PhoSim-NIRCam

PhoSim-NIRCam is a full end-to-end JWST/NIRCam image simulator built on the framework of the LSST image simulator PhoSim. It contains a comprehensive physical model of the JWST telescope + NIRCam, and simulates photons propagating through the whole system using a Monte Carlo approach.  PhoSim-NIRCam is easy to use, allowing the user to start creating realistic NIRCam images with minimal preparation.  It also provides a variety of advanced features that allow direct control of any element in the system.

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Beta version (02/26/18)
88 MB (452 MB unpacked)

Welcome to PhoSim-NIRCam!

What is PhoSim?

PhoSim (Photon Simulator) is an image simulator originally developed for the Large Synoptic Survey Telescope (LSST) by John Peterson and his group at Purdue University.  PhoSim is different from typical image simulators in astronomy in that it replicates the whole telescope and instrument system in the code (as well as the atmosphere in the case of LSST) and follows the propagation of photons using a Monte Carlo approach.  PhoSim, therefore, is a full end-to-end simulator, capable of creating highly realistic images that contain all the characteristics of the actual telescope + instrument system.  Furthermore, since PhoSim allows direct control of any element in the system, it can be used to diagnose real data, helping to identify the origin of any unexpected features and characteristics that may appear in the real system.

PhoSim-NIRCam

Although developed primarily for LSST, PhoSim itself is a physics-based code that can simulatie any optical/IR observing system when used with appropriately constructed configuration files. PhoSim-NIRCam has been developed by taking advantage of this feature, and is essentially PhoSim that comes with a particular set of configuration files constructed for JWST + NIRCam. Despite its complex inner working, PhoSim-NIRCam is easy to use, and is typically run as a one-line command with a CatalogFile and a CommandsFile.

Disclaimer: PhoSim-NIRCam is still in the early phase of develpment, and has not been tested extensively. So, please report to us any problem you might encounter! The "Known Issues/Development Plan" document (available from the "Quick Guide" menu at the top) lists the current limitations and develepment plans.

Information

LSST PhoSim

JWST PhoSim-NIRCam

JWST/NIRCam Images Simulated by PhoSim-NIRCam

The CANDELS GOODS-S F160W source catalog was used with PhoSim-NIRCam to create these images (a flat-fnu SED was assumed).  To avoid saturation, eleven 1310-sec images (comparable to DEEP8 NGROUPS=7) were combined to produce Tint = 4 hr images.  In this simulation, the NIRCam images do not necessarily look deeper than the CANDELS HST/F160W image because the former only contain sources that are seen in the latter.

JWST/NIRCam SW F200W Image

Total integration time: 4 hours (11 x 1310 sec);  Sky background: 0.1 MJy/sr.
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JWST/NIRCam LW F356W Image

Total integration time: 4 hours (11 x 1310 sec);  Sky background: 0.1 MJy/sr.
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HST/WFC3-IR F160W Image

The publicly available CANDELS image, which was used as the truth image for this simulation.

JWST/NIRCam LW Field Distortion

The yellow circles (r=1.5") mark the expected source locations in the distortion-free image.

The Developers

Purdue University
Colin Burke, John Peterson

University of Arizona
Eiichi Egami, Jarron Leisenring

Contact

Eiichi Egami
eegami@as.arizona.edu
JWST/NIRCam team
Steward Observatory, University of Arizona

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