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dc.contributor.authorMEDINA, S.-N.X
dc.contributor.authorDZIB, S.A
dc.contributor.authorURQUHART, J.S
dc.contributor.authorYANG, A.Y
dc.contributor.authorBRUNTHALER, A
dc.contributor.authorMENTEN, K.M
dc.contributor.authorWYROWSKI, F
dc.contributor.authorCOTTON, W.D
dc.contributor.authorCHEEMA, A
dc.contributor.authorDOKARA, R
dc.contributor.authorGONG, Y
dc.contributor.authorKHAN, S
dc.contributor.authorNGUYEN, H
dc.contributor.authorORTIZ-LEON, G.N
dc.contributor.authorRUGEL, M.R
dc.contributor.authorVEENA, V.S
dc.contributor.authorBEUTHER, H
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorCSENGERI, T
dc.contributor.authorPANDIAN, J.D
dc.contributor.authorROY, N
dc.date.issued2024
dc.description.abstractEnThe GLOSTAR survey studies star formation with the VLA and the Effelsberg 100m telescope in the Galactic plane (-2d<l<60d; |b|<1d) and the Cygnus X region with unprecedented sensitivity in both flux density (~50uJy/beam) and the capability of detecting emission with angular scales in the range from 1" to the largest radio structures in the Galaxy. We provide a complete GLOSTAR-VLA D-configuration radio source catalog for the covered part of the Galactic disk. A catalog for the pilot region (28d<l<36d) has been published in a previous paper and here we present the complementary catalog for the area within 2d<l<28d, 36d<l<60d and |b|<1d. Observations were taken with the VLA in a 4-8GHz band to image 100 degrees$^2$ of the inner Galactic disk at a reference frequency of 5.8GHz, using 260h of telescope time. We determined spectral indices inside the observed band and in the frequency range 1.4-5.8GHz by complementing our results with those from the THOR survey (1-2GHz). The final images have an angular resolution of 18" and an average sensitivity of 123uJy/beam. The sensitivity is better (~60uJy/beam) in areas free of extended emission. The Galactic disk catalog presented in this work, consists of 11211 radio sources. Of these, 1965 are known large-scale structure sources such as star-forming region complexes, well-known SNRs, SNR candidates or parts thereof. The remaining 9227 are discrete individual sources. Source parameters, namely flux densities, sizes, spectral indices, and classifications are reported. We identify 769 HII region candidates, 359 are newly classified as such. The mean value of spectral indices of 225 HII regions is 0.14$\pm$0.02, consistent with most of them emitting optically thin thermal radio emission. Combining our results with the previously published catalog of the pilot region, the final GLOSTAR-VLA D-configuration catalog contains 12981 radio sources.
dc.language.isoen
dc.title.enA global view on star formation: The GLOSTAR Galactic plane survey. XI. Radio source catalog IV: $2^\circ < \ell < 28^\circ$, $36^\circ < \ell < 60^\circ$ and $|b| < 1^\circ$
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/202449885
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv2407.12585
bordeaux.journalAstron.Astrophys
bordeaux.pageA196
bordeaux.volume689
bordeaux.peerReviewedoui
hal.identifierhal-04662756
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-04662756v1
bordeaux.COinSctx_ver=Z39.88-2004&amp;rft_val_fmt=info:ofi/fmt:kev:mtx:journal&amp;rft.jtitle=Astron.Astrophys&amp;rft.date=2024&amp;rft.volume=689&amp;rft.spage=A196&amp;rft.epage=A196&amp;rft.au=MEDINA,%20S.-N.X&amp;DZIB,%20S.A&amp;URQUHART,%20J.S&amp;YANG,%20A.Y&amp;BRUNTHALER,%20A&amp;rft.genre=article


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