Analysis on RXTE, INTEGRAL and ROTSE IIId observations of the X-ray Pulsar 4U 1907+09
S. Sahiner (1), S. C. Inam (2), A. Baykal (1), U. Kiziloglu (1) ((1), Middle East Technical University, (2) Baskent University)

TL;DR
This study combines RXTE, INTEGRAL, and ROTSE IIId data to analyze the timing, spectral properties, and optical behavior of the X-ray pulsar 4U 1907+09, providing an updated pulse period history and optical light curve.
Contribution
It offers a comprehensive timing and spectral analysis with an extended pulse period history and optical light curve, integrating multi-instrument observations for the first time.
Findings
Extended pulse period history of 4U 1907+09
Revised orbital distribution of X-ray dips
Long-term optical light curve of the source
Abstract
In this paper we present our recent timing and spectral analysis of the X-ray pulsar 4U 1907+09. Our X-ray data consist of an extended set of RXTE & INTEGRAL observations that were analyzed before ({\c{S}}ahiner et al. 2012). From the X-ray observations we extend the pulse period history of the source and obtain a revised orbital distribution of the X-ray dips. Using ROTSE IIId optical observations, we present the long term optical light curve of the source to have an understanding of long term optical behaviour.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysical Phenomena and Observations · Astronomical Observations and Instrumentation
