2023A&A...678A..72D


Query : 2023A&A...678A..72D

2023A&A...678A..72D - Astronomy and Astrophysics, volume 678A72 (2023/10-1)

Metrewave Galactic Plane with the uGMRT (MeGaPluG) Survey: Lessons from the pilot study.

DOKARA R., ROY N., MENTEN K., VIG S., DUTTA P., BEUTHER H., PANDIAN J.D., RUGEL M., RASHID M. and BRUNTHALER A.

Abstract (from CDS):

Context. The advent of wide-band receiver systems on interferometer arrays has enabled the undertaking of high-sensitivity and highresolution radio continuum surveys of the Galactic plane in a reasonable amount of telescope time. Yet, to date, there have been only a few such studies of the first quadrant of the Milky Way carried out at frequencies below 1 GHz. The Giant Metrewave Radio Telescope (GMRT) has recently upgraded its receivers with wide-band capabilities (now called the uGMRT), offering a prime opportunity to conduct high resolution surveys, while also demonstrating sensitivity to the extended structures.
Aims. We wish to assess the feasibility of conducting a large-scale snapshot survey, the Metrewave Galactic Plane with the uGMRT Survey (MeGaPluG), to simultaneously map extended sources and compact objects at an angular resolution lower than 10″ and a point source sensitivity of 0.15 mJy beam–1.
Methods. We performed an unbiased survey of a small portion of the Galactic plane, covering the W43/W44 regions (l = 29° - 35° and |b| < 1°) in two frequency bands: 300-500 MHz and 550-750 MHz. The 200 MHz wide-band receivers on the uGMRT were employed to observe the target field in several pointings, spending nearly 14 min on each pointing in two separate scans. We developed an automated pipeline for the calibration and a semi-automated self-calibration procedure was used to image each pointing using multi-scale CLEAN and outlier fields.
Results. We produced continuum mosaics of the surveyed region at a final common resolution of 25″ in the two bands that have central frequencies of 400 MHz and 650 MHz, with a point source sensitivity better than 5 mJy beam–1. A spectral index map was also obtained, which is helpful to distinguish between thermal and nonthermal emission. By cross-matching with other surveys, we validated the positions and flux densities obtained from our data. We plan to cover a larger footprint of the Galactic plane in the near future based on the lessons drawn from this study.

Abstract Copyright: © The Authors 2023

Journal keyword(s): surveys - radio continuum: ISM - ISM: supernova remnants - HII regions - Galaxy: general - local insterstellar matter

VizieR on-line data: <Available at CDS (J/A+A/678/A72): list.dat fits/*>

Simbad objects: 16

goto Full paper

goto View the references in ADS

Number of rows : 16
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 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
2 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
3 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
4 SNR G029.6+00.1 SNR 18 44 52 -02 56.5           ~ 61 1
5 SNR G029.7-00.3 SNR 18 46 22.8 -02 59 47           ~ 375 2
6 W 43 SFR 18 47 32 -01 56.5           ~ 604 0
7 GLOSTAR G031.256-00.041 SR? 18 48 31.6 -01 30 37           ~ 4 0
8 SNR G031.9+00.0 SNR 18 49 16.3 -00 55 01           ~ 368 2
9 SNR G032.22-00.21 SR? 18 50 53 -00 43.8           ~ 6 0
10 TGSSADR J185141.6+003739 Rad 18 51 41.68 +00 37 39.4           ~ 1 0
11 QSO J1851+005 QSO 18 51 46.72295 +00 35 32.3649           ~ 138 1
12 TGSSADR J185146.7+003531 Rad 18 51 46.75 +00 35 31.6           ~ 1 0
13 SNR G032.8-00.1 SNR 18 51 46.9 -00 03 19           ~ 110 2
14 SNR G033.6+00.1 SNR 18 52 29.000 +00 38 42.00           ~ 302 2
15 SNR G033.2-00.6 gam 18 53 41.1 -00 02 20           ~ 56 1
16 SNR G034.6-00.5 SNR 18 56 10.650 +01 13 21.30           ~ 1034 2

To bookmark this query, right click on this link: simbad:objects in 2023A&A...678A..72D and select 'bookmark this link' or equivalent in the popup menu