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 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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