SAE standards promote and facilitate safety, productivity, reliability, efficiency, and certification in mobility industries.

Optical Image (3 arcmin on a side, red = DSS 2 IR, green = DSS 2 red, blue = DSS 2 blue · Crab Weighted Monthly Mosaic Lightcurve for SWIFT J1419.0-2639

To bookmark this query, right click on this link: simbad:RX J1419.9+2706 and select 'bookmark this link' or equivalent in the popup menu

#j1419 hashtag on Twitter

Buy Sunbank Electronics/J1419-16-34 at PEI-Genesis. Check stock, pricing & view product specs. Authorized Distributor. Ships fast with no minimum order quantity.

other nameright ascension (J2000) declination (J2000) 5-GHz total flux density optical IDredshift 1418+546 14 h 19 m 46.5974 s + 54 ° 23 ´ 14.787 " 1.7 Jy BL Lac 0.152 · VLBApls image at 5 GHz color gif | contour gif | contour PostScript

The radio quasar NVSS J141922$-$083830 (J1419$-$0838) was initially classified as an uncategorised blazar-type object, following its detection in the $γ$-ray band with the Fermi space telescope. Later, using multi-waveband observations and modeling, its was found to be a flat-spectrum radio ...

The radio quasar NVSS J141922−083830 (J1419−0838) was initially classified as an uncategorised blazar-type object, following its detection in the γ $\gamma $ -ray band with the Fermi space telescope. Later, using multi-waveband observations and modeling, its was found to be a flat-spectrum ...

October 12, 2020 - To ensure we keep this website safe, please can you confirm you are a human by ticking the box below · If you are unable to complete the above request please contact us using the below link, providing a screenshot of your experience

Download Table | Properties of FIRST J1419+3940 measured following different imaging ap- proaches. from publication: Resolving the decades-long transient FIRST J141918.9+394036: an orphan long gamma-ray burst or a young magnetar nebula? | Ofek (2017) identified FIRST J141918.9+394036 (hereafter ...

July 1, 2020 - Nonetheless, no radio flare observation has been reported to date. Here we show that the radio transient FIRST J1419+3940, first observed in 1993 and still detectable, could have originated from a neutron star merger. We carry out numerical simulations of neutron star merger ejecta to demonstrate ...

July 4, 2020 - Download Citation | FIRST J1419+3940 as the First Observed Radio Flare from a Neutron Star Merger | During their violent merger, two neutron stars can shed a few percent of their mass. As this ejecta expands, it collides with the surrounding... | Find, read and cite all the research you need ...

Download Table | Radio Observations of J1419+3940 from publication: Discovery of the Luminous, Decades-long, Extragalactic Radio Transient FIRST J141918.9+394036 | We present the discovery of a slowly evolving, extragalactic radio transient, FIRST J141918.9+394036, identified by comparing a ...

Radio flares uniquely probe the neutron star merger populations as many events from past decades could still be detectable. Nonetheless, no radio flare observation has been reported to date. Here we show that the radio transient FIRST J1419+3940, first observed in 1993 and still detectable, ...

You need to enable JavaScript to run this app

July 1, 2020 - You need to enable JavaScript to run this app