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 EXO 2030+375 308.0462 37.6555 307.574628 37.484842 325.998165 53.954312 77.15821576 -1.21997822 58.3113 56070.8420717593 2012-05-23 20:12:35 56072.789849537 2012-05-25 18:57:23 407089010 77.9451 75 77.9531 77.9569 0 77.9451 2 1 0 2 1 0 0 72.515 72.515 168.2558 0 PROCESSED 57605.5425347222 2016-08-05 13:01:15 56449 2013-06-06 00:00:00 56083.2088888889 2012-06-05 05:00:48 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 072013 We propose to observe the Be/X-ray binary system EXO 2030+375 in the ascending part of one of its normal periastron flares for 75ks to study the onset of the pulsar activity. Quasi-periodic hour-long flux oscillations were recently observed during INTEGRAL serendipitous observations and by EXOSAT in 1985. They appear to happen at the viscous time-scale of a disk, evidencing some kind of instability in the transition zone between the magnetosphere and the accretion disk. The broad-band coverage and sensitivity of Suzaku will allow us to investigate in detail the opening of the magnetic gate for this high-magnetic field neutron star by studying the high time resolution light curve, the shape of its pulsed signal and the spectral properties. GALACTIC POINT SOURCES 4 A CARLO FERRIGNO EUR 7 AO7 UNVEIL ACCRETION ONSET DURING A NORMAL OUTBURST OF EXO 2030+375 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407089010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407089010'

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