|
PIT Hot News
|
18 February 2008
Improvements in the new PIT release: the 2008B
release of PIT includes the following modifications to support the special call for proposals:
- Enhancements to PIT
- The proposal checks will compare the target coordinates with the windows of optimum visibility for the semester and give appropriate warnings.
- Updated instrument resources
- Updated PIT help
31 August 2007
Improvements in the new PIT release: the 2008A
release of PIT includes the following modifications to support the special call for proposals:
- Enhancements to PIT
- The Band 3 tab includes an
entry box for the total requested time in Band 3 (in case this differs
from the standard request) as well as the minimum required Band 3 execution time.
- There
are new submission options on the Submit tab for accepting different
types of special proposals (poor weather, DD, DS, SV).
- Updated instrument resources
- Updated PIT help
05 May 2007
Improvements in the new PIT release: the 2007B.05
release of PIT includes the following modifications to support the special call for proposals:
- Enhancements to PIT
- Phoenix has been added to the Gemini South resource list
- Bug fixes
- Classical proposals may be submitted with observing conditions that are not 'Any'.
26 February 2007
Improvements in the new PIT release: the 2007B
release of PIT includes the following modifications:
- Enhancements to PIT
- A tab for entering considerations in case the program should end up in ranking band 3
- Classical
programs must provide all observing conditions constraints and if good
conditions are requested (better than IQ=85% and CC=70%, or WV=80%)
must provide information about bad weather backup plans as an
attachment to the scientific justification
- For a given proposal, only one telescope (Gemini North, Gemini South, Keck, or Subaru) may be chosen in the resources section
- Refined
guide star selection algorithms. The algorithms have been updated
to match the 2007A OT and various problems have been resolved.
- Queue
programs with timing contraints (e.g. coordinated observations with
other telescopes, limited numbers of observing windows) should give
these constraints in the scheduling tab.
- There are now two "Target is guide star" options, one for NICI and one for the facility AO system (Altair).
- User interface improvements
- New guide star assistant
- Arrows for re-ordering the co-investigator list
- The Mac version uses standard Mac key bindings
- PIT help updated
30 August 2006
Improvements in the new PIT release: the 2007A
release of PIT includes the following modifications:
- Enhancements to PIT
- User interface improvements
- Target of Opportunity mode (Standard or Rapid Response) selection
- Refined
guide star selection algorithms for NIFS and Altair. Altair AOWFS
is now called Altair NGS. A new Altair LGS algorithm is for
finding tip/tilt guide stars to be used with the laser AO beacon.
- General Target is Guide Star WFS algorithm for copying target information to a WFS component
- New UK NGO style sheet option
- USNO-B guide star catalog query added
- PIT help updated.
21 February 2006
Improvements in the new PIT release: the 2006B
release of PIT includes the following modifications:
- Enhancements to PIT
- Subaru added as a partner for the Gemini/Subaru time share.
- Instrument resources updated for 2006B: MOIRCS and Suprime-Cam on Subaru; NICI, Flamingos-2, and TEXES added for future
Campaign, SV and Demo Science observations (not available in the regular
2006B Call for Proposals).
- New
option for creating a PDF version of the proposal summary. Style
options for Gemini, NOAO, and the Chilean NGO are available.
- Postscript
attachments (.ps and .eps files) are no longer supported so that the
PDF export option will work reliably. It is recommended that postscript
figures be converted to PDF before attaching.
31 August 2005
Improvements in the new PIT release: the 2006A
release of PIT includes the following modifications:
- Enhancements to PIT
- Proposed observations can be checked to see whether potentially
duplicate datasets are in the Gemini Science Archive of the same target
(RA,dec tolerance of 30 arcsec) and same instrument (but not necessarily
the same instrument configuration).
- The RA and dec units must now be explicitly set as either hr/min/sec or
decimal degrees (RA) and deg/arcmin/arcsec or decimal degrees (dec). The
internal units are h:m:s and deg:arcmin:arcsec and converted for display.
- Previous data status information (reduced, analysed, published etc) and
related proposal details are now included in the proposal summary.
- Instrument resources updated for 2006A: bHROS added, GNIRS gratings
updated, added Altair field lens; NICI, NIFS and TEXES added for future
Campaign, SV and Demo Science observations (not available in the regular
2006A Call for Proposals).
- New option for submitting Demo Science (including campaign) and SV
proposals to a separate server at Gemini.
- Several new keywords added.
26 February 2005
Improvements in the new PIT release: the 2005B
release of PIT includes the following modifications:
- Enhancements to PIT
- Added field for status of previous Gemini data to new
"allocations" tab (reduced, analysed, published etc), which
combines previous allocation details with another new field, related
proposals submitted to other telescopes. The relevant on-line help pages
are updated.
- Partner lead scientist(s) of joint proposals are highlighted in the
proposal summary (above the PI details)
- Improved legibility of (HTML) partner summary table (smaller font - may
actually be slightly less legible in PIT but better in browsers and
hardcopy!). Note that a PDF summary will be added to supplement the HTML
summary, allowing inclusion of figures and other attachments in a single
document, in the 06A release.
- Summary corrected to list only the instrument resources that are used.
User interface modified to open automatically the instrument details for
the selected instrument.
- Instrument resources updated for 2005B: GMOS-S added H(alpha), H(alpha)
continuum and [SII] filters; GNIRS updated 0.675 arcsec slit and added
grating orders
26 August 2004
Improvements in the new PIT release: the 2005A
release of PIT includes the following modifications:
- Enhancements to PIT
- Submission of all joint proposals
now done in single-step to multiple partner backend servers. All partners
can now receive electronic submission of proposals.
- Instrument resources updated for 2005A: Michelle added echelle and
updated filters and slits; GNIRS added R=18000 grating and IFU, updated
slits; added Hokupa'a-85 (use is contingent on demonstration of
performance, see Call for Proposals for definitive details) and
corresponding AOWFS algorithm ; T-ReCS updated filters; GMOS-N removed u
filter; added HIRES (on Keck) for Gemini/Keck time exchange
25 February 2004
Improvements in the new PIT release: the
2004B
release of PIT includes the following modifications:
- Enhancements to PIT
- Instrument resources updated for 2004B: GNIRS added, IFU nod-and-shuffle
slits added for GMOS-South, Michelle gratings added and filters updated;
NIRI filters updated
- Additional checking from the "Check Proposal" button on the
"Submit" tab. Now checks that classical proposals have
"any" listed as the observing conditions for image quality,
cloud cover and water vapour, that guide stars are brighter (than 13mag)
if cloud cover is 90%-ile or poorer and that the default ("any")
observing conditions or example proposal are not submitted
accidentally.
- Word count added to abstract and to scientific and technical
justifications.
29 August 2003
Improvements in the new PIT release: the 2004A
release of PIT includes the following modifications:
- Bug Fixes
- Gemini North or Gemini South telescopes would occasionally be left in
the instrument resources even though there was no corresponding
instruments.
- HTML summary previously would lose the first character of the last line
in a text field if the previous line ended with a carriage return.
- Enhancements to PIT
- Guide star algorithms for Altair AO and chopping whilst using Peripheral
WFS added.
- Instrument resources updated for 2004A.
27 February 2003
Improvements in the 2003B PIT release: this release
includes the following modifications suggested by representatives of the National Gemini Offices:
- Enhancements to PIT
- Added checkbox on investigator page to identify "Principal
Contact" (PC) of joint proposals. Joint proposals (submitted to
multiple National TACs) must have one (and only one) Principal Contact.
The Principal Contact need not be the Principal Investigator. (PIT checks
that there is exactly one PC if multiple partners are selected on the
submit tab).
- Instrument resources updated for 2003B.
- Internal designation of image quality percentile bands made consistent
with values in GUI and public Observing Tool.
1 September 2002
Improvements in the 2003A PIT release: this release
includes the following modifications suggested by PIT users and/or
representatives of the National Gemini Offices:
- Bug Fixes
- Previous allocations could not always be read correctly from a file and
format of GUI was corrupted.
- Corrected PI status so that "GradNoThesis" is a valid status.
- Enhancements to PIT
- Image quality bands changed from [20%, 50%, 80%, Any] to [20%, 70%, 85%,
Any] to reduce sensitivity to underlying distribution (50% was at the
peak, by definition). Specific values in arcsec have also been adjusted
for currently observing seeing distributions - see the observing
condition constraints for details.
- Added check that total time requested is non zero to the built-in
verification.
- Instrument resources updated for 2003A.
- Updated URLs of guide star catalogues in catalogue assistant.
- Gamma ray bursts added to extragalactic keywords.
18 February 2002
Improvements in the 2002B PIT release: this release
includes the following modifications suggested by PIT users and/or
representatives of the National Gemini Offices:
- Bug Fixes
- Proposal verification no longer fails if the Default Resources are
deleted provided that every observation has override resources.
- Enhancements to PIT
- The time requested must now be entered explicitly by the
applicants. Previously the time summed over all observations was used and
was not editable. (This is still available as a guide). This simplifies
requesting different or partial allocations from an NTAC when the same
proposal is submitted to multiple NTACs for joint support.
- Support for PIT users whose machines connect to the internet via a proxy
server is now available from the file menu. (See more information on proxy
settings).
- An "update" feature has been added to streamline future
software distribution. It is intended that in future semesters only the
changed modules, and not the entire software package, will need to be
downloaded. At present this will probably either do nothing (Windows) or
dump diagnostic info to stdout (Solaris, Linux).
- Publications and previous time allocations may be loaded from
files. See the PIT
publications help page for file formats.
- Summary of instrument resources for the whole program and for each
observation added on the observations/resources page. See the PIT
observation resources help page for details.
- Tab added to scheduling page to justify optimal dates for scheduling.
- Previous allocations reinstated in HTML summary.
31 August 2001
Improvements in the 2002A PIT release: this release
includes the following modifications suggested by PIT users and/or
representatives of the National Gemini Offices:
- Bug Fixes
- Can select the same institution from the drop-down menu for consecutive
co-Is.
- Corrected instance of context-sensitive help pointing to wrong page.
- Save button on text pages (abstract, scientific and technical
justification, target list, TAC) now writes text file by default, reducing
possibility of over-writing entire XML proposal with contents of that
page's text box.
- Corrected one-day mismatch between the optimal or impossible dates as
specified by the user and as reported in the HTML summary
- Enhancements to PIT
- Resources (e.g. instrument configurations) are now defined and used
similar to observing constraints. A 'global default' configuration applies
to all observations in the proposed science program. This may be overridden
for one or more observations; each can have its own instrument
configuration. (See the PIT
resources help page for more details).
- Format of HTML summary tidied up; when printed, the first page now
includes all of the key information concerning the proposal. (See an
example from the GeminiDemo proposal included with PIT). Now
includes NTAC comments (if available).
- New or significantly modified help pages:
- GeminiData.xml file updated with 2002A instrument resources.
11 February 2001
Improvements in the 2001B.0 PIT release: this
release of PIT includes the following modifications suggested by PIT users and/or
representatives of the National Gemini Offices:
- Bug Fixes
- Overriding default observing condition constraint set now puts correct reference in XML
file.
- PWFS (or OIWFS, guide star) stars selected automatically by the catalog search assistant
can now be overridden.
- The symbols >, < and & can be used in text (title, abstract, science and tech
justification).
- The symbol & can be used in figure attachments (e.g. 'Figure 1 & 2').
- PWFS stars for objects with dec = -00:mm:ss.s are now correct. This was a problem with
the CADC server; ESO and Gemini servers gave correct results.
- The TAC-recommended time box no longer shrinks to narrow width when TAC comments extend
beyond the visible page and generate a scroll bar.
- Proposals with non-sidereal objects in the observation list no longer hang the HTML
summary and (in the Solaris version) give a Java error.
- Enhancements to PIT
- Information concerning the other partner countries is now collected for proposals
seeking joint support: check boxes for the names of the additional partners and added
collection of the total time requested from all partners. This information is reported in
the top section of the HTML summary.
- The co-ordinates for targets newly created in PIT must be given in the J2000 frame.
Formatted text files with targets may still contain B1950 co-ordinates; these are now
precessed to J2000 on-the-fly. Consequently the catalogue search assistant will find
available guide stars for all targets.
- The "integration time" has been re-labelled as "integration time +
overheads" on the observation page for each new target to emphasise that overheads
must be included.
- The source brightness field is now included when an external target list is saved or
loaded to a file.
- The partner-recommended time (on the TAC page) includes a minimum recommended time to
provide additional flexibility when constructing the schedule.
- For clarity, "guide star" was removed from the list of allowable wavefront
sensors, leaving (Peripheral) "Wave Front Sensor" and "On-Instrument
Wavefront Sensor" (including adaptive optics wavefront sensor) as the options.
- Additional catalogue search assistant algorithm added for GMOS on-instrument wavefront
sensor.
- GeminiData.xml file update with 2001B instrument resources.
- New Software
- A standalone script has been added that checks the Solaris operating system version and
the require patches.
- Connectivity to the guidestar catalogue servers can now be verified
using a web form. Testing of the connection to their back-end reception and processor
systems has been added by the UK (Canada & Australia?). The back-end system provides
verification of proposal submission (see more details
on the UK support page).
- Typographical Corrections in PIT
- "Principle Investigator" replaced with "Principal Investigator" on
eth PIT summary page.
- Gemini South added to the list of institutions.
- Institute of Astronomy (University of Hawaii) corrected to Institute for Astronomy.
- University of Oxford postal code corrected to OX1 3RH.
- HIA postal code updated to V9E 2E7.
12 March 2000
Improvements in the 2001A.0 PIT release: this release
includes the following modifications suggested by PIT users and/or representatives of the
National Gemini Offices:
- HTML summary now correctly recognises paragraph breaks in text and formats the output
- Speed of HTML summary generation has been improved dramatically; overall program
execution speed improved
- Automatic search for AOWFS and NIRI (f/14 camera) OIWFS stars is included; WFS patrol
fields updated
- Collect additional information to help technical assessment (especially target flux, WFS
brightness and separation; the latter two are collected automatically from the guide star
catalog server) and reported in the HTML summary
- Augment the pre-submission verification and expand the feedback when PIT verification is
run (now checks details of observations, file attachments)
- Further develop the help pages and add a beginner's Cookbook
- Tidy up the terminology when talking about WFS guide stars
- Update the GeminiDatan.xml file that contains the current semester dates and instrument
resources etc.
Last update February 14, 2008; Bryan Miller