Multiwavelength observations of the extraordinary accretion event AT2021lwx

Autor: P Wiseman, Y Wang, S Hönig, N Castro-Segura, P Clark, C Frohmaier, M D Fulton, G Leloudas, M Middleton, T E Müller-Bravo, A Mummery, M Pursiainen, S J Smartt, K Smith, M Sullivan, J P Anderson, J A Acosta Pulido, P Charalampopoulos, M Banerji, M Dennefeld, L Galbany, M Gromadzki, C P Gutiérrez, N Ihanec, E Kankare, A Lawrence, B Mockler, T Moore, M Nicholl, F Onori, T Petrushevska, F Ragosta, S Rest, M Smith, T Wevers, R Carini, T-W Chen, K Chambers, H Gao, M Huber, C Inserra, E Magnier, L Makrygianni, M Toy, F Vincentelli, D R Young

Publikováno v: Wiseman, P, Wang, Y, Honig, S, Castro-Segura, N, Clark, P, Frohmaier, C, Fulton, M D, Leloudas, G, Middleton, M, Muller-Bravo, T E, Mummery, A, Pursiainen, M, Smartt, S J, Smith, K, Sullivan, M, Anderson, J P, Acosta Pulido, J A, Charalampopoulos, P, Banerji, M, Dennefeld, M, Galbany, L, Gromadzki, M, Gutierrez, C P, Ihanec, N, Kankare, E, Lawrence, A, Mockler, B, Moore, T, Nicholl, M, Onori, F, Petrushevska, T, Ragosta, F, Rest, S, Smith, M, Wevers, T, Carini, R, Chen, T W, Chambers, K, Gao, H, Huber, M, Inserra, C, Magnier, E, Makrygianni, L, Toy, M, Vincentelli, F & Young, D R 2023, ' Multiwavelength observations of the extraordinary accretion event AT2021lwx ', Monthly Notices of the Royal Astronomical Society, vol. 522, no. 3, pp. 3992-4002 . https://doi.org/10.1093/mnras/stad1000
Wiseman, P, Wang, Y, Hönig, S, Castro-Segura, N, Clark, P, Frohmaier, C, Fulton, M D, Leloudas, G, Middleton, M, Müller-Bravo, T E, Mummery, A, Pursiainen, M, Smartt, S J, Smith, K, Sullivan, M, Anderson, J P, Pulido, J A A, Charalampopoulos, P, Banerji, M, Dennefeld, M, Galbany, L, Gromadzki, M, Gutiérrez, C P, Ihanec, N, Kankare, E, Lawrence, A, Mockler, B, Moore, T, Nicholl, M, Onori, F, Petrushevska, T, Ragosta, F, Rest, S, Smith, M, Wevers, T, Carini, R, Chen, T-W, Chambers, K, Gao, H, Huber, M, Inserra, C, Magnier, E, Makrygianni, L, Toy, M, Vincentelli, F & Young, D R 2023, ' Multiwavelength observations of the extraordinary accretion event AT2021lwx ', Monthly Notices of the Royal Astronomical Society, vol. 522, no. 3, 3992–4002 . https://doi.org/10.1093/mnras/stad1000

We present observations from X-ray to mid-infrared wavelengths of the most energetic non-quasar transient ever observed, AT2021lwx. Our data show a single optical brightening by a factor $>100$ to a luminosity of $7\times10^{45}$ erg s$^{-1}$, and a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5928d80421fd16f18763ce4fd3d7d802
https://doi.org/10.1093/mnras/stad1000

Constraints on the X-ray luminosity function of AGN at z = 5.7–6.4 with the Extragalactic Serendipitous Swift Survey

Autor: C L Barlow-Hall, J Delaney, J Aird, P A Evans, J P Osborne, M G Watson

Publikováno v: Barlow-Hall, C L, Delaney, J, Aird, J, Evans, P A, Osborne, J P & Watson, M G 2023, ' Constraints on the X-ray luminosity function of AGN at z = 5.7–6.4 with the Extragalactic Serendipitous Swift Survey ', Monthly Notices of the Royal Astronomical Society, vol. 519, no. 4, pp. 6055-6064 . https://doi.org/10.1093/mnras/stad100

X-ray luminosity functions (XLFs) of Active Galactic Nuclei (AGN) trace the growth and evolution of supermassive black hole populations across cosmic time, however, current XLF models are poorly constrained at redshifts of z>6, with a lack of spectro

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66d679b9d8c87d3ab0ea6b0d918dee10
https://hdl.handle.net/20.500.11820/9e301517-7154-4551-98e9-f0e04e0d7187

Revealing the structure of the lensed quasar Q 0957+561 II. Supermassive black hole mass via gravitational redshift

Autor: Joseph A. Muñoz, J. Jiménez-Vicente, Carina Fian, D. Chelouche, E. Mediavilla, Veronica Motta, Arnold Hanslmeier

Aims. We intend to use the impact of microlensing on the Fe III lambda lambda 2039 2113 emission line blend along with a measure of its gravitational redshift to estimate the mass of the quasar's central supermassive black hole (SMBH). Methods. We fi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a20c04a21e31b2f98fbfd3ee43fdfaa0
https://hdl.handle.net/10481/78228

Measuring the Hubble Constant with Double Gravitational Wave Sources in Pulsar Timing

Autor: Daniel D'Orazio, Jolien Creighton, Casey McGrath

Publikováno v: McGrath, C, D'Orazio, D J & Creighton, J 2022, ' Measuring the Hubble constant with double gravitational wave sources in pulsar timing ', Monthly Notices of the Royal Astronomical Society, vol. 517, no. 1, pp. 1242-1263 . https://doi.org/10.1093/mnras/stac2593

Pulsar timing arrays (PTAs) are searching for gravitational waves from supermassive black hole binaries (SMBHBs). Here we show how future PTAs could use a detection of gravitational waves from individually resolved SMBHB sources to produce a purely g

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::928b9fba0297332458ed5cb5cbf94a08
http://arxiv.org/abs/2208.06495

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.