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 | NGC 1313 | 49.5565 | -66.5364 | 49.405687 | -66.717354 | 341.391654 | -74.190914 | 283.40259478 | -44.62074971 | 201.281 | 54805.9606828704 | 2008-12-05 23:03:23 | 54808.2814699074 | 2008-12-08 06:45:19 | 703010010 | 91.4661 | 100 | 91.4981 | 91.4661 | 0 | 91.4981 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 78.7593 | 78.7593 | 200.4937 | 1 | PROCESSED | 57544.7004861111 | 2016-06-05 16:48:42 | 55188 | 2009-12-23 00:00:00 | 54822.6519328704 | 2008-12-22 15:38:47 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030038 | The nature of ultra luminous X-ray sources (ULX) is one of the most important unresolved issue in the modern astrophysics. We propose a 100 ks observation of an famous ULX, NGC 1313 X1, in order to search for Fe-K absorption lines, which are important spectral feature of Galactic black holes. Through the absorption feature, we will examine the nature of the ULX. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | KEN OHSUGA | JAP | 3 | AO3 | EXPLORING FE K-LINE ABSORPTION FEATURES FROM AN ULTRALUMINOUS X-RAY SOURCE, NGC 1313 X1 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703010010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703010010'
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