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 MRK 478 220.4959 35.3708 219.98335 35.583266 202.392109 47.875746 59.0913373 65.0766343 294.6097 55756.9652777778 2011-07-14 23:10:00 55758.8334837963 2011-07-16 20:00:13 706041010 85.3236 80 85.3316 85.3396 0 85.3236 3 2 0 2 1 0 0 77.6366 77.6366 161.3897 1 PROCESSED 57602.6370601852 2016-08-02 15:17:22 56151 2012-08-12 00:00:00 55783.7198842593 2011-08-10 17:16:38 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 062028 The NLS1 galaxy Mrk 478 has exceptionally unusual properties. It shows up to a factor of five variability while keeping its spectral shape constant. Previous short XMM-Newton observations show that it is probably reflection-dominated, where light-bending effects are at their extreme. This is the only known object that shows such high variability while remaining in a reflection-dominated state. All other known objects show reflection-dominated spectra only when in a faint state, making their study very difficult. This object is reflection-dominated yet bright enough to study with relatively short exposures.Here we propose to observe this object for 80 ks. The goal is to detect the reflection hump using Suzaku capabilities above 10 keV and probe light-bending around this black hole. EXTRAGALACTIC COMPACT SOURCES 7 A ABDERAHMEN ZOGHBI EUR 6 AO6 PROBING EXTREME RELATIVISITC LIGHT-BENDING IN MRK 478 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706041010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '706041010'

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