2024ApJ...976..163A


Query : 2024ApJ...976..163A

2024ApJ...976..163A - Astrophys. J., 976, 163 (2024/December-1)

Holographic Beam Measurements of the Canadian Hydrogen Intensity Mapping Experiment (CHIME).

AMIRI M., CHAKRABORTY A., FOREMAN S., HALPERN M., HILL A.S., HINSHAW G., LANDECKER T.L., MacEACHERN J., MASUI K.W., MENA-PARRA J., MILUTINOVIC N., NEWBURGH L., ORDOG A., PEN U.-L., PINSONNEAULT-MAROTTE T., REDA A., SIEGEL S.R., SINGH S., WANG H., WULF D. (The CHIME Collaboration)

Abstract (from CDS):

We present the first results of the holographic beam-mapping program for the Canadian Hydrogen Intensity Mapping Experiment (CHIME). We describe the implementation of a holographic technique as adapted for CHIME, and introduce the processing pipeline which prepares the raw holographic timestreams for analysis of beam features. We use data from six bright sources across the full 400-800 MHz observing band of CHIME to provide measurements of the copolar and cross-polar beam response in both amplitude and phase for all 1024 dual-polarized feeds in the array. In addition, we present comparisons with independent probes of the CHIME beam, which indicate the presence of polarized beam leakage. Holographic measurements of the beam have already been applied in science with CHIME, e.g., in estimating the detection significance of far-sidelobe fast radio bursts, and in validating the beam models used for CHIME's first detections of 21 cm emission (in cross-correlation with measurements of large-scale structure from galaxy surveys and the Lyα forest). Measurements presented in this paper, and future holographic results, will provide a unique data set to characterize the CHIME beam and improve the experiment's prospects for a detection of the baryon acoustic oscillation signal.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Holographic interferometry - Calibration

Simbad objects: 24

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Number of rows : 24
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 3C 10C Rad 00 25 16.44 +64 06 40.2           ~ 2 1
2 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
3 SNR G130.7+03.1 SNR 02 05 35.73 +64 49 41.3           ~ 661 4
4 NGC 1218 Sy1 03 08 26.22380005 +04 06 39.3007808   12.84       ~ 413 0
5 NGC 1275 Bla 03 19 48.1599902040 +41 30 42.108850836   13.10 12.48 11.09   ~ 4243 3
6 3C 111 Sy1 04 18 21.2772425736 +38 01 35.801359968   19.75 18.05     ~ 1002 2
7 NAME Per B SyG 04 37 04.37535450 +29 40 13.8179631   21.7       ~ 533 2
8 ICRF J052109.8+163822 Sy1 05 21 09.88596258 +16 38 22.0515459   19.37 18.84 18.480   ~ 910 1
9 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
10 ICRF J054236.1+495107 Sy1 05 42 36.13789710 +49 51 07.2337139   18.45 17.80 17.210   ~ 1573 1
11 2C 553 QSO 06 27 10.125 -05 53 06.21           ~ 165 1
12 3C 196 Sy1 08 13 36.0561170112 +48 13 02.644966020   18.36 17.79     ~ 578 2
13 MCG-02-24-007 LIN 09 18 05.66848602 -12 05 43.8060823   14.38 14.8     ~ 1077 1
14 3C 273 BLL 12 29 06.6998257176 +02 03 08.597629980   13.05 14.830 14.11   ~ 6022 1
15 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
16 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
17 3C 295 Sy1 14 11 20.6 +52 12 09   22.34 20.80 18.54   ~ 1021 4
18 MCG+01-43-006 SyG 16 51 07.9886687784 +04 59 35.547131472     18.25     ~ 502 1
19 4C -00.67 Sy2 17 20 28.1680537512 -00 58 46.582453920   15.36       ~ 345 1
20 NAME Kepler's SN SNR 17 30 40.51 -21 29 14.4           ~ 851 3
21 MCG+07-41-003 Bla 19 59 28.35656837 +40 44 02.0972325   16.22 15.10     ~ 2537 2
22 3C 409 Rad 20 14 27.597 +23 34 52.94           ~ 96 1
23 3C 454.3 Bla 22 53 57.7480438728 +16 08 53.561508864   16.57 16.10 15.22   ~ 3004 2
24 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1

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