21 Cataclysmic variables to be observed by William Herschel Telescope

Active Dates: Dec. 14, 2016 – Dec. 16, 2016


Abstract:

Roque Ruiz-Carmona (Ph.D. candidate, Institute of Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen, The Netherlands) has requested AAVSO assistance with his campaign to observe a set of 21 cataclysmic variables (CVs) with the William Herschel Telescope (WHT) at La Palma on 2016 December 16. This campaign is essentially identical in format to the ones successfully carried out by the AAVSO on his behalf in 2015 and in May 2016.

Justification:

To investigate the hypothesis that spiral density waves can only be detectable in high inclination systems and that the luminosity of the disk in outburst outshines the spiral pattern for the rest of the system. The sample of CVs to be monitored contains only eclipsing systems.

Requested Data Types:

Photometry



Targets
Name Magnitude Variability Type Photometry Notes Spectroscopy Notes
HT Cas 12.60 UGSU+E

Cadence: Not Specified

Precision: 100

Not Requested
AY Psc 14.40 UGZ/IW+E

Cadence: Not Specified

Precision: 100

Not Requested
CSS 081220:011614+092216 16.10 UG+E

Cadence: Not Specified

Precision: 100

Not Requested
ASASSN-15nv 15.30 UG+E

Cadence: Not Specified

Precision: 100

Not Requested

Spectroscopy Lines:

No spectroscopy lines provided

Photometry Filters:

No photometry filters provided

Comparison Stars:

No comparison stars provided


Co-Authorship

Observers are not eligible for co-authorship.

Additional Observer Input:

Not provided

Additional Submission Location:

Not provided


Forum URL

N/A


Notes:

Principal Investigator: Roque Ruiz-Carmona; Imported Campaign (Alert Notice #564)