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 | 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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