2020A&A...642A.146B


Query : 2020A&A...642A.146B

2020A&A...642A.146B - Astronomy and Astrophysics, volume 642A146-146 (2020/10-1)

USuRPER: Unit-sphere representation periodogram for full spectra.

BINNENFELD A., SHAHAF S. and ZUCKER S.

Abstract (from CDS):

We introduce an extension of the periodogram concept to time-resolved spectroscopy. USuRPER, the unit-sphere representation periodogram, is a novel technique that opens new horizons in the analysis of astronomical spectra. It can be used to detect a wide range of periodic variability of the spectrum shape. Essentially, the technique is based on representing spectra as unit vectors in a multidimensional hyperspace, hence its name. It is an extension of the phase-distance correlation periodogram we had introduced in previous papers, to very high-dimensional data such as spectra. USuRPER takes the overall shape of the spectrum into account, which means that it does not need to be reduced into a single quantity such as radial velocity or temperature. Through simulations, we demonstrate its performance in various types of spectroscopic variability: single-lined and double-lined spectroscopic binary stars, and pulsating stars. We also show its performance on actual data of a rapidly oscillating Ap star. USuRPER is a new tool to explore large time-resolved spectroscopic databases such as APOGEE, LAMOST, and the RVS spectra of Gaia. We have made a public GitHub repository with a Python implementation of USuRPER available to the community, to experiment with it and apply it to a wide range of spectroscopic time series.

Abstract Copyright: © ESO 2020

Journal keyword(s): methods: data analysis - methods: statistical - techniques: spectroscopic - binaries: spectroscopic - stars: oscillations - stars: individual: HD 115226

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 HD 115226 a2* 13 18 00.0189897768 -72 57 00.947433276   8.84 8.50     ApSr(Eu) 40 0

Query : 2020A&A...642A.146B

Basic data :
HD 115226 -- alpha2 CVn Variable
Other object types:
otypes_help
* (HD,CD,...), a2* (2016AJ), NIR (2MASS)
ICRS coord. (ep=J2000) :
13 18 00.0189897768 -72 57 00.947433276 (Optical) [ 0.0145 0.0149 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
13 14 15.9248244218 -72 41 12.474864763 [ 0.0145 0.0149 90 ]
Gal coord. (ep=J2000) :
304.9060701095527 -10.1804097905492 [ 0.0145 0.0149 90 ]
Proper motions mas/yr :
-12.752 -13.825 [0.018 0.020 90] A 2020yCat.1350....0G
Parallaxes (mas):
5.4817 [0.0186] A 2020yCat.1350....0G
Spectral type:
ApSr(Eu) D 1975MSS...C01....0H
Fluxes (6) :
B 8.84 [0.02] D 2000A&A...355L..27H
V 8.50 [0.01] D 2000A&A...355L..27H
G 8.482470 [0.002772] C 2020yCat.1350....0G
J 7.943 [0.019] C 2003yCat.2246....0C
H 7.901 [0.047] C 2003yCat.2246....0C
K 7.852 [0.020] C 2003yCat.2246....0C
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Identifiers (15) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

HD 115226 GSC 09250-01687 PPM 371829 Gaia DR2 5840189258001309824
CD-72 882 HIC 64883 Renson 33300 Gaia DR3 5840189258001309824
CPC 21.2 1975 HIP 64883 TIC 394272819 Gaia DR1 5840189258001309824
CPD-72 1373 2MASS J13180002-7257009 TYC 9250-1687-1

References (40 between 1850 and 2026) (Total 40)
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

Diameter : 1    Distance : 2    Var : 1    Plx : 5    PM : 4    SpT : 2   

   


External archives :

Link by name to the catalogue in VizieR :

HD 115226 CD-72 882 CPD-72 1373 GSC 09250-01687 HIC 64883
HIP 64883 2MASS J13180002-7257009 PPM 371829 TYC 9250-1687-1 Gaia DR2 5840189258001309824
Gaia DR3 5840189258001309824 Gaia DR1 5840189258001309824

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