Black holes and neutron stars have accretion instability

An X-ray afterglow of the GW170833 protoneutron star merger. Mon. Not. R. Astron. 483, 1912-1921

Piro, L. The remnant of a neutron star merger was constrained by X-ray observations. Mon. Not. R. Astron. 483, 1912–1921, was published in 2019.

Drout, M. R. et al. The light curves of the merger of stars are related to r-process nucleosynthesis. Science 358, 1570–1574 (2017).

Makhathini, S. et al. The panchromatic afterglow of GW170833: full uniform data set, modeling, comparison and implications. There are astrophys. J. 912, 154 in the years to come.

Buisson, D. J. K. et al. Discovery of thermonuclear (Type I) X-ray bursts in the X-ray binary Swift J1858.6–0814 observed with NICER and NuSTAR. There was a meeting on Mon. Not. R. Astron. 499 and 793 are published in 2020.

Bellini, A., Anderson, J. & Bedin, L. R. Astrometry and photometry with HST WFC3. I. Improved geometric-distortion corrections for 10 filters of the UVIS channel. Publ. Astron. Soc. ThePac 123, 622 was published in 2011.

McMullin, J. P., Waters, B., SchieBEL, D., Young, W., Golap, K., and Hill, F. in Astronomical Data Analysis Software and Systems. The day ended at 127–130 (Astronomical Society of the Pacific, 2007).

Pradel, N., Charlot, P. & Lestrade, J.-F. Astrometric accuracy of phase-referenced observations with the VLBA and EVN. Astron. Astrophys. 452, 1099–1106 (2006).

There was a correlation between the size of the jets and the number of active galactic nuclei. Astron. Astrophys. 598, L1 (2017).

Belloni, T., Klein-wolt, M., Méndez, M., and van Paradijs were part of the study. Astron. Astrophys. 355, 271–290 (2000).

Charlot, P. et al. The third realization of the international reference frame is very long baseline interferometry Astron. Astrophys. 644, A159 (2020).

A new type IIP supernova 2017eaw discovered in the infancy of the Zwicky Transient Facility: Bayesian analysis of gamma-ray bursts GRB 090510, GRB

Ackermann, M. et al. A hard power-law component was found in the observation of GRB 090510: a short-hard gamma-ray burst. There are astrophys. J. 716, 1178–1190 (2010).

Speagle, J. S. DYNESTY: a dynamic nested sampling package for estimating Bayesian posteriors and evidences. Mon. Not. R. Astron. Soc. 493, 3132–3158 (2020).

Rui, L. et al. Probing the final-stage progenitor evolution for type IIP supernova 2017eaw in NGC 6946. Mon. Not. R. Astron. The year 1990–2000.

M. T., Soumagnac and others were involved in research. A giant red supergiant was discovered in its infancy by the Zwicky Transient Facility. There are astrophys. J. Letters 902 is published in 2020.

Struble, M F., and Rood, H. J. collaborated on a collection of red shifts and dispersions for Abell clusters. Astrophys. J. Ser. 77 was published in 1991.

C. C. and Reddy, N. A. A steep faint-end slope of the UV luminosity function at z ~ 2–3: implications for the global stellar mass density and star formation in low-mass halos. Astrophys. J. 692, 778, and 81 were published in 2009.

C., A. I., and C. R. were involved in mapping compound cosmic telescopes. Astron. J. 781, 2 was published this year.

McCully, C., Keeton, C. R., Wong, K. C. & Zabludoff, A. I. The framework is used to efficiently model lines of sight. Mon. Not. R. Astron. 443 soc, 3:13300-1352, 2014).

Observational data for core collapse supernovae at redshift 2.5 and new results for the SPIE detector at the Large Binocular Telescope Observatory

Strolger, L.G. et al. Core collapse supernovae has a redshift 2.5 from the CANDELs and CLASH surveys. Astrophys. J. 825, 93.

Chen, W. Additional data for ‘Shock cooling of a red-supergiant supernova at redshift 3 in lensed images’. The journal Zenodo was published on October 10, 2002 and can be found there.

A redesign of the Multi package. The Calibration Workshop of the Space Telescope Science Institute took place in 2010.

Jones, D. O., Scolnic, D. M., & Rodney, S. A. PythonPhot: simple DAOPHOT-type photometry in Python. The source code for the Astrophysics is in the library.

Weymann, R.J., and Foltz, C. B. collaborated on a project. A moderate-resolution, high-throughput CCD channel for the MMT spectrograph. The title of the book is Publ. Astron. Soc. Pacif. 101, 713–724 was published in 1989.

The report was byRothberg, B. et al. Current status of the facility instrumentation suite at the Large Binocular Telescope Observatory. In Proc. There is an electronic device called the SPIE 10702. Evans, C. J. et al. wrote the book about ground- based and airborne tools for astronomy. 1070205 is part of the SpiE.

A full spectral fitting code is presented by Wilkinson, D. M. and Maraston, C. Mon. Not. R. Astron. There was a report on this topic in the paper “Soc 474, 4300–4350”.

Willmer, C N. A. and others. The Deep Evolutionary Exploratory Probe 2 galaxy redshift survey: the galaxy luminosity function to z ~ 1. There are astrophys. J. 661, 825, and 825 were published in 2006).

Hosseinzaden, G. et al. Weak mass loss from the red supergiant progenitor of the type II SN 2021yja. The print is at thearxiv.org.

Ho, A. Y. Q. et al. The Koala: a fast blue optical transient with luminous radio emission from a starburst dwarf galaxy at z = 0.27. Astrophys. J. 895, 49 (2020).

The Dark Energy Camera and The Dark Energy Survey are relevant to this topic. The electromagnetic counterpart of the binary neutron star merger LIGO/Virgo GW170817. I. Discovery of the optical counterpart using the dark energy camera. There are astrophys. J. 832, L16

Mangan, Dunwoody, R., and Meegan are from the Fermi GBM Team. GRB 211211A: Fermi GBM observation. The circular service for the GRB Coordinates Network was published in 2011.

Nicholl, M. Tight multimessenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light-curve synthesis. Mon. Not. R. Astron. Soc. 505, 3016–3032 (2021).

Gompertz, B. P., O’Brien, P. T., Wynn, G. A. & Rowlinson, A. Can magnetar spin-down power extended emission in some short GRBs? There was a meeting on Mon. Not. R. Astron. The journal 431, 1745–1743 was published in 2013).

Just, O., Bauswein, A., Ardevol Pulpillo, R., Goriely, S. & Janka, H. T. Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers. There was a celebration on Mon. Not. R. Astron. Soc. 448, 541–567 (2015).

Adriani, O. et al. The calorimetric electron telescope has been used to measure the spectrum from 11 GeV to 4.8 TeV. Lett. 120, 261102 (2018).

Minaev, P. & Pozanenko, A.; GRB IKI FuN. GRB 211211A: redshift estimation and SPI-ACS/INTEGRAL detection. GRB Coordinates Network, Circular Service, No. 31230 (2021).

Evans, P. A. et al. Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs. There was no work on Mon. Not. R. Astron. Soc. 397, 1177–1201 (2009).

Hook, I. M. et al. The Gemini–North Multi-Object Spectrograph: performance in imaging, long-slit, and multi-object spectroscopic modes. Publ. Astron. Soc. The states for the year 2004 are Pac 116 and 425.

Labrie, K., Anderson, K., Cárdenes, R., Simpson, C. & Turner, J. E. H. DRAGONS – Data Reduction for Astronomy from Gemini Observatory North and South. The conference is called the ASPConf. There is a Ser. 523, which was published last year.

Lang, D., Hogg, D. W., Mierle, K., Blanton, M. & Roweis, S. Astrometry.net: blind astrometric calibration of arbitrary astronomical images. Astron. J. 139, 1782–1800 (2010).

W. Kalberla and P. M. W. The survey of Galactic HI is conducted by the Latin American countries of Argentina and Bonn. The final data release of the combined LDS and IAR surveys. It was Astron. Astrophys. 440, 775–782 (2005).

Brown, W. R., Geller, M. J., Fabricant, D. G. & Kurtz, M. J. V- and R-band galaxy luminosity functions and low surface brightness galaxies in the century survey. Astron. J. 122, 714–728 (2001).

Fong, W.-f. et al. Short GRB host galaxies I: photometric and spectroscopic catalogs, host associations, and galactocentric offsets. Preprint can be found at http://arxiv.org/abs-2106.

Wright, E. L. The WISE has a mission description and initial on-orbit performance. Astron. J. 140, 1868–1881 (2010).

Conroy, C. & Gunn, J. E. The propagation of uncertainties in stellar population synthesis modeling. III. Model calibration, comparison, and evaluation. Astrophys. J. 712 was published in 2010.

Díaz, M. C. et al. Observations of the first similar source by the TOROS collaboration. There are astrophys. J. 856, L29

Gravitational-wave observations of the GRB 200522A: kilonova or collimated outflow from the binary neutron star merger

M. W., T., B. D., and others are involved in a multi-messenger inference of a binaries neutron star merger. Mon. Not. R. Astron. Soc. 489, 91–96 (2019).

Kasen, D., Metzger, B., Barnes, J., Quataert, E. & Ramirez-Ruiz, E. Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event. Nature 556, 80–84.

Khan, S. et al. Frequency-domain gravitational waves from nonprecessing black-hole binaries. I. A phenomenological model for the advanced detector era. D 93, 000016.

The tidal approximants were constructed from high-resolution numerical relativity simulations. Phys. Rev. D 96, 121501 (2017).

W. Fong and others. The broadband counterpart of the short GRB 200522A at z = 0.5536: a luminous kilonova or a collimated outflow with a reverse shock? There are astrophys. J. 906, 127 (2021).

Moskvitin, A., Spiridonova, O., Belkin, S., Pozanenko, A. & Pankov, N.; GRB IKI FuN. GRB 211211A: SAO RAS optical observations. GRB Coordinates Network, Circular Service, No. 31234 (2021).

McMullin, J. P., Waters, B., Schiebel, D., Young, W. & Golap, K. CASA architecture and applications. In Astronomical Data Analysis Software and Systems XVI: Astronomical Society of the Pacific Conference Series Vol. 376 (eds Shaw, R. A. et al.) 127 (2007).

Sanchez, D. A. & Deil, C. Enrico: a Python package to simplify Fermi-LAT analysis. In International Cosmic Ray Conference: International Cosmic Ray Conference Vol. 33, 2784 (2013).

Blumenthal, G. R. & Gould, R J. Bremsstrahlung, synchrotron radiation, and scattering of high energy electrons traversing diluting gases. Rev. Mod. Phys. 42, 237–271 (1970).

NuSTAR observations of the transient galactic black hole candidate Swift J1858.6-0814: a new sibling of V404 Cyg & V4641 Sgr

Belloni, M., Méndez, M., King, A.R., and van Paradijs studied an unstable central disk in a black hole. Astrophys. J. 479, L145–L148 (1997).

The variability in the microquasar GRS 1915+105 is due to radiation pressure instability. Astrophys. J. 544, L33–L36.

Janiuk, A., Grzedzielski, M., Capitanio, F. & Bianchi, S. Interplay between heartbeat oscillations and wind outflow in microquasar IGR J17091-3624. Astron. 574 is titled astrophys.

Hare, J. NuSTAR observations of the transient galactic black hole binary candidate Swift J1858.6–0814: a new sibling of V404 Cyg and V4641 Sgr? Astrophys. J. 890, 57 (2020).

Fender, R. P., Bell Burnell, S. J., Williams, P. M. & Webster, A. S. Flaring and quiescent infrared behaviour of Cygnus X-3. Mon. Not. R. Astron. The report was titled “Soc. 283, 798–804”.

The heliocentric and barycentricJulian dates achieved better than 1 minute accuracy. Publ. Astron. Soc. There was a report onPac 122, 935.

Edelson, R. A. & Krolik, J. H. The discrete correlation function: a new method for analyzing unevenly sampled variability data. There are astrophys. J. 333, 646 (1988).

Gandhi, P. and others. Rapid optical and X-ray timing observations of GX 339–4: multicomponent optical variability in the low/hard state. Mon. Not. R. Astron. Soc. 407, 2166–2192 (2010).

Paice, J. A. et al. Swift J1858.6-0814 had blue and rapid red flares. The Telegram of the Astronomer is numbered 12197.

F. M.,Vincentelli, and others. Discovery of a thermonuclear Type I X-ray burst in infrared: new limits on the orbital period of 4U 1728-34. The day was Mon. Not. R. Astron. L37–L41 will be added in 2020.

Harding, L. K. et al. The Hale telescope has a high-speed photometer at its prime focus. It’s Mon. Not. R. Astron. A summary of the work done in 3036 and 4049 by the society of 457.

There is a report titled, Nikzad, S. et al. Development of and field observations with delta-doped array are possible with high-efficiency UV/optical/ NIR detectors. J. Astron. In the middle of the night: Telesc. Instrum. Syst. 3, 036002 (2017).

The analysing atolls is done by Done, Gierliski, and Gladstone. Mon. Not. R. Astron. The work was done in the 13th and 22nd year of the society.

Vasilopoulos, G. The eruption of the super Eddington can be seen as a detection of constraints on the magnetic field strength. Mon. Not. R. Astron. 5535–5359 was published in 2020.

Tsygankov, S. S., Doroshenko, V., Lutovinov, A. A., Mushtukov, A. A. & Poutanen, J. SMC X-3: the closest ultraluminous X-ray source powered by a neutron star with non-dipole magnetic field. Astron. Astrophys. 605, A39 (2017).