Supernovae 2014dg in UGC 2855

This page is devoted to information on Supernova 2014dg in UGC 2855.   Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page.   Information on the original web pages for many of these images can be found on the links web page.

image Discovered by Koichi Itagaki (Japan).   This one is a Type Ia (z=0.004).   This supernova is in the Constellation Camelopardalis.

The following is a list of images of this SN, in chronological order. Click on the name in the "Image Credit" column to see the image. Times and dates are in UT unless otherwise noted. If you know of any others, please tell me!

Image CreditDateMagFilterComments
Koichi Itagaki 2014/09/11.725Discovery
Seiichirob Kiyota 2014/09/11.94815.9V
Yasuo Sano and Nayoro Hokkaido 2014/09/12.00015.1U
T. Yusa, Y. Suzuki, and K. Kato 2014/09/12.53515.4U
Andrea Mantero 2014/09/12.917
T. Noguchi 2014/09/13.45314.9U
Nick James 2014/09/13.86015.2V
JM Llapasset 2014/09/13.88715.3CV
Denis Buczynski 2014/09/14.90214.6RC
Giancarlo Cortini 2014/09/14.92015.0C
William Wiethoff 2014/09/16.175 mirror
Gregor Krannich 2014/09/16.81714.3V
Enrique Díez 2014/09/18.99314.4
Paolo Campaner 2014/09/23.04214.3U
Yasuo Sano 2014/09/26.000C
JM Llapasset 2014/09/26.10914.2CV
Juan-Luis Glez. Carballo 2014/09/29.92313.9V
JM Llapasset 2014/10/03.11014.5CV
Manfred Mrotzek 2014/10/04.050C
JM Llapasset 2014/10/13.78814.9CV
Rafael Benavides 2014/10/18.07314.5CV
Marc Serrau 2014/10/21.91814.3I
Gianpiero Locatelli 2014/10/22.867C
JM Llapasset 2014/10/25.11915.2CV
Esteban Aguilar 2014/10/25.84814.9CR
JM Llapasset 2014/11/02.79215.6CV
JM Llapasset 2014/11/02.80116.7g'
JM Llapasset 2014/11/12.88916.0CV
Felipe Peña 2014/11/15.86415.5CR
Jose Carrillo 2014/12/17.87816.9C
Wim Cuppens 2014/12/18.38016.3R mirror
JM Llapasset 2014/12/24.82416.6CV
Wim Cuppens 2015/01/31.37017.3R
LeenElineDylan (LED) 2015/01/31.37018.1R

Light curves and Spectra:

If you have observations of this Supernova, please send them to vsnet-obs


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