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24 results on '"Kasliwal, M M"'

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1. The Bactrian? Broad-lined Type-Ic supernova SN 2022xxf with extraordinary two-humped light curves

2. SN 2019odp: A Massive Oxygen-Rich Type Ib Supernova

3. Near-IR Type Ia SN distances: host galaxy extinction and mass-step corrections revisited

4. Establishing accretion flares from massive black holes as a major source of high-energy neutrinos

5. SRG/ART-XC discovery of SRGA J204318.2+443815: Towards the complete population of faint X-ray pulsars

6. The double-peaked radio light curve of PTF11qcj

7. PTF11mnb: the first analog of supernova 2005bf

8. Color Me Intrigued: the Discovery of iPTF 16fnm, a Supernova 2002cx-like Object

9. Confined Dense Circumstellar Material Surrounding a Regular Type II Supernova: The Unique Flash-Spectroscopy Event of SN 2013fs

10. A tale of two transients: GW170104 and GRB170105A

11. First Searches for Optical Counterparts to Gravitational-wave Candidate Events

12. Long-rising Type II supernovae from PTF and CCCP

13. Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914

14. A Fast Radio Burst Host Galaxy

15. A Wolf-Rayet-like progenitor of supernova SN 2013cu from spectral observations of a wind

16. Hubble Space Telescope studies of low-redshift Type Ia supernovae: Evolution with redshift and ultraviolet spectral trends

17. Discovery of a New Photometric Sub-class of Faint and Fast Classical Novae

18. A VLA search for 5 GHz radio transients and variables at low Galactic latitudes

19. Afterglow Observations of Fermi-LAT Gamma-Ray Bursts and the Emerging Class of Hyper-Energetic Events

20. The Massive Progenitor of the Type II-Linear SN 2009kr

21. Transients in the Local Universe

22. Supplement: Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up

23. Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger

24. LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW 150914

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