2025A&A...701A.266A


Query : 2025A&A...701A.266A

2025A&A...701A.266A - Astronomy and Astrophysics, volume 701A266 (2025/9-1)

ARVE: Analyzing Radial Velocity Elements I. The Code.

AL MOULLA K.

Abstract (from CDS):

Context. To overcome the radial velocity (RV) precision barrier imposed by stellar variability, there has been a recent surge of software aimed at simulating and modeling different aspects of these activity patterns, which currently limit the feasibility of detecting Earth-like exoplanets.
Aims. We present Analyzing Radial Velocity Elements (ARVE), a Python-based software which enables RV extraction using various customizable techniques, along with a subsequent analysis of the stellar and planetary signals present in the RVs. One of ARVE's unique features is its library of pre-computed auxiliary data, which includes synthetic spectra and spectral line masks that enable the code to efficiently perform certain routines with minimal input from the user.
Methods. ARVE is a class-based and modular code in which its functionalities are divided between four subclasses: functions, which handles general functions utilized by the other subclasses; data, which reads the input data, loads the auxiliary data, and extracts RVs from input high-resolution spectra; star, which characterizes the stellar activity components present in the RV time series; and planets, which performs fits of Keplerian signals in the data and offers injection-recovery tests of fictitious planets to determine the detection limits.
Results. We performed a demonstration of ARVE on three years of HARPS-N solar data. We investigated the evolution of granulation and supergranulation characteristic timescales with activity level. Additionally, we revealed the differences in planetary period-mass detection limits when extracting RVs with different methods.
Conclusions. As stellar activity mitigation techniques grow more diverse, we foresee that a tool such as ARVE could greatly benefit the community by offering a user-friendly and multi-functional approach to extracting and analyzing RV time series. With its current code structure, it is feasible to expand its functionality and increase compatibility by adding more spectrographs to future versions of ARVE.

Abstract Copyright: © The Authors 2025

Journal keyword(s): methods: numerical - techniques: radial velocities - techniques: spectroscopic - stars: activity

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 166620 PM* 18 09 37.4162111401 +38 27 27.998016381 7.86 7.27 6.40 5.63 5.14 K2V 481 0

Query : 2025A&A...701A.266A

Basic data :
HD 166620 -- High Proper Motion Star
Other object types:
otypes_help
* (2013A&A,AG,...), PM* (2007A&A,LHS,...), ** (**,WDS), MIR (AKARI,WISEA), Ro* (1996ApJ), V* (NSV), NIR (2MASS), IR (IRAS)
ICRS coord. (ep=J2000) :
18 09 37.4162111401 +38 27 27.998016381 (Optical) [ 0.0128 0.0153 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
18 07 58.0068993423 +38 27 12.872500239 [ 0.0128 0.0153 90 ]
Gal coord. (ep=J2000) :
065.3335484601812 +24.2074652985711 [ 0.0128 0.0153 90 ]
Proper motions mas/yr :
-316.454 -468.348 [0.018 0.020 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) -19.315 [0.0015] / z(spectroscopic) -0.000064 [0.000000] / cz -19.31 [0.00]
   (Opt) A 2018A&A...616A...7S
Parallaxes (mas):
90.1234 [0.0156] A 2020yCat.1350....0G
Spectral type:
K2V C 2003AJ....126.2048G
Fluxes (9) :
U 7.86 [~] C 2002yCat.2237....0D
B 7.27 [~] C 2002yCat.2237....0D
V 6.40 [~] C 2002yCat.2237....0D
R 5.63 [~] C 2002yCat.2237....0D
G 6.129808 [0.002762] C 2020yCat.1350....0G
I 5.14 [~] C 2002yCat.2237....0D
J 4.78 [~] C 2002yCat.2237....0D
H 4.27 [~] C 2002yCat.2237....0D
K 4.232 [0.021] C 2003yCat.2246....0C
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Identifiers (44) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

LHS 3363 GEN# +1.00166620 LSPM J1809+3827 TIC 75946144
** LUH 13A G 205-5 LTT 15374 TYC 3102-1975-1
AG+38 1655 GJ 706 2MASS J18093745+3827288 UBV 15461
AKARI-IRC-V1 J1809372+382725 HD 166620 NLTT 46046 UBV M 22712
ASCC 505680 HIC 88972 NSV 10316 USNO-B1.0 1284-00305405
BD+38 3095 HIP 88972 PLX 4171 uvby98 100166620
Ci 20 1078 HR 6806 PLX 4171.00 WDS J18096+3827A
Ci 18 2403 IRAS 18079+3826 PPM 81007 WEB 15090
CNS5 4496 JP11 2944 SAO 66700 WISEA J180937.13+382723.0
GC 24778 LAL 33439 SKY# 33024 Gaia DR3 4610177733290768896
GCRV 10624 LFT 1396 SPOCS 784 Gaia DR2 4610177733290768896

References (481 between 1850 and 2026) (Total 481)
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 : 15    Distance : 2    Var : 1    Rot : 12    Fe/H : 52    Plx : 5    PM : 13    SpT : 20   

   

Observing logs
Herschel : 4    ISO : 9    IUE : 4   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : HD 166620

Link by name to the catalogue in VizieR :

LHS 3363 AG+38 1655 AKARI-IRC-V1 J1809372+382725 BD+38 3095 G 205-5
GJ 706 HD 166620 HIC 88972 HIP 88972 HR 6806
IRAS 18079+3826 LSPM J1809+3827 2MASS J18093745+3827288 NLTT 46046 NSV 10316
PLX 4171 PPM 81007 SAO 66700 TYC 3102-1975-1 USNO-B1.0 1284-00305405
uvby98 100166620 WDS J18096+3827A WISEA J180937.13+382723.0 Gaia DR3 4610177733290768896 Gaia DR2 4610177733290768896

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