Klimov Tarpen Robotic Observatory

KTRO — Klimov Tarpen Robotic Observatory

“Tarpen” refers to the historical name associated with the Tushino area.

A compact robotic observatory designed to study measurement stability, reproducibility, and instrument response under real observational conditions.

KTRO is a semi-automated observational facility developed within the Psi–Continuum Experimental Program.

Its purpose is not large-scale survey astronomy or object discovery, but controlled and repeatable measurements.

KTRO system configuration

KTRO is conceived as a controlled platform for photometric stability studies, focused on long-term reproducibility, instrumental consistency, and methodological robustness.

KTRO is not about equipment.
It is about creating a stable observational reference system.

Project Overview

KTRO is being developed as a compact robotic observatory for controlled, repeatable astronomical measurements.

The project is oriented toward:

Rather than maximizing volume, KTRO is built to maximize control, traceability, and repeatability.

Why this matters

KTRO is not built to discover new objects — it is built to understand how measurements behave.
Measurement stability
Modern astrophysics relies on high-precision datasets, yet the stability of measurement systems themselves is rarely tested under controlled, repeatable conditions.
Reproducibility
KTRO provides a platform where the same observations can be repeated over months and seasons, allowing direct evaluation of reproducibility and systematic drift.
Instrument response
By operating a fixed, version-controlled pipeline, KTRO isolates how instruments and processing chains respond over time under identical conditions.
Methodological discipline
The project emphasizes controlled procedures over data volume, focusing on how reliable conclusions emerge from stable measurement systems.
KTRO complements large-scale cosmological datasets by providing a small-scale, controlled environment where measurement behavior can be directly examined.

The goal is not more data — but better-understood data.

Scientific Function within the Psi–Continuum Program

The Psi–Continuum framework operates at two scales:

KTRO serves as a controlled experimental testbed for measurement-system behavior.

While cosmological analyses rely on public datasets (SN Ia, BAO, H(z)), KTRO allows controlled repetition of measurements under known instrumental conditions.

The objective is methodological:

The guiding principle is consistent across scales:

Measurement systems must demonstrate stability, response coherence, and controlled deviations.

Observational Scope

Primary targets:

Observational protocol emphasizes:

The objective is reproducibility rather than discovery.

Instrumentation

Mount

Optical System

Planned Imaging Chain

The system is designed for mechanical stability, repeatable pointing, and progressive automation.

Development Phases

Phase 1 — Mechanical validation (completed)
Mount assembly, polar alignment testing, tracking validation.

Phase 2 — Semi-automation (ongoing)
Repeatable pointing routines, motor control refinement, pipeline integration.

Phase 3 — Long-term monitoring mode (planned)
Multi-month monitoring programs, cross-season stability checks, public data documentation where feasible.

Current Project Status

KTRO is currently in Phase 2 (semi-automation development).

At this stage, the project has already achieved:

The next milestone is transition from a semi-manual setup to a stable repeatable monitoring system suitable for long-term observational campaigns.

This transition depends not only on software and methodology, but also on completing the hardware chain required for fully reliable operation.

KTRO Build Status

KTRO is being assembled as a compact robotic observatory for reproducible photometric monitoring. The readiness level below is estimated directly from the number of completed core hardware modules.
Overall hardware readiness
2 of 9 key system modules are already deployed. The remaining modules are currently in progress.
22% complete — based on completed hardware cards
Estimated full operational readiness after hardware completion: ~85–90%
Completed
Sky-Watcher Explorer 150P
Primary optical tube already deployed as the telescope base of the KTRO system.
Completed
Completed
MaxVision EXOS-2 + OnStep V4 Pro
Equatorial mount and controller platform already operational as the mechanical base of the observatory.
Completed
In progress
ZWO ASI533MM Pro
Primary monochrome scientific camera for differential photometry, repeatable measurements, and long-term stability analysis.
Support component
In progress
ZWO EFW 2" Filter Wheel
Automated filter switching for controlled multi-band observations and a reproducible observing workflow.
Support component
In progress
Baader UBVRI Bessel Filter Set (V2)
Standard photometric filter set required for scientifically consistent and comparable measurements.
Support component
In progress
Baader MPCC Mark III
Coma correction module for improved field uniformity and more stable photometric quality across the frame.
Support component
In progress
ZWO EAFN Auto Focuser
Temperature-aware autofocus module for focus stability during repeatable long-duration observing sessions.
Support component
In progress
Mini PC (Intel N100 class)
Dedicated observatory-side computer for INDI, KStars, remote control, and automation pipeline operation.
Support component
In progress
Lunatico AAG CloudWatcher
Autonomous cloud and sky condition monitoring system required for safe unattended robotic operation.
Support component
Completed
2 modules: telescope and mount/controller platform.
In progress
7 modules remain to complete the operational hardware chain.
Current readiness
22% of key hardware modules completed.
Equipment support and shipment

Recipient: Dmitry V. Klimov
Region: Kaliningrad Region, Russia
Shipping details: provided upon request
Contact: d.klimov.psi@gmail.com

Please contact before purchase or shipment to confirm compatibility, current priority, and delivery details.

What support enables

Completing the KTRO hardware chain enables a transition from experimental setup to a stable observational system.
True photometric measurements
A cooled monochrome camera with calibrated filters enables scientifically consistent differential photometry, instead of qualitative observations.
Reproducible observing sessions
Automated filter switching, autofocus, and stable control allow identical observing conditions to be repeated across nights and seasons.
Fully automated operation
Integration of Mini PC, OnStep control, and environmental monitoring enables unattended robotic observing cycles with remote supervision.
Environmental awareness
CloudWatcher provides real-time sky condition assessment, allowing safe operation and consistent data quality control.
Stable data pipeline
A complete acquisition → calibration → reduction chain ensures traceable and reproducible data products.
Public observational dataset
The completed system enables structured long-term datasets that can be published and used for independent analysis.
Support does not only add hardware — it transforms KTRO into a controlled observational system capable of producing scientifically meaningful and reproducible data.

System Architecture

KTRO is designed as a complete observational chain: from optical acquisition and instrument control to calibrated data reduction and public publication.
Optical system
Sky-Watcher 150/750 telescope → Baader MPCC Mark III → ASI533MM Pro camera → 2" filter wheel → autofocus module
Mount and control
MaxVision EXOS-2 mount → OnStep V4 Pro controller → pointing, tracking, and repeatable motion control
Observatory-side computing
Mini PC → INDI / KStars / automation scripts → session control, device coordination, and monitoring
Environment and connectivity
Lunatico AAG CloudWatcher → sky-state monitoring → 4G communication link for remote supervision and control
Pipeline
Acquisition → calibration frames → reduction pipeline → quality checks → reproducible processed outputs
Data publication
Final data products → documentation → GitHub repository → public archival availability where feasible
System flow
Telescope + Camera Chain → Mount + OnStep → Mini PC → CloudWatcher + 4G Link → Reduction Pipeline → GitHub / Public Data
The architecture is intentionally compact: each subsystem serves reproducibility, remote operability, and traceable data flow.

Observational site

Rural site selected for controlled, repeatable observational conditions.
Sky quality

Bortle class 4–5 (estimated)

Conditions

Low light pollution, stable horizon, suitable for long-term monitoring.

Approximate location shown.

Reproducibility Policy

All data products will be made publicly available where possible.

All observational procedures are:

The program is methodological and complementary to professional observatories.

It aims to explore response diagnostics and stability structure under controlled small-scale conditions.

Status Summary

Current status: Phase 2 — semi-automation development
Hardware readiness: 22% complete
Completed modules: telescope; mount and controller
Priority: camera, filters, automation, weather monitoring

Structured long-term monitoring campaigns are planned for the sky conditions of the Nemansky region.