Variations of the dust properties of M82 with galactocentric distance
S Hutton, I Ferreras, V Yershov - Monthly Notices of the Royal …, 2015 - academic.oup.com
We use near ultraviolet and optical photometry to investigate the dust properties in the
nearby starburst galaxy M82. By combining imaging from the Swift/UVOT instrument and
optical data from the Sloan Digital Sky Survey, we derive the extinction curve parametrized …
nearby starburst galaxy M82. By combining imaging from the Swift/UVOT instrument and
optical data from the Sloan Digital Sky Survey, we derive the extinction curve parametrized …
A panchromatic analysis of starburst galaxy M82: Probing the dust properties
…, K Wu, P Kuin, A Breeveld, V Yershov… - Monthly Notices of …, 2014 - academic.oup.com
We combine near-ultraviolet (NUV), optical and IR imaging of the nearby starburst galaxy
M82 to explore the properties of the dust both in the interstellar medium of the galaxy and
the dust entrained in the superwind. The three NUV filters of Swift-Ultraviolet/Optical …
M82 to explore the properties of the dust both in the interstellar medium of the galaxy and
the dust entrained in the superwind. The three NUV filters of Swift-Ultraviolet/Optical …
The use and calibration of read-out streaks to increase the dynamic range of the Swift Ultraviolet/Optical Telescope
…, M Symeonidis, V Yershov… - Monthly Notices of …, 2013 - academic.oup.com
The dynamic range of photon counting micro-channel-plate (MCP) intensified charged-
coupled device (CCD) instruments such as the Swift Ultraviolet/Optical Telescope (UVOT)
and the XMM–Newton Optical Monitor (XMM-OM) is limited at the bright end by coincidence …
coupled device (CCD) instruments such as the Swift Ultraviolet/Optical Telescope (UVOT)
and the XMM–Newton Optical Monitor (XMM-OM) is limited at the bright end by coincidence …
Correlation of supernova redshifts with temperature fluctuations of the cosmic microwave background
VN Yershov, VV Orlov, AA Raikov - Monthly Notices of the Royal …, 2012 - academic.oup.com
Redshifts of supernova (SN) and gamma-ray burst (GRB) samples are compared with the
pixel temperatures of the Wilkinson Microwave Anisotropy Probe (WMAP) seven-year data,
the pixel locations corresponding to the SN and GRB sky coordinates. We have found a …
pixel temperatures of the Wilkinson Microwave Anisotropy Probe (WMAP) seven-year data,
the pixel locations corresponding to the SN and GRB sky coordinates. We have found a …
[CITATION][C] vanden Berk, D. 2010
…, TS Poole, P Roming, PJ Smith, M Still, V Yershov… - MNRAS
Calibration of the Swift-UVOT ultraviolet and visible grisms
…, M Mehdipour, M Still, V Yershov… - Monthly Notices of …, 2015 - academic.oup.com
We present the calibration of the Swift Ultraviolet and Optical Telescope (UVOT) grisms, of
which there are two, providing low-resolution field spectroscopy in the ultraviolet and optical
bands, respectively. The UV grism covers the range λ1700–5000 Å with a spectral resolution …
which there are two, providing low-resolution field spectroscopy in the ultraviolet and optical
bands, respectively. The UV grism covers the range λ1700–5000 Å with a spectral resolution …
Possible signature of distant foreground in the Planck data
VN Yershov, VV Orlov, AA Raikov - Monthly Notices of the Royal …, 2014 - academic.oup.com
By using the Planck map of the cosmic microwave background (CMB) radiation, we have
checked and confirmed the existence of a correlation between supernova (SN) redshifts, z
SN, and CMB temperature fluctuations at the SNe locations, T SN, which we previously …
checked and confirmed the existence of a correlation between supernova (SN) redshifts, z
SN, and CMB temperature fluctuations at the SNe locations, T SN, which we previously …
[CITATION][C] vanden Berk, D.(2010). Further calibration of the Swift ultraviolet/optical telescope
…, TS Poole, P Roming, PJ Smith, M Still, V Yershov… - MNRAS
Binary pulsars studies with multiwavelength sky surveys–I. Companion star identification
…, C Pallanca, SR Oates, VN Yershov… - Monthly Notices of …, 2014 - academic.oup.com
The identification of the stellar companions to binary pulsars is key to studying the evolution
of the binary system and how this is influenced by the interactions between the two stars. For
only a fraction of the known binary pulsars, the stellar companions have been identified …
of the binary system and how this is influenced by the interactions between the two stars. For
only a fraction of the known binary pulsars, the stellar companions have been identified …
A study of the asteroid (367943) Duende at Pulkovo Observatory
…, DL Gorshanov, VN Yershov… - Monthly Notices of …, 2016 - academic.oup.com
Using the telescopes ZA-320 M and MTM-500 M of Pulkovo Observatory (Russia), we have
carried out astrometric and photometric observations of the asteroid (367943) Duende (2012
DA14) immediately after its close approach to the Earth occurred on 2013 February 15. We …
carried out astrometric and photometric observations of the asteroid (367943) Duende (2012
DA14) immediately after its close approach to the Earth occurred on 2013 February 15. We …
