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Concerning the project

Observational program

Overview

GSC 0244 434

GSC 1040 399

GSC 1077 828

GSC 2750 854

GSC 2774 1779

GSC 2775 1188

GSC 2779 288

GSC 2978 366

GSC 4420 1984

HadV 26

HD 226957

IM Vul

KZ Dra

LR Com

MisV 1275

NSV 2470

NSV 13204

NSV 14559

TASS J0246

V355 Aur

V440 And

V523 Aur

V840 Her

V1011 Her

V1097 Her

XY Cnc

How to observe ?

Downloads

Ephemerides

Finding charts

Publications

Observation results

Status reports

Statistics

Useful links

The Prosper Projekt

Instructions for observers

Required format of observations

The format of observations (even individual points are useful!) should be the following (very similar to the MEDUZA format):

Position:1 11 25355565
Field:name of the starjulian datemagnitude date (UT)observer’s abbreviationestimate(s)
Example:QR And 2451139.25611.281998-11-21.756XYE4V2F

The observer's abbreviations are the same for PROSPER and MEDUZA group.

The observations send please to:


Contacts:

E-mail:

Web: http://prosper.ssph-brno.org

Snail-mail: RNDr. Miloslav Zejda, Nicholas Copernicus Observatory and Planetarium, Kraví hora 2, Brno, 616 00, Czech Republic


Some remarks to the charts

Each star has two independent charts. The first chart is intended particularly to visual observers. In the upper right corner of each view port, there is shown the level of the chart by Roman numerals. In the lower left corner there is an explanation of used magnitudes and orientation. Lower parts of the view ports contain also the information about scale. Stellar magnitudes are in visual passband and are in decimagnitudes. The variable is denoted by two lines in the last view port. Lowercase letters denote preliminary comparison stars, for these stars, V band magnitudes are given on the chart.

The second chart is intended to observers equipped with CCDs. The upper view port of the chart contains close vicinity of the variable star, lower left corner contains explanation of used magnitudes and orientation. Numbers near the stars are brightness’ in decimagnitudes. Box in the view port corresponds to the image in the bottom of the chart. The variable star is denoted by two lines both in the finding chart and the image. Arabic numerals give preliminary comparison star for which V and B-V were computed.

Useful tool for CCD observers could be "reference stars". They are one or more very bright stars, mostly seen by naked eye, which can be used for the setup of the telescope.

Stellar magnitudes were taken from Tycho-2 catalogue and recalculated to Johnson V using formulae supplied with the catalogue.

Charts for visual observers are shipped together with this issue of Perseus. CCD observers can find them on the Internet in TIFF and PS formats or they will be send to them upon request.