A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55
We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies...
Ausführliche Beschreibung
Autor*in: |
M. McNanna [verfasserIn] K. Bechtol [verfasserIn] S. Mau [verfasserIn] E. O. Nadler [verfasserIn] J. Medoff [verfasserIn] A. Drlica-Wagner [verfasserIn] W. Cerny [verfasserIn] D. Crnojević [verfasserIn] B. Mutlu-Pakdıl [verfasserIn] A. K. Vivas [verfasserIn] A. B. Pace [verfasserIn] J. L. Carlin [verfasserIn] M. L. M. Collins [verfasserIn] P. S. Ferguson [verfasserIn] D. Martínez-Delgado [verfasserIn] C. E. Martínez-Vázquez [verfasserIn] N. E. D. Noel [verfasserIn] A. H. Riley [verfasserIn] D. J. Sand [verfasserIn] A. Smercina [verfasserIn] E. Tollerud [verfasserIn] R. H. Wechsler [verfasserIn] T. M. C. Abbott [verfasserIn] M. Aguena [verfasserIn] O. Alves [verfasserIn] D. Bacon [verfasserIn] C. R. Bom [verfasserIn] D. Brooks [verfasserIn] D. L. Burke [verfasserIn] J. A. Carballo-Bello [verfasserIn] A. Carnero Rosell [verfasserIn] J. Carretero [verfasserIn] L. N. da Costa [verfasserIn] T. M. Davis [verfasserIn] J. De Vicente [verfasserIn] H. T. Diehl [verfasserIn] P. Doel [verfasserIn] I. Ferrero [verfasserIn] J. Frieman [verfasserIn] G. Giannini [verfasserIn] D. Gruen [verfasserIn] G. Gutierrez [verfasserIn] R. A. Gruendl [verfasserIn] S. R. Hinton [verfasserIn] D. L. Hollowood [verfasserIn] K. Honscheid [verfasserIn] D. J. James [verfasserIn] K. Kuehn [verfasserIn] J. L. Marshall [verfasserIn] J. Mena-Fernández [verfasserIn] R. Miquel [verfasserIn] M. E. S. Pereira [verfasserIn] A. Pieres [verfasserIn] A. A. Plazas Malagón [verfasserIn] J. D. Sakowska [verfasserIn] E. Sanchez [verfasserIn] D. Sanchez Cid [verfasserIn] B. Santiago [verfasserIn] I. Sevilla-Noarbe [verfasserIn] M. Smith [verfasserIn] G. S. Stringfellow [verfasserIn] E. Suchyta [verfasserIn] M. E. C. Swanson [verfasserIn] G. Tarle [verfasserIn] N. Weaverdyck [verfasserIn] P. Wiseman [verfasserIn] DES & DELVE Collaboration [verfasserIn] |
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E-Artikel |
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Sprache: |
Englisch |
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2024 |
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In: The Astrophysical Journal - IOP Publishing, 2022, 961(2024), 1, p 126 |
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Übergeordnetes Werk: |
volume:961 ; year:2024 ; number:1, p 126 |
Links: |
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DOI / URN: |
10.3847/1538-4357/ad07d0 |
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Katalog-ID: |
DOAJ096131888 |
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100 | 0 | |a M. McNanna |e verfasserin |4 aut | |
245 | 1 | 2 | |a A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 |
264 | 1 | |c 2024 | |
336 | |a Text |b txt |2 rdacontent | ||
337 | |a Computermedien |b c |2 rdamedia | ||
338 | |a Online-Ressource |b cr |2 rdacarrier | ||
520 | |a We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. | ||
650 | 4 | |a Local Group | |
650 | 4 | |a Low surface brightness galaxies | |
650 | 4 | |a Dwarf galaxies | |
653 | 0 | |a Astrophysics | |
700 | 0 | |a K. Bechtol |e verfasserin |4 aut | |
700 | 0 | |a S. Mau |e verfasserin |4 aut | |
700 | 0 | |a E. O. Nadler |e verfasserin |4 aut | |
700 | 0 | |a J. Medoff |e verfasserin |4 aut | |
700 | 0 | |a A. Drlica-Wagner |e verfasserin |4 aut | |
700 | 0 | |a W. Cerny |e verfasserin |4 aut | |
700 | 0 | |a D. Crnojević |e verfasserin |4 aut | |
700 | 0 | |a B. Mutlu-Pakdıl |e verfasserin |4 aut | |
700 | 0 | |a A. K. Vivas |e verfasserin |4 aut | |
700 | 0 | |a A. B. Pace |e verfasserin |4 aut | |
700 | 0 | |a J. L. Carlin |e verfasserin |4 aut | |
700 | 0 | |a M. L. M. Collins |e verfasserin |4 aut | |
700 | 0 | |a P. S. Ferguson |e verfasserin |4 aut | |
700 | 0 | |a D. Martínez-Delgado |e verfasserin |4 aut | |
700 | 0 | |a C. E. Martínez-Vázquez |e verfasserin |4 aut | |
700 | 0 | |a N. E. D. Noel |e verfasserin |4 aut | |
700 | 0 | |a A. H. Riley |e verfasserin |4 aut | |
700 | 0 | |a D. J. Sand |e verfasserin |4 aut | |
700 | 0 | |a A. Smercina |e verfasserin |4 aut | |
700 | 0 | |a E. Tollerud |e verfasserin |4 aut | |
700 | 0 | |a R. H. Wechsler |e verfasserin |4 aut | |
700 | 0 | |a T. M. C. Abbott |e verfasserin |4 aut | |
700 | 0 | |a M. Aguena |e verfasserin |4 aut | |
700 | 0 | |a O. Alves |e verfasserin |4 aut | |
700 | 0 | |a D. Bacon |e verfasserin |4 aut | |
700 | 0 | |a C. R. Bom |e verfasserin |4 aut | |
700 | 0 | |a D. Brooks |e verfasserin |4 aut | |
700 | 0 | |a D. L. Burke |e verfasserin |4 aut | |
700 | 0 | |a J. A. Carballo-Bello |e verfasserin |4 aut | |
700 | 0 | |a A. Carnero Rosell |e verfasserin |4 aut | |
700 | 0 | |a J. Carretero |e verfasserin |4 aut | |
700 | 0 | |a L. N. da Costa |e verfasserin |4 aut | |
700 | 0 | |a T. M. Davis |e verfasserin |4 aut | |
700 | 0 | |a J. De Vicente |e verfasserin |4 aut | |
700 | 0 | |a H. T. Diehl |e verfasserin |4 aut | |
700 | 0 | |a P. Doel |e verfasserin |4 aut | |
700 | 0 | |a I. Ferrero |e verfasserin |4 aut | |
700 | 0 | |a J. Frieman |e verfasserin |4 aut | |
700 | 0 | |a G. Giannini |e verfasserin |4 aut | |
700 | 0 | |a D. Gruen |e verfasserin |4 aut | |
700 | 0 | |a G. Gutierrez |e verfasserin |4 aut | |
700 | 0 | |a R. A. Gruendl |e verfasserin |4 aut | |
700 | 0 | |a S. R. Hinton |e verfasserin |4 aut | |
700 | 0 | |a D. L. Hollowood |e verfasserin |4 aut | |
700 | 0 | |a K. Honscheid |e verfasserin |4 aut | |
700 | 0 | |a D. J. James |e verfasserin |4 aut | |
700 | 0 | |a K. Kuehn |e verfasserin |4 aut | |
700 | 0 | |a J. L. Marshall |e verfasserin |4 aut | |
700 | 0 | |a J. Mena-Fernández |e verfasserin |4 aut | |
700 | 0 | |a R. Miquel |e verfasserin |4 aut | |
700 | 0 | |a M. E. S. Pereira |e verfasserin |4 aut | |
700 | 0 | |a A. Pieres |e verfasserin |4 aut | |
700 | 0 | |a A. A. Plazas Malagón |e verfasserin |4 aut | |
700 | 0 | |a J. D. Sakowska |e verfasserin |4 aut | |
700 | 0 | |a E. Sanchez |e verfasserin |4 aut | |
700 | 0 | |a D. Sanchez Cid |e verfasserin |4 aut | |
700 | 0 | |a B. Santiago |e verfasserin |4 aut | |
700 | 0 | |a I. Sevilla-Noarbe |e verfasserin |4 aut | |
700 | 0 | |a M. Smith |e verfasserin |4 aut | |
700 | 0 | |a G. S. Stringfellow |e verfasserin |4 aut | |
700 | 0 | |a E. Suchyta |e verfasserin |4 aut | |
700 | 0 | |a M. E. C. Swanson |e verfasserin |4 aut | |
700 | 0 | |a G. Tarle |e verfasserin |4 aut | |
700 | 0 | |a N. Weaverdyck |e verfasserin |4 aut | |
700 | 0 | |a P. Wiseman |e verfasserin |4 aut | |
700 | 0 | |a DES & DELVE Collaboration |e verfasserin |4 aut | |
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10.3847/1538-4357/ad07d0 doi (DE-627)DOAJ096131888 (DE-599)DOAJ6eeaf2d50e01496096fc1246608fe51f DE-627 ger DE-627 rakwb eng QB460-466 M. McNanna verfasserin aut A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. Local Group Low surface brightness galaxies Dwarf galaxies Astrophysics K. Bechtol verfasserin aut S. Mau verfasserin aut E. O. Nadler verfasserin aut J. Medoff verfasserin aut A. Drlica-Wagner verfasserin aut W. Cerny verfasserin aut D. Crnojević verfasserin aut B. Mutlu-Pakdıl verfasserin aut A. K. Vivas verfasserin aut A. B. Pace verfasserin aut J. L. Carlin verfasserin aut M. L. M. Collins verfasserin aut P. S. Ferguson verfasserin aut D. Martínez-Delgado verfasserin aut C. E. Martínez-Vázquez verfasserin aut N. E. D. Noel verfasserin aut A. H. Riley verfasserin aut D. J. Sand verfasserin aut A. Smercina verfasserin aut E. Tollerud verfasserin aut R. H. Wechsler verfasserin aut T. M. C. Abbott verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut D. Bacon verfasserin aut C. R. Bom verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut J. A. Carballo-Bello verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut L. N. da Costa verfasserin aut T. M. Davis verfasserin aut J. De Vicente verfasserin aut H. T. Diehl verfasserin aut P. Doel verfasserin aut I. Ferrero verfasserin aut J. Frieman verfasserin aut G. Giannini verfasserin aut D. Gruen verfasserin aut G. Gutierrez verfasserin aut R. A. Gruendl verfasserin aut S. R. Hinton verfasserin aut D. L. Hollowood verfasserin aut K. Honscheid verfasserin aut D. J. James verfasserin aut K. Kuehn verfasserin aut J. L. Marshall verfasserin aut J. Mena-Fernández verfasserin aut R. Miquel verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malagón verfasserin aut J. D. Sakowska verfasserin aut E. Sanchez verfasserin aut D. Sanchez Cid verfasserin aut B. Santiago verfasserin aut I. Sevilla-Noarbe verfasserin aut M. Smith verfasserin aut G. S. Stringfellow verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut N. Weaverdyck verfasserin aut P. Wiseman verfasserin aut DES & DELVE Collaboration verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 1, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:1, p 126 https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/article/6eeaf2d50e01496096fc1246608fe51f kostenfrei https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 1, p 126 |
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10.3847/1538-4357/ad07d0 doi (DE-627)DOAJ096131888 (DE-599)DOAJ6eeaf2d50e01496096fc1246608fe51f DE-627 ger DE-627 rakwb eng QB460-466 M. McNanna verfasserin aut A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. Local Group Low surface brightness galaxies Dwarf galaxies Astrophysics K. Bechtol verfasserin aut S. Mau verfasserin aut E. O. Nadler verfasserin aut J. Medoff verfasserin aut A. Drlica-Wagner verfasserin aut W. Cerny verfasserin aut D. Crnojević verfasserin aut B. Mutlu-Pakdıl verfasserin aut A. K. Vivas verfasserin aut A. B. Pace verfasserin aut J. L. Carlin verfasserin aut M. L. M. Collins verfasserin aut P. S. Ferguson verfasserin aut D. Martínez-Delgado verfasserin aut C. E. Martínez-Vázquez verfasserin aut N. E. D. Noel verfasserin aut A. H. Riley verfasserin aut D. J. Sand verfasserin aut A. Smercina verfasserin aut E. Tollerud verfasserin aut R. H. Wechsler verfasserin aut T. M. C. Abbott verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut D. Bacon verfasserin aut C. R. Bom verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut J. A. Carballo-Bello verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut L. N. da Costa verfasserin aut T. M. Davis verfasserin aut J. De Vicente verfasserin aut H. T. Diehl verfasserin aut P. Doel verfasserin aut I. Ferrero verfasserin aut J. Frieman verfasserin aut G. Giannini verfasserin aut D. Gruen verfasserin aut G. Gutierrez verfasserin aut R. A. Gruendl verfasserin aut S. R. Hinton verfasserin aut D. L. Hollowood verfasserin aut K. Honscheid verfasserin aut D. J. James verfasserin aut K. Kuehn verfasserin aut J. L. Marshall verfasserin aut J. Mena-Fernández verfasserin aut R. Miquel verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malagón verfasserin aut J. D. Sakowska verfasserin aut E. Sanchez verfasserin aut D. Sanchez Cid verfasserin aut B. Santiago verfasserin aut I. Sevilla-Noarbe verfasserin aut M. Smith verfasserin aut G. S. Stringfellow verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut N. Weaverdyck verfasserin aut P. Wiseman verfasserin aut DES & DELVE Collaboration verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 1, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:1, p 126 https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/article/6eeaf2d50e01496096fc1246608fe51f kostenfrei https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 1, p 126 |
allfields_unstemmed |
10.3847/1538-4357/ad07d0 doi (DE-627)DOAJ096131888 (DE-599)DOAJ6eeaf2d50e01496096fc1246608fe51f DE-627 ger DE-627 rakwb eng QB460-466 M. McNanna verfasserin aut A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. Local Group Low surface brightness galaxies Dwarf galaxies Astrophysics K. Bechtol verfasserin aut S. Mau verfasserin aut E. O. Nadler verfasserin aut J. Medoff verfasserin aut A. Drlica-Wagner verfasserin aut W. Cerny verfasserin aut D. Crnojević verfasserin aut B. Mutlu-Pakdıl verfasserin aut A. K. Vivas verfasserin aut A. B. Pace verfasserin aut J. L. Carlin verfasserin aut M. L. M. Collins verfasserin aut P. S. Ferguson verfasserin aut D. Martínez-Delgado verfasserin aut C. E. Martínez-Vázquez verfasserin aut N. E. D. Noel verfasserin aut A. H. Riley verfasserin aut D. J. Sand verfasserin aut A. Smercina verfasserin aut E. Tollerud verfasserin aut R. H. Wechsler verfasserin aut T. M. C. Abbott verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut D. Bacon verfasserin aut C. R. Bom verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut J. A. Carballo-Bello verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut L. N. da Costa verfasserin aut T. M. Davis verfasserin aut J. De Vicente verfasserin aut H. T. Diehl verfasserin aut P. Doel verfasserin aut I. Ferrero verfasserin aut J. Frieman verfasserin aut G. Giannini verfasserin aut D. Gruen verfasserin aut G. Gutierrez verfasserin aut R. A. Gruendl verfasserin aut S. R. Hinton verfasserin aut D. L. Hollowood verfasserin aut K. Honscheid verfasserin aut D. J. James verfasserin aut K. Kuehn verfasserin aut J. L. Marshall verfasserin aut J. Mena-Fernández verfasserin aut R. Miquel verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malagón verfasserin aut J. D. Sakowska verfasserin aut E. Sanchez verfasserin aut D. Sanchez Cid verfasserin aut B. Santiago verfasserin aut I. Sevilla-Noarbe verfasserin aut M. Smith verfasserin aut G. S. Stringfellow verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut N. Weaverdyck verfasserin aut P. Wiseman verfasserin aut DES & DELVE Collaboration verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 1, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:1, p 126 https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/article/6eeaf2d50e01496096fc1246608fe51f kostenfrei https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 1, p 126 |
allfieldsGer |
10.3847/1538-4357/ad07d0 doi (DE-627)DOAJ096131888 (DE-599)DOAJ6eeaf2d50e01496096fc1246608fe51f DE-627 ger DE-627 rakwb eng QB460-466 M. McNanna verfasserin aut A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. Local Group Low surface brightness galaxies Dwarf galaxies Astrophysics K. Bechtol verfasserin aut S. Mau verfasserin aut E. O. Nadler verfasserin aut J. Medoff verfasserin aut A. Drlica-Wagner verfasserin aut W. Cerny verfasserin aut D. Crnojević verfasserin aut B. Mutlu-Pakdıl verfasserin aut A. K. Vivas verfasserin aut A. B. Pace verfasserin aut J. L. Carlin verfasserin aut M. L. M. Collins verfasserin aut P. S. Ferguson verfasserin aut D. Martínez-Delgado verfasserin aut C. E. Martínez-Vázquez verfasserin aut N. E. D. Noel verfasserin aut A. H. Riley verfasserin aut D. J. Sand verfasserin aut A. Smercina verfasserin aut E. Tollerud verfasserin aut R. H. Wechsler verfasserin aut T. M. C. Abbott verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut D. Bacon verfasserin aut C. R. Bom verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut J. A. Carballo-Bello verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut L. N. da Costa verfasserin aut T. M. Davis verfasserin aut J. De Vicente verfasserin aut H. T. Diehl verfasserin aut P. Doel verfasserin aut I. Ferrero verfasserin aut J. Frieman verfasserin aut G. Giannini verfasserin aut D. Gruen verfasserin aut G. Gutierrez verfasserin aut R. A. Gruendl verfasserin aut S. R. Hinton verfasserin aut D. L. Hollowood verfasserin aut K. Honscheid verfasserin aut D. J. James verfasserin aut K. Kuehn verfasserin aut J. L. Marshall verfasserin aut J. Mena-Fernández verfasserin aut R. Miquel verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malagón verfasserin aut J. D. Sakowska verfasserin aut E. Sanchez verfasserin aut D. Sanchez Cid verfasserin aut B. Santiago verfasserin aut I. Sevilla-Noarbe verfasserin aut M. Smith verfasserin aut G. S. Stringfellow verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut N. Weaverdyck verfasserin aut P. Wiseman verfasserin aut DES & DELVE Collaboration verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 1, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:1, p 126 https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/article/6eeaf2d50e01496096fc1246608fe51f kostenfrei https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 1, p 126 |
allfieldsSound |
10.3847/1538-4357/ad07d0 doi (DE-627)DOAJ096131888 (DE-599)DOAJ6eeaf2d50e01496096fc1246608fe51f DE-627 ger DE-627 rakwb eng QB460-466 M. McNanna verfasserin aut A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. Local Group Low surface brightness galaxies Dwarf galaxies Astrophysics K. Bechtol verfasserin aut S. Mau verfasserin aut E. O. Nadler verfasserin aut J. Medoff verfasserin aut A. Drlica-Wagner verfasserin aut W. Cerny verfasserin aut D. Crnojević verfasserin aut B. Mutlu-Pakdıl verfasserin aut A. K. Vivas verfasserin aut A. B. Pace verfasserin aut J. L. Carlin verfasserin aut M. L. M. Collins verfasserin aut P. S. Ferguson verfasserin aut D. Martínez-Delgado verfasserin aut C. E. Martínez-Vázquez verfasserin aut N. E. D. Noel verfasserin aut A. H. Riley verfasserin aut D. J. Sand verfasserin aut A. Smercina verfasserin aut E. Tollerud verfasserin aut R. H. Wechsler verfasserin aut T. M. C. Abbott verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut D. Bacon verfasserin aut C. R. Bom verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut J. A. Carballo-Bello verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut L. N. da Costa verfasserin aut T. M. Davis verfasserin aut J. De Vicente verfasserin aut H. T. Diehl verfasserin aut P. Doel verfasserin aut I. Ferrero verfasserin aut J. Frieman verfasserin aut G. Giannini verfasserin aut D. Gruen verfasserin aut G. Gutierrez verfasserin aut R. A. Gruendl verfasserin aut S. R. Hinton verfasserin aut D. L. Hollowood verfasserin aut K. Honscheid verfasserin aut D. J. James verfasserin aut K. Kuehn verfasserin aut J. L. Marshall verfasserin aut J. Mena-Fernández verfasserin aut R. Miquel verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malagón verfasserin aut J. D. Sakowska verfasserin aut E. Sanchez verfasserin aut D. Sanchez Cid verfasserin aut B. Santiago verfasserin aut I. Sevilla-Noarbe verfasserin aut M. Smith verfasserin aut G. S. Stringfellow verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut N. Weaverdyck verfasserin aut P. Wiseman verfasserin aut DES & DELVE Collaboration verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 1, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:1, p 126 https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/article/6eeaf2d50e01496096fc1246608fe51f kostenfrei https://doi.org/10.3847/1538-4357/ad07d0 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 1, p 126 |
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English |
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In The Astrophysical Journal 961(2024), 1, p 126 volume:961 year:2024 number:1, p 126 |
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In The Astrophysical Journal 961(2024), 1, p 126 volume:961 year:2024 number:1, p 126 |
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Local Group Low surface brightness galaxies Dwarf galaxies Astrophysics |
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M. McNanna @@aut@@ K. Bechtol @@aut@@ S. Mau @@aut@@ E. O. Nadler @@aut@@ J. Medoff @@aut@@ A. Drlica-Wagner @@aut@@ W. Cerny @@aut@@ D. Crnojević @@aut@@ B. Mutlu-Pakdıl @@aut@@ A. K. Vivas @@aut@@ A. B. Pace @@aut@@ J. L. Carlin @@aut@@ M. L. M. Collins @@aut@@ P. S. Ferguson @@aut@@ D. Martínez-Delgado @@aut@@ C. E. Martínez-Vázquez @@aut@@ N. E. D. Noel @@aut@@ A. H. Riley @@aut@@ D. J. Sand @@aut@@ A. Smercina @@aut@@ E. Tollerud @@aut@@ R. H. Wechsler @@aut@@ T. M. C. Abbott @@aut@@ M. Aguena @@aut@@ O. Alves @@aut@@ D. Bacon @@aut@@ C. R. Bom @@aut@@ D. Brooks @@aut@@ D. L. Burke @@aut@@ J. A. Carballo-Bello @@aut@@ A. Carnero Rosell @@aut@@ J. Carretero @@aut@@ L. N. da Costa @@aut@@ T. M. Davis @@aut@@ J. De Vicente @@aut@@ H. T. Diehl @@aut@@ P. Doel @@aut@@ I. Ferrero @@aut@@ J. Frieman @@aut@@ G. Giannini @@aut@@ D. Gruen @@aut@@ G. Gutierrez @@aut@@ R. A. Gruendl @@aut@@ S. R. Hinton @@aut@@ D. L. Hollowood @@aut@@ K. Honscheid @@aut@@ D. J. James @@aut@@ K. Kuehn @@aut@@ J. L. Marshall @@aut@@ J. Mena-Fernández @@aut@@ R. Miquel @@aut@@ M. E. S. Pereira @@aut@@ A. Pieres @@aut@@ A. A. Plazas Malagón @@aut@@ J. D. Sakowska @@aut@@ E. Sanchez @@aut@@ D. Sanchez Cid @@aut@@ B. Santiago @@aut@@ I. Sevilla-Noarbe @@aut@@ M. Smith @@aut@@ G. S. Stringfellow @@aut@@ E. Suchyta @@aut@@ M. E. C. Swanson @@aut@@ G. Tarle @@aut@@ N. Weaverdyck @@aut@@ P. Wiseman @@aut@@ DES & DELVE Collaboration @@aut@@ |
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M. McNanna misc QB460-466 misc Local Group misc Low surface brightness galaxies misc Dwarf galaxies misc Astrophysics A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 |
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QB460-466 A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 Local Group Low surface brightness galaxies Dwarf galaxies |
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M. McNanna K. Bechtol S. Mau E. O. Nadler J. Medoff A. Drlica-Wagner W. Cerny D. Crnojević B. Mutlu-Pakdıl A. K. Vivas A. B. Pace J. L. Carlin M. L. M. Collins P. S. Ferguson D. Martínez-Delgado C. E. Martínez-Vázquez N. E. D. Noel A. H. Riley D. J. Sand A. Smercina E. Tollerud R. H. Wechsler T. M. C. Abbott M. Aguena O. Alves D. Bacon C. R. Bom D. Brooks D. L. Burke J. A. Carballo-Bello A. Carnero Rosell J. Carretero L. N. da Costa T. M. Davis J. De Vicente H. T. Diehl P. Doel I. Ferrero J. Frieman G. Giannini D. Gruen G. Gutierrez R. A. Gruendl S. R. Hinton D. L. Hollowood K. Honscheid D. J. James K. Kuehn J. L. Marshall J. Mena-Fernández R. Miquel M. E. S. Pereira A. Pieres A. A. Plazas Malagón J. D. Sakowska E. Sanchez D. Sanchez Cid B. Santiago I. Sevilla-Noarbe M. Smith G. S. Stringfellow E. Suchyta M. E. C. Swanson G. Tarle N. Weaverdyck P. Wiseman DES & DELVE Collaboration |
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search for faint resolved galaxies beyond the milky way in des year 6: a new faint, diffuse dwarf satellite of ngc 55 |
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QB460-466 |
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A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 |
abstract |
We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. |
abstractGer |
We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. |
abstract_unstemmed |
We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host. |
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A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">DOAJ096131888</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240413142625.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">240413s2024 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3847/1538-4357/ad07d0</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)DOAJ096131888</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DOAJ6eeaf2d50e01496096fc1246608fe51f</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QB460-466</subfield></datafield><datafield tag="100" ind1="0" ind2=" "><subfield code="a">M. McNanna</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="2"><subfield code="a">A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2024</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). 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