2016MNRAS.457..542B


Query : 2016MNRAS.457..542B

2016MNRAS.457..542B - Mon. Not. R. Astron. Soc., 457, 542-574 (2016/March-3)

Difference image analysis: automatic kernel design using information criteria.

BRAMICH D.M., HORNE K., ALSUBAI K.A., BACHELET E., MISLIS D. and PARLEY N.

Abstract (from CDS):

We present a selection of methods for automatically constructing an optimal kernel model for difference image analysis which require very few external parameters to control the kernel design. Each method consists of two components; namely, a kernel design algorithm to generate a set of candidate kernel models, and a model selection criterion to select the simplest kernel model from the candidate models that provides a sufficiently good fit to the target image. We restricted our attention to the case of solving for a spatially invariant convolution kernel composed of delta basis functions, and we considered 19 different kernel solution methods including six employing kernel regularization. We tested these kernel solution methods by performing a comprehensive set of image simulations and investigating how their performance in terms of model error, fit quality, and photometric accuracy depends on the properties of the reference and target images. We find that the irregular kernel design algorithm employing unregularized delta basis functions, combined with either the Akaike or Takeuchi information criterion, is the best kernel solution method in terms of photometric accuracy. Our results are validated by tests performed on two independent sets of real data. Finally, we provide some important recommendations for software implementations of difference image analysis.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: data analysis - methods: statistical - techniques: image processing - techniques: photometric

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 7789 OpC 23 57 19.4 +56 43 28   7.68 6.7     ~ 575 0

Query : 2016MNRAS.457..542B

Basic data :
NGC 7789 -- Open Cluster
Other object types:
otypes_help
OpC (2013A&A,OCl), Cl* (2020A&A,C,...)
ICRS coord. (ep=J2000) :
23 57 19.4 +56 43 28 (Optical) [ ] E 2023A&A...674A..37G
FK4 coord. (ep=B1950 eq=1950) :
23 54 47.4 +56 26 46 [ ]
Gal coord. (ep=J2000) :
115.5250 -05.3671 [ ]
Proper motions mas/yr :
-0.922 -1.933 [0.003 0.003 90] C 2020A&A...633A..99C
Radial velocity / Redshift / cz :
V(km/s) -54.91 [0.12] / z(spectroscopic) -0.000183 [0.000000] / cz -54.90 [0.12]
   (Opt) A 2021A&A...647A..19T
Parallaxes (mas):
0.453 [0.001] C 2020A&A...633A..99C
Angular size (arcmin):
25.3 25.3 0 (Opt) D 2020A&A...633A..99C
Fluxes (2) :
B 7.68 [~] E ~
V 6.7 [~] E ~
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Hierarchy : number of linked objects
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: 4811
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Identifiers (6) :
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NGC 7789 Cl Melotte 245 [KPR2004b] 518
C 2354+564 OCl 269.0 [KPS2012] MWSC 3779

References (575 between 1850 and 2026) (Total 575)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 12    Distance : 9    Fe/H : 17    Plx : 8    PM : 13   

   


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Data at NED - NASA/IPAC Extragalactic Database : NGC 7789

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NGC 7789

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