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 II PEG 358.7744 28.6284 358.137778 28.350132 11.171995 26.557383 108.23861581 -32.63076231 231.1411 56301.1877314815 2013-01-09 04:30:20 56303.6487962963 2013-01-11 15:34:16 407038010 17.0176 100 111.5065 111.5145 0 17.0176 3 3 0 3 1 0 0 107.9058 107.9058 212.6198 2 PROCESSED 57608.5074305556 2016-08-08 12:10:42 56724 2014-03-08 00:00:00 56363.602037037 2013-03-12 14:26:56 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070102 We propose a Suzaku observation of the powerful flare star II Peg with the high sensitivity of HXD. MAXI/GSC results from 2009 to 2011 show that this source exhibits the highest flaring activity with the largest luminosities and the largest fluxes. Then detection of the non-thermal emission is the most expected from this source at the on-set of a flare. We are to observe this target simultaneously with radio, infrared, optical, and X-ray bands for the first time. Our goal is (1) to detect impulsive non-thermal emission at the powerful II Peg flare (2) to obtain wide-band SED variability from radio to hard X-ray band, and (3) to establish unified view of stellar flare mechanism via the wide radio-X-ray band. GALACTIC POINT SOURCES 4 C YOHKO TSUBOI JAP 7 AO7 NON-THERMAL EMISSION ON THE POWERFUL STELLAR FLARE FROM II PEG XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407038010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407038010'

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