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 HD6903 17.4507 19.662 16.780979 19.395948 23.622213 11.325445 128.84764567 -42.9987034 70.0004 55031.3824305556 2009-07-19 09:10:42 55032.3578703704 2009-07-20 08:35:20 404034010 36.8135 35 36.8295 36.8135 0 36.8215 2 2 0 2 1 0 0 29.6727 29.6727 84.2639 0 PROCESSED 57547.8823958333 2016-06-08 21:10:39 55419 2010-08-11 00:00:00 55048.3029976852 2009-08-05 07:16:19 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041201 Suzaku XIS spectra of two G0 III Hertzsprung gap giants will complete a multi-observatory survey of the anomalous coronal behavior of this "X-ray deficient" class. The abrupt rise in coronal luminosities from the warmer giants to their cooler cousins, only slightly further advanced in evolution, might signal disruption of a "fossil" magnetosphere by a newly born solar-like dynamo. Key discriminators are the coronal energy distribution, composition (FIP bias), and sporadic hard emission associated with flaring. The proposed targets are the brightest not previously observed in X-rays at CCD resolution, and both have supporting HST UV spectra. Expanding the high energy sample of this key class of objects is essential for probing their contrary, but perhaps deeply significant, behavior. GALACTIC POINT SOURCES 4 B THOMAS AYRES USA 4 AO4 ANOMALOUS CORONAE IN THE MIDST OF THE HERTZSPRUNG GAP XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404034010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404034010'

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