ESO telescope proposal template adapted for Research Techniques in Astronomy (RTA) at the University of Nottingham. Updated for 2018/19.
\begin
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%
% ESO LA SILLA PARANAL OBSERVATORY
% --------------------------------
% NORMAL PROGRAMME PHASE 1 TEMPLATE
% ---------------------------------
%
% Adapted for:
% Research Techniques in Astronomy (RTA)
% at the University of Nottingham
% by Steven Bamford, Nov 2017
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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%
% I M P O R T A N T N O T E
% ----------------------------
%
% By submitting this proposal, the Principal Investigator takes full
% responsibility for the content of the proposal, in particular with
% regard to the names of CoI's and the agreement to act in accordance
% with the ESO policy and regulations, should observing time be
% granted.
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% - LaTeX *is* sensitive towards upper and lower case letters.
% - Everything after a `%' character is taken as comments.
% - DO NOT CHANGE ANY OF THE MACRO NAMES (words beginning with `\')
% - DO NOT INSERT ANY TEXT OUTSIDE THE PROVIDED MACROS
\documentclass{esoform}
% The list of LaTeX definitions of commonly used astronomical symbols
% is already included in the style file common2e.sty (see Table 1 in
% the Users' Manual). If you have your own macros or definitions,
% please insert them here, between the \documentclass{esoform}
% and the \begin{document} commands.
%
% PLEASE USE NEITHER YOUR OWN MACROS NOR ANY TEX/LATEX MACROS
% IN THE \Title, \Abstract, \PI, \CoI, and \Target MACROS.
%
% WARNING: IT IS THE RESPONSIBILITY OF THE APPLICANTS TO STAY WITHIN THE
% CURRENT BOX LIMITS AND ELIMINATE POTENTIAL OVERFILL/OVERWRITE PROBLEMS
\begin{document}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% CONTENTS OF THE FIRST PAGE %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
%---- BOX 1 -----------------------------------------------------------
%
% You should use this template for period 103A applications ONLY.
%
% DO NOT EDIT THE MACRO BELOW.
% Type below, within the curly braces {}, the title of your observing
% programme (up to two lines).
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% DO NOT USE ANY TEX/LATEX MACROS IN THE TITLE
\Title{This Is The Proposal Title This Is The Proposal Title}
% Type below the numeric code corresponding to the subcategory of
% your programme.
% Please see the Call for Proposals and the ESOFORM User Manual for more details.
\SubCategoryCode{X0}
%---- BOX 2 -----------------------------------------------------------
%
% Type below a concise abstract of your proposal (up to 9 lines).
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% DO NOT USE ANY TEX/LATEX MACROS IN THE ABSTRACT
\Abstract{This is a concise abstract of the proposal which may have up
to 9 lines.}
%---- BOX 3 -----------------------------------------------------------
%
% Description of the observing run(s) necessary for the completion of
% your programme. The macro takes ten parameters: run ID, period,
% instrument, time requested, month preference, moon requirement,
% seeing requirement, transparency requirement, observing mode and
% run type.
%
% 1. RUN ID
% Valid values: A, B, ..., Z
%
% 2. PERIOD
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 3. INSTRUMENT
% Valid values: ARTEMIS EFOSC2 ESPRESSO-1UT ESPRESSO-4UT FLAMES FORS2 GRAVITY HARPS HAWKI KMOS LABOCA MATISSE MUSE NACO OMEGACAM PIONIER SEPIA SINFONI SOFI SOFOSC SPHERE Special3.6 SpecialAPEX SpecialNTT ULTRACAM UVES VIRCAM XSHOOTER nFLASH
%
% Please see the Call for Proposals and the ESOFORM User Manual for more details.
%
% 4. TIME REQUESTED
% In hours for Service Mode, in nights for Visitor Mode.
% In either case the time can be rounded up to 1 decimal place.
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 5. MONTH PREFERENCE
% Valid values: oct, nov, dec, jan, feb, mar, apr, may, jun, jul, aug, sep, any
%
% 6. MOON REQUIREMENT (dark, grey, none)
% Valid values: d, g, n
%
% 7. SEEING REQUIREMENT (arcsec or none)
% Valid values: 0.4, 0.6, 0.8, 1.0, 1.2, 1.4, n
%
% 8. TRANSPARENCY REQUIREMENT (photometric, clear, thin)
% Valid values: PHO, CLR, THN
%
% 9. OBSERVING MODE (visitor or service)
% Valid values: v, s
%
% 10. RUN TYPE
% Leave blank
\ObservingRun{A}{103}{FORS2}{4h}{nov}{n}{0.8}{PHO}{s}{}
\ObservingRun{A/alt}{103}{FORS2}{3n=2x1+2H2}{nov}{n}{0.8}{PHO}{v}{}
\ObservingRun{B}{103}{XSHOOTER}{2n=2x1}{dec}{n}{0.6}{CLR}{v}{}
\ObservingRun{C}{103}{NACO}{0.4n}{nov}{n}{0.8}{THN}{v}{}
\ObservingRun{D}{103}{XSHOOTER}{1h}{nov}{n}{1.4}{THN}{s}{}
\ObservingRun{E}{104}{XSHOOTER}{1h}{sep}{n}{n}{THN}{s}{}
%---- BOX 4 -----------------------------------------------------------
%
% Not Applicable to RTA
%---- BOX 5 -----------------------------------------------------------
%
% Take advantage of this box to provide any special remark (up to three
% lines).
% This macro is optional and can be commented out.
% It is also NOT checked at the pdfLaTeX compilation.
\SpecialRemarks{This macro is optional and can be commented out. }
%---- BOX 6 -----------------------------------------------------------
% Enter your group ID here
\Group{Group ID}
% Do not include any names in the proposal to allow for anonymous review
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% THE TWO PAGES OF THE SCIENTIFIC DESCRIPTION AND FIGURES %%%%%%%%%%
%%%%%%%%%%%%%%%%%&&&%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
%---- BOX 7 -----------------------------------------------------------
%
% THIS DESCRIPTION IS RESTRICTED TO TWO PAGES
%
% THE RELATIVE LENGTHS OF EACH OF THE SECTIONS ARE VARIABLE,
% BUT THEIR SUM (INCLUDING FIGURES & REFS.) IS RESTRICTED TO TWO PAGES
%
% BE SURE TO CHECK THAT THE END OF YOUR CASE HAS NOT BEEN TRUNCATED!
%
% All macros in this box are NOT checked at the pdfLaTeX compilation.
%
% Blank lines will start a new paragraph, but not add any vertical whitespace.
% Note that \\ will not work as expected.
%
% If you wish to include some vertical whitespace (to relieve the wall of text),
% then use \newline, \smallskip, \medskip and \bigskip.
%
% To emphasise text, you may use \textbf, \emph, etc.
%
% Simple bullet points can be achieved with $\bullet$.
%----------------------------------------------------------------
\ScientificRationale{Scientific rationale: scientific background of
the project, pertinent references; previous work plus justification
for present proposal.\medskip
Lorem ipsum dolor sit amet, consectetur adipiscing elit. Etiam faucibus iaculis
aliquam. Aliquam libero est, lacinia et neque ac, dignissim viverra
arcu. Suspendisse semper congue dolor, eget convallis ligula feugiat et. Nulla
facilisi. Duis condimentum venenatis erat quis rhoncus. Nam risus dolor,
tincidunt nec faucibus nec, commodo condimentum quam. Cras aliquet finibus
pharetra. Donec ultrices neque quis justo fermentum ultricies. Fusce eget nunc
non mauris semper maximus. Donec ultricies lectus nec lectus euismod
rutrum. Curabitur scelerisque, libero ac ultricies iaculis, sapien ipsum
tincidunt velit, at lobortis nisi massa eu risus. Aenean mi libero, egestas nec
dui sit amet, consequat egestas lacus. Vivamus aliquam mi massa. Donec non ante
augue. Nunc vitae congue est, et interdum ipsum:
$\bullet$ This,\newline
$\bullet$ That,\newline
$\bullet$ The other.
Nunc quis est felis. Donec feugiat enim ante, vel rutrum ligula ornare
vitae. Fusce sed accumsan nisi. Ut sit amet vulputate ligula. Etiam mollis quam
vel justo posuere venenatis. Cras quis leo quis nibh consectetur
accumsan. Suspendisse ac mauris non nisi sodales vulputate. In hac habitasse
platea dictumst. Aenean iaculis, metus quis commodo aliquet, eros metus
condimentum nisi, a mollis est purus ut nisi.
}
%----------------------------------------------------------------
\ImmediateObjective{Immediate objective of the proposal: state what is
actually going to be observed and what shall be extracted from the
observations, so that the feasibility becomes clear.\medskip
Lorem ipsum dolor sit amet, consectetur adipiscing elit. Ut condimentum,
lectus quis placerat bibendum, magna nisl pharetra enim, in tincidunt lorem
nunc at augue. Donec sed vehicula erat. Cras et sem ligula. Etiam condimentum
sem non leo placerat, imperdiet dictum nisl tincidunt. Sed id nisl
augue. Duis consequat nibh justo, faucibus tristique urna mattis ac. Maecenas
semper posuere tristique. Maecenas ac libero eu turpis molestie congue.
Vivamus id turpis id ligula faucibus varius at eget turpis. Praesent metus
enim, rutrum eu sapien ut, convallis congue risus. Fusce nec elementum magna,
at ultricies risus. Curabitur lectus sapien, pharetra eget nibh in, bibendum
tempor nibh. Cras sit amet nulla sapien. Mauris aliquam purus pharetra
faucibus posuere. Nulla placerat risus quam, vitae elementum orci imperdiet
in. Mauris a velit eros. Duis tempus dolor nec est rhoncus, eget bibendum
justo tincidunt. Suspendisse ultrices molestie dolor, quis lobortis
enim. Vestibulum id eros a metus dictum rhoncus. Donec laoreet ex quis dui
vehicula vestibulum. Nullam congue, neque at suscipit vehicula, sapien lectus
sagittis eros, at molestie ipsum est eget lectus. Interdum et malesuada fames
ac ante ipsum primis in faucibus. Ut lacinia viverra lacus, non porta augue
feugiat vel. \textbf{Nam vulputate felis eget lacinia auctor.} }
%
%---- THE SECOND PAGE OF THE SCIENCE CASE CAN INCLUDE FIGURES ----------
%
% Up to ONE page of figures can be added to your proposal.
% The text and figures of the scientific description must not
% exceed TWO pages in total.
% If you use color figures, do make sure that they are still readable
% if printed in black and white. Figures must be in PDF or JPEG format.
% Each figure has a size limit of 1MB.
% MakePicture and MakeCaption are optional macros and can be commented out.
\MakePicture{galaxy.pdf}{angle=90,width=10cm}
\MakeCaption{Fig.~1: A caption for your figure can be inserted here.}
\MakeCaption{References can also be included using MakeCaption.
For example:\medskip
\textbf{References:}\newline
Blah B., 2017, MNRAS, 999, 666, 111\newline
Meself M., et al., 2015, ApJ, 000, 111, 222\newline
Meself M., et al., 2015, AJ, 1234, 123, 321
}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% THE PAGE OF TECHNICAL JUSTIFICATIONS %%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
%---- BOX 8 -----------------------------------------------------------
%
% Provide below a careful justification of the requested lunar phase
% and of the requested number of nights or hours. Provide all
% information necessary to reproduce your ETC calculations. When
% applicable, specify the magnitude system employed (e.g., Vega, AB).
% All macros in this box are NOT checked at the pdfLaTeX compilation.
\WhyLunarPhase{Provide here a careful justification of the requested lunar
phase.
Lorem ipsum dolor sit amet, consectetur adipiscing elit. Etiam faucibus iaculis
aliquam. Aliquam libero est, lacinia et neque ac, dignissim viverra
arcu. Suspendisse semper congue dolor, eget convallis ligula feugiat et. Nulla
facilisi.}
\WhyNights{Provide a careful justification of the requested number of nights or
hours for each observing run here. ESO Exposure Time Calculators exist for
all Paranal and La Silla instruments and are available at the following web
address: http://www.eso.org/observing/etc.
Lorem ipsum dolor sit amet, consectetur adipiscing elit. Etiam faucibus iaculis
aliquam. Aliquam libero est, lacinia et neque ac, dignissim viverra
arcu. Suspendisse semper congue dolor, eget convallis ligula feugiat et. Nulla
facilisi. Duis condimentum venenatis erat quis rhoncus. Nam risus dolor,
tincidunt nec faucibus nec, commodo condimentum quam. Cras aliquet finibus
pharetra. Donec ultrices neque quis justo fermentum ultricies. Fusce eget nunc
non mauris semper maximus. Donec ultricies lectus nec lectus euismod
rutrum. Curabitur scelerisque, libero ac ultricies iaculis, sapien ipsum
tincidunt velit, at lobortis nisi massa eu risus. Aenean mi libero, egestas nec
dui sit amet, consequat egestas lacus. Vivamus aliquam mi massa. Donec non ante
augue.}
\TelescopeJustification{Justification for the use of the selected telescope
(i.e., VLT) with respect to other available alternatives.}
\ModeJustification{Explain if a particular observing mode (visitor or service)
is specifically needed for this programme. If either can, in principle, be
used then please enter N/A. }
% Please specify the type of calibrations needed.
% In case of special calibration the second parameter is used to enter specific details.
% Valid values: standard, special
\Calibrations{standard}{}
%\Calibrations{special}{Adopt a special calibration}
%
%---- BOX 9a -- ESO Archive ------------------------------------------
%
% Are the data requested in this proposal in the ESO Archive
% (http://archive.eso.org)? If yes, explain the need for new data.
% This macro is NOT checked at the pdfLaTeX compilation.
\RequestedDataRemark{No data in ESO archive for any targets listed.}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% THE PAGE OF THE TARGET/FIELD LIST %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
%---- BOX 11 ----------------------------------------------------------
%
% Complete list of targets/fields requested. The macro takes nine
% parameters: run ID, target field/name, RA, Dec, time on target, magnitude,
% diameter, additional information, reference star.
%
% 1. RUN ID
% Valid values: run IDs specified in BOX 3
%
% 2. TARGET FIELD/NAME
%
% 3. RA (J2000)
% Format: hh mm ss.f, or hh mm.f, or hh.f
% Use 00 00 00 for unknown coordinates
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 4. Dec (J2000)
% Format: dd mm ss, or dd mm.f, or dd.f
% Use 00 00 00 for unknown coordinates
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 5. TIME ON TARGET
% Format: hours (overheads and calibration included)
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 6. MAGNITUDE
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 7. ANGULAR DIAMETER
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 8. ADDITIONAL INFORMATION
% Any relevant additional information may be inserted here.
% For APEX and CRIRES runs, the requested PWV upper limit MUST
% be specified for each target using this field.
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 9. REFERENCE STAR ID
% See Users' Manual.
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% Long lists of targets will continue on the last page of the
% proposal.
%
% DO NOT USE ANY TEX/LATEX MACROS FOR THE TARGETS
\Target{ABC}{NGC 104}{00 24 06}{-72 04 58}{3.0}{5}{30 min}{47 Tuc}{}
\Target{A}{NGC 253}{00 47 33.1}{-25 17 17.8}{10.0}{8}{}{Seyfert gal.}{}
\Target{BC}{NGC 1851}{05 14 06.3}{-40 02 50}{8.0}{8.8}{}{glob. cluster}{}
\Target{B}{NGC 1316}{03 22 41.5}{-37 12 33}{15.0}{9.7}{10 min}{Fornax A}{}
\Target{B}{NGC 1365}{03 33 36}{-36 08 27}{15.0}{10}{}{Seyfert gal.}{}
\Target{C}{NGC 2997}{09 45 38}{-31 11 25}{10.0}{}{}{Sc galaxy}{S133231219553}
\Target{D}{Alpha Ori}{06 45 08.9}{-16 42 58}{1}{-1.4}{6 mas}{Sirius}{}
\Target{E}{Alpha Ori}{06 45 08.9}{-16 42 58}{1}{-1.4}{6 mas}{Sirius}{}
% *****************
% ** PWV limits **
% For CRIRES and all APEX instruments users must specify the PWV upper
% limits for each target. For example:
%\Target{}{Alpha CMa}{06 45 08.9}{-16 42 58}{1}{-1.4}{6 mas}{PWV=1.0mm, Sirius}{}
%\Target{}{HD 104237}{12 00 05.6}{-78 11 33}{1}{}{}{PWV<0.7mm;LST=9h00-15h00}{}
%
% *****************
% Use TargetNotes to include any comments that apply to several or all
% of your targets.
% This macro is NOT checked at the pdfLaTeX compilation.
\TargetNotes{A note about the targets and/or strategy of selecting the targets during the run.}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% TWO PAGES OF SCHEDULING REQUIREMENTS %%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
%---- BOX 12 ----------------------------------------------------------
%
% Uncomment the following line if the proposal involves time-critical
% observations, or observations to be performed at specific time
% intervals. Please leave these brackets blank. Details of time
% constraints can be entered in Special Remarks and using the
% other flags in Box 13.
%
%
\HasTimingConstraints{}
%
% The timing constraint macros listed below
% are optional and can be commented out:
% \HasTimingConstraints, \RunSplitting, \Link and \TimeCritical
% They are also NOT checked at the pdfLaTeX compilation.
% 1. RUN SPLITTING, FOR A GIVEN ESO TELESCOPE (Visitor Mode only)
%
% 1st argument: run ID
% Valid values: run IDs specified in BOX 3
%
% 2nd argument: run splitting requested for sub-runs
% This parameter is NOT checked at the pdfLaTeX compilation.
\RunSplitting{B}{1,10s,1}
% 2. LINK FOR COORDINATED OBSERVATIONS BETWEEN DIFFERENT RUNS.
\Link{B}{after}{A}{10}
\Link{C}{after}{B}{}
\Link{C}{simultaneous}{D}{}
% 3. UNSUITABLE PERIOD(S) OF TIME
%
% 1st argument: run ID
% Valid values: run IDs specified in BOX 3
%
% 2nd argument: Chilean start date for the unsuitable time
% Format: dd-mmm-yyyy
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 3rd argument: Chilean end date for the unsuitable time
% Format: dd-mmm-yyyy
% This parameter is NOT checked at the pdfLaTeX compilation.
\UnsuitableTimes{A}{15-jul-19}{18-jul-19}{Insert explanation of unsuitable time here.}
\UnsuitableTimes{B}{15-jul-19}{18-jul-19}{Insert explanation of unsuitable time here.}
\UnsuitableTimes{C}{20-jul-19}{23-jul-19}{Insert explanation of unsuitable time here.}
%
%---- BOX 12 contd.. -- Scheduling Requirements
%
% SPECIFIC DATE(S) FOR TIME-CRITICAL OBSERVATIONS
% Please note: The dates must correspond to the LOCAL CHILEAN observing dates.
%
% The 2nd and 3rd parameters are NOT checked at the pdfLaTeX compilation.
% 1st argument: run ID
% Valid values: run IDs specified in BOX 3
%
% 2nd argument: Chilean start date for the critical period.
% Format: dd-mmmm-yyyy
%
% 3rd argument: Chilean end date for the critical period.
% Format: dd-mmmm-yyyy
\TimeCritical{A}{12-may-19}{14-may-19}{Insert reason for time-critical observations.}
\TimeCritical{D}{1-may-19}{2-may-19}{Insert reason for time-critical observations.}
\TimeCritical{D}{17-may-19}{18-may-19}{Insert reason for time-critical observations.}
\TimeCritical{D}{23-may-19}{24-may-19}{Insert reason for time-critical observations.}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
%---- BOX 13 ----------------------------------------------------------
%
% INSTRUMENT CONFIGURATIONS:
%
% Uncomment only the lines related to instrument configuration(s)
% needed for the acquisition of your planned observations.
%
% 1st argument: run ID
% Valid values: run IDs specified in BOX 3
%
% 2nd argument: instrument
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 3rd argument: mode
% This parameter is NOT checked at the pdfLaTeX compilation.
% Please note that RRM mode is only available for some specific
% instrument configurations.
%
% 4th argument: additional information
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% All parameters are mandatory and cannot be empty. Do NOT specify
% Instrument Configurations for alternative runs.
% Examples (to be commented or deleted)
\INSconfig{A}{FORS2}{Detector}{MIT}
\INSconfig{A}{FORS2}{IMG}{ESO filters: provide list HERE}
\INSconfig{B}{XSHOOTER}{300-2500nm}{IFU}
\INSconfig{B}{XSHOOTER}{IFU}{100k-2x2, 100k-2x2,NDR}
\INSconfig{C}{NACO}{IMG 54 mas/px VIS-WFS}{provide list of filters HERE}
\INSconfig{D}{XSHOOTER}{300-2500nm}{IFU}
\INSconfig{D}{XSHOOTER}{IFU}{100k-2x2, 100k-2x2,NDR}
\INSconfig{E}{XSHOOTER}{300-2500nm}{IFU}
\INSconfig{E}{XSHOOTER}{IFU}{100k-2x2, 100k-2x2,NDR}
%
% Real list of instrument configurations
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Paranal
%
%-----------------------------------------------------------------------
%---- NAOS/CONICA at the VLT-UT1 (ANTU) -------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{NACO}{PRE-IMG}{provide list of filters HERE}
%
% Specify the NGS name, distance from target and magnitude
%(Vmag preferred, otherwise Rmag) in the target list,
% and uncomment the following line
%\INSconfig{}{NACO}{NGS}{-}
%
%\INSconfig{}{NACO}{Special Cal}{Select if you have special calibrations}
%\INSconfig{}{NACO}{Pupil Track}{Select if you need pupil tracking mode}
%\INSconfig{}{NACO}{Cube}{Select if you need cube mode}
%
%\INSconfig{}{NACO}{SAM IR-WFS}{Provide list of masks and filters HERE}
%\INSconfig{}{NACO}{SAMPol IR-WFS}{Provide list of masks and filters HERE}
%
%\INSconfig{}{NACO}{IMG 54 mas/px IR-WFS}{provide list of filters HERE}
%\INSconfig{}{NACO}{IMG 27 mas/px IR-WFS}{provide list of filters HERE}
%\INSconfig{}{NACO}{IMG 13 mas/px IR-WFS}{provide list of filters HERE}
%
%\INSconfig{}{NACO}{CORONA AGPM IR-WFS}{provide list of filters (L',NB-3.74,NB-4.05) HERE}
%
%\INSconfig{}{NACO}{POL 54 mas/px IR-WFS}{provide list of filters HERE}
%\INSconfig{}{NACO}{POL 27 mas/px IR-WFS}{provide list of filters HERE}
%\INSconfig{}{NACO}{POL 13 mas/px IR-WFS}{provide list of filters HERE}
%
%-----------------------------------------------------------------------
%---- FORS2 at the VLT-UT1 (ANTU) --------------------------------------
%-----------------------------------------------------------------------
%
%If you require the E2V (Blue) detector uncomment the following line
%\INSconfig{}{FORS2}{Detector}{E2V}
%
%If you require the MIT (RED) detector uncomment the following line
%\INSconfig{}{FORS2}{Detector}{MIT}
%
% If you require the High-Resolution collimator uncomment the following line
%\INSconfig{}{FORS2}{collimator}{HR}
%
% Uncomment the line(s) corresponding to the imaging mode(s) you require and
% provide the list of filters needed for your observations:
%
%\INSconfig{}{FORS2}{PRE-IMG}{ESO filters: provide list HERE}
%\INSconfig{}{FORS2}{IMG}{ESO filters: provide list HERE}
%\INSconfig{}{FORS2}{IMG}{User's own filters (to be described in text)}
%\INSconfig{}{FORS2}{IPOL}{ESO filters: provide list HERE}
%\INSconfig{}{FORS2}{IPOL}{User's own filters (to be described in text)}
%
% Uncomment the line(s) corresponding to the spectroscopic mode(s) you require and
% provide the list of grism+filter combination needed for your observations:
%
%\INSconfig{}{FORS2}{LSS}{Provide list of grism+filter combinations HERE}
%\INSconfig{}{FORS2}{MOS}{Provide list of grism+filter combinations HERE}
%\INSconfig{}{FORS2}{PMOS}{Provide list of grism+filter combinations HERE}
%\INSconfig{}{FORS2}{MXU}{Provide list of grism+filter combinations HERE}
%
% Uncomment the following line for Rapid Response Mode observations
%
%\INSconfig{}{FORS2}{RRM}{yes}
%
% Uncomment the following line for use of the Virtual Image Slicer
%\INSconfig{}{FORS2}{Virtual Image Slicer}{VM only}
%
%-----------------------------------------------------------------------
%---- KMOS at the VLT-UT1 (ANTU) ---------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{KMOS}{IFU}{provide list of settings (IZ, YJ, H, K, HK) here}
%
%-----------------------------------------------------------------------
%---- FLAMES at the VLT-UT2 (KUEYEN) -----------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{FLAMES}{UVES}{Specify the UVES setup below}
%\INSconfig{}{FLAMES}{GIRAFFE-MEDUSA}{Specify the GIRAFFE setup below}
%\INSconfig{}{FLAMES}{GIRAFFE-IFU}{Specify the GIRAFFE setup below}
%\INSconfig{}{FLAMES}{GIRAFFE-ARGUS}{Specify the GIRAFFE setup below}
%\INSconfig{}{FLAMES}{Combined: UVES + GIRAFFE-MEDUSA}{Specify the UVES and GIRAFFE setups below}
%\INSconfig{}{FLAMES}{Combined: UVES + GIRAFFE-IFU}{Specify the UVES and GIRAFFE setups below}
%\INSconfig{}{FLAMES}{Combined: UVES + GIRAFFE-ARGUS}{Specify the UVES and GIRAFFE setups below}
%
% If you have selected UVES, either standalone or in combined mode,
% please specify the UVES standard setup(s) to be used
%\INSconfig{}{FLAMES}{UVES}{standard setup Red 520}
%\INSconfig{}{FLAMES}{UVES}{standard setup Red 580}
%\INSconfig{}{FLAMES}{UVES}{standard setup Red 580 + simultaneous calibration}
%\INSconfig{}{FLAMES}{UVES}{standard setup Red 860}
%
%\INSconfig{}{FLAMES}{GIRAFFE}{fast readout mode 625kHz VM only}
%\INSconfig{}{FLAMES}{GIRAFFE}{slow readout mode 50kHz VM only}
%
% If you have selected GIRAFFE, either standalone or in combined mode
% please specify the GIRAFFE standard setups(s) to be used
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR01 379.0}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR02 395.8}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR03 412.4}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR04 429.7}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR05 447.1 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR05 447.1 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR06 465.6}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR07 484.5 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR07 484.5 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR08 504.8}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR09 525.8 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR09 525.8 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR10 548.8}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR11 572.8}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR12 599.3}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR13 627.3}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR14 651.5 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR14 651.5 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR15 665.0}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR15 679.7}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR16 710.5}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR17 737.0 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR17 737.0 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR18 769.1}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR19 805.3 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR19 805.3 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR20 836.6 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR20 836.6 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR21 875.7}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR22 920.5 A}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup HR22 920.5 B}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR01 385.7}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR02 427.2}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR03 479.7}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR04 543.1}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR05 614.2}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR06 682.2}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR07 773.4}
%\INSconfig{}{FLAMES}{GIRAFFE}{standard setup LR08 881.7}
%
%\INSconfig{}{FLAMES}{GIRAFFE}{fast readout mode 625kHz VM only}
%
%-----------------------------------------------------------------------
%---- X-SHOOTER at the VLT-UT2 (KUEYEN)
%-----------------------------------------------------------------------
%
%\INSconfig{}{XSHOOTER}{300-2500nm}{SLT}
%\INSconfig{}{XSHOOTER}{300-2500nm}{IFU}
%
% Slits (SLT only):
%
%UVB arm, available slits in arcsec: 0.5, 0.8, 1.0, 1.3, 1.6, 5.0
%VIS arm, available slits in arcsec: 0.4, 0.7, 0.9, 1.2, 1.5, 5.0
%NIR arm, available slits in arcsec: 0.4, 0.6, 0.6JH, 0.9, 0.9JH, 1.2, 5.0
% The 0.6JH and 0.9JH include a stray light K-band blocking filter
% that allow sky limited studies in J and H bands.
%
%The slits for IFU are fixed and do not need to be mentioned here.
%
% Replace SLIT-UVB, SLIT-VIS, SLIT-NIR with the choice of the slits:
%\INSconfig{}{XSHOOTER}{SLT}{SLIT-UVB,SLIT-VIS,SLIT-NIR}
%
% Detector readout mode:
%
% UVB and VIS arms: available readout modes and binning:
% 100k-1x1, 100k-1x2, 100k-2x2, 400k-1x1, 400k-1x2, 400k-2x2
% The NIR readout mode is fixed to NDR.
%
%\INSconfig{}{XSHOOTER}{IFU}{readout UVB,readout VIS,readout NIR}
%\INSconfig{}{XSHOOTER}{SLT}{readout UVB,readout VIS,readout NIR}
%
% Imaging mode
% replace 'list of filters' by the actual filters you wish to use among:
% U, B, V, R, I, Uprime, Gprime, Rprime, Iprime, Zprime
% Please note that the imaging mode can only be used in combination with slit or IFU observations
%\INSconfig{}{XSHOOTER}{IMG}{list of filters}
%
%\INSconfig{}{XSHOOTER}{RRM}{yes}
%
% Uncomment the following line for use of the Virtual Image Slicer
%\INSconfig{}{XSHOOTER}{Virtual Image Slicer}{VM only}
%
%-----------------------------------------------------------------------
%---- UVES at the VLT-UT2 (KUEYEN) -------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{UVES}{BLUE}{Standard setting: 346}
%\INSconfig{}{UVES}{BLUE}{Standard setting: 437}
%\INSconfig{}{UVES}{BLUE}{Non-std setting: provide central wavelength HERE}
%
%\INSconfig{}{UVES}{RED}{Standard setting: 520}
%\INSconfig{}{UVES}{RED}{Standard setting: 580}
%\INSconfig{}{UVES}{RED}{Standard setting: 600}
%\INSconfig{}{UVES}{RED}{Iodine cell standard setting: 600}
%\INSconfig{}{UVES}{RED}{Standard setting: 860}
%\INSconfig{}{UVES}{RED}{Non-std setting: provide central wavelength HERE}
%
%\INSconfig{}{UVES}{DIC-1}{Standard setting: 346+580}
%\INSconfig{}{UVES}{DIC-1}{Standard setting: 390+564}
%\INSconfig{}{UVES}{DIC-1}{Standard setting: 346+564}
%\INSconfig{}{UVES}{DIC-1}{Standard setting: 390+580}
%\INSconfig{}{UVES}{DIC-1}{Non-std setting: provide central wavelength HERE}
%
%\INSconfig{}{UVES}{DIC-2}{Standard setting: 437+860}
%\INSconfig{}{UVES}{DIC-2}{Standard setting: 346+860}
%\INSconfig{}{UVES}{DIC-2}{Standard setting: 390+860}
%
%\INSconfig{}{UVES}{DIC-2}{Standard setting: 437+760}
%\INSconfig{}{UVES}{DIC-2}{Standard setting: 346+760}
%\INSconfig{}{UVES}{DIC-2}{Standard setting: 390+760}
%\INSconfig{}{UVES}{DIC-2}{Non-std setting: provide central wavelength HERE}
%
%\INSconfig{}{UVES}{Field Derotation}{yes}
%\INSconfig{}{UVES}{Image slicer-1}{yes}
%\INSconfig{}{UVES}{Image slicer-2}{yes}
%\INSconfig{}{UVES}{Image slicer-3}{yes}
%\INSconfig{}{UVES}{Iodine cell}{yes}
%\INSconfig{}{UVES}{Longslit Filters}{Provide list of filters HERE}
%
%\INSconfig{}{UVES}{RRM}{yes}
%
% Uncomment the following line for use of the Virtual Image Slicer
%\INSconfig{}{UVES}{Virtual Image Slicer}{VM only}
%
%-----------------------------------------------------------------------
%---- SPHERE at the VLT-UT3 (MELIPAL) -----------------------------------
%-----------------------------------------------------------------------
%
% Pupil or field tracking?
% Mode choices: IRDIS-CI, IRDIS-DBI,
% IRDIFS, IRDIFS-EXT,
% ZIMPOL-I
% (Not relevant for IRDIS-DPI, IRDIS-LSS, ZIMPOL-P1 or ZIMPOL-P2)
%--------------------
% IRDIFS:
% Coronagraph combination choices:
% IRDIFS: None, N-ALC-YJH-S, N-ALC-YJH-L, N-CLC-SW-L, N-SAM-7H
% IRDIFS-EXT: None, N-ALC-YJH-S, N-ALC-YJH-L, N-ALC-Ks, N-SAM-7H
% Filter choices for IRDIS in IRDIFS mode
% IRDIFS: DB-H23, DB-ND23, DB-H34, BB-H
% IRDIFS-EXT: DB-K12, BB-Ks
%---------------------
% IRDIS imaging (alone):
% Coronagraph combination choices for IRDIS imaging modes (see UM for details)
% IRDIS-CI, IRDIS-DPI:
% None, N-ALC-Y, N-ALC-YJ-S, N-ALC-YJ-L, N-ALC-YJH-S,
% N-ALC-YJH-L, N-ALC-Ks, N-SAM-7H
% IRDIS-DBI: None, N-ALC-Y, N-ALC-YJ-S, N-ALC-YJ-L, N-ALC-YJH-S,
% N-ALC-YJH-L, N-ALC-Ks, N-SAM-7H
% Filter choices:
% IRDIS-CI, IRDIS-DPI:
% BB-Y, BB-J, BB-H, BB-Ks, NB-Hel, NB-CntJ, NB-CntH,
% NB-CntK1, NB-BrG, NB-CntK2, NB-PaB, NB-FeII, NB-H2, NB-CO
% IRDIS-DBI: DB-Y23, DB-J23, DB-H23, DB-NDH23, DB-H34, DB-K12
%---------------------
% IRDIS spectroscopy:
% Coronagraphic slit/grism combinations for IRDIS-LSS:
% IRDIS-LSS: N-S-LR-WL, N-S-MR-WL,
% N_S_APO_LR_WL, N_S_APO_MR_WL, N_S_APO_MR_NL
%---------------------
% ZIMPOL imaging:
% Coronagraph choices:
% ZIMPOL-I: None, V-CLC-M-WF, V-CLC-M-NF, V-CLC-L-WF, V-CLC-XL-WF, V-SAM-7H
% Filter choices:
% ZIMPOL-I: RI, R-PRIM, I-PRIM, V, V-S, V-L, N-R, 730-NB, N-I, I-L,
% KI, TiO-717, CH4-727, Cnt748, Cnt820, HeI, OI-630,
% CntHa, B-Ha, N-Ha, Ha-NB
%--------------------
% ZIMPOL polarimetry:
% Coronagraph choices:
% ZIMPOL-P1: None, V-CLC-S-WF, V-CLC-M-WF, V-CLC-L-WF, V-CLC-XL-WF, V-CLC-MT-WF
% ZIMPOL-P2: None, V-CLC-S-WF, V-CLC-M-WF, V-CLC-L-WF, V-CLC-XL-WF, V-CLC-MT-WF
% Filter choices:
% ZIMPOL-P1: RI, R-PRIM, I-PRIM, V, N-R, N-I, KI, TiO-717,
% CH4-727, Cnt748, Cnt820, CntHa, N-Ha, B-Ha
% ZIMPOL-P2: RI, R-PRIM, I-PRIM, V, N-R, N-I, KI, TiO-717,
% CH4-727, Cnt748, Cnt820, CntHa, N-Ha, B-Ha
% Readout mode choice for ZIMPOL
% ZIMPOL-P1: FastPol, SlowPol
% ZIMPOL-P2: FastPol, SlowPol
%-------------------
%
% One entry per mode. Repeat the entry for each mode.
%
%\INSconfig{}{SPHERE}{Pupil}{mode}
%\INSconfig{}{SPHERE}{Field}{mode}
%
% One entry per combination. Repeat the entry for each combination.
%
%\INSconfig{}{SPHERE}{IRDIFS}{Coronagraph/filter or SAM mask combination for IRDIFS}
%\INSconfig{}{SPHERE}{IRDIFS-EXT}{Coronagraph/filter or SAM mask combination for IRDIFS-EXT}
%
%\INSconfig{}{SPHERE}{IRDIS-CI}{Coronagraph/filter or SAM mask combination for IRDIS-CI}
%\INSconfig{}{SPHERE}{IRDIS-DBI}{Coronagraph/filter or SAM mask combination for IRDIS-DBI}
%\INSconfig{}{SPHERE}{IRDIS-DPI}{Coronagraph/filter or SAM mask combination for IRDIS-DPI}
%\INSconfig{}{SPHERE}{IRDIS-LSS}{Coronagraphic slit/grism combination for IRDIS-LSS}
%
%\INSconfig{}{SPHERE}{ZIMPOL-I}{Coronagraph/filter or SAM mask combination for ZIMPOL-I}
%
%\INSconfig{}{SPHERE}{ZIMPOL-P1}{Coronagraph/filter/readout mode for ZIMPOL-P1}
%\INSconfig{}{SPHERE}{ZIMPOL-P2}{Coronagraph/filter/readout mode for ZIMPOL-P2}
%
%------------------
% Uncomment the following line if the run requires the Rapid Response Mode
% 'Mode' should be one of IRDIFS, IRDIFS-EXT, IRDIS-CI, IRDIS-DBI,
% IRDIS-DPI, IRDIS-LSS, ZIMPOL-I, ZIMPOL-P1, ZIMPOLP2,
%
%\INSconfig{}{SPHERE}{RRM}{Mode}
%
%-----------------------------------------------------------------------
%---- SINFONI at the VLT-UT3 (MELIPAL) ---------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{SINFONI}{PRE-IMG}{provide list of setting(s) (J,H,K,H+K)}
%
%\INSconfig{}{SINFONI}{IFS 250mas/pix no-AO}{provide list of setting(s) (J,H,K,H+K) HERE}
%\INSconfig{}{SINFONI}{IFS 100mas/pix no-AO}{provide list of setting(s) (J,H,K,H+K) HERE}
%
% If you plan to use a NGS, please specify the NGS name and magnitude (Rmag preferred,
% otherwise Vmag) in target list.
%\INSconfig{}{SINFONI}{IFS 250mas/pix NGS}{provide list of setting(s) (J,H,K,H+K) HERE}
%\INSconfig{}{SINFONI}{IFS 100mas/pix NGS}{provide list of setting(s) (J,H,K,H+K) HERE}
%\INSconfig{}{SINFONI}{IFS 25mas/pix NGS}{provide list of setting(s) (J,H,K,H+K) HERE}
%
% Select if you have special calibrations
%\INSconfig{}{SINFONI}{Special Cal}{-}
%
% Select if you need pupil tracking mode
%\INSconfig{}{SINFONI}{Pupil Track}{-}
%
% Select for RRM
%\INSconfig{}{SINFONI}{RRM}{yes}
%
%-----------------------------------------------------------------------
%---- HAWKI at the VLT-UT4 (YEPUN) -----------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{HAWKI}{PRE-IMG}{provide list of filters (Y,J,H,Ks,CH4,BrG,H2,NB1190,NB1060,NB2090) HERE}
%
%\INSconfig{}{HAWKI}{IMG}{provide list of filters (Y,J,H,Ks,CH4,BrG,H2,NB1190,NB1060,NB2090) HERE}
%\INSconfig{}{HAWKI}{FASTJITT}{Provide list of filters (Y,J,H,Ks,CH4,BrG,H2,NB1190,NB1060,NB2090) HERE}
%
%\INSconfig{}{HAWKI}{AO-IMG}{provide list of filters (Y,J,H,Ks,CH4,BrG,H2,NB1190,NB1060,NB2090) HERE}
%\INSconfig{}{HAWKI}{AO-FASTJITT}{Provide list of filters (Y,J,H,Ks,CH4,BrG,H2,NB1190,NB1060,NB2090) HERE}
%
% Uncomment for RRM (NoAO only)
%\INSconfig{}{HAWKI}{RRM}{yes}
%
%-----------------------------------------------------------------------
%---- MUSE at the VLT-UT4 (YEPUN) -----------------------------------
%-----------------------------------------------------------------------
%
% If you plan to use MUSE in NOAO mode, please uncomment one of these lines.
%\INSconfig{}{MUSE}{WFM-NOAO-N}{-}
%\INSconfig{}{MUSE}{WFM-NOAO-E}{-}
%
% If you plan to use the LGS, please specify the Tip-Tilt star name and magnitude (Rmag preferred,
% otherwise Vmag) in the target list.
%\INSconfig{}{MUSE}{WFM-AO-N LGS}{-}
%\INSconfig{}{MUSE}{WFM-AO-E LGS}{-}
%
% If you plan to use the LGS in WFM without a Tip-Tilt star (seeing enhancer mode)
%\INSconfig{}{MUSE}{WFM-AO-N LGS-noTTS}{-}
%\INSconfig{}{MUSE}{WFM-AO-E LGS-noTTS}{-}
%
% If you plan to use the LGS in NFM, please specify the Tip-Tilt star
% name and infrared H-band magnitude in the target list
%\INSconfig{}{MUSE}{NFM-AO-N LGS}{-}
%
% Uncomment the following line for Rapid Response Mode observations (NOAO mode only)
%\INSconfig{}{MUSE}{RRM}{yes}
%
%-----------------------------------------------------------------------
%---- ESPRESSO at the VLT-ICCF -----------------------------------------
%-----------------------------------------------------------------------
%
% ESPRESSO in 1 UT mode:
%
%\INSconfig{}{ESPRESSO-1UT}{HR}{1x1, 2x1}
%\INSconfig{}{ESPRESSO-1UT}{UHR}{1x1}
%
% ESPRESSO in 4 UT mode:
%
%\INSconfig{}{ESPRESSO-4UT}{MR}{4x2, 8x4}
%
%-----------------------------------------------------------------------
%---- GRAVITY ----------------------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{GRAVITY}{Single-Field}{provide list of grating(s) (LR,MR,HR) HERE}
%\INSconfig{}{GRAVITY}{Dual-Field}{provide list of grating(s) (LR,MR,HR) HERE}
%\INSconfig{}{GRAVITY}{Astrometry}{provide list of grating(s)(LR,MR,HR) HERE}
%
%%For UT runs, uncomment the following line and specify the Wave Front Sensor to be used: either MACAO or CIAO Off axis:
%\INSconfig{}{GRAVITY}{WFS}{MACAO or CIAO-OFF}
%
%----------------------------------------------------------------------
%---- MATISSE at the VLTI ---------------------------------------------
%----------------------------------------------------------------------
%% For L band the dispersive element must be specified. For N
% band in P103 only the low resolution is available and always
% observed in parallel to L band.
%
%\INSconfig{}{MATISSE}{L}{Give list of dispersive elements to be used (LR,MR,HR)}
%\INSconfig{}{MATISSE}{N}{LR}
%
%-----------------------------------------------------------------------
%---- PIONIER ----------------------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{PIONIER}{GRISM}{1.65}
%\INSconfig{}{PIONIER}{FREE}{1.65}
%
%-----------------------------------------------------------------------
%---- VIRCAM at VISTA --------------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{VIRCAM}{IMG}{provide list of filters here}
%
%-----------------------------------------------------------------------
%---- OMEGACAM at VST --------------------------------------------------
% This instrument is only available for GTO, Chilean and filler programmes.
%-----------------------------------------------------------------------
%
%\INSconfig{}{OMEGACAM}{IMG}{provide list of filters here}
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% La Silla
%
%-----------------------------------------------------------------------
%---- EFOSC2 (or SOFOSC) at the NTT ------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{EFOSC2}{PRE-IMG}{EFOSC2 filters: provide list here}
%\INSconfig{}{EFOSC2}{Imaging-filters}{EFOSC2 filters: provide list here}
%\INSconfig{}{EFOSC2}{Imaging-filters}{ESO non EFOSC filters: provide ESOfilt No}
%\INSconfig{}{EFOSC2}{Imaging-filters}{User's own filters (to be described in text)}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#1:320-1090}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#2:510-1100}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#3:305-610}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#4:409-752}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#5:520-935}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#6:386-807}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#7:327-524}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#8:432-636}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#11:338-752}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#13:369-932}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#14:310-509}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#16:602-1032}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#17:689-876}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#18:470-677}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#19:440-510}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Grism\#20:605:715}
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Aperture: 0.5'', ... ,10.0''}
%
%\INSconfig{}{EFOSC2}{Spectro-long-slit}{Aperture: Shiftable}
%\INSconfig{}{EFOSC2}{Spectro-MOS}{PunchHead=0.95''}
%\INSconfig{}{EFOSC2}{Spectro-MOS}{PunchHead=1.12''}
%\INSconfig{}{EFOSC2}{Spectro-MOS}{PunchHead=1.45''}
%\INSconfig{}{EFOSC2}{Polarimetry}{$\lambda / 2$ retarder plate}
%\INSconfig{}{EFOSC2}{Polarimetry}{$\lambda / 4$ retarder plate}
%\INSconfig{}{EFOSC2}{Coronograph}{yes}
%
%-----------------------------------------------------------------------
%---- SOFI (or SOFOSC) at the NTT --------------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{SOFI}{PRE-IMG-LargeField}{Provide list of filters HERE}
%\INSconfig{}{SOFI}{Imaging-LargeField}{Provide list of filters HERE}
%\INSconfig{}{SOFI}{Burst}{Provide list of filters HERE}
%\INSconfig{}{SOFI}{FastPhot}{Provide list of filters HERE}
%\INSconfig{}{SOFI}{Polarimetry}{Provide list of filters HERE}
%\INSconfig{}{SOFI}{Spectroscopy-long-slit}{Blue Grism, Provide list of slits HERE}
%\INSconfig{}{SOFI}{Spectroscopy-long-slit}{Red Grism, Provide list of slits HERE}
%\INSconfig{}{SOFI}{Spectroscopy-high-res}{H, Provide list of slits HERE}
%\INSconfig{}{SOFI}{Spectroscopy-high-res}{K, Provide list of slits HERE}
%
%-----------------------------------------------------------------------
%---- ULTRACAM at the NTT ----------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{ULTRACAM}{-}{-}
%
%-----------------------------------------------------------------------
%---- HARPS at the 3.6 -------------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{HARPS}{spectro-Thosimult}{HARPS}
%\INSconfig{}{HARPS}{WAVE}{HARPS}
%\INSconfig{}{HARPS}{spectro-ObjA(B)}{HARPS}
%\INSconfig{}{HARPS}{spectro-ObjA(B)}{EGGS}
%\INSconfig{}{HARPS}{spectro-polarimetry}{linear}
%\INSconfig{}{HARPS}{spectro-polarimetry}{circular}
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Chajnantor
%
%-----------------------------------------------------------------------
%---- ARTEMIS at APEX ----------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{ARTEMIS}{IMG}{350 and 450 um}
%
%-----------------------------------------------------------------------
%---- LABOCA at APEX ----------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{LABOCA}{IMG}{-}
%
%-----------------------------------------------------------------------
%---- nFLASH at APEX ----------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{nFLASH}{-}{Please enter Central Frequencies from 200 to 270 GHz and from 385 to 500 GHz}
%
%-----------------------------------------------------------------------
%---- SEPIA at APEX ----------------------------------------------
%-----------------------------------------------------------------------
%
%\INSconfig{}{SEPIA}{Band-5}{Please enter Central Frequency 159 to 211 GHz}
%\INSconfig{}{SEPIA}{Band-7}{Please enter Central Frequency 272 to 376 GHz}
%\INSconfig{}{SEPIA}{Band-9}{Please enter Central Frequency 602 to 720 GHz}
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% Interferometry PAGE %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
% The \VLTITarget macro is only needed when requesting
% interferometry, in which case it is MANDATORY to uncomment it and
% fill in the information. It takes the following parameters:
%
% 1st argument: run ID
% Valid values: run IDs specified in BOX 3
%
% 2nd argument: target name
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 3rd argument: visual magnitude
% Values with up to two decimal places are allowed here.
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 4th argument: magnitude at wavelength of observation
% Values with up to two decimal places are allowed here.
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 5th argument: wavelength of observation (in microns)
% Values with up to two decimal places are allowed here.
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 6th argument: size at wavelength of observation (in mas)
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 7th argument: baseline
% UT observations are scheduled in terms of 4-telescope baselines for PIONIER, MATISSE and GRAVITY.
%
% AT observations are scheduled in terms of 4-telescope
% configurations (quadruplets) for any instrument.
% For AT observations with any instrument, please specify
% one of the 3 (or 4 for GRAVITY) available AT quadruplets at this stage.
%
% 8th parameter: Range of visibilities for the specified configuration.
% Please specify the maximum and minimum visibility values
% corresponding to the chosen configuration at hour angle 0
% separated by "/".
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 9th parameter: correlated magnitude
% (for the visibility values specified in the 8th parameter)
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% 10th parameter: time on target in hours
% Values with up to two decimal places are allowed here.
% This parameter is NOT checked at the pdfLaTeX compilation.
%
% PIONIER
% A0-G1-J2-J3 : corresponding to the "large" configuration
% D0-G2-J3-K0 : corresponding to the "medium" configuration
% A0-B2-C1-D0 : corresponding to the "small" configuration
% UT1-UT2-UT3-UT4
%
% MATISSE
% A0-G1-J2-J3 : corresponding to the "large" configuration
% D0-G2-J3-K0 : corresponding to the "medium" configuration
% A0-B2-C1-D0 : corresponding to the "small" configuration
% UT1-UT2-UT3-UT4
%
% GRAVITY
% A0-G1-J2-J3 : corresponding to the "large" configuration, only offered in single-field mode
% D0-G2-J3-K0 : corresponding to the "medium" configuration, only offered in single-field mode
% A0-B2-C1-D0 : corresponding to the "small" configuration, offered in both single-field and dual-field modes
% A0-G1-J2-K0 : corresponding to the "astrometric" configuration, only offered in dual-field mode
% UT1-UT2-UT3-UT4
%
%\VLTITarget{E}{Alpha Ori}{-1.4}{-1.4}{10.6}{6}{UT1-UT2-UT3-UT4}{0.60/0.10}{-0.2/4.0}{2}
%\VLTITarget{F}{Alpha Ori}{-1.4}{-1.4}{10.6}{6}{AO-G1-J2-J3}{0.80/0.40}{-0.9/-0.2}{1}
% You can specify here a note applying to all or some of your VLTI
% targets. You should take advantage of this note to indicate
% suitable alternative baselines for your observations.
% This macro is NOT checked at the pdfLaTeX compilation.
%\VLTITargetNotes{Note about the VLTI targets, e.g., Run E can also be carried out using UT1-UT3-UT4.}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% THE END %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\MakeProposal
\end{document}