2022PASP..134k4509C


Query : 2022PASP..134k4509C

2022PASP..134k4509C - Publ. Astron. Soc. Pac., 134, part no 11, 4509 (2022/November-1041)

APERO: A PipelinE to Reduce Observations-Demonstration with SPIRou.

COOK N.J., ARTIGAU E., DOYON R., HOBSON M., MARTIOLI E., BOUCHY F., MOUTOU C., CARMONA A., USHER C., FOUQUE P., ARNOLD L., DELFOSSE X., BOISSE I., CADIEUX C., VANDAL T., DONATI J.-F. and DESLIERES A.

Abstract (from CDS):

With the maturation of near-infrared high-resolution spectroscopy, especially when used for precision radial velocity, data reduction has faced unprecedented challenges in terms of how one goes from raw data to calibrated, extracted, and corrected data with required precisions of thousandths of a pixel. Here we present A PipelinE to Reduce Observations (APERO), specifically focused on Spectro Polarimètre Infra ROUge (SPIROU), the near-infrared spectropolarimeter on the Canada-France-Hawaii Telescope (SPectropolarimètre InfraROUge, CFHT). In this paper, we give an overview of APERO and detail the reduction procedure for SPIROU. APERO delivers telluric-corrected 2D and 1D spectra as well as polarimetry products. APERO enables precise stable radial velocity measurements on the sky (via the LBL algorithm), which is good to at least ∼2 m s–1 over the current 5 yr lifetime of SPIROU.

Abstract Copyright: © 2022. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved

Journal keyword(s): Astronomy data reduction - Spectropolarimetry - Radial velocity - Spectroscopy - Calibration - Near infrared astronomy

Simbad objects: 21

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Number of rows : 21
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 PM J01276+7217 PM* 01 27 40.9728637224 +72 17 47.186355408     12.989 12.687   ~ 24 0
2 HD 36395 PM* 05 31 27.3957852161 -03 40 38.024004501 10.626 9.443 7.968 6.996 5.913 M1.5Ve 574 0
3 TOI-530b Pl 06 53 39.0655003863 +12 52 54.652087949           ~ 17 0
4 HD 265866 PM* 06 54 48.9580633365 +33 16 05.438282419   11.47   9.650   M3V 277 0
5 V* AD Leo PM* 10 19 36.2808181226 +19 52 12.010446571   10.82 9.52 9.19   dM3 1469 1
6 BD-03 2978b Pl 10 42 14.0836906368 -03 50 06.260144388           ~ 150 0
7 * tau Boo b Pl 13 47 15.7381720026 +17 27 24.809555600           ~ 312 1
8 CD-24 12689 Or* 16 27 40.2857881416 -24 22 04.130226300   12.91 11.533 11.11 10.00 K5e 301 0
9 NAME Barnard's star BY* 17 57 48.4984700685 +04 41 36.113879676 12.497 11.24 9.511 8.298 6.741 M4V 907 2
10 HD 173740 PM* 18 42 46.8946714770 +59 37 36.721161413   11.32 9.78     M3.5V 381 1
11 LSPM J1844+3633 PM* 18 44 42.3658884696 +36 33 44.530295652   15.1   13.4   ~ 28 0
12 TOI-1452b Pl 19 20 41.7258970920 +73 11 43.537714476           ~ 27 0
13 HD 189733 BY* 20 00 43.7129433648 +22 42 39.073143456 9.241 8.578 7.648 7.126 6.68 K2V 991 1
14 HD 189733b Pl 20 00 43.7129433648 +22 42 39.073143456           ~ 1610 1
15 HD 197481 BY* 20 45 09.5324974119 -31 20 27.237889841   10.05 8.627 9.078 6.593 M1VeBa1 1344 0
16 * gam Equ a2* 21 10 20.5000721160 +10 07 53.691967776 5.03 4.94 4.68 4.43 4.32 A9VpSrCrEu 564 0
17 TOI-1278b BD? 21 21 54.9403734715 +35 38 55.777318896           ~ 23 0
18 LSPM J2147+6245b Pl 21 47 24.7901788584 +62 45 13.903846920           ~ 26 0
19 HD 209290 PM* 22 02 10.2750978279 +01 24 00.832158070 11.838 10.616 9.146 8.213 7.245 M0.5V 285 0
20 TRAPPIST-1 LM* 23 06 29.3684948589 -05 02 29.037301866     18.798 16.466 14.024 M7.5e 1306 0
21 Ross 248 BY* 23 41 55.0363002516 +44 10 38.818911116   14.19   11.1   M5.0V 361 0

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