Chandra X-Ray Observatory (CXC)

Chandra Observation Scheduling and Observer Support


Overview

After the Peer Review, the Chandra Director's Office (CDO) sends a message to observers of approved programs, requesting that they confirm basic observing parameters for their targets.

After observers confirm basic parameters, a long-term schedule (LTS) can be generated. The LTS includes all observations for the given cycle. This consists of both targets that need to be assigned to specific weeks, plus targets assigned to a "pool". Pool targets are unconstrained observations that are used to fill out the weekly short-term schedules (STS).

The LTS is updated each week to incorporate changes as the cycle progresses.

After the initial LTS is built for a cycle, the Chandra uplink support Interface scientists ("USINT", or "uplink scientists") contact observers to requests a more detailed second confirmation of observation parameters. If these parameters are not confirmed in a timely fashion, the target may need to be rescheduled, sometimes after a considerable delay.

The final planned short-term schedule (STS) for the week is posted on the public web soon after the schedule is approved for upload to Chandra.

Early scheduling of Targets

Targets are placed in the LTS according to constraints imposed by both science and spacecraft requirements. Observers should be aware that some targets may be scheduled early. During the transition period before the nominal start of a new cycle, the LTS usually includes a mix of targets from both cycles.

Reviewing Target Information

Observers can review observation parameters in the Chandra database at any time using either WebChaSeR or from the pages linked off the table returned by the Target Search Form.

Observers are encouraged to review these pages to confirm the observation setup well in advance of their LTS observation date and either submit changes or else confirm that the configuration is correct to their uplink contact scientist.

Uplink Support (USINT) for Observers

After the initial parameter confirmation done by CDO, each Chandra observation is assigned an uplink support (USINT) scientist from the DOSS or Calibration groups at the CXC based upon the selected instrument. The uplink scientist is responsible for contacting each observer to confirm their observation configuration in more depth in advance of releasing the observation for scheduling in an STS.

The support process includes a series of steps:

  1. The uplink scientist sends a standard form letter for the relevant instrument. The user is asked to respond within a certain time frame based upon a projected observation date.
  2. Upon response from the user, the uplink scientist requests any necessary changes to the observation configuration and releases the observation for scheduling. Should the user not respond by the specified deadline, the observation cannot be scheduled and may be significantly delayed.
  3. The observation is selected as a candidate for observation in a specific week and enters the scheduling process.
  4. Should the observation be confirmed, it will appear in the short term schedule (STS) for that week on the CXC web pages.
  5. After the observation setup is confirmed, the uplink scientist will only contact the observation PI/observer again if their scheduled observation is not actually done (e.g., due to radiation, safe mode, TOO, or other unforeseen circumstances).
  6. When the observation is completed and the data received on the ground, the PI/observer is informed by the CXC data systems group, who sends them the quick look images and, later, the data itself.

Observation Planning Schedule

This table applies to observations scheduled during the nominal cycle and may not apply to targets chosen for early observation. Early targets may undergo an abbreviated schedule, with faster required response times.

ActionUsual Timing
(days are counted back from the first day of the target's LTS week)
First Contact from the Director's OfficeWithin one month of the announcement of approved targets for the new cycle
USINT Contacts the Observer Start of Cycle (earlier if targets are selected for early scheduling)
Observer Response to USINT contact required32 days (Failure to respond to USINT can cause significant delays in the scheduling of an observation, possibly as long as a year in extreme cases.)
Observing Parameters are finalized in the CXC database25 days
Observation request is submitted for scheduling23 days

A generic form of the current contact letters and information can be found at one of the following links:

Long Term Schedule (LTS)

This is generated for each observing cycle. It places about 50% of the targets into one week bins, taking note of all observing constraints. In order to achieve an efficient final schedule, the remaining unconstrained targets are placed in the pool and are selected for observation by the Mission Planning team as they become visible to Chandra.

The LTS is updated roughly once a week, and is available on the LTS page. Pool targets, which are those most likely to move around, are labeled clearly in each schedule.

Short Term Schedule (STS)

This is generated weekly in preparation for upload to Chandra on the Sunday of each week. It is also updated on the public web site soon after notification of final approval for an STS goes out.

This is the official observation plan but we note that unanticipated events, such as TOOs, increased solar activity, satellite problems (etc.), can interrupt the schedule - resulting in some of the observations not being completed. In this case, an updated STS is generated and posted on the web and affected observers are notified.

TOO/DDT support

Due to the unpredictable nature of the observations, TOO and DDT targets are not usually assigned an uplink scientist until after a trigger has been approved. If they have not been assigned a USINT person before triggering an observation, the observers of these proposals may request help from the CXC through the HelpDesk.

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The Chandra X-Ray Center (CXC) is operated for NASA by the Smithsonian Astrophysical Observatory. 60 Garden Street, Cambridge, MA 02138 USA.   Email: cxcweb@head.cfa.harvard.edu Smithsonian Institution, Copyright © 1998-2012. All rights reserved.