The Photo-z Infrared Telescope (PIRT) -- a space instrument for rapid follow up of high-redshift gamma-ray bursts and electromagnetic counterparts to gravitational wave events
M. Seiffert, A. Balady, T.-C. Chang, R. Dyer, H. Fausey, S. Guiriec,, M. Hart, R.O. Morris, J.I. Rodriguez, P. Roming, M. Rud, D. Russell, R., Sambruna, R. Terrile, V. Torossian, A.J. van der Horst, N.E. White, P., Willems, A. Woodmansee, E.T. Young

TL;DR
PIRT is a space infrared telescope designed for rapid follow-up of high-redshift gamma-ray bursts and gravitational wave counterparts, enabling quick localization and characterization in coordination with other observatories.
Contribution
This paper introduces the design and expected performance of PIRT, a new space-based instrument for rapid identification and study of distant GRBs and GW event counterparts.
Findings
PIRT can identify GRBs with redshift z > 6.
Expected localization accuracy better than 1 arcsecond.
Enables timely follow-up with ground-based telescopes and JWST.
Abstract
The Photo-z InfraRed Telescope (PIRT) is an instrument on the Gamow Explorer, currently proposed for a NASA Astrophysics Medium Explorer. PIRT works in tandem with a companion wide-field instrument, the Lobster Eye X-ray Telescope (LEXT), that will identify x-ray transients likely to be associated with high redshift gamma-ray bursts (GRBs) or electromagnetic counterparts to gravitational wave (GW) events. After receiving an alert trigger from LEXT, the spacecraft will slew to center the PIRT field of view on the transient source. PIRT will then begin accumulating data simultaneously in five bands spanning 0.5 - 2.5 microns over a 10 arc-minute field of view. Each PIRT field will contain many hundreds of sources, only one of which is associated with the LEXT transient. PIRT will gather the necessary data in order to identify GRB sources with redshift , with an expected source…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Pulsars and Gravitational Waves Research · Astronomy and Astrophysical Research
