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 | YY MEN | 74.6207 | -75.281 | 75.005816 | -75.353979 | 292.803657 | -80.004198 | 287.41045099 | -33.23069192 | 7.2587 | 54996.0772916667 | 2009-06-14 01:51:18 | 54998.5606365741 | 2009-06-16 13:27:19 | 404036010 | 106.9498 | 100 | 106.9578 | 106.9578 | 0 | 106.9498 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 104.0902 | 104.0902 | 214.5398 | 0 | PROCESSED | 57547.6240393518 | 2016-06-08 14:58:37 | 55378 | 2010-07-01 00:00:00 | 55008.2997106482 | 2009-06-26 07:11:35 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 041202 | The single K giant YY Men is one of the most active stars within 300 pc of the Sun, having produced 2 of the most powerful radio flares and 1 of the most powerful and long-duration optical flares ever detected. Its corona is one of the hottest and brightest known, with a *typical* X-ray luminosity of 32.0-32.5 (log erg/s) which most other cool stars only reach during major flares. We propose to obtain a 100-ksec observation of this hyperactive star to get a high S/N XIS exposure of its spectrum, particularly in the 5-10 keV region in which the XIS excels. We will study the He- and H-like Fe lines, search for 6.4 keV fluorescent emission, search for the presence of ultrahigh temperature and nonthermal spectral components, and look for correlations with simultaneous ATCA radio observations. | GALACTIC POINT SOURCES | 4 | B | STEPHEN DRAKE | USA | 4 | AO4 | THE EXTREME CORONAL PROPERTIES OF THE HYPERACTIVE K GIANT YY MEN | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404036010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404036010'
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