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 | TAU SCO | 248.9733 | -28.218 | 248.193759 | -28.116325 | 251.450612 | -6.120226 | 351.53478934 | 12.80506422 | 280.0312 | 54729.4179398148 | 2008-09-20 10:01:50 | 54729.7578009259 | 2008-09-20 18:11:14 | 403034040 | 13.9711 | 10 | 13.9711 | 13.9711 | 0 | 13.9711 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 12.8912 | 12.8912 | 29.35 | 0 | PROCESSED | 57543.857974537 | 2016-06-04 20:35:29 | 55148 | 2009-11-13 00:00:00 | 54780.4954050926 | 2008-11-10 11:53:23 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031121 | We are proposing to observe the magnetic hot star tau Sco (B0.2V) with six Suzaku pointings of 10 ksec each. This star has a highly structured surface magnetic field at around 500 G, and its unusually hard emission has been associated with wind confinement in closed magnetic loops. Our proposal is to test this claim. The surface field sports a torus-like structure of closed loops with a magnetic axis that is tilted by nearly 90 degrees from the stellar rotation axis. We selected six phases to optimize the detection of hard X-ray variability from occultation of hot plasma confined in the torus field arrangement as it rotates about the star. The Suzaku data will be important for confronting models of interactions between line-driven winds and magnetic fields in massive stars. | GALACTIC POINT SOURCES | 4 | A | RICHARD IGNACE | USA | 3 | AO3 | X-RAYS FROM MAGNETICALLY CONFINED HOT PLASMA IN TAU SCO | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403034040/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403034040'
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