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 ETA CARINAE 161.2181 -59.7282 160.732192 -59.464935 202.181916 -58.969104 287.59637986 -0.67920855 289.0006 54274.2459259259 2007-06-23 05:54:08 54275.9015509259 2007-06-24 21:38:14 402039010 58.3961 50 58.4041 58.3961 0 58.4041 2 2 0 2 1 0 0 51.552 51.552 143.0099 1 PROCESSED 57539.0368981482 2016-05-31 00:53:08 54695 2008-08-17 00:00:00 54322.5140856482 2007-08-10 12:20:17 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021026 XMM-Newton observations in 2003 suggest that X-ray emission from Eta Carinae has a hard X-ray component above 10 keV in addition to the thermal emission with kT ~3-5 keV. The excess is apparently strongest near the 2-10 keV X-ray maximum, and possibly produced by very hot plasma or 1st-order Fermi acceleration of particles which then inverse Compton-upscatter UV seed photons from the stellar photospheres. We propose a 50 ksec observation of Eta Carinae with the Suzaku telescope during AO2, compare the X-ray spectrum with earlier observations and determine the level of emission at E >9 keV. GALACTIC POINT SOURCES 4 B KENJI HAMAGUCHI USA 2 AO2 HARD X-RAY EMISSION FROM ETA CARINAE HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402039010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402039010'

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