P200 Observer Information

Nighttime long exposure of the open Hale Telescope dome. (Palomar/Caltech)

Contents

1. P200 telescope
2. P200 schedule/instrument settings
3. P200 instruments
4. P200 software resources
5. P200 CCDs and filters

Our present limited operations guidelines.

Please see Palomar Remote Observing resources.
Updated Mon 08 Jun 2020 7:18 am PDT

P200 Telescope

Nightly operations of the Palomar 200-inch Hale Telescope (P200) are conducted from a data/control room, and facilitated by telescope operators and support astronomer personnel. Typically observations are conducted in the same data room; in limited circumstances remote observations are supported—see Palomar Remote Observing. Allocation of P200 observing time is handled through independent time allocation process within eligible constituencies, and the allocations are merged into an integrated observing schedule.

P200 supports limited remote observing capabilities for CHIMERA, DBSP, TSpec, WaSP, and WIRC. Interested/eligible parties can find more information on Palomar Remote Observing at our COO Remote Observing page.

P200 Schedule/Instrument Settings

The Lead Observer (LO) identified for each P200 night is the single contact point for all scheduling and logistical matters associated with the observing run. If no distinct LO is designated, the program Principal Investigator serves as LO. Please see the on-line P200 Observing Schedule if you have questions about the LO-designation for an upcoming run.

LOs are responsible for identifying instrument settings at least two weeks before an observing run. Instrument settings (aka Palomar "green sheets") for instruments such as DBSP are defined through the on-line reservation form (available through the observer login portal, or through help request to the Palomar support team).

Questions concerning observing setups or any other logistical issues should be sent to the Palomar support team.

P200 Instruments

The Hale Telescope instruments provide a wide range of imaging and spectroscopic capabilities in the optical and near-infrared.

The Hale's seeing-limited imaging instruments include two wide-field cameras: the Wafer-scale imager for Palomar (WaSP) CCD imager in the optical and the Wide-field Infrared Camera (WIRC) HgCdTe imager in the infrared, both mounted at the prime focus of the telescope and covering 24 and 8.9 arcminutes across, respectively. The high-speed CHIMERA imager operates in electron-multiplied photon-counting mode at prime focus for precision photometry. At Cassegrain focus, the Cosmic Web Imager (CWI) is an imaging spectrograph (integral-field unit) that images a 1-arcmin FoV over a range of wavelengths simultaneously. The traditional single-object spectrographs, the optical Double Spectrograph (DBSP) and the infrared Triple Spectrograph (TripleSpec), both also install at the Cassegrain focus.

PALM-3000 is the facility high-Strehl ratio AO system for the Hale Telescope. It works in conjunction with a suite of back-end instruments, including the workhorse imaging spectrometer Palomar High Angular Resolution Observer (PHARO) and Palomar Radial Velocity Instrument (PARVI), an ultra-stable diffraction-limited, high-resolution infrared spectrograph focused on exoplanet science using both the radial velocity technique and high-contrast, high-dispersion coronagraphy.

Palomar’s newest initiatives are NGPS, a modern highly-efficient workhorse moderate-resolution optical spectrograph under development to replace the nearly 40-year-old DBSP, and SIGHT, a compact facility ultraviolet laser-guide-star adaptive optics system that will integrate with the P200 telescope to provide broadband wavelength seeing improvement to a range of optical-to-infrared wavelengths at any location on the sky. NGPS and SIGHT are both expected to enter routine science operation in 2023.

The following is a summary of P200 instrument information/resources:

Public instruments are those set up and maintained by the Palomar Observatory staff, and are available for all constituencies to use.

Private instruments are those built, set up, and maintained by individuals or groups for their own research. Other observers wishing to use these instruments must to arrange, in advance, a collaboration with the builder.

Semiprivate instruments are similar to the private instruments except that the builders have agreed to make them available to others without the need for a formal collaboration, although consultation may be advisable. Scheduling restrictions may apply, however.

P200 Software Resources

• FACSUM: P200 observation aid tool (HTML, PDF)
• DBSP Guider Software: DBSP guider software (HTML, PDF)
• DBSP Quick-Look Tool: DBSP quick-look data reduction software (HTML, PDF)

P200 CCDs and Filters

A summary of technical specifications for the P200 CCDs is available here.

A P200 filter list, sensitivities and sky background measurements are also available.