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Variable stars

Tracking T CrB

by OBSN · 26 Mar 2024
Objectives

Perform the most precise photometry possible

Methodology

We will attempt to perform the most precise photometry possible using FotoDif (the classic version, not FotoDifSN) and the comparison stars proposed below. We must use all three comparison stars . - Tycho can also be used. - Multiband photometry is appreciated; it has a very different behavior in B and V. - Look, it's a bright star. Be careful not to oversaturate it; a slight blur might help. - We recommend reading the tutorial on how to perform good photometry, which we have on this same website . Right now T CrB is still an object for the end of the night, although from 2 a.m. onwards it already has a decent height. Thank you for your measurements!

Target objects
T Crb RA 15h 59m 30.2   Dec +25° 55′ 13″
Campaign data 1,538 observations
Contributors 34 observers
N
NISL external
796 obs
M
MJOD external
262 obs
B
BCAH external
118 obs
E
ERE external
72 obs
R
RMU external
52 obs
N
NRNA external
31 obs
V
VALF external
29 obs
M
MMAO external
28 obs
G
GFDB external
26 obs
L
LFEA external
25 obs
G
GPF external
16 obs
F
FESA external
10 obs
S
SJGA external
10 obs
R
RJUD external
7 obs
C
CANE external
6 obs
F
FRGA external
6 obs
B
BJOK external
5 obs
G
GALF external
5 obs
A
AANF external
5 obs
L
LCR external
4 obs
E
EALA external
3 obs
M
MAND external
3 obs
T
TJOB external
3 obs
H
HJLA external
3 obs
J
JCB external
2 obs
A
ATE external
2 obs
C
CMAW external
2 obs
T
TCRB external
1 obs
J
Josep
1 obs
P
Pep
1 obs
P
Pep
1 obs
C
CFEC external
1 obs
F
FERC external
1 obs
A
ACL external
1 obs
Tracking T CrB Light curve