DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 NGC6251_LOBE_BGD2 245.3877 82.3337 246.650515 82.446813 101.124392 73.239187 115.79036875 31.61025625 299.99 55789.4176967593 2011-08-16 10:01:29 55789.6225 2011-08-16 14:56:24 706005020 11.178 10 11.178 11.178 0 11.178 1 1 0 1 1 0 0 9.788 9.788 17.6879 0 PROCESSED 57602.7824421296 2016-08-02 18:46:43 56173 2012-09-03 00:00:00 55805.1871527778 2011-09-01 04:29:30 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060004 We propose a Suzaku observation of "Gamma-ray lobe" accociated with a FR-I/II radio galaxy NGC6251. This is the second discovery next to Cen-A lobe with Fermi-LAT above 100 MeV. Compared to huge angular extent of Cen-A (~10 degree), the lobe of NGC 6251 is comfortably fit within an XIS-FOV, but its physical size is almost the same as Cen-A(~Mpc). We can therefore estimate the total power accumulated in lobe with much less uncertainties, and pressure balance between non-thermal electrons and external thermal cluster medium, that may reveal possible contributions of hidden protons in the lobe. We propose a 40 ksec observation of NGC 6251 centered on the NW-lobe, with additional 20 ksec x 2 observations at "OFF-src" positions to improve the background estimate. EXTRAGALACTIC COMPACT SOURCES 7 A JUN KATAOKA JAP 6 AO6 SUZAKU OBSERVATION OF "GAMMA-RAY LOBE'' IN A RADIO GALAXY NGC6251 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706005020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '706005020'

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