Service Observing Schedule ||| 2003B Service Observing Schedule

2004A Service Observing Schedule ||| 2004B Service Observing Schedule

2005A Service Observing Schedule ||| 2005B Service Observing Schedule

2006A Service Observing Schedule |||2006B Service Observing Schedule

2007A Service Observing Schedule |||2007B Service Observing Schedule

2008A Service Observing Schedule |||2008B Service Observing Schedule

2009A Service Observing Schedule |||2009B Service Observing Schedule

2010A Service Observing Schedule |||2010B Service Observing Schedule

2011A Service Observing Schedule |||2011B Service Observing Schedule

2012A Service Observing Schedule |||2012B Service Observing Schedule


2013A Service Observing Schedule

Date Grating Setup Plan Targets Log Programs Notes
February 14747/Ib 130201.plan target log 130201.log GSU 12A-04, NOAO 12b-0174, NOAO 12A-388
SUNY 12B-11, VAND 12B-01
Clear
February 22626/Ia GSU12B.plan target log 130202.log GSU 12B-01 Clear
February 32626/Ia 130203.plan target log 130203.log NOAO 11b-44, NOAO 12b-0232
SUNY 12b-11, Yale 12b-09
Clear; thin cloud
February 42626/Ia GSU12B.plan target log 130204.log GSU 12B-01 Clear; Humid
February 51313/I 130205.plan target log Data 130205.log YALE 12a-02 Clear, Humid; program not completed
February 62626/Ia GSU12B.plan target log 130206.log GSU 12B-01 Partly cloudy
February 72626/Ia 130207.plan target log 130207.log NOAO 12b-0232, SUNY 12b-11 This Cloud
February 82626/Ia GSU12B.plan target log 130208.log GSU 12B-01 This Cloud
February 94747/II 130209.plan target log 130209.log HAO 13a-01, SUNY 13A-11 Humid; program not completed
February 102626/Ia GSU12B.plan target log 130210.log GSU 12B-01 Clear
February 112626/Ia 130211.plan target log 130211.log NOAO 12b-0232, SUNY 12b-11 Cleat; technical issues; program not completed
February 122626/Ia GSU12B.plan target log 130212.log GSU 12B-01 Clear
February 134747/IIb, 47/Ib 130213.plan target log 130213.log GSU 12A-04, NOAO 12a-0338
SUNY 12B-31, SUNY 13a-11
Clear
February 142626/Ia GSU12B.plan target log 130214.log GSU 12B-01 Clear
February 151313/I 130215.plan target log Data 130215.log Macri; SUNY 13A-11; Yale 12B-02 Clear; substitute observer
February 162626/Ia GSU12B.plan target log 130216.log GSU 12B-01 Clear
February 172626/Ia 130217.plan target log Data 130217.log GSU 12A-04; NOAO 11B-44, NO 12B-0232
SUNY 13A-11, Yale 12b-09
Clear
February 182626/Ia GSU12B.plan target log 130218.log GSU 12B-01 Clear
February 191313/I 130219.plan target log Data 130219.log Macri; SUNY 13A-11; Yale 12B-02 Clear
February 202626/Ia 130220.plan target log 130220.log NOAO 12B-0232, SUNY 13A-11 Clear

Notes:



Useage Summary

A more-or-less current accounting of the useage for the current semester is maintained here.


Except for authorized TOOs, all requests for changes to the schedule must be approved by the scheduler or the PI.

All requests to schedule TOOs, authorized or not, must be made to the scheduler.


Standard Setups

The following is a list of spectrograph setups we have used. The most common service observing setups are 13/I, 26/I, 47/Ib, 47/II, 47/IIb, and 58/I. Other setups may be requested when the science requires them, but scheduling efficiency is increased if the standard ones are used as much as possible.

Note: Gratings may not be changed during the night. Grating tilts may be changed, at the cost of some observing efficiency.

Standard Setups Regularly used for Monitoring Programs
Setup
Name
SlitFilterColl
Focus
Grating
Blaze
Res (A)
Tilt
Wav. Range
Comp
exp (sec)
YstartYsizeYspec
13/I110.5clear58513
4450
17.2
11.58
3146-9374
He-Ar
120
200 280 TBD
26/I 110.5 clear 565 26
3550
4.3
15.93
3532-5300
He-Ar
30
214 280 TBD
26/Ia 110.5 clear 565 26
3550
4.3
16.14
3660-5440
He-Ar
30
214 280 TBD
35/I 110.5 OG570 630 35
6750
4.3
19.64
5901-7700
Neon
20
TBD 280 TBD
47/Ib 110.5 GG495 595 47
7100
3.1
22.64
5652-6972
Neon
20
200 280 164
47/II 83.0 CuSO4 620 47
3550
1.6
27.39
3878-4552
He-Ar
45
200 280 TBD
56/II 83.0 CuSO4 620 56
4900
2.2
22.90
4017-4938
He-Ar
60
225 280 TBD

Defined, non-Standard Setups
Setup
Name
Slit Filter Coll
Focus
Grating
Blaze
Res (A)
Tilt
Wav. Range
Comp
exp (sec)
Ystart Ysize Yspec
9/I 110.5 clear 610 9
4000
8.6
13.21
3505-6956
He-Ar
30
214 280 TBD
9/Ib 110.5 clear 560 9
4000
8.6
13.35
3750-7185
He-Ar
30
214 280 TBD
9/Ic 110.5 clear 560 9
4000
8.6
13.09
3330-6800
He-Ar
30
214 280 TBD
11/I300 clear TBD 11
8000
16.4
TBD
4000-10000
He-Ar
50
200 280 TBD
13/Ib110.5 BG38 585 13
4450
17.2
11.58
3500-6500
He-Ar
50
200 280 TBD
13/Ic83.0   490 13
4450
17.2
11.78
3500-9700
He-Ar
50
200 280 TBD
13/Ir110.5 GG495 585 13
4450
17.2
11.58
5000-9374
He-Ar
50
200 280 TBD
16/I 110.5 clear 480 16
5550
4.8
16.21
4200-6150
He-Ar
30
220 280 TBD
26/Ib 110.5 clear 565? 26
3550
4.3
16.50
3800-5575
He-Ar
30
214 280 TBD
26/Ic 110.5 clear 565 26
3550
4.3
15.55
3300-5075
He-Ar
30
214 280 TBD
32/I 110 OG570 640 32
4900
8.6
15.13
5994-9608
Neon
10
285 150 TBD
32/Ib 110 WG360 640 32
4900
8.6
13.45
3800-7250
He-Ar
20
285 150 TBD
35/Ib 110.5 OG570 630 35
6750
4.3
19.81
6000-7800
Neon
20
TBD 280 TBD
35/II 90 CuSO4 630 35
6750
4.3
???
3700-4600
HeNeAr
30
TBD 280 TBD
47/I 110.5 GG495 595 47
7100
3.1
23.45
6010-7335
Neon
20
200 280 164
47/Ic 155 OG570 650? 47
7100
3.1
27.58
7815-9150
Neon
10
200 280 164
47/Id 155 OG570 650? 47
7100
3.1
22.42
5550-6870
Neon
10
200 280 164
47/Ie 110.5 GG495 595 47
7100
3.1
23.98
6240-7560
Neon
10
200 280 164
47/If 110.5 GG495 595 47
7100
3.1
24.40
6475-7675
Neon
10
20 0 280 164
47/Ig 110.5 GG495 595 47
7100
3.1
26.70
7500-8700
Neon
10
20 0 280 164
47/Ih 110.5 GG495 595 47
7100
3.1
24.26
6400-7600
Neon
10
20 0 280 164
47/IIb 83.0 BG 39 620 47
3550
1.6
28.27
4070-4744
He-Ar
45
200 280 TBD
47/IIc 83.0 CuSO4 620 47
3550
1.6
27.91
3990-4664
He-Ar
45
200 280 TBD
47/IId 200 BG 39 595 47
3550
1.6
28.28
4066-4740
He-Ar
45
285 150 TBD
47/IIe 200 BG 39 595 47
3550
1.6
29.63
4426-5100
He-Ar
45
285 150 TBD
58/I 83.0 GG 495 595 58
8000
6.5
16.9
~6000-9000
Neon
20
285 150 TBD

Where are my data?

Our observer only takes the data, he does not give it to you. You must download your own data.

scp the data from either

(yymmdd is the civil date at the start of the night)

Get the v17 password from Fred Walter, or Howard Bond.

Note that as of November 2008 CTIO has tightened their computer security, and are discouraging scp downloads. They are encouraging use of VPN (see this memo).

The data are generally kept on-line at CTIO for a week or two after they have been taken. The raw data are archived at Stony Brook and at Yale.

An IDL pipeline for reducing RC spectra

An IDL-based pipeline for reducing 1.5m RC spectra is now available. The manual is available in this pdf file. The full distribution, including calibration data and data to test the software on, is here.

The pipeline should run under Linux, with IDL versions 6.2 and later. You will need the IDL Astronomy User's Library in your path.

Caveat: this has not been extensively tested on other systems, so you may run into missing procedures and undefined environment variables (or hardware links). Please let me know of any problems and I will correct the problems.

An IDL pipeline for reducing echelle spectra

An IDL-based pipeline for reducing 1.5m queue echelle spectra is now available. A brief guide is available in this file. The full distribution, including calibration data, is here.

This will work only for data taken using the full chip readout.

The pipeline should run under the Linux O/S, with IDL versions 6.2 and later. You will need the IDL Astronomy User's Library in your path.

Caveat: this has not been tested on other systems, so you may run into missing procedures and undefined environment variables (or hardware links). Please let me know of any problems and I will correct the problems.

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