the transient sky eran ofek caltech shri kulkarni arne rau mansi kasliwal brian cameron avishay...
TRANSCRIPT
The Transient Sky
Eran Ofek CALTECH
Shri KulkarniArne RauMansi KasliwalBrian CameronAvishay Gal-YamDale Frail
Collaborators:
Talk LayoutTransients along the EM spectrum (review)
Motivation & the future
Ongoing optical searches
Individual transients (optical)
M85 OT 2006-1
SN2006gy
Kulkarni, Ofek et al. (2006 Nature submitted)Rau et al. (2006)Ofek et al. in prep
Ofek et al. (2006 ApJL submitted)
Transients along the EM (-rays)
Gamma rays
Long-GRBs
Short GRBs
Soft -ray repeaters
Massive stars
NS mergers?
Neutron Stars (NS)
?
Transients along the EM (-rays)Ofek et al. (2006 ApJ accepted)
Z=0.09
Progenitor age<10Myr
if NS merger:for kick velocity>35km/s
velocity
sizeregionage
Transients along the EM (~cm)
RadioSearching for radio transients
Levinson, Ofek et al. (2002)
Future: ATA SKA
Comparison of 2 radio surveys
Found: 2 genuine transients
Transients in nearby galaxies
Gal-Yam, Ofek et al. (2006)
Ofek et al. in prep
Transients along the EM (visible)
Many searches
But usually focused on specific classes…
Solar systemSupernovaeMicrolensing…
Motivation
New / rare kind of transients
Peculiar members of known families
Test models
Standard candle systematics
Summary of physical motivation
The future - LSST
8.4m mirror6.5m effective diameter
Field of view = 9.65 sq. deg
The future - LSST
LSST details
6 filters: ugrizY
~7000 sq. deg. per night
First light: 2013, Cerro Pachon
~1min transients alert
Single image: r~24 mag After 10yrs r~28 mag
Sky for everyone - No proprietary period!
Back to the present(Our) ongoing searches
Nearby clusters
Fornax, Perseus
SDSS-II
cadence improvingFollow up
Palomar 5mMPG 2.2mLCO 2.5m
Palomar robotic 60”
Palomar 48” (10 sq. deg)
Nearby galaxies surveyPalomar robotic 60”
Kulkarni, Ofek, Rau, Kasliwal
Another strategy…
Individual transients
M85 OT 2006-1
SN2006gy
Kulkarni, Ofek et al. (2006)Rau et al. (2006)Ofek et al. in prep
Ofek et al. (2006; ApJL submitted)
In the past year:
Follow-up of 6 transients
Examples:
M85 Optical Transient 2006-1Kulkarni, Ofek et al. (2006; Nature submitted)Rau et al. (2006; ApJL submitted)Ofek et al. in prep
M85 Optical Transient 2006-1
M85 Optical Transient 2006-1
Width~350km/s
M85 Optical Transient 2006-1Late time Spitzer observation
M85 Optical Transient 2006-1Late time Spitzer observation
M85 Optical Transient 2006-1
Green to red color evolution
60 day plateau
Peak abs. mag I~-13
Expansion velocity ~350 km/s
Cool black-body at late time
E~1047 erg (in 3 months)
a-spherical expansion?
M85 Optical Transient 2006-1
…like: M31-RV & V838 Mon
M85 Optical Transient 2006-1
…like: M31-RV & V838 Mon
Favored model:
Stellar merger(Soker & Tylenda)
M85 Optical Transient 2006-1
Searching for his brothers
SN 2006gy Ofek et al. (2006 ApJL submitted)
Discovered: 2006 Sep 18 (Quimby et al.)
H line
AGN(?) - Prieto et al. (2006)
Type-IIn supernova (SN) ? Harutyunyan et al.Foley et al. (2006)
However,early type galaxyAbs mag @ peak ~-22~50 days rise time
SN Nucleus
Dust lane
FWHM ~0.”1
SN 2006gy Ofek et al. (2006 ApJL submitted)
SN 2006gy Ofek et al. (2006 ApJL submitted)
SN 2006gy Ofek et al. (2006 ApJL submitted)
S0 template with EB-V=0.16 extinction
SN+galaxy @ day~45
SN+galaxy @ day~7
SN 2006gy Ofek et al. (2006 ApJL submitted)
SN 2006gy Ofek et al. (2006 ApJL submitted)
VLA – no detection
Swift/XRT – no detection
Chandra (PI: Pooly)
VariableX-ray source @ galaxy center
Hybrid IIn/Ia SN (Type-IIa)
SN 2002ic -20.1 ~20 late type galaxy
SN 2005gj -20.4 ~55 blue Irr. MB~-17
SN 1997cy -20.1 <30 blue LSB MB~-17.7
SN 1999E <-19.5 <140 MB~-15 spiral
SN 2006gy -22.2 ~50 S0 galaxy
NameAbs V-m
ag
Rise time [d]
Environment
SN 2006gy Ofek et al. (2006 ApJL submitted)
energy
Total radiated energy ~1.2x1051 erg during 2 months
Type-Ia SN features in spectra
Assuming SN2006gy is a type-Ia SN
kinetic energy of a Ia SN (~1-2x1051 erg)
radiation
SN 2006gy Ofek et al. (2006 ApJL submitted)
Assuming SN2006gy is a type-Ia SN
kinetic energy of a Ia SN (~1-2x1051 erg)
radiationRequires:
Mass-loss rate ~10-2 M /yr
Over ~100yr
Common envelope? (Livio & Riess 2003)
SN 2006gy Ofek et al. (2006 ApJL submitted)
Summary
First year – “listening” mode:
The “known”: 1 LBV(?), 2+1(?) dwarf novae
The “known unknown”:
Out of 6 targets:
The “unknown unknown”
M85 OT 2006-1
SN 2006gy
Still waiting…
End
Transients along the EM (-rays)Ofek (2006b); Ofek et al. (2006a)
Extragalactic SGRs
M85 Optical Transient 2006-1
M85 Optical Transient 2006-1Comparison with other types of transients
Transients along the EM (~cm)
VLA J172059+38
VLA J121550+13 in NGC 4216
SN 2006gy Ofek et al. (2006)
Peak absolute V-band magnitude ~-22.2
Summary
Total radiated energy ~1.2x1051 erg during 2 months
Type-Ia SN features in spectra
SDSS-15207
SDSS-15207
Chandra (PI: Pooley)
XRT – no detectionVLA – no detection
SN 2006gy Ofek et al. (2006 ApJL submitted)
M85 Optical Transient 2006-1
Searching for his brothersin nearby galaxies…