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
|
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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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