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observing

QX Pup

Update (July 7, 2015):  I-band coverage of QX Pup by AAVSO observers since 2010 clearly shows that the period given in the 4th Edition of the GCVS of 648: days is incorrect. A phase plot by Sebastián Otero of these data shows that the period of QX Pup in Ic is 551 days.

 

The Field of QX Pup

This is a multiple set of projects, so pick and choose what aspects of them interest you.

High Energy Network activities in 2009

Activities of the AAVSO International High Energy Network, FY 2008-2009
 

High Energy Network Overview

The AAVSO International High Energy Network came about as an evolution of the AAVSO International GRB Network. The GRB Network was established at the First High Energy Workshop for Amateur Astronomers in April, 2000. The GRB network was a great success, detecting many GRB afterglows and discovering a few on our own. The follow-up of GRB optical afterglows continues to be a major focus of the Network today.

Sky Calendar

Sorry! This page is still under development.

Observing Variable Stars

Multiwavelength observations of SS Cygni

Update: 2010 May 10

AAVSO Veterans, Peace Corps, VISTA, and more

Watch this page as we add information from you and from our archives!

Are you a veteran? Are you currently serving or have you served in the Armed Forces of the United States, your own country, or another country? The Red Cross or Red Crescent?  The Peace Corps? VISTA? Other similar organizations?

If yes, have you had interesting experiences related to your service and variable star observing or astronomy in general? Would you be willing to share them with us?

Observer Awards for Variable Star Observing

Without the nightly observations of amateur astronomers, the professional astronomer would find it difficult, if not impossible, to collect the quantity of data that is needed to further the study of stars, the Sun, novae and supernovae, comets, and meteors.

Standardized Magnitude

The standardized magnitude for the variable is given by

Vstd = (Vins - Cins) + Cstd

where Vins is the instrumental magnitude of the variable, Cins is the instrumental value of the comparison, and Cstd is the chart magnitude for the comparison (or the equivalent for ensemble photometry).

Note that 'standardized' does NOT mean that Landolt Standards were used as comparison stars.

Tags: 

AAVSO Unique Identifier

What Is The Name of That Star?

"What is the name of that star?" This is a question that many a young observer has asked their mentors. As astronomers we know that stars have many names - proper names, Bayer and Flamsteed Designations, and the Henry Draper Catalogue, for example.

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