2024A&A...687A.302F


Query : 2024A&A...687A.302F

2024A&A...687A.302F - Astronomy and Astrophysics, volume 687A302 (2024/7-1)

CHEOPS in-flight performance A comprehensive look at the first 3.5 yr of operations.

FORTIER A., SIMON A.E., BROEG C., OLOFSSON G., DELINE A., WILSON T.G., MAXTED P.F.L., BRANDEKER A., COLLIER CAMERON A., BECK M., BEKKELIEN A., BILLOT N., BONFANTI A., BRUNO G., CABRERA J., DELREZ L., DEMORY B.-O., FUTYAN D., FLOREN H.-G., GUNTHER M.N., HEITZMANN A., HOYER S., ISAAK K.G., SOUSA S.G., STALPORT M., TURIN A., VERHOEVE P., AKINSANMI B., ALIBERT Y., ALONSO R., BANHIDI D., BARCZY T., BARRADO D., BARROS S.C.C., BAUMJOHANN W., BAYCROFT T., BECK T., BENZ W., BIRO B.I., BODI A., BONFILS X., BORSATO L., CHARNOZ S., CSEH B., CSIZMADIA S., CSANYI I., CUBILLOS P.E., DAVIES M.B., DAVIS Y.T., DELEUIL M., DEMANGEON O.D.S., DEREKAS A., DRANSFIELD G., DUCROT E., EHRENREICH D., ERIKSON A., FARINA C., FOSSATI L., FRIDLUND M., GANDOLFI D., GARAI Z., GARCIA L., GILLON M., GOMEZ MAQUEO CHEW Y., GOMEZ-MUNOZ M.A., GRANATA V., GUDEL M., GUTERMAN P., HEGEDUS T., HELLING C., JEHIN E., KALUP C., KILKENNY D., KISS L.L., KRISKOVICS L., LAM K.W.F., LASKAR J., LECAVELIER DES ETANGS A., LENDL M., LOPEZ PINA A., LUNTZER A., MAGRIN D., MILLER N.J., MODREGO CONTRERAS D., MORDASINI C., MUNARI M., MURRAY C.A., NASCIMBENI V., OTTACHER H., OTTENSAMER R., PAGANO I., PAL A., PALLE E., PASETTI A., PEDERSEN P.P., PETER G., PETRUCCI R., PIOTTO G., PIZARRO-RUBIO A., POLLACCO D., PRIBULLA T., QUELOZ D., RAGAZZONI R., RANDO N., RAUER H., RIBAS I., SABIN L., SANTOS N.C., SCANDARIATO G., SCHANCHE N., SCHROFFENEGGER U., SCUTT O.J., SEBASTIAN D., SEGRANSAN D., SELI B., SMITH A.M.S., SOUTHWORTH R., STANDING M.R., SZABO G.M., SZAKATS R., THOMAS N., TIMMERMANS M., TRIAUD A.H.M.J., UDRY S., VAN GROOTEL V., VENTURINI J., VILLAVER E., VINKO J., WALTON N.A., WELLS R. and WOLTER D.

Abstract (from CDS):

Context. Since the discovery of the first exoplanet almost three decades ago, the number of known exoplanets has increased dramatically. By beginning of the 2000s it was clear that dedicated facilities to advance our studies in this field were needed. The CHaracterising ExOPlanet Satellite (CHEOPS) is a space telescope specifically designed to monitor transiting exoplanets orbiting bright stars. In September 2023, CHEOPS completed its nominal mission duration of 3.5 yr and remains in excellent operational conditions. As a testament to this, the mission has been extended until the end of 2026.
Aims. Scientific and instrumental data have been collected throughout in-orbit commissioning and nominal operations, enabling a comprehensive analysis of the mission's performance. In this article, we present the results of this analysis with a twofold goal. First, we aim to inform the scientific community about the present status of the mission and what can be expected as the instrument ages. Secondly, we intend for this publication to serve as a legacy document for future missions, providing insights and lessons learned from the successful operation of CHEOPS.
Methods. To evaluate the instrument performance in flight, we developed a comprehensive monitoring and characterisation (M&C) programme. It consists of dedicated observations that allow us to characterise the instrument's response and continuously monitor its behaviour. In addition to the standard collection of nominal science and housekeeping data, these observations provide valuable input for detecting, modelling, and correcting instrument systematics, discovering and addressing anomalies, and comparing the instrument's actual performance with expectations.
Results. The precision of the CHEOPS measurements has enabled the mission objectives to be met and exceeded. The satellite's performance remains stable and reliable, ensuring accurate data collection throughout its operational life. Careful modelling of the instrumental systematics allows the data quality to be significantly improved during the light curve analysis phase, resulting in more precise scientific measurements.
Conclusions. CHEOPS is compliant with the driving scientific requirements of the mission. Although visible, the ageing of the instrument has not affected the mission's performance. The satellite's capabilities remain robust, and we are confident that we will continue to acquire high-quality data during the mission extension.

Abstract Copyright: © The Authors 2024

Journal keyword(s): space vehicles: instruments - techniques: photometric - telescopes - planets and satellites: detection - planets and satellites: terrestrial planets

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 31

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Number of rows : 31
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 WT 2353 PM* 00 29 12.3029193648 -30 27 13.466857032   13.05 11.95     ~ 102 0
2 WASP-12b Pl 06 30 32.7966092352 +29 40 20.263502460           ~ 847 1
3 WASP-12 * 06 30 32.7966092352 +29 40 20.263502460   12.14 11.57     G0V 358 1
4 * 53 Cnc LP? 08 52 28.5899126304 +28 15 32.968291068 9.35 7.85 6.23     M3III 61 0
5 * rho01 Cnc e Pl 08 52 35.8111044043 +28 19 50.954994470           ~ 682 1
6 * rho01 Cnc PM* 08 52 35.8111044043 +28 19 50.954994470 7.45 6.82   5.4   K0IV-V 1223 1
7 StKM 1-805 Em* 09 52 53.0238196464 +31 17 32.582691204   13.30 11.878 11.465   M0 10 0
8 HD 88111 PM* 10 09 07.6204989384 -25 47 50.697956256   9.96 9.18     G8/K0V 8 0
9 HD 88742 PM* 10 13 24.7290968722 -33 01 54.194829479 7.06 6.97 6.38     G0V 167 0
10 NGC 3201 GlC 10 17 36.82 -46 24 44.9           ~ 1001 0
11 TYC 5502-1037-1 PM* 10 44 47.3117501400 -12 27 18.847956276   13.35 11.92     ~ 5 0
12 HD 108236 PM* 12 26 17.8919204184 -51 21 46.215656244   9.89 9.24     G5V 62 0
13 HD 110067 PM* 12 39 21.5036859792 +20 01 40.035976644   9.22 8.43     K0V 54 0
14 BD-07 3477 HS* 12 44 20.2386233232 -08 40 16.846099536   10.46 10.594 10.895   sdB2VIIHe3 303 1
15 * 61 Vir PM* 13 18 24.3139864471 -18 18 40.297748582 5.710 5.440 4.740     G6.5V 742 1
16 Ross 1020 PM* 13 22 56.7475808912 +24 28 03.598852682   14.55   12.577   M4V 98 0
17 HD 122303 PM* 14 01 03.1882316643 -02 39 17.519814662 12.343 11.177 9.707 8.745 7.66 M0V 204 0
18 HD 125612 PM* 14 20 53.5176649416 -17 28 53.489705520   8.93 8.32     G3V 147 1
19 HD 133112b Pl 15 02 44.8678907928 -03 01 52.986571896           ~ 144 0
20 HD 133112 PM* 15 02 44.8678907928 -03 01 52.986571896   6.788 6.618     A4/5IV/V 86 0
21 BD-07 4003 BY* 15 19 26.8269387505 -07 43 20.189497466 13.403 11.76 10.560 9.461 8.911 M3V 717 2
22 * nu.02 Lup d Pl 15 21 48.1499105161 -48 19 03.469906910           ~ 24 1
23 HD 146389 PM* 16 15 50.3653280520 +10 01 57.284258556   9.866 9.39 9.22   F8 70 1
24 BD-12 4523 BY* 16 30 18.0583947383 -12 39 45.321217732 12.829 11.638 10.072 8.917 7.421 M3V 365 0
25 WASP-103b Pl 16 37 15.5765824488 +07 11 00.109678740           ~ 215 1
26 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
27 HD 175986 ** 19 03 29.6331376968 -68 45 20.091805452   6.422 5.861     G0IV 50 0
28 HD 181433 PM* 19 25 09.5666936172 -66 28 07.676956827   9.42 8.38     K3III-IV 144 1
29 HD 190360 PM* 20 03 37.4050868074 +29 53 48.492435887   6.44   5.2   G7IV-V 490 1
30 HD 215152 PM* 22 43 21.3028100652 -06 24 02.953048623   9.12 8.13 7.83 8.46 K3V 141 1
31 V* BR Psc BY* 23 49 12.5250852078 +02 24 04.405476893 11.532 10.427 8.993 8.029 6.946 dM1 370 0

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