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.
observation_id
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
exposure
awarded_exposure
xtend_exposure
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
xtend_data_mode1
xtend_data_mode2
1 201107010 WR140 305.1173 43.85438 304.69527 43.69509 327.37108 60.49166 80.93044 4.17659 237.18784 60636.83060 2024-11-22 19:56:04 60641.19241 2024-11-27 04:37:04 232.152 160.000 168.319 1 300000A0 168.319 0.000 0.000 0.000 11110 11310 PROCESSED 2025-07-17 08:13:29 2025-12-11 00:00:00 2024-12-11 19:17:05 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012182 Cosmic dust is a primary building block of the Earth, and its formation is a fundamental question. The massive colliding wind binary system, WR140, produces massive dust near periastron of its 7.9-year-long orbit. During the dust emission rise in previous binary cycles, the CIII line excess enhanced, and the X-ray emission declined oppositely, suggesting strong cooling of the WWC plasma produced a condition for dust formation. The star experiences another periastron passage on November 22nd, 2024. We propose 3 XRISM observations around that time to study the location and motion of the WWC plasma using the Fe XXV emission line. We also expect to detect the fluorescent Fe line, which strongly constrains the distance of the WWC apex from the stellar surface. STELLAR CORONAE, WINDS, AND YOUNG STARS 2 A KENJI HAMAGUCHI USA 1 NOR DYNAMICS OF THE EXPLOSIVE DUST FORMATION NEAR PERIASTRON IN WR140 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201107010/ Quick Look 304.96797 43.33095 305.7091 43.67595 305.22904 44.21621 304.48312 43.86759 304.54236 43.17226 305.28413 43.51432 304.80949 44.05646 304.06287 43.71083 326.69086 60.07695 327.96722 60.13482 327.86066 60.77402 326.55758 60.71485 80.4358 3.97106 81.02589 3.72335 81.27544 4.31442 80.68421 4.56258 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '201107010'

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