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Analytical Resolution of the Dark Night Sky (Olbers') Paradox
DOI: 10.1002/asna.201913540 Bibcode: 2019AN....340..510H

Harari, Zaki

We derive a spatiotemporal analytical resolution of the dark night sky, or Olbers' paradox, first showing that in an infinitely large universe the cumulative solid angle of the light that is projected upon the celestial sphere by an infinite population of directly observable stars is indeed finite. Using the GAIA DR2 data, we show that the number …

2019 Astronomische Nachrichten
Gaia 1
ExoMars Schiaparelli Direct-to-Earth Observation using GMRT
DOI: 10.1029/2018RS006707 Bibcode: 2019RaSc...54..314E

Asmar, S. W.; De, K.; Gupta, Y. +3 more

During the ExoMars Schiaparelli separation event on 16 October 2016 and Entry, Descent, and Landing (EDL) events 3 days later, the Giant Metrewave Radio Telescope (GMRT) near Pune, India, was used to directly observe UHF transmissions from the Schiaparelli lander as they arrive at Earth. The Doppler shift of the carrier frequency was measured and …

2019 Radio Science
ExoMars-16 1
Gaia DR2 and the Virtual Observatory: VO in Operations New Era
Bibcode: 2019ASPC..523..445S

Merín, Bruno; Hambly, Nigel C.; Allen, Mark +15 more

During the last decade, the IVOA (International Virtual Observatory Alliance) has been tasked with the difficult task of defining standards to interchange astronomical data. These efforts have been supported by many IVOA partners in general and by the ESAC Science Data Centre (ESDC) in particular, that have been collaborating in the definition of …

2019 Astronomical Data Analysis Software and Systems XXVII
Gaia 1
A Detailed Investigation on the Infrared-excess Binary EG Cassiopeiae
DOI: 10.1088/1538-3873/ab3b9c Bibcode: 2019PASP..131l4201Y

Yang, Yuangui; Yuan, Huiyu; Dai, Haifeng

In this study, new data concerning the EB-type eclipsing binary EG Cas are presented as observed using three telescopes in China. A spectral type of F0V was determined from the low-precision spectrum. By solving the radial velocity and BV light curves, the absolute parameters of this system are preliminarily deduced. The results imply that EG Cas …

2019 Publications of the Astronomical Society of the Pacific
Gaia 1
New outburst from the luminous supersoft source SSS1 in NGC 300 with periodic modulation
DOI: 10.1093/mnras/stz2940 Bibcode: 2019MNRAS.490.4804C

Haberl, F.; Maitra, C.; Carpano, S.

The nearby galaxy NGC 300 is hosting two luminous transient supersoft X-ray sources with bolometric luminosities above 3 × 1038 erg s-1, assuming simple blackbody spectra with temperatures around 60-70 eV. For one of these, SSS1, a periodic modulation of 5.4 h was observed in an XMM-Newton observation from 2001 Jan…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 1
Neutral-gas-phase metal abundances in Zn II-selected quasar absorption line systems near redshift z = 1.2
DOI: 10.1093/mnras/sty3165 Bibcode: 2019MNRAS.483.1168M

Turnshek, David A.; Rao, Sandhya M.; Monier, Eric M. +2 more

We present 10 metallicity measurements for quasar absorbers near z = 1.2 that were selected for having unusually significant Zn II absorption in their Sloan Digital Sky Survey (SDSS) spectra. Follow-up UV space spectroscopy of the Lyα region shows that all 10 have damped Lyα (DLA) absorption, corresponding to neutral hydrogen column densities in t…

2019 Monthly Notices of the Royal Astronomical Society
eHST 1
Flares activity of selected stars from GTSh10 catalog by CRTS data
DOI: 10.48550/arXiv.1903.05920 Bibcode: 2019A&AT...31..333G

Gorbachev, M. A.; Shlyapnikov, A. A.

Based on the database of photometric observations of the CRTS project over an interval of more than 9 years, the activity of red dwarfs from the GTSh10 catalog was analyzed. The total number of analyzed objects, a list ares, amplitudes and moments of recorded events are presented. For the most interesting objects, from the point of view are activi…

2019 Astronomical and Astrophysical Transactions
Gaia 1
SB 796: a high-velocity RRc star
DOI: 10.1093/mnras/sty2828 Bibcode: 2019MNRAS.482.5327G

Soszyński, Igor; Gomel, Roy; Faigler, Simchon +6 more

We report here on a detailed study of a c-type RR Lyrae variable (RRc variable), SB 796, serendipitously discovered in a search of the WASP public data for stars that display large photometric periodic modulation. SB 796 displays a period of P = 0.26585 d and semi-amplitude of ∼0.1 mag. Comparison of the modulation shape and period with the detail…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 1
Long-Term Activity of a Little Known Dwarf Nova DT Octantis
DOI: 10.1134/S199034131904014X Bibcode: 2019AstBu..74..490S

Šimon, V.; Edelmann, H.

We analyze the long-term activity of a little known dwarf nova (DN) DT Oct. We use photographic observations from the Bamberg Observatory (Southern Patrol Photographic Sky Survey), CCD data from ASAS-3 survey, and AAVSO data (both CCD and visual). We determined the recurrence times of the superoutbursts, TCso, and of the normal outburst…

2019 Astrophysical Bulletin
Gaia 1
A new binary star system of EA type in Perseus: UCAC4 735-019611
Bibcode: 2019OEJV..194....1B

Brincat, S. M.; Galdies, C.; Grech, W.

Discovery of a new binary star system (UCAC4 735-019611=USNO-B1.0 1469-0068570=2MASS J01561032+5657563) in the Perseus constellation is presented. It was discovered during asteroid photometric work. The shape of the light curve and its characteristics (period of 2.12701±0.00001d, amplitude of V=0.55 mag, initial minimum period epoch HJD 2457363.37…

2019 Open European Journal on Variable Stars
Gaia 1