Archive for October, 2013

New Paper on exoplanets – the SEAWOLF project

Posted October 31, 2013 By grigoris

Trawling for transits in a sea of noise: A Search for Exoplanets by Analysis of WASP Optical Lightcurves and Follow-up (SEAWOLF)

E. Gaidos, D. R. Anderson, S. Lepine, K. D. Colon, G. Maravelias, N. Narita, E. Chang, J. Beyer, A. Fukui, J. D. Armstrong, A. Zezas, B. J. Fulton, A. W. Mann, R. G. West, F. Faedi

Studies of transiting Neptune-size planets orbiting close to nearby bright stars can inform theories of planet formation because mass and radius and therefore mean density can be accurately estimated and compared with interior models. The distribution of such planets with stellar mass and orbital period relative to their Jovian-mass counterparts can test scenarios of orbital migration, and whether “hot” (period < 10d) Neptunes evolved from “hot” Jupiters as a result of mass loss. We searched 1763 late K and early M dwarf stars for transiting Neptunes by analyzing photometry from the Wide Angle Search for Planets and obtaining high-precision (<10−3) follow-up photometry of stars with candidate transit signals. One star in our sample (GJ 436) hosts a previously reported hot Neptune. We identified 92 candidate signals among 80 other stars and carried out 148 observations of predicted candidate transits with 1-2 m telescopes. Data on 70 WASP signals rules out transits for 39 of them; 28 other signals are ambiguous and/or require more data. Three systems have transit-like events in follow-up photometry and we plan additional follow-up observations. On the basis of no confirmed detections in our survey, we place an upper limit of 10.25% on the occurrence of hot Neptunes around late K and early M dwarfs (95% confidence). A single confirmed detection would translate to an occurrence of 5.3±4.4%. The latter figure is similar to that from Doppler surveys, suggesting that GJ 436b may be the only transiting hot Neptune in our sample. Our analysis of Kepler data for similar but more distant late-type dwarfs yields an occurrence of 0.32±0.21%. Depending on which occurrence is applicable, we estimate that the Next Generation Transit Survey will discover either ~60 or ~1000 hot Neptunes around late K and early M-type dwarfs.


Updating clock time through terminal

Posted October 22, 2013 By grigoris

In my Fedora 14 desktop I keep losing minutes without knowing how and why (doesn’t the clock update automatically?).
At the beginning I tried to change the file /etc/ntp.conf (edit it and change the parameter server to: ‘server’; 1) as perhaps the server did not respond correctly.
I tried to update by:

but the result was not the expected one, but an error: “… the NTP socket is in use, exiting”
I stopped (/etc/init.d/ntpd stop) and tried to updated (ntpdate but another error was raised: “… no server suitable for synchronization found” (reasonable though since …ntd was down!).

By looking a little bit around the solution [2] was to update while running as:
ntpdate -u

and…that’s it! I removed the extra entry in the /etc/ntp.conf (to keep the original servers only) and it worked again.

Now let’s see if it’s going to keep up or I will need to manually update the clock from time to time.

[1]: – Synchronize the system clock to Network Time Protocol (NTP) under Fedora or Red Hat Linux
[2]: – Socket is in use